list of Solar System objects by size
{{Short description|Largest objects of the Solar System}}
File:solar system mass distribution ppm chart.svg chart of the relative mass distribution of the Solar System, each cubelet denoting 2{{e|24}} kg]]
This article includes a list of the most massive known objects of the Solar System and partial lists of smaller objects by observed mean radius. These lists can be sorted according to an object's radius and mass and, for the most massive objects, volume, density, and surface gravity, if these values are available.
These lists contain the Sun, the planets, dwarf planets, many of the larger small Solar System bodies (which includes the asteroids), all named natural satellites, and a number of smaller objects of historical or scientific interest, such as comets and near-Earth objects.
Many trans-Neptunian objects (TNOs) have been discovered; in many cases their positions in this list are approximate, as there is frequently a large uncertainty in their estimated diameters due to their distance from Earth.
Solar System objects more massive than 1021 kilograms are known or expected to be approximately spherical. Astronomical bodies relax into rounded shapes (spheroids), achieving hydrostatic equilibrium, when their own gravity is sufficient to overcome the structural strength of their material. It was believed that the cutoff for round objects is somewhere between 100 km and 200 km in radius if they have a large amount of ice in their makeup;{{cite web |title=The Dwarf Planets |last=Brown |first=M. |publisher=Caltech |url=http://www.gps.caltech.edu/~mbrown/dwarfplanets/ |access-date=2008-09-25 |archive-url=https://web.archive.org/web/20110116181239/http://www.gps.caltech.edu/~mbrown/dwarfplanets/ |archive-date=2011-01-16 |url-status=live }} however, later studies revealed that icy satellites as large as Iapetus (1,470 kilometers in diameter) are not in hydrostatic equilibrium at this time,{{cite web|url=https://www.planetary.org/blogs/emily-lakdawalla/2012/3389.html |title=Iapetus' peerless equatorial ridge |publisher=The Planetary Society |access-date=2020-01-04}} and a 2019 assessment suggests that many TNOs in the size range of 400–1,000 kilometers may not even be fully solid bodies, much less gravitationally rounded.{{cite web |url=http://www2.lowell.edu/~grundy/abstracts/2019.G-G.html |title=Gǃkúnǁʼhòmdímà and Gǃòʼé ǃhú |publisher=.lowell.edu |access-date=2020-01-04 |archive-date=2019-04-07 |archive-url=https://web.archive.org/web/20190407045339/http://www2.lowell.edu/~grundy/abstracts/preprints/2019.G-G.pdf }} Objects that are ellipsoids due to their own gravity are here generally referred to as being "round", whether or not they are actually in equilibrium today, while objects that are clearly not ellipsoidal are referred to as being "irregular."
Spheroidal bodies typically have some polar flattening due to the centrifugal force from their rotation, and can sometimes even have quite different equatorial diameters (scalene ellipsoids such as {{dp|Haumea}}). Unlike bodies such as Haumea, the irregular bodies have a significantly non-ellipsoidal profile, often with sharp edges.
There can be difficulty in determining the diameter (within a factor of about 2) for typical objects beyond Saturn {{xref|(see: {{slink|2060 Chiron|Physical characteristics}}, for an example)}}. For TNOs there is some confidence in the diameters, but for non-binary TNOs there is no real confidence in the masses/densities. Many TNOs are often just assumed to have Pluto's density of 2.0 g/cm3, but it is just as likely that they have a comet-like density of only 0.5 g/cm3.{{cite web |date=2006 |title=Small Body Density and Porosity: New Data, New Insights |publisher=Lunar and Planetary Science XXXVII |first1=D. T. |last1=Britt |first2=G. J. |last2=Consolmagno |first3=W. J. |last3=Merline |url=http://www.lpi.usra.edu/meetings/lpsc2006/pdf/2214.pdf |access-date=2008-12-16 |archive-url=https://web.archive.org/web/20081217064607/http://www.lpi.usra.edu/meetings/lpsc2006/pdf/2214.pdf |archive-date=2008-12-17 }}
For example, if a TNO is incorrectly assumed to have a mass of 3.59{{e|20}} kg based on a radius of 350 km with a density of 2 g/cm3 but is later discovered to have a radius of only 175 km with a density of 0.5 g/cm3, its true mass would be only 1.12{{e|19}} kg.
The sizes and masses of many of the moons of Jupiter and Saturn are fairly well known due to numerous observations and interactions of the Galileo and Cassini orbiters; however, many of the moons with a radius less than ≈100 km, such as Jupiter's Himalia, have far more uncertain masses.{{cite web |url=http://ssd.jpl.nasa.gov/?sat_phys_par |publisher=JPL (Solar System Dynamics) |title=Planetary Satellite Physical Parameters |date=2008-10-24 |access-date=2008-12-16}} Further out from Saturn, the sizes and masses of objects are less clear. There has not yet been an orbiter around Uranus or Neptune for long-term study of their moons. For the small outer irregular moons of Uranus, such as Sycorax, which were not discovered by the Voyager 2 flyby, even different NASA web pages, such as the National Space Science Data Center{{cite web |title=Uranian Satellite Fact Sheet |publisher=NASA (National Space Science Data Center) |last=Williams |first=D. R. |url=http://nssdc.gsfc.nasa.gov/planetary/factsheet/uraniansatfact.html |date=2007-11-23 |access-date=2008-12-12 |archive-url=https://web.archive.org/web/20100105183741/http://nssdc.gsfc.nasa.gov/planetary/factsheet/uraniansatfact.html |archive-date=2010-01-05 |url-status=live }} and JPL Solar System Dynamics, give somewhat contradictory size and albedo estimates depending on which research paper is being cited.
There are uncertainties in the figures for mass and radius, and irregularities in the shape and density, with accuracy often depending on how close the object is to Earth or whether it has been visited by a probe.
Graphical overview
File:Solar-system-top50-diameter.svg
File:Sun vs planets en.svg|Relative masses of the bodies of the Solar System. Objects smaller than Saturn are not visible at this scale.
File:Masses of the planets en.svg|Relative masses of the Solar planets. Jupiter at 71% of the total and Saturn at 21% dominate the system.
File:Masses of Solid Solar System bodies en.svg|Relative masses of the solid bodies of the Solar System. Earth at 48% and Venus at 39% dominate. Bodies less massive than Pluto are not visible at this scale.
File:Masses of all moons.png|Relative masses of the rounded moons of the Solar System. Mimas, Enceladus, and Miranda are too small to be visible at this scale.
Objects with radii over 400 km
File:Mass and radius large solar system objects.png
The following objects have a nominal mean radius of 400 km or greater. It was once expected that any icy body larger than approximately 200 km in radius was likely to be in hydrostatic equilibrium (HE).{{cite web
|title = How many dwarf planets are there in the outer solar system?
|publisher = California Institute of Technology
|last = Brown |first= Michael E.
|url = http://web.gps.caltech.edu/~mbrown/dps.html
|access-date = 28 April 2019}} However, {{dp|Ceres}} (r = 470 km) is the smallest body for which detailed measurements are consistent with hydrostatic equilibrium,{{Cite journal |doi = 10.1038/nature18955|pmid = 27487219|bibcode = 2016Natur.537..515P|title = A partially differentiated interior for (1) Ceres deduced from its gravity field and shape|year = 2016|last1 = Park|first1 = R. S.|last2 = Konopliv|first2 = A. S.|last3 = Bills|first3 = B. G.|last4 = Rambaux|first4 = N.|last5 = Castillo-Rogez|first5 = J. C.|last6 = Raymond|first6 = C. A.|last7 = Vaughan|first7 = A. T.|last8 = Ermakov|first8 = A. I.|last9 = Zuber|first9 = M. T.|last10 = Fu|first10 = R. R.|last11 = Toplis|first11 = M. J.|last12 = Russell|first12 = C. T.|last13 = Nathues|first13 = A.|last14 = Preusker|first14 = F.|journal = Nature|volume = 537|issue = 7621|pages = 515–517|s2cid = 4459985| url=https://resolver.sub.uni-goettingen.de/purl?gro-2/86708 }} whereas Iapetus (r = 735 km) is the largest icy body that has been found to not be in hydrostatic equilibrium.{{cite web|url=http://www.planetary.org/blogs/emily-lakdawalla/2012/3389.html|title=Iapetus' peerless equatorial ridge}} The known icy moons in this range are all ellipsoidal (except Proteus), but trans-Neptunian objects up to 450–500 km radius may be quite porous.{{cite journal |last1=Grundy |first1=W.M. |last2=Noll |first2=K.S. |last3=Buie |first3=M.W. |last4=Benecchi |first4=S.D. |last5=Ragozzine |first5=D. |last6=Roe |first6=H.G. |title=The mutual orbit, mass, and density of transneptunian binary Gǃkúnǁʼhòmdímà ({{mp|(229762) 2007 UK|126}}) |journal=Icarus |date=December 2019 |volume=334 |pages=30–38 |doi=10.1016/j.icarus.2018.12.037 |s2cid=126574999 |url=http://www2.lowell.edu/~grundy/abstracts/preprints/2019.G-G.pdf |archive-url=https://web.archive.org/web/20190407045339/http://www2.lowell.edu/~grundy/abstracts/preprints/2019.G-G.pdf |archive-date=2019-04-07 }}
For simplicity and comparative purposes, the values are manually calculated assuming that the bodies are all spheres. The size of solid bodies does not include an object's atmosphere. For example, Titan looks bigger than Ganymede, but its solid body is smaller. For the giant planets, the "radius" is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure.{{cite web|url=http://nssdc.gsfc.nasa.gov/planetary/factsheet/uranusfact.html|title=Uranus Fact Sheet}}
Because Sedna and Máni have no known moons, directly determining their mass is impossible without sending a probe (estimated to be from 1.7x1021 to 6.1×1021 kg for Sedna{{cite web |title=90377 Sedna |work=Universe Guide |date=12 September 2022 |url=https://www.universeguide.com/kuiperbeltobject/316/sedna |access-date=2023-08-06 |last1=Guide |first1=Universe }}).
class="wikitable sortable" |
rowspan=2 style="font-weight: normal;" | Body{{notetag|name=A|text=Name of body, including alternative names using Roman numerals to designate moons (such as "Saturn I" for Mimas), and numbers to designate minor planets}}
! rowspan=2 class="unsortable"| Image ! colspan=2 style="font-weight: normal;" | Radius{{notetag|name=B|Mean radius including uncertainties}} ! colspan=2 | Volume ! colspan=2 | Mass ! colspan="2" |Surface area ! data-sort-type="number" | Density ! colspan=2 style="font-weight: normal;" | Gravity{{notetag|name=Gravity|text=Given as surface gravity (1 bar for gaseous planets)}} ! rowspan=2 | Type ! rowspan=2 data-sort-type="number"|Discovery |
---|
data-sort-type="number" | (km)
! data-sort-type="number" | (R🜨) ! data-sort-type="number" | (109 km3) ! data-sort-type="number" | ({{abbr|V🜨|Given in multiples of Earth's volume}}) ! data-sort-type="number" | (1021 kg) ! data-sort-type="number" | (M🜨) !(106 km2) !🜨 ! data-sort-type="number" | (g/cm3) ! data-sort-type="number" | (m/s2) ! data-sort-type="number" | (🜨) |
style="background-color: #FBEC5D;" align=center
|Sun |bgcolor=black| File:The Sun in white light.jpg |{{small|109.2}}NASA/JPL, [https://solarsystem.nasa.gov/solar-system/sun/by-the-numbers/ Our Sun, by the numbers] Accessed 2020 Oct 22 |{{sort|2|prehistoric}} |
style="background-color: #C4C4C4;" align=center
|bgcolor=black| File:Jupiter OPAL 2024.png !{{val|69911|6}}NASA/JPL [https://ssd.jpl.nasa.gov/?planet_phys_par Planets and Pluto: Physical Characteristics] Last updated 2020-May-29 |10.97 |1,431,280 |1,321 |317.83 |120.41 |2.528 |gas giant planet; has rings |{{sort|5|prehistoric}} |
style="background-color: #C4C4C4;" align=center
|bgcolor=black| File:Saturn square crop.jpg !{{val|58232|6}} |9.140 |827,130 |764 |95.162 |83.54 |1.065 |gas giant planet; has rings |{{sort|8|prehistoric}} |
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| Uranus |bgcolor=black| File:Uranus Voyager2 color calibrated.png |3.981 |68,340 |63.1 |14.536 |15.85 |0.886 |ice giant planet; has rings | 1781 |
style="background-color: #C4C4C4;" align=center
|bgcolor=black| File:Neptune Voyager2 color calibrated.png |3.865 |62,540 |57.7 |17.147 |14.94 |1.137 |ice giant planet; has rings | 1846 |
style="background-color: #D5D5D5;" align=center
|bgcolor=black| File:The Blue Marble (remastered).jpg |1 |1,083.21 |1 |1 |1 |9.81 |1 |{{sort|1|prehistoric}} |
style="background-color: #D5D5D5;" align=center
|bgcolor=black| File:Venus 2 Approach Image.jpg |0.9499 |928.43 |0.857 |0.815 |0.903 |0.905 |{{sort|4|prehistoric}} |
style="background-color: #D5D5D5;" align=center
|Mars |bgcolor=black| File:Mars - August 30 2021 - Flickr - Kevin M. Gill.png |0.5320 |163.18 |0.151 |0.107 |0.283 |0.379 |{{sort|6|prehistoric}} |
style="background-color: #FFE8E8;" align=center
|Ganymede |bgcolor=black| File:Ganymede JunoGill 2217.jpg !{{val|2634.1|0.3}} |0.4135 |76.30 |0.0704 !{{val|148.2}} |0.0248 |0.171 !{{val|1.936}} |1.428 |0.146 |moon of Jupiter (icy) | 1610 |
style="background-color: #FFFFCC;" align=center
|Titan |bgcolor=black| File:Titan in true color.jpg !{{val|2574.73|0.09|fmt=gaps}} |0.4037{{efn|name=equatorial|text=Radius estimated using equatorial radius and assuming body is spherical}} |71.50 |0.0658 !{{val|134.5}} |0.0225 |0.163 !{{val|1.880|0.004}} |1.354 |0.138 |moon of Saturn (icy) | 1655 |
style="background-color: #D5D5D5;" align=center
|bgcolor=black| File:Mercury in true color.jpg |0.3829 |60.83 |0.0562 |0.0553 |0.147 |0.377 |{{sort|7|prehistoric}} |
style="background-color: #FFE8E8;" align=center
|Callisto |bgcolor=black| File:Callisto - July 8 1979 (38926064465).jpg |0.3783 |58.65 |0.0541 !{{val|107.6}} |0.018 |0.143 !{{val|1.834|0.003}} |1.23603 |0.126 |moon of Jupiter (icy) | 1610 |
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|Io |bgcolor=black| File:Io highest resolution true color.jpg |0.2859 |25.32 |0.0234 !{{val|89.32}} |0.015 |0.082 !{{val|3.528|0.006}} |1.797 |0.183 |moon of Jupiter (terrestrial) | 1610 |
style="background-color: #B0E0E6;" align=center
|Moon |bgcolor=black| File:FullMoon2010.jpg !{{val|1737.4|.1}}[https://ssd.jpl.nasa.gov/?sat_phys_par Planetary Satellite Physical Parameters] |0.2727 |21.958 |0.0203 !{{val|73.46}}[https://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html Moon Fact Sheet] |0.0123 |0.074 |1.625 |0.166 |moon of Earth (terrestrial) |{{sort|3|prehistoric}} |
style="background-color: #FFE8E8;" align=center
|Europa |bgcolor=black| File:Europa in natural color.png |0.2450 |15.93 |0.0147 !{{val|48.00}} |0.008035 |0.06 !{{val|3.013|0.005}} |1.316 |0.134 |moon of Jupiter (terrestrial) | 1610 |
style="background-color: #DDEEFF;" align=center
|Triton |bgcolor=black| File:Triton.usgs23.png !{{val|1353.4|0.9}}{{efn|name=equatorial}} |0.2124{{efn|name=equatorial}} |10.38 |0.0096 !{{val|21.39|0.03}} |0.003599 |0.045 !{{val|2.061}} |0.782 |0.0797 |moon of Neptune (icy) | 1846 |
style="background-color: #E6E6E6;" align="center"
|Pluto |bgcolor=black| File:Pluto in True Color - High-Res.jpg !{{val|1188.3|0.8|fmt=gaps}} |0.187 |7.057 |0.00651 !{{val|13.03|0.03}} |0.0022 |17.79 |0.034 !{{val|1.854|0.006}} |0.620 |0.063 |dwarf planet; plutino; multiple | 1930 |
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|Eris |style="background:#420001;"| File:Eris and dysnomia2.jpg !{{val|1163|6|fmt=gaps}}{{efn|name=various|text=Radius has been determined by various methods, such as optical (Hubble), thermal (Spitzer), or direct imaging via spacecraft}} {{cite journal |last1=Sicardy |first1=B. |display-authors=etal. |date=2011 |title=Size, density, albedo and atmosphere limit of dwarf planet Eris from a stellar occultation |journal=European Planetary Science Congress Abstracts |volume=6 |page=137 |url=http://meetingorganizer.copernicus.org/EPSC-DPS2011/EPSC-DPS2011-137-8.pdf |access-date=2011-09-14 |bibcode=2011epsc.conf..137S }} |0.1825{{efn|name=various}} |6.59 |0.0061 |0.0028 |17 |0.033 !{{val|2.52|0.07}} |{{Gr|16.7|1163}} |0.083 | 2003 |
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|{{dp|Haumea}} |bgcolor=black| File:Haumea Hubble.png !{{val|798|6}} to 816{{Cite web|title=The size, shape, density and ring of the dwarf planet Haumea|url=http://www.astrosurf.com/sogorb/occultations/nature24051.pdf}} | 0.12 |1.98{{efn|name=WolframVolume|text=Calculated in Wolfram Alpha using semi axes of {{val|1050|x|840|x|537}} ([https://www.wolframalpha.com/input/?i=ellipsoid+volume+semi-axis+lengths+1050+840+537 Ellipsoid volume: 1.98395×10^9 km3])}} |0.0018 |0.00066 |8.14 |0.016 {{cite journal|author1=Dunham, E. T.|author2=Desch, S. J.|author3=Probst, L.|date=April 2019|title=Haumea's Shape, Composition, and Internal Structure|journal=The Astrophysical Journal|volume=877|issue=1|page=11|arxiv=1904.00522|bibcode=2019ApJ...877...41D|doi=10.3847/1538-4357/ab13b3|s2cid=90262114 |doi-access=free }} {{efn|name=haumea|Best fit, assuming Haumea is in hydrostatic equilibrium}} |0.401 |0.0409 |dwarf planet; | 2004 |
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|Titania |bgcolor=black| File:Titania (moon) color, cropped.jpg |0.1237{{efn|name="three radii" |text=Radius estimated by using three radii and assuming body is spheroid}} |2.06 |0.0019 !{{val|3.40|0.06}} |0.00059 |0.015 !{{val|1.711|0.005}} |0.378 |0.0385 | 1787 |
style="background-color: #FFFFCC;" align="center"
|Rhea |bgcolor=black| File:Rhea hi-res PIA07763.jpg !{{val|763.8|1.0}}{{efn|name="three radii"}} |0.1199{{efn|name="three radii"}} |1.87 |0.0017 !{{val|2.307}} |0.00039 |0.014 !{{val|1.236|0.005}} |0.26 |0.027 | 1672 |
style="background-color: #CCFFCC;" align=center
|Oberon |bgcolor=black| File:Oberon in true color by Kevin M. Gill.jpg !{{val|761.4|2.6}}{{efn|name=equatorial}} |0.1195{{efn|name=equatorial}} |1.85 |0.0017 !{{val|3.08|0.09}} |0.0005 |0.014 !{{val|1.63|0.05}} |0.347 |0.035 | 1787 |
style="background-color: #FFFFCC;" align="center"
|Iapetus |bgcolor=black| File:Iapetus 706 1419 1.jpg |0.1153 |1.66 |0.0015 !{{val|1.806}} |0.00033 |6.8 |0.013 !{{val|1.088|0.013}} |0.223 |0.0227 | 1671 |
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|{{dp|Makemake}} |bgcolor=black| File:Makemake moon Hubble image with legend (cropped).jpg !{{val|715|19 |
11}}{{cite journal|author=M.E. Brown|year=2013|arxiv=1304.1041|title=On the size, shape, and density of dwarf planet Makemake|journal=The Astrophysical Journal Letters|volume=767|issue=1|pages=L7(5pp)|doi=10.1088/2041-8205/767/1/L7|bibcode = 2013ApJ...767L...7B |s2cid=12937717}}
|0.112 |1.53 |0.0014 !{{val|3.1|p=≈ }} |0.00053 |6.4 |0.013 !{{val|2.1|p=≈ }} |0.57 |0.0581 | 2005 |
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|Gonggong |bgcolor=black| File:2007 OR10 and its moon.png !{{val|615|25}}{{cite journal |title=The mass and density of the dwarf planet (225088) 2007 OR10 |first1=Csaba |last1=Kiss |first2=Gabor |last2=Marton |first3=Alex H. |last3=Parker |first4=Will |last4=Grundy |first5=Aniko |last5=Farkas-Takacs |first6=John |last6=Stansberry |first7=Andras |last7=Pal |first8=Thomas |last8=Muller |first9=Keith S. |last9=Noll |first10=Megan E. |last10=Schwamb |first11=Amy C. |last11=Barr |first12=Leslie A. |last12=Young |first13=Jozsef |last13=Vinko |journal=Icarus |pages=3–10 |arxiv=1903.05439 |doi=10.1016/j.icarus.2019.03.013 |bibcode=2018DPS....5031102K |volume=334|year=2019 |s2cid=119370310 }} |0.0983 |1.03 |0.0009 !{{val|1.75|0.07}} |0.00029 |4.753 |0.009 !{{val|1.72|0.16}} |0.3 |0.0306 |dwarf planet; resonant SDO (3:10) | 2007 |
style="background-color: #E5E5FF;" align=center
|Charon |bgcolor=black| File:Charon in True Color - High-Res.jpg !{{val|606.0|0.5}} |0.0951 |0.932 |0.0009 !{{val|1.586|0.015}} |0.00025 |0.009 !{{val|1.70|0.02}} |0.288 |0.0294 | 1978 |
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|Umbriel |bgcolor=black| File:PIA00040 Umbrielx2.47.jpg |0.0918 |0.837 |0.0008 !{{val|1.28|0.03}} |0.00020 |0.008 !{{val|1.39|0.16}} |0.234 |0.024 | 1851 |
style="background-color: #CCFFCC;" align="center"
|Ariel |bgcolor=black| File:Ariel in monochrome.jpg |0.0909 |0.813 |0.0007 !{{val|1.25|0.02}} |0.000226 |0.008 !{{val|1.66|0.15}} |0.269 |0.027 | 1851 |
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|Dione |bgcolor=black| File:Dione in natural light.jpg |0.0881 |0.741 |0.0007 !{{val|1.095}} |0.000183 |0.008 !{{val|1.478|0.003}} |0.232 |0.0237 | 1684 |
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|Quaoar |bgcolor=black| File:Quaoar-weywot hst.jpg !{{val|543|2}} |0.0879 |0.737 |0.0007 !{{val|1.20|0.05}}{{Cite Q|Q116754015|display-authors=1}} |0.0002 |3.83 |0.008 |0.3 |0.0306 |dwarf planet; cubewano; binary; has rings | 2002 |
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|Tethys |bgcolor=black| File:PIA18317-SaturnMoon-Tethys-Cassini-20150411.jpg |0.0834 |0.624 |0.0006 !{{val|0.617}} |0.000103 |0.007 !{{val|0.984|0.003}}Roatsch Jaumann et al. 2009, p. 765, Tables 24.1–2 |0.145 |0.015 | 1684 |
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|Ceres |bgcolor=black| File:Ceres - RC3 - Haulani Crater (22381131691) (cropped).jpg |0.0742 |0.433 |0.0004 {{cite web |title = Dawn Journal, May 28, 2015 |last = Rayman |first = M. D. |publisher = Jet Propulsion Laboratory |url = http://dawnblog.jpl.nasa.gov/2015/05/28/dawn-journal-may-28-2015/ |date = 28 May 2015 |access-date = 23 July 2015 |archive-url = https://web.archive.org/web/20150530075157/http://dawnblog.jpl.nasa.gov/2015/05/28/dawn-journal-may-28-2015/ |archive-date = 30 May 2015 }} |0.000157 !{{val|2.17}} |0.28 |0.029 | 1801 |
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|Orcus |bgcolor=black| File:Orcus-vanth hst2.jpg !{{val|455|25|20}} |0.0719 |0.404 |0.0004 |0.000092 | | |0.2 |0.0204 |dwarf planet; plutino; binary | 2004 |
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|Sedna |bgcolor=black| File:Sedna PRC2004-14d.jpg !{{val|453|157|129}} |0.0785 |0.516 |0.0005 ! | | | ! | | |dwarf planet; sednoid; detached object | 2003 |
align="center"
|Salacia |bgcolor=black| File:Salacia Hubble.png !{{val|423|11}} |0.0664 |0.373 |0.0003 |0.000082 | | !{{val|1.5|0.1}}{{cite journal |title=Mutual Orbit Orientations of Transneptunian Binaries |url=http://www2.lowell.edu/~grundy/abstracts/preprints/2019.TNB_orbits.pdf |first1=W. M. |last1=Grundy |first2=K. S. |last2=Noll |first3=H. G. |last3=Roe |first4=M. W. |last4=Buie |first5=S. B. |last5=Porter |first6=A. H. |last6=Parker |first7=D. |last7=Nesvorný |first8=S. D. |last8=Benecchi |first9=D. C. |last9=Stephens |first10=C. A. |last10=Trujillo |journal=Icarus |year=2019 |doi=10.1016/j.icarus.2019.03.035 |bibcode=2019Icar..334...62G |issn=0019-1035 |volume=334 |pages=62–78 |s2cid=133585837 |access-date=2019-10-26 |archive-date=2020-01-15 |archive-url=https://web.archive.org/web/20200115091416/http://www2.lowell.edu/~grundy/abstracts/preprints/2019.TNB_orbits.pdf }} |{{Gr|0.4922|446.5}} |0.0168 | 2004 |
colspan="15" style="font-size: 0.9em; font-weight: normal; text-align: left; padding: 6px 4px;"|
:{{legend2|#FBEC5D|border=1px solid #bbb|star}} {{legend2|#C4C4C4|border=1px solid #bbb|giant planet}} {{legend2|#D5D5D5|border=1px solid #bbb|terrestrial planet}} {{legend2|#E6E6E6|border=1px solid #AAF3CD|presumed dwarf planet}} {{legend2|#B0E0E6|border=1px solid #AAF3CD|moon of Earth}} {{legend2|#FFE8E8|border=1px solid #AAF3CD|moon of Jupiter}} {{legend2|#FFFFCC|border=1px solid #E6E600|moon of Saturn}} {{legend2|#CCFFCC|border=1px solid #00FF00|moon of Uranus}} {{legend2|#DDEEFF|border=1px solid #8FC7FF|moon of Neptune}} {{legend2|#E5E5FF|border=1px solid #8FC7FF|moon of Pluto}} |
Smaller objects by mean radius
= From 200 to 399 km =
All imaged icy moons with radii greater than 200 km except Proteus are clearly round, although those under 400 km that have had their shapes carefully measured are not in hydrostatic equilibrium. The known densities of TNOs in this size range are remarkably low ({{val|1|-|1.2|u=g/cm3}}), implying that the objects retain significant internal porosity from their formation and were never gravitationally compressed into fully solid bodies.
{{sticky header}}
class="wikitable sortable sticky-header-multi" |
style="font-weight:normal; width:110px;"| Body{{notetag|name=A}}
! class="unsortable"| Image ! data-sort- type="number" style="width:85px; font-weight:normal;"| Radius{{notetag|name=B}} ! data-sort-type="number" vkwidth=75 | Mass ! data-sort- type="number" style="width:65px;"| Density ! Type{{notetag|name=default|text=Figures from default source Johnston's Archive—List of Known Trans-Neptunian Objects,{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} if otherwise not mentioned in the References column}} ! class="unsortable" style="width: 3.8em; text-align: center;" | Refs{{notetag|name=Refs}} |
---|
Máni {{small|307261}} |bgcolor=black| File:2002 MS4 Hubble 8x upscale.png |align=center | {{val|398|12}} |align=center | – |align=center | – |align=center | {{cite journal |display-authors = etal |first1 = F. L. |last1 = Rommel |first2 = F. |last2 = Braga-Ribas |first3 = J. L. |last3 = Ortiz |first4 = B. |last4 = Sicardy |first5 = P. |last5 = Santos-Sanz |first6 = J. |last6 = Desmars |title = A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS4 measured from stellar occultations |journal = Astronomy & Astrophysics |date = October 2023 |volume = 678 |id = A167 |pages = 25 |doi-access = free |doi = 10.1051/0004-6361/202346892 |arxiv = 2308.08062 |bibcode = 2023A&A...678A.167R |s2cid = 260926329}} |
{{mpl-|55565|2002 AW|197}} {{small|55565}} | style="background:#181818;"| File:55565-2002aw197 hst.jpg |align=center | {{val|384|19}} |align=center | – |align=center | – |cubewano |align=center | {{Cite journal |arxiv=1403.6309 |last1=Vilenius |first1= E. |display-authors=etal. |title="TNOs are Cool": A survey of the trans-Neptunian region X. Analysis of classical Kuiper belt objects from Herschel and Spitzer observations |journal=Astronomy & Astrophysics |volume=564 |pages=A35 |year=2014 |doi=10.1051/0004-6361/201322416 |bibcode=2014A&A...564A..35V |s2cid=118513049 }} |
Varda {{small|174567}} | style="background:#181818;"| File:Varda-ilmare hst.jpg |align=center | {{val|373|8}} |align=center | {{val|245|6}} |align=center | {{val|1.23|.04}} |align=center | {{cite journal |display-authors = etal |first1 = D. |last1 = Souami |first2 = F. |last2 = Braga-Ribas |first3 = B. |last3 = Sicardy |first4 = B. |last4 = Morgado |first5 = J. L. |last5 = Ortiz |first6 = J. |last6 = Desmars |date = August 2020 |title = A multi-chord stellar occultation by the large trans-Neptunian object (174567) Varda |journal = Astronomy & Astrophysics |volume = 643 |pages = A125 |doi = 10.1051/0004-6361/202038526 |arxiv = 2008.04818 |
{{mpl-|532037|2013 FY|27}} {{small|532037}} |bgcolor=black| File:2013 FY27 small.png |align=center | {{val|370|40}} |align=center | – |align=center | – |
{{mpl-|208996|2003 AZ|84}} {{small|208996}} | style="background:#181818;"| File:2003AZ84 Hubble small.png |align=center | {{val|362}} ~ {{val|386|6}} (assuming HE) |align=center | 150 ~ 210 (assuming HE) |align=center | {{val|0.76 |
|align=center | {{Cite journal
|display-authors = 6
|first1 = A. |last1 = Dias-Oliveira
|first2 = B. |last2 = Sicardy
|first3 = J. L. |last3 = Ortiz
|first4 = F. |last4 = Braga-Ribas
|first5 = R. |last5 = Leiva
|first6 = R. |last6 = Vieira-Martins
|first7 = G. |last7 = Benedetti-Rossi
|first8 = J. I. B. |last8 = Camargo
|first9 = M. |last9 = Assafin
|last10 = Gomes-Jú
|first11 = A. R. |last11 = nior
|first12 = T. |last12 = Baug
|first13 = T. |last13 = Chandrasekhar
|first14 = J. |last14 = Desmars
|first15 = R. |last15 = Duffard
|first16 = P. |last16 = Santos-Sanz
|date = July 2017
|title = Study of the Plutino Object (208996) 2003 AZ84 from Stellar Occultations: Size, Shape, and Topographic Features
|journal = The Astronomical Journal
|volume = 154
|issue = 1
|page = 13
|bibcode = 2017AJ....154...22D
|doi = 10.3847/1538-3881/aa74e9
|arxiv = 1705.10895|s2cid = 119098862 |doi-access = free }}
|-
|
| align="center" |350
| align="center" |–
| align="center" |–
|eTNO
|-
|{{mpl|2021 DR|15}}
|bgcolor=black|
|align=center | {{val|356}}
|align=center | –
|align=center | –
|SDO
|-
|Ixion
{{small|28978}}
| style="background:#181818;"| Image:28978-ixion hst.jpg
|align=center | {{val|354.8|.1}}
|align=center | –
|align=center | –
|align=center | {{cite journal
|first1 = Stephen E. |last1 = Levine
|first2 = Carlos A. |last2 = Zuluaga
|first3 = Michael J. |last3 = Person
|first4 = Amanda A. |last4 = Sickafoose
|first5 = Amanda A. |last5 = Bosh
|first6 = Michael |last6 = Collins
|date = April 2021
|title = Occultation of a Large Star by the Large Plutino (28978) Ixion on 2020 October 13 UTC
|journal = The Astronomical Journal
|volume = 161
|page = 210
|number = 5
|doi = 10.3847/1538-3881/abe76d
|bibcode = 2021AJ....161..210L|doi-access= free}}
|-
|{{mpl-|90568|2004 GV|9}}
{{small|90568}}
| style="background:#3c3c3c;"| File:2004-gv9 hst.jpg
|align=center | {{val|340|17}}
|align=center | –
|align=center | –
|cubewano
|align=center | {{cite journal
|title="TNOs are Cool": A survey of the trans-Neptunian region VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects
|author=Vilenius, E.
|author2=Kiss, C.
|author3=Mommert, M.
|year=2012
|journal=Astronomy & Astrophysics
|pages=A94
|volume=541
|doi=10.1051/0004-6361/201118743
|arxiv=1204.0697
|display-authors=etal
|bibcode = 2012A&A...541A..94V|s2cid=54222700
}}
|-
|{{mpl-|145452|2005 RN|43}}
{{small|145452}}
| style="background:#3c3c3c;"| File:2005-rn43 hst.jpg
|align=center | {{val|340|+28|-37}}
|align=center | –
|align=center | –
|cubewano
|-
|Varuna
{{small|20000}}
| style="background:#181818;"| File:20000-varuna hst.jpg
|align=center | {{val|327|77|51}}
|align=center | {{val|160|p=≈ }}
|align=center | {{val|0.99|.09|.02}}
|cubewano
|align=center | {{cite journal
|title=The thermal emission of Centaurs and Trans-Neptunian objects at millimeter wavelengths from ALMA observations
|first1=E. |last1=Lellouch
|first2=R. |last2=Moreno
|first3=T. |last3=Müller
|first4=S. |last4=Fornasier
|first5=P. |last5=Sanstos-Sanz
|first6=A. |last6=Moullet
|first7=M. |last7=Gurwell
|first8=J. |last8=Stansberry
|first9=R. |last9=Leiva
|first10=B. |last10=Sicardy
|first11=B. |last11=Butler
|first12=J. |last12=Boissier
|date=September 2019
|journal=Monthly Notices of the Royal Astronomical Society
|volume=488
|issue=3
|pages=3035–3044
|doi=10.1093/mnras/stz1880
|doi-access=free |arxiv=1709.06747}}
|-
|{{mpl-|55637|2002 UX|25}}
{{small|55637}}
| style="background:#310001;"| File:20131105 2002 UX25 hst.png
|align=center | {{val|332|15}}
|align=center | {{val|125|3}}
|align=center | {{val|0.82|0.11}}
|cubewano; binary
|align=center | {{·}}{{cite journal|author=M.E. Brown
|title=The density of mid-sized Kuiper belt object 2002 UX25 and the formation of the dwarf planets
|journal=The Astrophysical Journal
|volume=778
|issue=2
|pages=L34
|arxiv=1311.0553
|date=4 November 2013
|doi=10.1088/2041-8205/778/2/L34
|bibcode=2013ApJ...778L..34B|s2cid=17839077
}}
|-
|{{mpl-|145451|2005 RM|43}}
{{small|145451}}
| style="background:#3c3c3c;"| File:145451-2005rm43.jpg
|align=center | {{val|322}}
|align=center | –
|align=center | –
|SDO
|align=center | {{cite web
|title = TNO Results
|url = https://lesia.obspm.fr/lucky-star/results.php
|work = ERC Lucky Star Project
|publisher = Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (LESIA)
|access-date = 4 June 2023}}{{cite web
|title = Occultation by 2005 RM43 in 23 DEC 2018
|url = https://lesia.obspm.fr/lucky-star/campaigns/results/2005RM43_24_12_2018_prelim2.pdf
|work = ERC Lucky Star Project
|publisher = Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (LESIA)
|date = 24 December 2018
|access-date = 4 June 2023}}
|-
|Gǃkúnǁʼhòmdímà
{{small|229762}}
|bgcolor=black| File:2007 UK126 Hubble (crop).png
|align=center | {{val|321|14}}
|align=center | {{val|136.1|3.3}}
|align=center | {{val|1.02|0.17}}
|SDO; binary
|align=center | {{cite journal
|first1 = G. |last1 = Benedetti-Rossi
|first2 = B. |last2 = Sicardy
|first3 = M. W. |last3 = Buie
|first4 = J. L. |last4 = Ortiz
|first5 = R. |last5 = Vieira-Martins
|first6 = J. M. |last6 = Keller
|first7 = F. |last7 = Braga-Ribas
|first8 = J. I. B. |last8 = Camargo
|first9 = M. |last9 = Assafin
|first10 = N. |last10 = Morales
|first11 = R. |last11 = Duffard
|first12 = A. |last12 = Dias-Oliveira
|first13 = P. |last13 = Santos-Sanz
|display-authors = 6
|date = December 2016
|title = Results from the 2014 November 15th Multi-chord Stellar Occultation by the TNO (229762) 2007 UK126
|journal = The Astronomical Journal
|volume = 152
|issue = 6
|page = 11
|bibcode = 2016AJ....152..156B
|doi = 10.3847/0004-6256/152/6/156
|arxiv = 1608.01030
|s2cid = 119249473
|doi-access = free
|-
|{{mpl|2014 UZ|224}}
| bgcolor="black" | File:2014UZ224-ALMA.jpg
| align="center" | {{val|317.5|28.5|30.5}}
| align="center" | –
| align="center" | –
|SDO
| align="center" | {{cite journal
|title=Discovery and Physical Characterization of a Large Scattered Disk Object at 92 AU
|display-authors=etal
|first1=David W. |last1=Gerdes
|first2=Masao |last2=Sako
|first3=Stephanie |last3=Hamilton
|first4=Ke |last4=Zhang
|first5=Tali |last5=Khain
|first6=Juliette C. |last6=Becker
|journal=The Astrophysical Journal Letters
|volume=839
|pages=L15
|number=1
|date=2017
|doi=10.3847/2041-8213/aa64d8
|arxiv=1702.00731|bibcode=2017ApJ...839L..15G
|s2cid=35694455
|doi-access=free
}}
|-
|{{mpl-|470599|2008 OG|19}}
{{small|470599}}
|bgcolor=black|
|align=center | {{val|309.5|28|56.5}}
|align=center | –
|align=center | {{val|0.609|0.004}}
|SDO
|align=center | {{cite journal
|last1=Fernández-Valenzuela |first1=Estela
|last2=Ortiz |first2=Jose Luis
|last3=Duffard |first3=René
|title=2008 OG19: A highly elongated Trans-Neptunian Object
|journal=Monthly Notices of the Royal Astronomical Society
|volume= 456|issue= 3|pages= 2354–2360|year=2015
|doi= 10.1093/mnras/stv2739
|doi-access=free
|arxiv=1511.06584
|bibcode= 2016MNRAS.456.2354F|s2cid=73720001
|-
|{{mpl-|574372|2010 JO|179}}
{{small|574372}}
|bgcolor=black|
|align=center | {{val|309|p=≈ }}
|align=center | –
|align=center | –
|SDO
|-
|Dysnomia
{{small|Eris I}}
| style="background:#420001;"| File:Eris and dysnomia2.jpg
|align=center | {{val|307.5|60|50}}
|align=center | {{val|500}}
|align=center | {{val|0.7|0.5}}
|moon of Eris
|align=center | {{cite journal
|first1 = Michael E. |last1 = Brown
|first2 = Bryan |last2 = Butler
|title = Masses and densities of dwarf planet satellites measured with ALMA
|journal = The Planetary Science Journal
|date = October 2023
|volume = 4
|issue = 10
|id = 193
|pages = 6
|doi-access = free
|doi = 10.3847/PSJ/ace52a
|arxiv = 2307.04848
|bibcode = 2023PSJ.....4..193B
|s2cid = 259766266}}
|-
|{{mpl-|278361|2007 JJ|43}}
{{small|278361}}
|bgcolor=black|
|align=center | {{val|305|85|70}}
|align=center | –
|align=center | –
|cubewano
|-
|{{mpl-|523692|2014 EZ|51}}
{{small|523692}}
|bgcolor=black|
|align=center | {{val|288|p=> }}
|align=center | –
|align=center | –
|SDO
|align=center | {{cite web
|title = (523692) 2014 EZ51, 2019 February 25 occultation
|last1 = Loader |first1 = B.
|last2 = Hanna |first2 = W.
|url = http://www.occultations.org.nz/planet/2019/results/20190225_523692_2014EZ51_UCAC4_322-079801_Plot_Colour.png
|website = occultations.org.nz
|date = 25 February 2019
|access-date = 5 January 2020}}
|-
|{{mpl|2012 VP|113}}
|bgcolor=black|
|align=center | {{val|287|p=≈ }}
|align=center | –
|align=center | –
|align=center | {{cite web | url=http://www.johnstonsarchive.net/astro/tnoslist.html | title=List of known trans-Neptunian objects }}
|-
|{{mpl-|78799|2002 XW|93}}
{{small|78799}}
|bgcolor=black|
|align=center | {{val|283|36|37}}
|align=center | –
|align=center | –
|other TNO
|align=center | {{cite web
|title = Asteroid (78799) 2002 XW93
|work = Small Bodies Data Ferret
|url = https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=78799
|access-date = 17 November 2018
|archive-date = 18 November 2018
|archive-url = https://web.archive.org/web/20181118081527/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=78799
|url-status = dead
}}
|-
|{{mpl-|612911|2004 XR|190}}
{{small|612911}}
| style="background:#3c3c3c;"| File:2004-xr190 hst.jpg
|align=center | {{val|278|p=≈ }}
|align=center | –
|align=center | –
|SDO
|-
|{{mpl-|612533|2002 XV|93}}
{{small|612533}}
|bgcolor=black| File:2002xv93.jpg
|align=center | {{val|275|+11|-12}}
|align=center | –
|align=center | –
|align=center | {{cite journal | last1 = Mommert | first1 = Michael| last2 = Harris | first2 = A. W. | last3 = Kiss | first3 = C. | last4 = Pál | first4 = A. | last5 = Santos-Sanz | first5 = P. | last6 = Stansberry | first6 = J. | last7 = Delsanti | first7 = A. | last8 = Vilenius | first8 = E. | last9 = Müller | first9 = T. G. | first10 = N. | last10 = Peixinho| first11 = E. | last11 = Lellouch| first12 = N. | last12 = Szalai| first13 = F. | last13 = Henry| first14 = R. | last14 = Duffard| first15 = S. | last15 = Fornasier| first16 = P. | last16 = Hartogh| first17 = M. | last17 = Mueller| first18 = J. L. | last18 = Ortiz| first19 = S. | last19 = Protopapa| first20 = M. | last20 = Rengel| first21 = A. | last21 = Thirouin| title = TNOs are cool: A survey of the trans-Neptunian region—V. Physical characterization of 18 Plutinos using Herschel-PACS observations| doi = 10.1051/0004-6361/201118562 | journal = Astronomy & Astrophysics | volume = 541 | pages = A93 | date = May 2012| bibcode = 2012A&A...541A..93M | arxiv = 1202.3657 | s2cid = 119253817|display-authors=7}}
|-
|{{mpl|2015 RR|245}}
{{small|523794}}
|bgcolor=black|
|align=center | {{val|270|p=≈ }}
|align=center | –
|align=center | –
|resonant KBO {{small|(2:9)}}
|-
|{{mpl-|455502|2003 UZ|413}}
{{small|455502}}
| style="background:#3c3c3c;"| File:455502-2003uz413.jpg
|align=center | {{val|268|p=≈ }}
|align=center | –
|align=center | –
|-
|Vesta
{{small|4}}
|bgcolor=black| File:Vesta in natural color.jpg
|align=center | {{val|262.7|0.1}}
|align=center | {{val|259}}
|align=center | {{val|3.46}}
|belt asteroid type V
|align=center | {{cite journal
|author=Russell, C. T.
|display-authors=etal
|title=Dawn at Vesta: Testing the Protoplanetary Paradigm
|journal=Science
|volume=336
|issue=6082
|pages=684–686
|date=2012
|doi=10.1126/science.1219381 |pmid=22582253
|bibcode = 2012Sci...336..684R
|s2cid=206540168
|-
|{{mpl-|84922|2003 VS|2}}
{{small|84922}}
| style="background:#3c3c3c;"| File:84922-2003vs2 hst.jpg
|align=center | {{val|262|4}}
|align=center | –
|align=center | –
|-
|Pallas
{{small|2}}
|bgcolor=black| File:Potw1749a Pallas crop.png
|align=center | {{val|256|2}}
|align=center | {{val|204|3}}
|align=center | {{val|2.92|0.08}}
|belt asteroid type B
|align=center | Marsset, M., Brož, M., Vernazza, P. et al. The violent collisional history of aqueously evolved (2) Pallas. Nat Astron 4, 569–576 (2020). https://doi.org/10.1038/s41550-019-1007-5P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. Astronomy & Astrophysics 54, A56
|-
|{{mpl-|120348|2004 TY|364}}
{{small|120348}}
|bgcolor=black|
|align=center | {{val|256|+19|-20}}
|align=center | –
|align=center | –
|cubewano
|align=center |{{cite journal
|display-authors = 6
|first1 = E. |last1 = Lellouch
|first2 = P. |last2 = Santos-Sanz
|first3 = P. |last3 = Lacerda
|first4 = M. |last4 = Mommert
|first5 = R. |last5 = Duffard
|first6 = J. L. |last6 = Ortiz
|first7 = T. G. |last7 = Müller
|first8 = S. |last8 = Fornasier
|first9 = J. |last9 = Stansberry
|first10 = Cs. |last10 = Kiss
|first11 = E. |last11 = Vilenius
|first12 = M. |last12 = Mueller
|first13 = N. |last13 = Peixinho
|first14 = R. |last14 = Moreno
|first15 = O. |last15 = Groussin
|first16 = A. |last16 = Delsanti
|first17 = A. W. |last17 = Harris
|date = September 2013
|title = "TNOs are Cool": A survey of the trans-Neptunian region. IX. Thermal properties of Kuiper belt objects and Centaurs from combined Herschel and Spitzer observations
|url = http://www.aanda.org/articles/aa/pdf/2013/09/aa22047-13.pdf
|journal = Astronomy and Astrophysics
|volume = 557
|page = 19
|bibcode = 2013A&A...557A..60L
|doi = 10.1051/0004-6361/201322047
|access-date= 27 April 2019|arxiv= 1202.3657}}
|-
|Enceladus
{{small|Saturn II}}
|bgcolor=black| File:PIA17202-SaturnMoon-Enceladus-ApproachingFlyby-20151028.jpg
|align=center | {{val|252.1|0.2}}
|align=center | {{val|108.0|0.1}}
|align=center | {{val|1.609|0.005}}
|moon of Saturn
|-
|{{mpl-|84522|2002 TC|302}}
{{small|84522}}
| style="background:#3c3c3c;"| File:84522-2002tc302 hst.jpg
|align=center | {{val|250|7}}
|align=center | –
|align=center | –
|align=center | {{cite journal
|title = The large Trans-Neptunian Object {{mp|2002 TC|302}} from combined stellar occultation, photometry and astrometry data
|first1 = J. L. |last1 = Ortiz
|first2 = P. |last2 = Santos-Sanz
|first3 = B. |last3 = Sicardy
|first4 = G. |last4 = Benedetti-Rossi
|first5 = E. |last5 = Duffard
|first6 = N. |last6 = Morales
|journal = Astronomy & Astrophysics |arxiv = 2005.08881
|date = 18 May 2020|volume = A134 |page = 639 |doi = 10.1051/0004-6361/202038046 |s2cid = 218673812 }}
|-
|{{mpl-|202421|2005 UQ|513}}
{{small|202421}}
|bgcolor=black|
|align=center | {{val|249|32|38}}
|align=center | –
|align=center | –
|cubewano
|-
|Miranda
{{small|Uranus V}}
|bgcolor=black| File:Miranda mosaic in color - Voyager 2.png
|align=center | {{val|235.8|0.7}}
|align=center | {{val|65.9|7.5}}
|align=center | {{val|1.2|0.15}}
|moon of Uranus
{{cite journal|year=1988|doi=10.1016/0019-1035(88)90054-1|bibcode=1988Icar...73..427T|pages=427–441 |volume=73 | first=P. C.|last=Thomas|title=Radii, shapes, and topography of the satellites of Uranus from limb coordinates|journal=Icarus|issue=3}}
|-
|Dziewanna
{{small|471143}}
| style="background:#181818;"| File:471143-dziewanna hst.jpg
|align=center | {{val|235|+18|-5}}
|align=center | –
|align=center | –
|SDO
|-
|{{mpl-|145480|2005 TB|190}}
{{small|145480}}
| style="background:#3c3c3c;"| File:145480-2005tb190 hst.jpg
|align=center | {{val|232|31}}
|align=center | –
|align=center | –
|align=center | {{cite journal
|display-authors=etal
|last=Santos-Sanz |first=P.
|date=2012
|title="TNOs are Cool": A Survey of the Transneptunian Region IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS
|journal=Astronomy & Astrophysics
|volume=541
|pages=A92
|arxiv=1202.1481
|doi=10.1051/0004-6361/201118541
|bibcode=2012A&A...541A..92S|s2cid=118600525 }}
|-
|{{mpl-|26375|1999 DE|9}}
{{small|26375}}
|bgcolor=black|
|align=center | {{val|231|23}}
|align=center | –
|align=center | –
|align=center | {{cite book
|first1 = John |last1 = Stansberry
|first2 = Will |last2 = Grundy
|first3 = Mike |last3 = Brown
|first4 = Dale |last4 = Cruikshank
|first5 = John |last5 = Spencer
|first6 = David |last6 = Trilling
|first7 = Jean-Luc |last7 = Margot
|date = 2008
|chapter = Physical Properties of Kuiper Belt and Centaur Objects: Constraints from the Spitzer Space Telescope
|chapter-url = https://www.lpi.usra.edu/books/ssbn2008/7017.pdf
|title = The Solar System Beyond Neptune
|pages = 161–179
|publisher = University of Arizona Press
|isbn = 978-0-8165-2755-7
|arxiv = astro-ph/0702538
|bibcode = 2008ssbn.book..161S}}
|-
|{{mpl-|120132|2003 FY|128}}
{{small|120132}}
|bgcolor=black|
|align=center | {{val|230|11}}
|align=center | –
|align=center | –
|SDO
|-
|{{mpl-|84719|2002 VR|128}}
{{small|84719}}
|bgcolor=black|
|align=center | {{val|224|+24|-22}}
|align=center | –
|align=center | –
|-
|Vanth
{{small|Orcus I}}
| style="background:#181818;"|File:Orcus-vanth hst2.jpg
|align=center | {{val|221|5}}
|align=center | {{val|87|8}}
|align=center | {{val|1.5|1.0|0.5}}
|moon of 90482 Orcus
|align=center |{{cite journal
|first1=A. A. |last1=Sickafoose
|first2=A. S. |last2=Bosh
|first3=S. E. |last3=Levine
|first4=C. A. |last4=Zuluaga
|first5=A. |last5=Genade
|first6=K. |last6=Schindler
|first7=T. A. |last7=Lister
|first8=M. J. |last8=Person
|title=A stellar occultation by Vanth, a satellite of (90482) Orcus
|journal=Icarus
|volume=319
|pages=657–668
|date=February 2019
|doi=10.1016/j.icarus.2018.10.016
|arxiv=1810.08977
|bibcode=2019Icar..319..657S|s2cid=119099266
|-
|Hygiea
{{small|10}}
|bgcolor=black| File:SPHERE image of Hygiea.jpg
|align=center | {{val|216|4}}
|align=center | {{val|87.4|6.9}}
|align=center | {{val|2.06|0.20}}
|belt asteroid type C
|align=center |{{cite journal
|title=A basin-free spherical shape as an outcome of a giant impact on asteroid Hygiea
|url=https://www.eso.org/public/archives/releases/sciencepapers/eso1918/eso1918a.pdf
|display-authors=etal
|last1=Vernazza |first1=P.
|last2=Jorda |first2=L.
|last3=Ševeček |first3=P.
|last4=Brož |first4=M.
|last5=Viikinkoski |first5=M.
|last6=Hanuš |first6=J.
|journal=Nature Astronomy
|volume=273
|issue=2
|doi=10.1038/s41550-019-0915-8
|bibcode=2020NatAs...4..136V
|pages=136–141|year=2020
|hdl=10045/103308
|s2cid=209938346
|hdl-access=free
|-
|{{mpl-|444030|2004 NT|33}}
{{small|444030}}
|bgcolor=black|
|align=center | {{val|212|44|40}}
|align=center | –
|align=center | –
|cubewano
|-
|Proteus
{{small|Neptune VIII}}
|bgcolor=black| File:Proteus (Voyager 2).jpg
|align=center | {{val|210|7}}
|align=center | {{val|44}}
|align=center | {{val|1.3|p=≈ }}
|moon of Neptune
|-
|{{mpl-|303775|2005 QU|182}}
{{small|303775}}
|bgcolor=black|
|align=center | {{val|208|37}}
|align=center | –
|align=center | –
|SDO
|-
|Chaos
{{small|19521}}
|bgcolor=#181818| File:19521-chaos hst.jpg
|align=center | {{val|208|42|15}} equivalent
|align=center | –
|align=center | –
|cubewano
|-
|{{mpl-|119951|2002 KX|14}}
{{small|119951}}
| style="background:#3c3c3c;"| File:119951-2002kx14 hst.jpg
|align=center | {{val|207.5|0.5}}
|align=center | –
|align=center | –
|cubewano
|align=center |{{cite journal
|title=Stellar occultation by (119951) 2002 KX14 on April 26, 2012
|url=https://www.aanda.org/articles/aa/pdf/2014/11/aa24648-14.pdf
|display-authors=etal
|first1=A. |last1=Alvarez-Candal
|first2=J. L. |last2=Ortiz
|first3=N. |last3=Morales
|first4=Y. |last4=Jiménez-Teja
|first5=R. |last5=Duffard
|first6=B. |last6=Sicardy
|journal=Astronomy & Astrophysics
|volume=571
|issue=A48
|page=8
|date=November 2014
|doi=10.1051/0004-6361/201424648
|bibcode=2014A&A...571A..48A
|access-date=14 October 2019|doi-access=free
}}
|-
|{{mpl-|469372|2001 QF|298}}
{{small|469372}}
|bgcolor=#181818| File:(469372) 2001 QF298 hst.jpg
|align=center | {{val|204|+20|-22}}
|align=center | –
|align=center | –
|-
|Huya
{{small|38628}}
|bgcolor=black| File:Huya Hubble.png
|align=center | {{val|203|8}}
|align=center | {{val|50|p=> }}
|align=center | {{val|1.43|p=> }}
|align=center | {{Cite journal |first1=S. |last1=Fornasier |display-authors=etal. |arxiv=1305.0449 |title=TNOs are Cool: A survey of the trans-Neptunian region. VIII. Combined Herschel PACS and SPIRE observations of 9 bright targets at 70–500 μm |journal=Astronomy & Astrophysics |volume=555 |pages=A15 |date=6 May 2013 |doi=10.1051/0004-6361/201321329 |bibcode=2013A&A...555A..15F |s2cid=119261700 }}{{·}}{{cite journal
|title=Rotational properties of the binary and non-binary populations in the Trans-Neptunian belt
|url=https://www.aanda.org/articles/aa/full_html/2014/09/aa23567-14/aa23567-14.html
|first1=A. |last1=Thirouin
|first2=K. S. |last2=Knoll
|first3=J. L. |last3=Ortiz
|first4=N. |last4=Morales
|date=September 2014
|journal=Astronomy & Astrophysics
|volume=569
|number=A3
|page=20
|doi=10.1051/0004-6361/201423567
|arxiv=1407.1214|bibcode=2014A&A...569A...3T|s2cid=119244456
}}
|-
|{{mpl-|175113|2004 PF|115}}
{{small|175113}}
|bgcolor=black|
|align=center | {{val|203|+49|-38}}
|align=center | –
|align=center | –
|-
! colspan=14 style="font-size: 0.9em; font-weight: normal; text-align: left; padding: 6px 4px" |
Legend:
:SDO – scattered disc object
:cubewano – classical Kuiper belt object
:plutino – 2:3 orbital resonance with Neptune
|}
= From 100 to 199 km =
This list contains a selection of objects estimated to be between 100 and 199 km in radius (200 and 399 km in diameter). The largest of these may have a hydrostatic-equilibrium shape, but most are irregular. Most of the trans-Neptunian objects (TNOs) listed with a radius smaller than 200 km have "assumed sizes based on a generic albedo of 0.09" since they are too far away to directly measure their sizes with existing instruments. Mass switches from 1021 kg to 1018 kg (Zg). Main-belt asteroids have orbital elements constrained by (2.0 AU < a < 3.2 AU; q > 1.666 AU) according to JPL Solar System Dynamics (JPLSSD).{{cite web
|title=JPL definition of Main-belt Asteroid (MBA)
|publisher=JPL Solar System Dynamics
|url=http://ssd.jpl.ar.gov/sbdb_help.cgi?class=MBA
|access-date=12 March 2009}}{{dead link|date=September 2017 |bot=InternetArchiveBot |fix-attempted=yes }} Many TNOs are omitted from this list as their sizes are poorly known.
class="wikitable sortable sticky-header-multi" |
style="font-weight:normal; width:110px;"| Body{{notetag|name=A}}
! class="unsortable"| Image ! data-sort- type="number" style="width:85px; font-weight:normal;"| Radius{{notetag|name=B}} ! data-sort- type="number" style="width:75px;"| Mass ! Type ! class="unsortable" style="font-weight: normal; width: 3.8em; text-align: center;" | Refs{{notetag|name=Refs}} |
---|
{{mpl-|144897|2004 UX|10}} {{small|144897}} |bgcolor=black| |align=center | {{val|199|20}} |align=center | {{val|30|p=≈ }} |align=center |{{·}}{{cite journal | last1 = Thirouin | first1 = A. | last2 = Ortiz | first2 = J. L. | last3 = Duffard | first3 = R. | last4 = Santos-Sanz | first4 = P. | last5 = Aceituno | first5 = F. J. | last6 = Morales | first6 = N. | doi = 10.1051/0004-6361/200912340 | title = Short-term variability of a sample of 29 trans-Neptunian objects and Centaurs | journal = Astronomy & Astrophysics | volume = 522 | pages = A93 | year = 2010 | arxiv = 1004.4841|bibcode = 2010A&A...522A..93T | s2cid = 54039561 }} |
{{mpl-|33340|1998 VG|44}} {{small|33340}} |bgcolor=black| |align=center | {{val|199|20}} |align=center | {{val|47|p=≈ }} |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
{{mpl-|15789|1993 SC}} {{small|15789}} |bgcolor=black| |align=center | {{val|199|20}} |align=center | {{val|47|p=≈ }} |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
Mimas {{small|Saturn I}} |bgcolor=black| File:Mimas Cassini.jpg |align=center | {{val|198.2|0.3}} |align=center | {{val|37.49|0.03}} |
{{mpl-|35671|1998 SN|165}} {{small|35671}} |bgcolor=black| |align=center | {{val|196|20}} |align=center | |
{{mpl-|42301|2001 UR|163}} {{small|42301}} | style="background:#3c3c3c;"| File:42301-2001ur163 hst.jpg |align=center | {{val|176|p=≈ }} |align=center | |resonant KBO {{small|(4:9)}} |
{{mpl-|24835|1995 SM|55}} {{small|24835}} |bgcolor=black| |align=center | {{val|173}} (assuming albedo of 0.7) |align=center | ? |align=center | ? |cubewano |align=center | |
{{mpl-|126154|2001 YH|140}} {{small|126154}} |bgcolor=black| |align=center | {{val|172|20}} |align=center | {{val|85|p=≈ }} |resonant KBO {{small|(3:5)}} |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
1993 FW {{small|181708}} |bgcolor=black| |align=center | {{val|170.5}} |align=center | |TNO, second discovered |align=center |{{cite web | url=http://web.gps.caltech.edu/~mbrown/dps.html | title=Astronomer Mike Brown }} |
{{mpl-|552555|2010 ER|65}} {{small|552555}} |bgcolor=black| |align=center | {{val|170|20}} |align=center | {{val|30|p=≈ }} |SDO |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
Nereid {{small|Neptune II}} | bgcolor="black" | File:Nereid-Voyager2.jpg | align="center" | {{val|170|25}} | align="center" | |
{{mpl-|15874|1996 TL|66}} {{small|15874}} |bgcolor=black| |align=center | {{val|170|10}} |align=center | |SDO |
{{mpl-|230965|2004 XA|192}} {{small|230965}} |bgcolor=black| |align=center | {{val|170|60|47.5}} |align=center | |SDO |
{{mpl-|471137|2010 ET|65}} {{small|471137}} |bgcolor=black| |align=center | {{val|170|20}} |align=center | {{val|30|p=≈ }} |SDO |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
{{mpl-|119979|2002 WC|19}} {{small|119979}} | style="background:black;"| File:2002 WC19.jpg |align=center | {{val|169|p=≈ }} |align=center | {{val|77|5}} |resonant KBO {{small|(1:2)}}; binary |align=center |{{cite web |title = (119979) 2002 WC19 |publisher = Johnston's Archive |date = 27 May 2019 |first = Wm. Robert |last = Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-119979.html |
{{mpl-|612931|2005 CA|79}} {{small|612931}} |bgcolor=black| |align=center | {{val|167|20}} |align=center | {{val|60|p=≈ }} |resonant KBO {{small|(1:2)}} |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
Interamnia {{small|704}} |bgcolor=black| File:704 Interamnia VLT (2021), deconvolved.pdf |align=center | {{val|166|3}} |align=center | {{val|35.2|5.1}} |belt asteroid type F |align=center |{{cite journal |display-authors=etal |first1=J. |last1=Hanuš |first2=P. |last2=Vernazza |first3=M. |last3=Viikinkoski |first4=M. |last4=Ferrais |first5=N. |last5=Rambaux |first6=E. |last6=Podlewska-Gaca |title=(704) Interamnia: A transitional object between a dwarf planet and a typical irregular-shaped minor body |journal=Astronomy & Astrophysics |volume=633 |pages=A65 |arxiv=1911.13049 |doi=10.1051/0004-6361/201936639 |bibcode=2020A&A...633A..65H |year=2020 |s2cid=208512707 }}{{·}} |
Ilmarë {{small|Varda I}} | style="background:#181818;"| File:Varda-ilmare hst.jpg |align=center | {{val|163|18}} |align=center | |moon of 174567 Varda |align=center |{{cite web |title = (450894) 2008 BT18 |work = Johnston's Archive |date = 31 January 2015 |author = Johnston, Wm. Robert |url = http://www.johnstonsarchive.net/astro/astmoons/am-174567.html |access-date = 28 April 2019}} |
Europa {{small|52}} |bgcolor=black| File:52 Europa VLT (2021), deconvolved.pdf |align=center | {{val|160|2}} |align=center | {{val|23.9|3.8}} |belt asteroid type C |
Hiʻiaka {{small|Haumea I}} |bgcolor=#181818| File:Haumea Hubble.png |align=center | {{val|160|p=≈ }} |align=center | {{val|17.9|1.1}} |align=center |{{cite journal| doi = 10.1088/0004-6256/137/6/4766| last1 = Ragozzine| first1 = D.| last2 = Brown| first2 = M. E.| year = 2009| title = Orbits and Masses of the Satellites of the Dwarf Planet Haumea (2003 EL61)| journal = The Astronomical Journal| volume = 137| issue = 6| pages = 4766–4776| arxiv = 0903.4213| bibcode = 2009AJ....137.4766R| s2cid = 15310444}}{{·}} |
{{mpl-|307251|2002 KW|14}} {{small|307251}} |bgcolor=black| |align=center | {{val|160|20}} |align=center | {{val|30|p=≈ }} |cubewano |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
{{mpl-|469306|1999 CD|158}} {{small|469306}} |bgcolor=black| |align=center | {{val|155|20}} |align=center | {{val|48|p=≈ }} |resonant KBO {{small|(4:7)}} |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
{{mpl-|470316|2007 OC|10}} {{small|470316}} |bgcolor=black| |align=center | {{val|155|20}} |align=center | {{val|30|p=≈ }} |SDO |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
{{mpl-|145453|2005 RR|43}} {{small|145453}} |bgcolor=black| |align=center | {{val|150|20}} |align=center | {{val|60|p=≈ }} |cubewano |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
Davida {{small|511}} |bgcolor=black| File:511 Davida VLT (2021), deconvolved.pdf |align=center | {{val|149|2}} |align=center | {{val|26.6|7.3}} |belt asteroid type C |
{{mpl-|55636|2002 TX|300}} {{small|55636}} | style="background:#3c3c3c;"| File:55636-2002tx300 hst.jpg |align=center | {{val|143|5}} |align=center | |align=center |{{cite journal |display-authors=6 |last1=Elliot|first1=J. L. |last2=Person|first2=M. J. |last3=Zuluaga|first3=C. A. |last4=Bosh|first4=A. S. |last5=Adams|first5=E. R. |last6=Brothers|first6=T. C. |last7=Gulbis|first7=A. A. S. |last8=Levine|first8=S. E. |last9=Lockhart|first9=M. |date=2010 |title=Size and albedo of Kuiper belt object 55636 from a stellar occultation |url=http://www.dtic.mil/cgi-bin/GetTRDoc?AD=ADA541934&Location=U2&doc=GetTRDoc.pdf |archive-url=https://web.archive.org/web/20140222100203/http://www.dtic.mil/cgi-bin/GetTRDoc?AD=ADA541934&Location=U2&doc=GetTRDoc.pdf |archive-date=February 22, 2014 |journal=Nature |volume=465 |issue=7300 |pages=897–900 |doi=10.1038/nature09109 |pmid=20559381 |bibcode=2010Natur.465..897E|s2cid=4431420}} |
Actaea {{small|Salacia I}} |bgcolor=black| File:Salacia Hubble.png |align=center | {{val|143|12}} |align=center | |moon of 120347 Salacia |align=center |{{cite web |title = (120347) Salacia and Actaea |publisher = Johnston's Archive |date = 20 September 2014 |first = Wm. Robert |last = Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-120347.html |access-date = 13 June 2019}} |
Sylvia {{small|87}} |bgcolor=black| File:87 Sylvia VLT (2021), deconvolved.pdf |align=center | {{val|137|2}} |align=center | {{val|14.3|0.5}} |
{{mpl-|120178|2003 OP|32}} {{small|120178}} |bgcolor=black| |align=center | {{val|137|20}} |align=center | {{val|45|p=≈ }} |cubewano |align=center |{{cite web |date=25 May 2019 |title=List of Known Trans-Neptunian Objects |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/tnoslist.html |access-date=31 May 2019}} |
Lempo {{small|47171}} | style="background:#490405;"| File:1999TC36-Trujillo-HST.png |align=center | {{val|136|9}} |align=center | |align=center |{{cite web |title = (47171) Lempo, Paha, and Hiisi |publisher = Johnston's Archive |date = 8 October 2017 |first = Wm. Robert |last = Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-47171.html |access-date = 10 June 2019}} |
Eunomia {{small|15}} |bgcolor=black| File:15 Eunomia VLT (2021), deconvolved.pdf |align=center | {{val|135|2}} |align=center | {{val|30.5|1.9}} |belt asteroid type S |
Hyperion {{small|Saturn VII}} | bgcolor="black" | File:Hyperion true.jpg | align="center" | {{val|135|4}} | align="center" | {{val|5.62|0.05}} | align="center" |{{cite journal| doi = 10.1016/j.icarus.2010.01.025| last1 = Thomas| first1 = P. C.| date = July 2010| title = Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission| journal = Icarus| volume = 208| issue = 1| pages = 395–401| url = http://www.ciclops.org/media/sp/2011/6794_16344_0.pdf| bibcode = 2010Icar..208..395T| access-date = 2014-04-12| archive-date = 2018-12-23| archive-url = https://web.archive.org/web/20181223003125/http://www.ciclops.org/media/sp/2011/6794_16344_0.pdf}}{{·}}{{Cite web|title=Planetary Satellite Physical Parameters|url=https://ssd.jpl.nasa.gov/?sat_phys_par|website=JPL, NASA}} |
Euphrosyne {{small|31}} |bgcolor=black| File:31 Euphrosyne VLT (2021), deconvolved.pdf |align=center | {{val|134|2}} |align=center | {{val|16.5|2.6}} |
{{mpl-|26308|1998 SM|165}} {{small|26308}} | style="background:#420001;"| File:1998SM165-Trujillo-HST.jpg |align=center | {{val|134|14}} |align=center | {{val|6.87|1.8}} |resonant KBO {{small|(1:2)}} |align=center |{{cite web |title = (26308) 1998 SM165 and S/2001 (26308) 1 |work = Johnston's Archive |date = 21 September 2014 |first = Wm. Robert |last = Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-79360.html |
Cybele {{small|65}} |bgcolor=black| File:000065-asteroid shape model (65) Cybele.png |align=center | {{val|131.5|1.5}} |align=center | {{val|14.8|1.8}} |outer belt asteroid type C |align=center |Marsset et al. (2022) The equilibrium shape of (65) Cybele: primordial or relic of a large impact? |
Chariklo {{small|10199}} |bgcolor=black| File:10199 Chariklo Hubble.jpg |align=center | {{val|130|p=≈ }} |align=center | |align=center |{{cite web |title = LCDB Data for (10199) Chariklo |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=10199%7CChariklo |access-date = 28 April 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040733/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=10199%7CChariklo }} |
Juno {{small|3}} |bgcolor=black| File:3 Juno VLT (2021).png |align=center | {{val|127|1}} |align=center | {{val|27.0|2.4}} |belt asteroid type S |
Hiisi {{small|Lempo II}} | style="background:#490405;"| File:1999TC36-Trujillo-HST.png |align=center | {{val|126|8}} |align=center | |secondary of 47171 Lempo |
Hektor {{small|624}} |bgcolor=black| File:624 Hektor.png |align=center | {{val|125|13}} |align=center | {{val|7.9|1.4}} |Jupiter trojan ({{L4}}) type D; binary |align=center |{{Cite journal |display-authors = 6 |first1 = F. |last1 = Marchis |first2 = J. |last2 = Durech |first3 = J. |last3 = Castillo-Rogez |first4 = F. |last4 = Vachier |first5 = M. |last5 = Cuk |first6 = J. |last6 = Berthier |first7 = M. H. |last7 = Wong |first8 = P. |last8 = Kalas |first9 = G. |last9 = Duchene |first10 = M. A. |last10 = van Dam |first11 = H. |last11 = Hamanowa |first12 = M. |last12 = Viikinkoski |date = March 2014 |title = The Puzzling Mutual Orbit of the Binary Trojan Asteroid (624) Hektor |journal = The Astrophysical Journal Letters |volume = 783 |issue = 2 |page = 6 |bibcode = 2014ApJ...783L..37M |doi = 10.1088/2041-8205/783/2/L37 |arxiv = 1402.7336 |
Sila {{small|79360}} |bgcolor=#181818| File:Sila-nunam.jpg |align=center | {{val|124|15}} |align=center | {{val|10.8|0.22}} |align=center |{{cite web |title = (79360) Sila-Nunam |work = Johnston's Archive |date = 20 September 2014 |first = Wm. Robert |last = Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-79360.html |access-date = 28 April 2019}} |
{{mpl-|309239|2007 RW|10}} {{small|309239}} |bgcolor=black| |align=center | {{val|124|15}} |align=center | |quasi-satellite of Neptune |
Altjira {{small|148780}} |bgcolor=#181818| File:148780-altjira-hubble.jpg |align=center | {{val|123|19|70}} |align=center | |cubewano; binary |
Nunam {{small|79360}} |bgcolor=#181818| File:Sila-nunam.jpg |align=center | {{val|118|15}} |align=center | |secondary of 79360 Sila |
Bamberga {{small|324}} |bgcolor=black| File:Potw1749a Bamberga crop.png |align=center | {{val|114|2}} |align=center | {{val|10.2|0.9}} |belt asteroid type C |
Patientia {{small|451}} |bgcolor=black| |align=center | {{val|112.9|2.3}} |align=center | {{val|10.9|5.3}} |belt asteroid type C |
Psyche {{small|16}} |bgcolor=black| File:Psyche VLT.png |align=center | {{val|112|2}} |align=center | {{val|26.2|2.9}} |belt asteroid type M |
Ceto {{small|65489}} | style="background:black;"| File:ceto-phorcys hst.jpg |align=center | {{val|112|5}} |align=center | {{val|5.4|0.4}} |
Herculina {{small|532}} |bgcolor=black| File:532Herculina (Lightcurve Inversion).png |align=center | {{val|111.2|2.4}} |align=center | |belt asteroid type S |
S/2007 (148780) 1 {{small|Altjira I}} |bgcolor=#181818| File:148780-altjira-hubble.jpg |align=center | {{val|110|17|62}} |align=center | |secondary of 148780 Altjira |
Hesperia {{small|69}} |bgcolor=black| File:69Hesperia (Lightcurve Inversion).png |align=center | {{val|110|15}} |align=center | {{val|5.86|1.18}} |belt asteroid type M |align=center |{{·}}{{cite journal|display-authors=6|last=Shepard|first=Michael K.|author2=Harris, Alan W.|author3=Taylor, Patrick A.|author4=Clark, Beth Ellen|author5=Ockert-Bell, Maureen|author6=Nolan, Michael C.|author7=Howell, Ellen S.|author7-link=Ellen Howell|author8=Magri, Christopher|author9=Giorgini, Jon D.|author10=Benner, Lance A. M.|title=Radar observations of Asteroids 64 Angelina and 69 Hesperia|journal=Icarus|volume=215 |issue=2 |pages=547–551 |date=2011|url=http://echo.jpl.nasa.gov/asteroids/MBAs/shepard.etal.2011.angelina+hesperia.pdf|doi=10.1016/j.icarus.2011.07.027|bibcode=2011Icar..215..547S |arxiv=1104.4114}} |
Thisbe {{small|88}} |bgcolor=black| File:88 Thisbe VLT (2021), deconvolved.pdf |align=center | {{val|109|2}} |align=center | {{val|11.6|2.2}} |belt asteroid type B |
Doris {{small|48}} |bgcolor=black| File:48 Doris VLT (2021), deconvolved.pdf |align=center | {{val|108|2}} |align=center | {{val|6.9|2.9}} |belt asteroid type C |
Chiron {{small|2060 or 95P}} | style="background:#3c3c3c;"| File:2060 Chiron Hubble.jpg |align=center | {{val|108|5}} |align=center | |
Phoebe {{small|Saturn IX}} |bgcolor=black| File:Phoebe cassini.jpg |align=center | {{val|106.5|0.7}} |align=center | {{val|8.29|0.01}} |
Satellite of (38628) Huya {{small|Huya I}} |bgcolor=black| File:Huya Hubble.png |align=center | {{val|106|15}} |align=center | |moon of 38628 Huya |
Fortuna {{small|19}} |bgcolor=black| File:19 Fortuna VLT (2021), deconvolved.pdf |align=center | {{val|105.5|1.0}} |align=center | {{val|8.8|1.4}} |belt asteroid type G |
Camilla {{small|107}} |bgcolor=black| File:107Camilla (Lightcurve Inversion).png |align=center | {{val|105|4}} |align=center | {{val|11.2|0.3}} |outer belt asteroid type C; trinary |align=center |{{cite journal |display-authors = 6 |first1 = A. K. |last1 = Mainzer |first2 = J. M. |last2 = Bauer |first3 = R. M. |last3 = Cutri |first4 = T. |last4 = Grav |first5 = E. A. |last5 = Kramer |first6 = J. R. |last6 = Masiero |first7 = C. R. |last7 = Nugent |first8 = S. M. |last8 = Sonnett |first9 = R. A. |last9 = Stevenson |first10 = E. L. |last10 = Wright |date = June 2016 |title = NEOWISE Diameters and Albedos V1.0 |url = https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_COMPIL_5_NEOWISEDIAM_V1_0/data/neowise_mainbelt.tab |journal = NASA Planetary Data System |volume = 247 |pages = EAR–A–COMPIL–5–NEOWISEDIAM–V1.0 |bibcode = 2016PDSS..247.....M |access-date = 31 October 2018}}{{·}} |
Themis {{small|24}} |bgcolor=black| File:24 Themis VLT (2021), deconvolved.pdf |align=center | {{val|104|2}} |align=center | {{val|6.2|2.9}} |belt asteroid type C |
Amphitrite {{small|29}} |bgcolor=black| File:Potw1749a Amphitrite crop.png |align=center | {{val|102|1}} |align=center | {{val|12.7|2.0}} |belt asteroid type S |
Egeria {{small|13}} |bgcolor=black| File:13 Egeria VLT (2021), deconvolved.pdf |align=center | {{val|101|2}} |align=center | {{val|9.2|2.1}} |belt asteroid type G |
Iris {{small|7}} |bgcolor=black| File:Iris asteroid eso.jpg |align=center | {{val|100|5}} |align=center | {{val|13.5|2.3}} |belt asteroid type S |
colspan=7 style="font-size: 0.9em; font-weight: normal; text-align: left; padding: 6px 4px" | Legend:
:centaur – asteroids orbiting between the outer planets :Jupiter trojan – asteroids located in Jupiter's {{L4}} and {{L5}} Lagrange points |
= From 50 to 99 km =
This list contains a selection of objects 50 and 99 km in radius (100 km to 199 km in average diameter). The listed objects currently include most objects in the asteroid belt and moons of the giant planets in this size range, but many newly discovered objects in the outer Solar System are missing, such as those included in the following reference. Asteroid spectral types are mostly Tholen, but some might be SMASS.
class="wikitable sortable sticky-header-multi" |
style="font-weight:normal; width:110px;"| Body{{notetag|name=A}}
! class="unsortable"| Image ! data-sort- type="number" style="width:85px; font-weight:normal;"| Radius{{notetag|name=B}} ! data-sort- type="number" style="width:75px;"| Mass ! Type ! class="unsortable" style="font-weight: normal; width: 3.8em; text-align: center;" | Refs{{notetag|name=Refs|text=Reference column specifically for radius (r) and mass (M) citations}} |
---|
Elektra {{small|130}} |bgcolor=black| File:130 Elektra VLT (2021), deconvolved.pdf |align=center | {{val|99.5|1}} |align=center | {{val|6.4|0.2}} |
Bienor {{small|54598}} |bgcolor=black| |align=center | {{val|99|3|3.5}} |align=center | |
Hebe {{small|6}} |bgcolor=black| File:6hebe.png |align=center | {{val|97.5|1.5}} |align=center | {{val|12.4|2.4}} |belt asteroid type S |
Larissa {{small|Neptune VII}} |bgcolor=black| File:Larissa 1.jpg |align=center | {{val|97|3}} |align=center | {{val|4.2|p=≈ }} |moon of Neptune |align=center |{{·}}{{refn|name=mass estimate|group=lower-alpha|The mass estimate is based on the assumed density of 1.2 g/cm3, and a volume of 3.5 {{e|6}} km3 obtained from a detailed shape model in Stooke (1994). {{cite journal| doi = 10.1007/BF00572198| last = Stooke| first = Philip J.| year = 1994| title = The surfaces of Larissa and Proteus| journal = Earth, Moon, and Planets| volume = 65| issue = 1| pages = 31–54| bibcode = 1994EM&P...65...31S| s2cid = 121825800}} |
Ursula {{small|375}} |bgcolor=#181818| File:375Ursula-LB1.jpg |align=center | {{val|96.8|1.3}} |align=center | {{val|8.4|5.3}} |belt asteroid type C |align=center |{{cite journal |display-authors = 6 |first1 = Fumihiko |last1 = Usui |first2 = Daisuke |last2 = Kuroda |first3 = Thomas G. |last3 = Müller |first4 = Sunao |last4 = Hasegawa |first5 = Masateru |last5 = Ishiguro |first6 = Takafumi |last6 = Ootsubo |first7 = Daisuke |last7 = Ishihara |first8 = Hirokazu |last8 = Kataza |first9 = Satoshi |last9 = Takita |first10 = Shinki |last10 = Oyabu |first11 = Munetaka |last11 = Ueno |first12 = Hideo |last12 = Matsuhara |first13 = Takashi |last13 = Onaka |date = October 2011 |title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey |journal = Publications of the Astronomical Society of Japan |volume = 63 |issue = 5 |pages = 1117–1138 |bibcode = 2011PASJ...63.1117U |doi = 10.1093/pasj/63.5.1117 |doi-access= free |
S/2018 (532037) 1
|bgcolor=black| |align=center | {{val|95|p=≈ }} |align=center | |moon of 2013 FY27 |
Eugenia {{small|45}} |bgcolor=black| file:45 Eugenia VLT (2021), deconvolved.pdf |align=center | {{val|94|1}} |align=center | {{val|5.8|0.1}} |
Hermione {{small|121}} |bgcolor=black| File:Hermione06 2.jpg |align=center | {{val|94|3}} |align=center | {{val|5.0|0.3}} |outer belt asteroid type C; binary |align=center | {{cite web |first1 = Wm. Robert |last1 = Johnston |title = (121) Hermione and S/2002 (121) 1 ("LaFayette") |publisher = Johnston's Archive |date = 21 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-00121.html |
Daphne {{small|41}} |bgcolor=black| file:41 Daphne VLT (2021), deconvolved.pdf |align=center | {{val|94|7}} |align=center | {{val|6.1|0.9}} |
Aurora {{small|94}} |bgcolor=black| File:94Aurora (Lightcurve Inversion).png |align=center | {{val|93.8|3.6}}{{dubious|date=January 2020}} |align=center | {{val|6.2|3.6}} |belt asteroid type C |
Bertha {{small|154}} |bgcolor=black| file:000154-asteroid shape model (154) Bertha.png |align=center | {{val|93.4|0.9}} |align=center | {{val|9.2|5.2}}{{dubious|date=January 2020}} |belt asteroid type C |
Janus {{small|Saturn X}} |bgcolor=black| File:PIA12714 Janus crop.jpg |align=center | {{val|89.5|1.4}} |align=center | {{val|1.898|0.001}} |moon of Saturn |
Teharonhiawako {{small|88611}} | style="background:#3c3c3c;"| File:teharonhiawako-sawiskera hst.jpg |align=center | {{val|89|16|18}} |align=center | {{val|2.44|0.03}}{{dubious|date=January 2020}} |align=center |{{·}}{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (88611) Teharonhiawako and Sawiskera |publisher = Johnston's Archive |date = 20 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-88611.html |access-date = 13 June 2019}} |
Aegle {{small|96}} |bgcolor=black| |align=center | {{val|88.9|0.8}} |align=center | {{val|6.4|6.3}} |belt asteroid type T |
Galatea {{small|Neptune VI}} | bgcolor="black" | File:Galatea moon.jpg | align="center" | {{Val|88|4}} | align="center" | {{val|2.12|0.08}} |moon of Neptune {{cite journal | doi = 10.1126/science.253.5023.995 | last = Porco | first = C.C. | year = 1991 | title = An Explanation for Neptune's Ring Arcs | journal = Science | volume = 253 | issue = 5023 | pages = 995–1001 | pmid = 17775342 | bibcode = 1991Sci...253..995P | s2cid = 742763 }} |
Phorcys {{small|Ceto I}} | style="background:black;"| File:ceto-phorcys hst.jpg |align=center | {{val|87|8 |
9}}
|align=center | {{val|1.67|p=≈ }} |secondary of 65489 Ceto |align=center |{{·}}{{cite journal |last=Grundy |first=W.M. |author2=Stansberry, J.A. |author3=Noll K.S. |author4=Stephens, D.C. |display-authors= etal |title=The orbit, mass, size, albedo, and density of (65489) Ceto/Phorcys: A tidally-evolved binary Centaur |journal=Icarus |date=2007 |arxiv=0704.1523 |bibcode = 2007Icar..191..286G |doi = 10.1016/j.icarus.2007.04.004 |volume=191 |issue=1 |pages=286–297|s2cid=1532765 }} |
Palma {{small|372}} |bgcolor=black| File:372Palma (Lightcurve Inversion).png |align=center | {{val|86.8|1.4}}{{dubious|date=January 2020}} |align=center | {{val|5.2|0.6}} |belt asteroid type B |align=center |{{cite journal |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = C. |last6 = Nugent |first7 = M. S. |last7 = Cabrera |date = 10 October 2012 |title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids |journal = The Astrophysical Journal Letters |volume = 759 |pages = L8 |number = 1 |bibcode = 2012ApJ...759L...8M |doi = 10.1088/2041-8205/759/1/L8|arxiv= 1209.5794 |s2cid = 46350317 |
Metis {{small|9}} |bgcolor=black| File:9 Metis VLT (2021), deconvolved.pdf |align=center | {{val|86.5|1}} |align=center | {{val|8.0|1.9}} |belt asteroid type S |
Alauda {{small|702}} |bgcolor=#181818| File:702Ala-mag13-occult.jpg |align=center | {{val|86|28}} |align=center | {{val|6.06|0.36}}{{dubious|date=January 2020}} |align=center |{{·}}{{cite journal |first1 = P. |last1 = Rojo |first2 = J. L. |last2 = Margot |date = February 2011 |title = Mass and Density of the B-type Asteroid (702) Alauda |journal = The Astrophysical Journal |volume = 727 |issue = 2 |page = 5 |bibcode = 2011ApJ...727...69R |doi = 10.1088/0004-637X/727/2/69 |arxiv = 1011.6577|s2cid = 59449907 }} |
Hilda {{small|153}} | bgcolor="#181818" | File:Hilda-LB1-mag14.jpg | align="center" | {{val|85.3|1.6}} | align="center" | |outer belt asteroid; Hildas |
Himalia {{small|Jupiter VI}} | bgcolor="black" | File:Cassini-Huygens Image of Himalia.png | align="center" | {{val|85}} | align="center" | {{val|4.2|0.6}} |moon of Jupiter | align="center" | {{·}}{{cite journal |last=Emelyanov |first=N.V. |author2= Archinal, B. A. |author3=A'hearn, M. F. |display-authors=etal |title=The mass of Himalia from the perturbations on other satellites | url=https://www.aanda.org/articles/aa/pdf/2005/30/aahe201.pdf |journal=Astronomy and Astrophysics |volume=438 |issue=3 |pages=L33–L36 |date=2005 |doi=10.1051/0004-6361:200500143|bibcode=2005A&A...438L..33E|doi-access=free}} |
Namaka {{small|Haumea II}} | bgcolor=#181818 | File:Haumea Hubble.png | align="center" | {{val|85|p=≈ }} | align="center" | {{val|1.8|1.5}} |moon of Haumea |
Weywot {{small|Quaoar I}} | style="background:#181818;" | File:quaoar-weywot hst.jpg | align="center" | {{val|85|p=≈ }} | align="center" | {{val|5|p=< ≈ }} |moon of 50000 Quaoar | align="center" | |
Freia {{small|76}} | bgcolor="black" | File:76Freia (Lightcurve Inversion).png | align="center" | {{val|84.2|1.0}} | align="center" | {{val|2.0|4.2}}{{dubious|date=January 2020}} |
Albion {{small|15760}} | bgcolor="black" | | align="center" | {{val|83.5}} | |TNO, first KBO discovered | align="center" |{{cite web | url=http://www.johnstonsarchive.net/astro/tnoslist.html | title=List of known trans-Neptunian objects }} |
Amalthea {{small|Jupiter V}} | bgcolor="black" | File:Amalthea (moon).png | align="center" | {{Val|83.45|2.4}} | align="center" | {{val|2.08|0.15}} |moon of Jupiter | align="center" |{{cite journal| doi = 10.1006/icar.1998.5976| last1 = Thomas | first1 = P. C.| last2 = Burns | first2 = J. A.| last3 = Rossier | first3 = L.| last4 = Simonelli | first4 = D.| last5 = Veverka | first5 = J.| last6 = Chapman | first6 = C. R.| last7 = Klaasen | first7 = K.| last8 = Johnson | first8 = T. V.| last9 = Belton | first9 = M. J. S.| author10 = Galileo Solid State Imaging Team| date =September 1998| title = The Small Inner Satellites of Jupiter| journal = Icarus| volume = 135| issue = 1| pages = 360–371| bibcode = 1998Icar..135..360T| doi-access = free}}{{·}}{{cite journal| doi = 10.1126/science.1110422| last1 = Anderson | first1 = J. D.| last2 = Johnson | first2 = T. V.| last3 = Schubert | first3 = G.| last4 = Asmar | first4 = S.| last5 = Jacobson | first5 = R. A.| last6 = Johnston | first6 = D.| last7 = Lau | first7 = E. L.| last8 = Lewis | first8 = G.| last9 = Moore | first9 = W. B.| date = 27 May 2005| last10 = Taylor | first10 = A.| last11 = Thomas | first11 = P. C.| last12 = Weinwurm | first12 = G.| title = Amalthea's Density is Less Than That of Water| journal = Science| volume = 308| issue = 5726| pages = 1291–1293| pmid = 15919987| bibcode = 2005Sci...308.1291A| s2cid = 924257 }} |
Agamemnon {{small|911}} | bgcolor="black" | File:911 Agamemnon.png | align="center" | {{val|83.3|2.0}} | align="center" | |Jupiter trojan ({{L4}}) type D |
Elpis {{small|59}} | bgcolor="black" | | align="center" | {{val|82.6|2.3}} | align="center" | {{val|3|0.5}} |
Eleonora {{small|354}} |bgcolor=black| file:354 Eleonora VLT (2021), deconvolved.pdf |align=center | {{val|82.5|1.5}} |align=center | {{val|7.5|2.7}} |belt asteroid type A |
Nemesis {{small|128}} |bgcolor=black| file:128 Nemesis VLT (2021), deconvolved.pdf |align=center | {{val|81.5|2.5}} |align=center | {{val|3.4|1.7}} |belt asteroid type C |
Puck {{small|Uranus XV}} | bgcolor="black" | File:Puck.png | align="center" | {{val|81|2}} | align="center" | |moon of Uranus |
S/2015 (136472) 1 {{small|Makemake I}} |bgcolor=black| File:Makemake moon Hubble image with legend (cropped).jpg | align="center" | {{val|80|p=≈ }} | align="center" | |moon of Makemake |
Sycorax {{small|Uranus XVII}} |bgcolor=black| File:Uranus-sycorax2.gif |align=center | {{val|78.5|11.5|7.5}} |align=center | |moon of Uranus |align=center |{{cite journal |title = Properties of the Irregular Satellite System around Uranus Inferred from K2, Herschel, and Spitzer Observations |display-authors = etal |first1 = A. |last1 = Farkas-Takács |first2 = Cs. |last2 = Kiss |first3 = A. |last3 = Pál |first4 = L. |last4 = Molnár |first5 = Gy. M. |last5 = Szabó |first6 = O. |last6 = Hanyecz |date = September 2017 |journal = The Astronomical Journal |volume = 154 |issue = 3 |id = 119 |page = 13 |doi = 10.3847/1538-3881/aa8365 |arxiv = 1706.06837 |bibcode = 2017AJ....154..119F|s2cid = 118869078 |doi-access = free }} |
Io {{small|85}} |bgcolor=black| File:85Io (Lightcurve Inversion).png |align=center | {{val|77.4|1.9}}{{dubious|date=January 2020}} |align=center | {{val|2.6|1.5}} |
Minerva {{small|93}} |bgcolor=black| File:93Minerva (Lightcurve Inversion).png |align=center | {{val|77.08|0.65}} |align=center | {{val|3.5|0.4}} |
Alexandra {{small|54}} |bgcolor=black| File:54Alexandra (Lightcurve Inversion).png |align=center | {{val|77.07|0.32}} |align=center | {{val|6.2|3.5}}{{dubious|date=January 2020}} |belt asteroid type C |
Laetitia {{small|39}} |bgcolor=black| |align=center | {{val|77|2}} |align=center | {{val|4.7|1.1}} |belt asteroid type S |align=center |{{cite journal |first1 = B. |last1 = Carry |title = Density of asteroids |journal = Planetary and Space Science |volume = 73 |issue = 1 |pages = 98–118 |date = December 2012 |doi = 10.1016/j.pss.2012.03.009 |bibcode = 2012P&SS...73...98C |arxiv = 1203.4336|s2cid = 119226456 |
Nemausa {{small|51}} |bgcolor=black| File:51 Nemausa VLT (2021), deconvolved.pdf |align=center | {{val|75|1.5}} |align=center | {{val|3.9|1.6}} |belt asteroid type G |
Kalliope {{small|22}} | bgcolor="black" | file:22 Kalliope VLT (2021), deconvolved.pdf | align="center" | {{val|75|2.5}} | align="center" | {{val|7.7|0.4}} |
Despina {{small|Neptune V}} | bgcolor="black" | File:Despina.jpg | align="center" | {{val|75|3}} | align="center" | |moon of Neptune |
Manwë {{small|385446}} | style="background:#3c3c3c;"| File:manwe-thorondor hst.jpg |align=center | {{val|75|p=≈ }} |align=center | {{val|1.41|p=≈ }} |resonant KBO {{small|(4:7)}}; binary |align=center |{{cite arXiv |title=The Complex Rotational Light Curve of (385446) Manwë-Thorondor, a Multi-Component Eclipsing System in the Kuiper Belt |first1=David L. |last1=Rabinowitz |first2=Susan D. |last2=Benecchi |first3=William M. |last3=Grundy |first4=Anne J. |last4=Verbiscer |first5=Audrey |last5=Thirouin |date=November 2019 |class=astro-ph.EP |
Pales {{small|49}} |bgcolor=black| |align=center | {{val|74.9|p=≈ }} |align=center | {{val|4.2|2.2}} |belt asteroid type C |align=center |{{cite web |url=http://www.psi.edu/pds/resource/imps.html |author=Tedesco |display-authors=etal |title=Supplemental IRAS Minor Planet Survey (SIMPS) |access-date=29 December 2008 |work=IRAS-A-FPA-3-RDR-IMPS-V6.0 |publisher=Planetary Data System |date=2004 |archive-url=https://web.archive.org/web/20090817051318/http://www.psi.edu/pds/resource/imps.html |
Parthenope {{small|11}} |bgcolor=black| file:11 Parthenope VLT (2021), deconvolved.pdf |align=center | {{val|74.5|1}} |align=center | {{val|5.5|0.4}} |belt asteroid type S |
Arethusa {{small|95}} |bgcolor=black| File:95Arethusa (Lightcurve Inversion).png |align=center | {{val|74.0|2.4}} |align=center | |belt asteroid type C |
Pulcova {{small|762}} |bgcolor=#181818| File:762 Pulcova Hubble.jpg |align=center | {{val|73.7|0.4}} |align=center | {{val|1.4|0.1}} |align=center |{{·}}{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (762) Pulcova |publisher = Johnston's Archive |date = 21 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-00762.html |access-date = 10 June 2019}} |
Flora {{small|8}} |bgcolor=black| file:8 Flora VLT (2021), deconvolved.pdf |align=center | {{val|73|1}} |align=center | {{val|4.0|1.6}} |belt asteroid type S |
Ino {{small|173}} |bgcolor=black| file:173 Ino VLT (2021), deconvolved.pdf |align=center | {{val|72.5|1.5}} |align=center | {{val|2.2|1.3}} |belt asteroid type Xc |
Adeona {{small|145}} |bgcolor=black| file:145 Adeona VLT (2021), deconvolved.pdf |align=center | {{val|72|1.5}} |align=center | {{val|2.4|0.3}} |belt asteroid type Xc |
Irene {{small|14}} |bgcolor=black| File:14Irene (Lightcurve Inversion).png |align=center | {{val|72|1}} |align=center | {{val|2.9|1.9}} |belt asteroid type S |
Melpomene {{small|18}} |bgcolor=black| file:18 Melpomene VLT (2021), deconvolved.pdf |align=center | {{val|70.5|1}} |align=center | {{val|4.5|0.9}} |belt asteroid type S |
Lamberta {{small|187}} |bgcolor=black| file:Lamberta VLT.png |align=center | {{val|70.5|1}} |align=center | {{val|1.9|0.3}} |belt asteroid type Ch |
Aglaja {{small|47}} |bgcolor=black| |align=center | {{val|71|4}} |align=center | {{val|3.2|1.7}} |belt asteroid type C |
Patroclus {{small|617}} |bgcolor=#181818| File:617 Patroclus Hubble.jpg |align=center | {{val|70.2|0.4}} |align=center | {{val|1.36|0.11}} |
Julia {{small|89}} |bgcolor=black| File:Potw1749a Julia crop.png |align=center | {{val|70|1.4}} |align=center | {{val|4.3|3.2}} |belt asteroid type S |
Typhon {{small|42355}} | style="background:#181818;"| File:typhon-echidna hst.jpg |align=center | {{val|69|4.5}} |align=center | {{val|0.87|0.03}} |align=center |{{·}}{{cite web |title = (42355) Typhon and Echidna |publisher = Johnston's Archive |date = 31 January 2015 |first = Wm. Robert |last = Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-42355.html |access-date = 14 June 2019}} |
Massalia {{small|20}} |bgcolor=black| File:A112.M119.shape.png |align=center | {{val|67.8|1.8}} |align=center | {{val|5|1.04}} |belt asteroid type S |
Portia {{small|Uranus XII}} | style="background:#181818;"| File:Portia1.jpg |align=center | {{val|67.6|4}} |align=center | |moon of Uranus |
Emma {{small|283}} |bgcolor=black| File:283Emma (Lightcurve Inversion).png |align=center | {{val|66.2|0.1}} |align=center | {{val|1.38|0.03}} |
Paha {{small|Lempo I}} | style="background:#490405;"| File:1999TC36-Trujillo-HST.png |align=center | {{val|66|4|4.5}} |align=center | {{val|0.746|0.001}} |moon of 47171 Lempo |align=center | {{·}}{{cite journal |last1=Benecchi |first1=S.D |last2=Noll |first2=K. S. |last3=Grundy |first3=W. M. |last4=Levison |first4=H. F. |title=(47171) 1999 TC36, A Transneptunian Triple |journal=Icarus |volume=207 |issue=2 |pages=978–991 |date=2010 |doi=10.1016/j.icarus.2009.12.017 |bibcode=2010Icar..207..978B |arxiv=0912.2074|s2cid=118430134 }} |
Lucina {{small|146}} |bgcolor=black| File:146Lucina (Lightcurve Inversion).png |align=center | {{val|65.9}}±? |align=center | |belt asteroid type C |align=center |{{cite journal | last1 = Pravec | first1 = P. | last2 = Harris | first2 = A. W. | last3 = Kusnirak | first3 = P. | last4 = Galad | first4 = A. | last5 = Hornoch | first5 = K. | title = Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations | journal = Icarus | volume = 221 | issue = 1 | pages = 365–387 | year = 2012 | doi = 10.1016/j.icarus.2012.07.026 | bibcode = 2012LPICo1667.6089P}} |
Sawiskera {{small|Teharonhiawako I}} | style="background:#3c3c3c;"| File:teharonhiawako-sawiskera hst.jpg |align=center | {{val|65.5|12|13}} |align=center | |secondary of 88611 Teharonhiawako |
Achilles {{small|588}} |bgcolor=black|File:Modelled shape of 588 Achilles from its light curve.png |align=center | {{val|65.0|0.3}} |align=center | |Jupiter trojan ({{L4}}) type DU |
Panopaea {{small|70}} |bgcolor=black| |align=center | {{val|64.0|0.4}} |align=center | {{val|4.33|1.09}} |belt asteroid type C |
Thule {{small|279}} |bgcolor=black| |align=center | {{val|63.3|1.8}} |align=center | |outer belt asteroid type D |
Borasisi {{small|66652}} | style="background:#181818;"| File:borasisi-pabu hst.jpg |align=center | {{val|63|12.5 |
25.5}}
|align=center | {{val|3.433|0.027}} |align=center |{{·}}{{cite journal | last1 = Grundy | first1 = W. M. | last2 = Noll | first2 = K. S. | last3 = Nimmo | first3 = F. | last4 = Roe | first4 = H. G. | last5 = Buie | first5 = M. W. | last6 = Porter | first6 = S. B. | last7 = Benecchi | first7 = S. D. | last8 = Stephens | first8 = D. C. | last9 = Levison | first9 = H. F. | doi = 10.1016/j.icarus.2011.03.012 | last10 = Stansberry | first10 = J. A. | title = Five new and three improved mutual orbits of transneptunian binaries | journal = Icarus | volume = 213 | issue = 2 | page = 678 | date = 2011 | url = http://es.ucsc.edu/~fnimmo/website/Grundy_KBO.pdf|bibcode = 2011Icar..213..678G |arxiv = 1103.2751| s2cid = 9571163 }} |
Hestia {{small|46}} |bgcolor=black| |align=center | {{val|62.07|1.7}} |align=center | {{val|3.5}} |align=center |{{·}}{{cite journal |last=Michalak |first=G. |title=Determination of asteroid masses |journal=Astronomy & Astrophysics |volume=374 |issue=2 |pages=703–711 |date=2001 |doi=10.1051/0004-6361:20010731 |bibcode=2001A&A...374..703M|doi-access=free}} |
Leto {{small|68}} |bgcolor=black| File:68Leto (Lightcurve Inversion).png |align=center | {{val|61.3|1.6}} |align=center | {{val|3.28|1.9}} |belt asteroid type S |
Undina {{small|92}} |bgcolor=black| |align=center | {{val|60.46|0.85}} |align=center | {{val|4.43|0.25}} |belt asteroid type X |
Bellona {{small|28}} |bgcolor=#181818| File:28Bell-LB1-mag12.jpg |align=center | {{val|60.45|1.90}} |align=center | {{val|2.62|0.15}} |belt asteroid type S |align=center |{{cite web |type=2018-10-18 last obs |title=JPL Small-Body Database Browser: 28 Bellona |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=28 |
Diana {{small|78}} |bgcolor=black| |align=center | {{val|60.30|1.35}} |align=center | {{val|1.27|0.13}} |belt asteroid type C |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 78 Diana |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=78 |
Anchises {{small|1173}} |bgcolor=black| File:001173-asteroid shape model (1173) Anchises.png |align=center | {{val|60.2|1.5}} |align=center | |Jupiter trojan ({{L5}}) type P |
Bernardinelli-Bernstein {{small|C/2014 UN271}} |bgcolor=black| File:2014 UN271 Jan 2022 Hubble crop.png |align=center | {{val|60|7}} |align=center | |
Galatea {{small|74}} |bgcolor=black| |align=center | {{val|59.4|1.4}} |align=center | {{val|6.13|5.36}} |belt asteroid type C |align=center |{{cite web |type=2018-05-22 last obs |title=JPL Small-Body Database Browser: 74 Galatea |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=74 |
Deiphobus {{small|1867}} |bgcolor=black| |align=center | {{val|59.1|0.8}} |align=center | |Jupiter trojan ({{L5}}) type D |align=center |{{cite web |type=2018-06-21 last obs |title=JPL Small-Body Database Browser: 1867 Deiphobus (1971 EA) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1867 |access-date=2 May 2019}} |
Äneas {{small|1172}} |bgcolor=black| |align=center | {{val|59.01|0.40}} |align=center | |Jupiter trojan ({{L5}}) type D |align=center |{{cite web |type=2018-07-03 last obs |title=JPL Small-Body Database Browser: 1172 Aneas (1930 UA) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1172 |access-date=1 May 2019}} |
Kleopatra {{small|216}} |bgcolor=black| File:216 Kleopatra VLT (2021), deconvolved.pdf |align=center | {{val|59|1}} |align=center | {{val|3.0|0.3}} |
Athamantis {{small|230}} |bgcolor=black| File:230 Athamantis VLT (2021), deconvolved.pdf |align=center | {{val|59|1}} |align=center | {{val|2.3|1.1}} |belt asteroid type S |
Diomedes {{small|1437}} |bgcolor=black| File:001437-asteroid shape model (1437) Diomedes.png |align=center | {{val|58.89|0.59}} |align=center | |Jupiter trojan ({{L4}}) type D |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 1437 Diomedes (1937 PB) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1437 |access-date=30 April 2019}} |
Terpsichore {{small|81}} |bgcolor=black| |align=center | {{val|58.9|0.4}} |align=center | {{val|6.19|5.31}} |belt asteroid type C |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 81 Terpsichore |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=81 |
Epimetheus {{small|Saturn XI}} |bgcolor=black| File:PIA09813 Epimetheus S. polar region.jpg |align=center | {{val|58.1|1.8}} |align=center | {{val|0.5266|0.0006}} |moon of Saturn |
Victoria {{small|12}} |bgcolor=black| File:12 Victoria VLT (2021), deconvolved.pdf |align=center | {{val|58|1}} |align=center | {{val|2.7|1.3}} |belt asteroid type S |
Circe {{small|34}} |bgcolor=black| File:34Circe (Lightcurve Inversion).png |align=center | {{val|57.7|1.0}} |align=center | {{val|3.66|0.03|p=≈ }} |belt asteroid type C |
Leda {{small|38}} |bgcolor=black| File:38Leda (Lightcurve Inversion).png |align=center | {{val|57.7|0.7}} |align=center | {{val|5.71|5.47}} |belt asteroid type C |
Odysseus {{small|1143}} |bgcolor=black| |align=center | {{val|57.3|0.3}} |align=center | |Jupiter trojan ({{L4}}) type D |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 1143 Odysseus (1930 BH) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1143 |access-date=2 May 2019}} |
Alcathous {{small|2241}} |bgcolor=black| |align=center | {{val|56.8|0.9}} |align=center | |Jupiter trojan ({{L5}}) type D |align=center |{{cite web |type=2018-06-17 last obs |title=JPL Small-Body Database Browser: 2241 Alcathous (1979 WM) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2241 |access-date=2 May 2019}} |
Melete {{small|56}} |bgcolor=black| File:A666.M1106.shape(1).png |align=center | {{val|56.62|0.85}} |align=center | {{val|4.61}} |belt asteroid type P |
Mnemosyne {{small|57}} |bgcolor=black| |align=center | {{val|56.3|1.4}} |align=center | {{val|12.6|2.4|p=≈ }} |belt asteroid type S |align=center |{{cite web |type=2018-06-25 last obs |title=JPL Small-Body Database Browser: 57 Mnemosyne |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=57 |
Nestor {{small|659}} |bgcolor=black| |align=center | {{val|56.2|0.9}} |align=center | |Jupiter trojan ({{L4}}) type XC |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 659 Nestor (A908 FE) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=659 |access-date=2 May 2019}} |
Harmonia {{small|40}} |bgcolor=black| File:40Harmonia (Lightcurve Inversion).png |align=center | {{val|55.6|0.2}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2018-09-15 last obs |title=JPL Small-Body Database Browser: 40 Harmonia |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=40 |access-date=3 May 2019}} |
Leleākūhonua {{small|541132}} |bgcolor=black| |align=center | {{val|55|7|5}} |align=center | |align=center |{{cite journal |display-authors = etal |first1 = Marc W. |last1 = Buie |first2 = Rodrigo |last2 = Leiva |first3 = John M. |last3 = Keller |first4 = Josselin |last4 = Desmars |first5 = Bruno |last5 = Sicardy |first6 = J. J. |last6 = Kavelaars |date = April 2020 |title = A Single-chord Stellar Occultation by the Extreme Trans-Neptunian Object (541132) Leleākūhonua |journal = The Astronomical Journal |volume = 159 |issue = 5 |page = 230 |id = 230 |doi = 10.3847/1538-3881/ab8630 |bibcode = 2020AJ....159..230B|arxiv= 2011.03889 |s2cid = 219039999 |doi-access = free }} |
Euterpe {{small|27}} |bgcolor=black| File:27Euterpe (Lightcurve Inversion).png |align=center | {{val|54.9|0.8}} |align=center | {{val|1.67|1.01}} |belt asteroid type S |
Antilochus {{small|1583}} |bgcolor=black| |align=center | {{val|54.4|0.3}} |align=center | |Jupiter trojan ({{L4}}) type D |
Thorondor {{small|Manwë I}} | style="background:#3c3c3c;"| File:manwe-thorondor hst.jpg |align=center | {{val|54}} |align=center | {{val|0.5}} |secondary of 385446 Manwë |
Thalia {{small|23}} |bgcolor=black| File:23Thalia (Lightcurve Inversion).png |align=center | {{val|53.8|1.1}} |align=center | {{val|1.96|0.09}} |belt asteroid type S |align=center |{{cite web |type=2018-10-21 last obs |title=JPL Small-Body Database Browser: 23 Thalia |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=23 |
Erato {{small|62}} |bgcolor=black| File:62Erato (Lightcurve Inversion).png |align=center | {{val|53.5|0.3}} |align=center | |belt asteroid type BU/type Ch |align=center |{{cite web |type=2018-05-24 last obs |title=JPL Small-Body Database Browser: 62 Erato |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=62 |access-date=3 May 2019}} |
Astraea {{small|5}} |bgcolor=black| File:5Astraea (Lightcurve Inversion).png |align=center | {{val|53.3|1.6}} |align=center | {{val|2.9}} |belt asteroid type S |align=center |{{cite web |type=2018-09-16 last obs |title=JPL Small-Body Database Browser: 5 Astraea |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=5 |
Pabu {{small|Borasisi I}} | style="background:#181818;"| File:borasisi-pabu hst.jpg |align=center | {{val|52.5|10|21}} |align=center | |secondary of 66652 Borasisi |
Eos {{small|221}} |bgcolor=black| |align=center | {{val|51.76|2.8}} |align=center | {{val|5.87|0.34|p=≈ }} |
Aegina {{small|91}} |bgcolor=black| |align=center | {{val|51.7|0.2}} |align=center | |belt asteroid type C |align=center |{{cite web |type=2018-07-31 last obs |title=JPL Small-Body Database Browser: 91 Aegina |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=91 |access-date=3 May 2019}} |
Leukothea {{small|35}} |bgcolor=black| File:A532.M868.shape.png |align=center | {{val|51.5|0.6}} |align=center | |belt asteroid type C |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 35 Leukothea |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=35 |access-date=3 May 2019}} |
Menoetius {{small|Patroclus I}} |bgcolor=#181818| File:617 Patroclus Hubble.jpg |align=center | {{val|51.4|0.25}} |align=center | |secondary of 617 Patroclus |align=center |{{cite web |title = LCDB Data for (617) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=617%7C |access-date = 1 May 2019 |archive-date = 19 October 2020 |archive-url = https://web.archive.org/web/20201019075539/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=617%7C }} |
Isis {{small|42}} |bgcolor=black| File:42Isis (Lightcurve Inversion).png |align=center | {{val|51.4|1.4}} |align=center | {{val|1.58|0.52}} |belt asteroid type S |
Klotho {{small|97}} |bgcolor=black| File:97Klotho (Lightcurve Inversion).png |align=center |{{val|50.4|0.3}} |align=center |{{val|1.33|0.13}} |belt asteroid type M |
Troilus {{small|1208}} |bgcolor=#3c3c3c| File:1208 Troilus Hubble.jpg |align=center | {{val|50.3|0.5}} |align=center | |Jupiter trojan ({{L5}}) type FCU |align=center |{{cite web |type=2018-07-22 last obs |title=JPL Small-Body Database Browser: 1208 Troilus (1931 YA) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1208 |access-date=2 May 2019}} |
= From 20 to 49 km =
This list includes few examples since there are about 589 asteroids in the asteroid belt with a measured radius between 20 and 49 km.{{cite web|url=http://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=all;obj_kind=all;obj_numbered=all;ast_orbit_class=IMB;ast_orbit_class=MBA;ast_orbit_class=OMB;OBJ_field=0;ORB_field=0;combine_mode=AND;c1_group=OBJ;c1_item=Ap;c1_op=%3C=;c1_value=100;c2_group=OBJ;c2_item=Ap;c2_op=%3E=;c2_value=40;table_format=HTML;max_rows=50;format_option=comp;c_fields=AcBhBgBjBiBnBsAiAp;.cgifields=format_option;.cgifields=ast_orbit_class;.cgifields=combine_mode;.cgifields=table_format;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=com_orbit_class&query=1&c_sort=ApD|title=JPL Small-Body Database Search Engine|first=Alan|last=Chamberlin}} Many thousands of objects of this size range have yet to be discovered in the trans-Neptunian region. The number of digits is not an endorsement of significant figures. The table switches from {{e|18}} kg to {{e|15}} kg (Eg). Most mass values of asteroids are assumed.{{cite journal |last=Baer |first=James|author2=Steven R. Chesley
|title=Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris
|journal=Celestial Mechanics and Dynamical Astronomy
|volume=100|issue=2008|pages=27–42 |doi=10.1007/s10569-007-9103-8 |date=2008|bibcode= 2008CeMDA.100...27B |doi-access=free}}
class="wikitable sortable sticky-header-multi" |
style="font-weight:normal; width:100px;"| Body{{notetag|name=A}}
! class="unsortable" | Image ! data-sort- type="number" style="width:85px; font-weight:normal;"| Radius{{notetag|name=B}} ! data-sort- type="number" style="width:75px;"| Mass ! Type – notes ! class="unsortable" style="font-weight: normal; width: 3.8em; text-align: center;" | Refs{{notetag|name=Refs|text=Reference column specifically for radius (r) and mass (M) citations}} |
---|
Asterope {{small|233}} |bgcolor=black| |align=center | {{val|49.8|0.6}} |align=center | |align=center |{{cite web |type=2018-10-24 last obs |title=JPL Small-Body Database Browser: 233 Asterope |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=233 |access-date=3 May 2019}} |
Pholus {{small|5145}} |bgcolor=black| |align=center | {{val|49.5|+7.5 |
7}}
|align=center | |
Thebe {{small|Jupiter XIV}} |bgcolor=black|File:Thebe.jpg |align=center |{{val|49.3|2}} |align=center | |moon of Jupiter |
Lutetia {{small|21}} |bgcolor=black|File:Rosetta triumphs at asteroid Lutetia.jpg |align=center |{{val|49|1}} |align=center |{{val|1700|20}} |belt asteroid type M |
Kalypso {{small|53}} |bgcolor=black| File:A1012.M1732.shape.png |align=center | {{val|48.631|13.299}} |align=center | {{val|5630|5000|p=≈ }} |belt asteroid type XC |align=center |{{cite web |type=2018-10-18 last obs |title=JPL Small-Body Database Browser: 53 Kalypso |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=53 |
Notburga {{small|626}} |bgcolor=black| File:000626-asteroid shape model (626) Notburga.png |align=center | {{val|48.42|2.335}} | |belt asteroid type XC |
Proserpina {{small|26}} |bgcolor=black| File:A713.M1189.shape.png |align=center |{{val|47.4|0.85}} |align=center |{{val|748|895}} |belt asteroid type S |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 26 Prosperina |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=26 |
Juliet {{small|Uranus XI}} |bgcolor=black| File:Julietmoon.png |align=center |{{val|46.8|4}} |align=center | |moon of Uranus |
Urania {{small|30}} |bgcolor=black| File:30Urania (Lightcurve Inversion).png |align=center | {{val|44|1}} |align=center | {{val|1300|900}} |belt asteroid type S |
Ausonia {{small|63}} |bgcolor=black| File:63Ausonia (Lightcurve Inversion).png |align=center | {{val|46.5|1.5}} |align=center | {{val|1200|200}} |belt asteroid type S |
Beatrix {{small|83}} |bgcolor=black| |align=center |{{val|44.819|1.326}} |align=center | |belt asteroid type X |
Concordia {{small|58}} |bgcolor=black| |align=center |{{val|44.806|0.419}} |align=center | |belt asteroid type C |
Echidna {{small|Typhon I}} | style="background:#181818;"|File:typhon-echidna hst.jpg |align=center |{{val|44.5|3}} |align=center | |moon of 42355 Typhon |
Automedon {{small|2920}} |bgcolor=black| |align=center | {{val|44.287|0.898}} |align=center | |Jupiter trojan ({{L4}}) type D |align=center |{{cite web |type=2018-10-15 last obs |title=JPL Small-Body Database Browser: 2920 Automedon (1981 JR) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2920 |access-date=2 May 2019}} |
Antiope {{small|90}} |bgcolor=black| |align=center |{{val|43.9|0.5}} |align=center |{{val|828|22}} |align=center |{{cite web |title = (90) Antiope and S/2000 (90) 1 |publisher = Johnston's Archive |date = 21 September 2014 |first = Wm. Robert |last = Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-42355.html |
Prometheus {{small|Saturn XVI}} |bgcolor=black|File:Prometheus 12-26-09a.jpg |align=center |{{val|43.1|2.7}} |align=center |{{val|159.5|1.5}} |moon of Saturn |
Danaë {{small|61}} |bgcolor=black| |align=center |{{val|42.969|1.076}} |align=center |{{val|2890|2780}} |belt asteroid type S |align=center |{{cite web |type=2018-07-13 last obs |title=JPL Small-Body Database Browser: 61 Danae |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=61 |
Thetis {{small|17}} |bgcolor=black| File:17Thetis-LB1.jpg |align=center |{{val|42.449|1.014}} |align=center |{{val|1200}} |belt asteroid type S |align=center |{{cite web |type=2018-05-13 last obs |title=JPL Small-Body Database Browser: 17 Thetis |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=17 |
Pandora {{small|55}} |bgcolor=black| File:55Pandora (Lightcurve Inversion).png |align=center |{{val|42.397|1.251}} |align=center | |belt asteroid type M |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 55 Pandora |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=55 |access-date=4 May 2019}} |
Huenna {{small|379}} |bgcolor=black| |align=center |{{val|42.394|0.779}} |align=center |{{val|383|19}} |belt asteroid type B/type C; binary |align=center |{{cite web |type=2018-08-30 last obs |title=JPL Small-Body Database Browser: 379 Huenna (A894 AA) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=379 |access-date=3 May 2019}}{{·}}{{cite journal |display-authors=6 |last=Marchis |first=Franck |author2=P. Descamps |author3=J. Berthier |author4=D. hestroffer |author5=F. vachier |author6=M. Baek |author7=A. Harris |author8=D. Nesvorny |title=Main Belt Binary Asteroidal Systems With Eccentric Mutual Orbits |journal=Icarus |volume=195 |issue=1 |pages=295–316 |date=2008 |arxiv=0804.1385 |doi=10.1016/j.icarus.2007.12.010 |bibcode=2008Icar..195..295M|s2cid=119244052 }} |
Virginia {{small|50}} |bgcolor=black| |align=center | {{val|42.037|0.121}} |align=center | {{val|2310|700}} |align=center |{{cite web |type=2018-10-19 last obs |title=JPL Small-Body Database Browser: 50 Virginia |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=50 |
Feronia {{small|72}} |bgcolor=black|File:72Feronia (Lightcurve Inversion).png |align=center |{{val|41.975|2.01}} |align=center |{{val|3320|8490|p=≈ }} |belt asteroid type TDG |
S/2000 (90) 1 {{small|Antiope I}} |bgcolor=black| |align=center |{{val|41.9|0.5}} |align=center | |secondary of 90 Antiope |
Poulydamas {{small|4348}} |bgcolor=black| |align=center |{{val|41.016|0.313}} |align=center | |Jupiter trojan ({{L5}}) type C |align=center |{{cite web |type=2018-07-13 last obs |title=JPL Small-Body Database Browser: 4348 Poulydamas (1988 RU) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=4348 |access-date=4 May 2019}} |
Logos {{small|58534}} |bgcolor=#3c3c3c|File:Logos-zoe-hst.jpg |align=center |{{val|41|9}} |align=center |{{val|458|6.9}} |align=center |{{cite web |title = (58534) Logos and Zoe |work = Johnston's Archive |date = 20 September 2014 |author = Johnston, Wm. Robert |url = http://www.johnstonsarchive.net/astro/astmoons/am-58534.html |
Pandora {{small|Saturn XVII}} |bgcolor=black|File:Pandora PIA07632.jpg |align=center |{{val|40.7|1.5}} |align=center |{{val|137.1|1.9}} |moon of Saturn |
Thalassa {{small|Neptune IV}} | style="background:#fffff8;"| File:Neptune Trio.jpg |align=center |{{val|40.7|2.8}} |align=center | |moon of Neptune |
Niobe {{small|71}} |bgcolor=black| File:A614.M1014.shape.png |align=center |{{val|40.43|0.4}} |align=center | |belt asteroid type S |
Pomona {{small|32}} |bgcolor=black| File:32Pomona (Lightcurve Inversion).png |align=center |{{val|40.38|0.8}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2018-06-12 last obs |title=JPL Small-Body Database Browser: 32 Pomona |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=32 |access-date=4 May 2019}} |
Belinda {{small|Uranus XIV}} |bgcolor=black|File:Belinda.gif |align=center |{{val|40.3|8}} |align=center | |moon of Uranus |
Elara {{small|Jupiter VII}} |bgcolor=black| File:Elara - New Horizons.png |align=center |{{val|39.95|1.7}} |align=center | |moon of Jupiter |align=center |{{cite journal |display-authors = etal |first1 = T. |last1 = Grav |first2 = J. M. |last2 = Bauer |first3 = A. K. |last3 = Mainzer |first4 = J. R. |last4 = Masiero |first5 = C. R. |last5 = Nugent |first6 = R. M. |last6 = Cutri |date = August 2015 |title = NEOWISE: Observations of the Irregular Satellites of Jupiter and Saturn |journal = The Astrophysical Journal |volume = 809 |issue = 1 |id = 3 |page = 9 |doi = 10.1088/0004-637X/809/1/3 |arxiv = 1505.07820 |bibcode = 2015ApJ...809....3G|s2cid = 5834661 }} |
Cressida {{small|Uranus IX}} |bgcolor=black| File:Cressida.png |align=center |{{val|39.8|2}} |align=center | |moon of Uranus |
Amycus {{small|55576}} |bgcolor=black| |align=center |{{val|38.15|6.25}} |align=center | |
Hylonome {{small|10370}} | style="background:#3c3c3c;"| File:10370 Hylonome Hubble.jpg |align=center |{{val|37.545}} |align=center | |align=center |{{cite web |title = LCDB Data for (10370) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=10370%7C |access-date = 4 May 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040734/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=10370%7C }} |
Socus {{small|3708}} |bgcolor=black| |align=center | {{val|37.831|0.404}} |align=center | |Jupiter trojan ({{L5}}) type C |
Nysa {{small|44}} |bgcolor=black| File:44Nysa (Lightcurve Inversion).png |align=center |{{val|37.83|0.37}} |align=center | |belt asteroid type E |
Rosalind {{small|Uranus XIII}} |bgcolor=black| File:Rosalindmoon.png |align=center |{{val|36|6}} |align=center | |moon of Uranus |
Maja {{small|66}} |bgcolor=black| File:A737.M1234.shape(1).png |align=center |{{val|35.895|0.46}} |align=center | |belt asteroid type C |
Ariadne {{small|43}} |bgcolor=black| File:43Ariadne (Lightcurve Inversion).png |align=center |{{val|35.67|0.627}} |align=center |{{val|1210|220|p=≈ }} |belt asteroid type S |align=center |{{cite web |type=2018-10-20 last obs |title=JPL Small-Body Database Browser: 43 Ariadne |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=43 |
Iphigenia {{small|112}} |bgcolor=black| |align=center |{{val|35.535|0.26}} |align=center |{{val|1970|6780|p=≈ }} |belt asteroid type C |
Xiangliu {{small|Gonggong I}} |bgcolor=black| |align=center |{{val|35|15|p=≈ }} |align=center | |moon of (225088) Gonggong |align=center | |
Dike {{small|99}} |bgcolor=black| File:A688.M1144.shape.png |align=center |{{val|33.677|0.208}} |align=center | |belt asteroid type C |align=center |{{cite web |type=2018-10-24 last obs |title=JPL Small-Body Database Browser: 99 Dike |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=99 |access-date=4 May 2019}} |
Echeclus {{small|60558 or 174P}} |bgcolor=black| |align=center |{{val|32.3|0.8}} |align=center | |
Desdemona {{small|Uranus X}} |bgcolor=black| File:Desdemonamoon.png |align=center |{{val|32|4}} |align=center | |moon of Uranus |
Eurybates {{small|3548}} | style="background:#3f3f3f;"| File:3548 Eurybates Hubble.jpg |align=center | {{val|31.943|0.149}} |align=center | |Jupiter trojan ({{L4}}) type CP |
Eurynome {{small|79}} |bgcolor=black| File:79Eurynome (Lightcurve Inversion).png |align=center |{{val|31.739|0.476}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2018-08-18 last obs |title=JPL Small-Body Database Browser: 79 Eurynome |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=79 |access-date=4 May 2019}} |
Eurydike {{small|75}} |bgcolor=black| |align=center |{{val|31.189|0.802}} |align=center | |belt asteroid type M |align=center |{{cite web |type=2019-05-08 last obs |title=JPL Small-Body Database Browser: 75 Eurydike |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=75 |access-date=3 June 2019}} |
Halimede {{small|Neptune IX}} | style="background:#6d6d6c;"| File:Halimede.jpg |align=center |{{val|31|p=≈ }} |align=center | |moon of Neptune |
Phocaea {{small|25}} |bgcolor=black| File:25Phocaea (Lightcurve Inversion).png |align=center |{{val|30.527|1.232}} |align=center |{{val|599|60}} |belt asteroid type S |
Naiad {{small|Neptune III}} |bgcolor=black| File:Naiad Voyager.png |align=center |{{val|30.2|3.2}} |align=center | |moon of Neptune |
Schwassmann– Wachmann 1 {{small|29P}} |bgcolor=black| File:29P Schwassmann Wachmann.jpg |align=center |{{val|30.2|3.7}} |align=center | |align=center |{{cite web |type=2018-10-16 last obs |title=JPL Small-Body Database Browser: 29P/Schwassmann-Wachmann 1 |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1000079 |access-date=4 May 2019}} |
Neso {{small|Neptune XIII}} | style="background:#181818;"| File:Neso VLT-FORS1 2002-09-03 annotated.gif |align=center |{{val|30|p=≈ }} |align=center | |moon of Neptune |
Angelina {{small|64}} |bgcolor=black| File:A990.M1696.shape(1).png |align=center |{{val|29.146|0.541}} |align=center | |belt asteroid type E |align=center |{{cite web |type=2019-05-09 last obs |title=JPL Small-Body Database Browser: 64 Angelina |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=64 |access-date=3 June 2019}} |
Pasiphae {{small|Jupiter VIII}} | style="background:#3c3c3c;"| File:Pasiphaé.jpg |align=center |{{val|28.9|0.4}} |align=center | |moon of Jupiter |
Alkmene {{small|82}} |bgcolor=black| File:82Alkmene (Lightcurve Inversion).png |align=center |{{val|28.811|0.357}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2019-05-09 last obs |title=JPL Small-Body Database Browser: 82 Alkmene |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=82 |access-date=3 June 2019}} |
Nessus {{small|7066}} | style="background:#3c3c3c;"| File:7066 Nessus Hubble.jpg |align=center |{{val|28.5|8.5}} |align=center | |align=center |{{cite journal |display-authors = 6 |first1 = R. |last1 = Duffard |first2 = N. |last2 = Pinilla-Alonso |first3 = P. |last3 = Santos-Sanz |first4 = E. |last4 = Vilenius |first5 = J. L. |last5 = Ortiz |first6 = T. |last6 = Mueller |first7 = S. |last7 = Fornasier |first8 = E. |last8 = Lellouch |first9 = M. |last9 = Mommert |first10 = A. |last10 = Pal |first11 = C. |last11 = Kiss |first12 = M. |last12 = Mueller |first13 = J. |last13 = Stansberry |first14 = A. |last14 = Delsanti |first15 = N. |last15 = Peixinho |first16 = D. |last16 = Trilling |date = April 2014 |title = "TNOs are Cool": A survey of the trans-Neptunian region. XI. A Herschel-PACS view of 16 Centaurs |journal = Astronomy and Astrophysics |volume = 564 |page = 17 |bibcode = 2014A&A...564A..92D |doi = 10.1051/0004-6361/201322377 |arxiv = 1309.0946|s2cid = 119177446 }} |
Polana {{small|142}} |bgcolor=black| |align=center |{{val|27.406|0.139}} |align=center | |belt asteroid type F |align=center |{{cite web |type=2019-05-08 last obs |title=JPL Small-Body Database Browser: 142 Polana |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=142 |access-date=4 May 2019}} |
Bianca {{small|Uranus VIII}} |bgcolor=black| File:Biancamoon.png |align=center |{{val|27|2}} |align=center | |moon of Uranus |
Mathilde {{small|253}} |bgcolor=black|File:(253) mathilde crop.jpg |align=center |{{val|26.4}} |align=center |{{val|103.3|4.4}} |belt asteroid type C |align=center |{{cite web |type=2018-10-22 last obs |title=JPL Small-Body Database Browser: 253 Mathilde |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=253 |access-date=4 May 2019}}{{·}}{{cite journal|author=D. K. Yeomans|title=Estimating the mass of asteroid 253 Mathilde from tracking data during the NEAR flyby|journal=Science|volume=278|issue=5346|date=1997|pages=2106–9|pmid=9405343|doi=10.1126/science.278.5346.2106|bibcode=1997Sci...278.2106Y|display-authors=etal}} |
Hidalgo {{small|944}} |bgcolor=black| File:Hidalgoanimation2003.gif |align=center |{{val|26.225|1.8}} |align=center | |
Orus {{small|21900}} | style="background:#181818;"| File:21900 Orus Hubble.jpg |align=center | {{val|25.405|0.405}} |align=center | |
Amalthea {{small|113}} |bgcolor=black| |align=center |{{val|25.069|0.633}} |align=center | |
Prospero {{small|Uranus XVIII}} | style="background:#484848;"| File:Prospero - Uranus moon.jpg |align=center |{{val|25|p=≈ }} |align=center | |moon of Uranus |
Setebos {{small|Uranus XIX}} | style="background:#626363;"| File:Uranus - Setebos image.jpg |align=center |{{val|24|p=≈ }} |align=center | |moon of Uranus |
Carme {{small|Jupiter XI}} | style="background:#7d7d7a;"| File:Carmé.jpg |align=center |{{val|23.35|0.45}} |align=center | |moon of Jupiter |
Klytia {{small|73}} |bgcolor=black| File:73Klytia (Lightcurve Inversion).png |align=center |{{val|22.295|0.471}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2019-05-11 last obs |title=JPL Small-Body Database Browser: 73 Klytia |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=73 |access-date=5 June 2019}} |
Sao {{small|Neptune XI}} |bgcolor=black| File:Sao VLT-FORS1 2002-09-03 annotated.gif |align=center |{{val|22|p=≈ }} |align=center | |moon of Neptune |
Echo {{small|60}} |bgcolor=black| File:A990.M1696.shape(1).png |align=center |{{val|21.609|0.286}} |align=center |{{val|315|32}} |belt asteroid type S |align=center |{{cite web |type=2019-05-11 last obs |title=JPL Small-Body Database Browser: 60 Echo |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=60 |
Metis {{small|Jupiter XVI}} |bgcolor=black|File:Metis.jpg |align=center |{{val|21.5|2}} |align=center |{{val|119.893|p=≈ }} |moon of Jupiter |align=center |{{·}}{{cite web|date=25 April 2019 |title=Metis By the Numbers|publisher=NASA Solar System Exploration |url=https://solarsystem.nasa.gov/moons/jupiter-moons/metis/by-the-numbers/|access-date=3 May 2019}} |
Ophelia {{small|Uranus VII}} |bgcolor=black| File:Opheliamoon.png |align=center |{{val|21.4|4}} |align=center | |moon of Uranus |
Lysithea {{small|Jupiter X}} |bgcolor=black|File:Lysithea 2MASS JHK color composite.png |align=center |{{val|21.1|0.35}} |align=center | |moon of Jupiter |
Caliban {{small|Uranus XVI}} | style="background:#490405;"| File:Caliban discovery.jpg |align=center |{{val|21|10|6}} |align=center | |moon of Uranus |
Laomedeia {{small|Neptune XII}} | style="background:#181818;"| File:Laomedeia VLT-FORS1 2002-09-03 annotated.gif |align=center |{{val|21|p=≈ }} |align=center | |moon of Neptune |
Cordelia {{small|Uranus VI}} |bgcolor=black| File:Cordeliamoon.png |align=center |{{val|20.1|3}} |align=center | |moon of Uranus |
Psamathe {{small|Neptune X}} | style="background:#50524f;"| File:Psmathe feat.jpg |align=center |{{val|20|p=≈ }} |align=center | |moon of Neptune |
= From 1 to 19 km =
This list contains some examples of Solar System objects between 1 and 19 km in radius. This is a common size for asteroids, comets and irregular moons.
class="wikitable sortable sticky-header-multi" |
style="font-weight:normal; width:130px;"| Body{{notetag|name=A}}
! class="unsortable" | Image ! data-sort- type="number" style="width:85px; font-weight:normal;"| Radius{{notetag|name=B}} ! data-sort- type="number" style="width:75px;"| Mass ! Type – notes ! class="unsortable" style="font-weight: normal; width: 3.8em; text-align: center;" | Refs{{notetag|name=Refs|text=Reference column specifically for radius (r) and mass (M) citations}} |
---|
Urda {{small|167}} |bgcolor=black| File:167Urda (Lightcurve Inversion).png |align=center |{{val|19.968|0.132}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2018-05-11 last obs |title=JPL Small-Body Database Browser: 167 Urda |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=167 |access-date=5 June 2019}} |
Hydra {{small|Pluto III}} |bgcolor=black|File:Hydra Enhanced Color.jpg |align=center |{{val|19.65}} |align=center |{{val|48|42}} |moon of Pluto |align=center |{{cite journal |last1=Verbiscer |first1=A. J. |last2=Porter |first2=S. B. |last3=Buratti |first3=B. J. |last4=Weaver |first4=H. A. |last5=Spencer |first5=J. R. |last6=Showalter |first6=M. R. |last7=Buie |first7=M. W. |last8=Hofgartner |first8=J. D. |last9=Hicks |first9=M. D. |last10=Ennico-Smith |first10=K. |last11=Olkin |first11=C. B. |last12=Stern |first12=S. A. |last13=Young |first13=L. A. |last14=Cheng |first14=A. |title=Phase Curves of Nix and Hydra from the New Horizons Imaging Cameras |journal=The Astrophysical Journal |date=2018 |volume=852 |issue=2 |pages=L35 |doi=10.3847/2041-8213/aaa486|bibcode=2018ApJ...852L..35V |doi-access=free }}{{·}}{{cite journal|last1=Stern|first1=S. A.|last2=Bagenal|first2=F.|last3=Ennico|first3=K.|last4=Gladstone|first4=G. R.|title=The Pluto system: Initial results from its exploration by New Horizons|journal=Science|date=15 October 2015|volume=350|issue=6258|pages=aad1815|doi=10.1126/science.aad1815|pmid=26472913|display-authors=etal|arxiv = 1510.07704 |bibcode = 2015Sci...350.1815S |s2cid=1220226}} |
Siarnaq {{small|Saturn XXIX}} | style="background:#181818;"| File:Siarnaq-discovery-CFHT.gif |align=center |{{val|19.65|2.95}} |align=center | |moon of Saturn |
Koronis {{small|158}} |bgcolor=black| File:158Koronis (Lightcurve Inversion).png |align=center |{{val|19.513|0.231}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2018-05-08 last obs |title=JPL Small-Body Database Browser: 158 Koronis |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=158 |access-date=12 June 2019}} |
Nix {{small|Pluto II}} |bgcolor=black|File:Nix best view.jpg |align=center |{{val|19.017}} |align=center |{{val|45|40}} |moon of Pluto |
Ganymed {{small|1036}} |bgcolor=black|File:001036-asteroid shape model (1036) Ganymed.png |align=center |{{val|18.838|0.199}} |align=center |{{val|167|318|p=≈ }} |
Okyrhoe {{small|52872}} |bgcolor=black| |align=center |{{val|18|0.6}} |align=center | |align=center |{{cite web |type=2018-08-18 last obs |title=JPL Small-Body Database Browser: 52872 Okyrhoe (1998 SG35) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=52872 |access-date=4 May 2019}} |
Blarney {{small|2320}} |bgcolor=black| |align=center |{{val|18}} |align=center | |belt asteroid |align=center |{{cite web | url=https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=2320 | title=Small-Body Database Lookup }} |
Helene {{small|Saturn XII}} | style="background:#616161;"|File:Helene over Saturn.jpg |align=center |{{val|17.6|0.4}} |align=center | |moon of Saturn; Dione trojan ({{L4}}) |
Sinope {{small|Jupiter IX}} | style="background:#3b3b36;"| File:Sinopé.jpg |align=center |{{val|17.5|0.3}} |align=center | |moon of Jupiter |
Hippocamp {{small|Neptune XIV}} |bgcolor=black|File:Hippocamp-heic1904b.jpg |align=center |{{val|17.4|1}} |align=center |{{val|50|p=≈ }} |moon of Neptune |align=center |{{cite journal|last1= Showalter|first1=M. R.|last2=de Pater|first2= I.|last3= Lissauer|first3=J. J.|last4= French|first4=R. S.|url=https://www.spacetelescope.org/static/archives/releases/science_papers/heic1904/heic1904a.pdf|title= The seventh inner moon of Neptune|journal= Nature|volume= 566|issue= 7744|year= 2019|pages= 350–353|doi= 10.1038/s41586-019-0909-9|pmid=30787452|pmc=6424524|bibcode=2019Natur.566..350S}}{{·}} |
Leucus {{small|11351}} | style="background:#3c3c3c;"| File:11351 Leucus Hubble.jpg |align=center | {{val|17.078|0.323}} |align=center | |Jupiter trojan ({{L4}}) type D |
Stephano {{small|Uranus XX}} | style="background:#4f5050;"|File:Stephano - Uranus moon.jpg |align=center |{{val|16|p=≈ }} |align=center | |moon of Uranus |
Arrokoth {{small|486958}} |bgcolor=black|File:UltimaThule CA06 color 20190516.png |align=center |{{val|15.85|0.25}} |align=center | |
Ida {{small|243}} |bgcolor=black|File:243 Ida large.jpg |align=center |{{val|15.7}} |align=center |{{val|42|6}} |align=center |{{cite book |last=Britt |first=D. T. |author2=Yeomans, D. K.|author3= Housen, K.|author4= Consolmagno, G. |title=Asteroid Density, Porosity, and Structure |journal=Asteroids III |date=2002 |pages=485–500 |doi=10.2307/j.ctv1v7zdn4.37 |url=http://www.lpi.usra.edu/books/AsteroidsIII/pdf/3022.pdf |access-date=2008-10-27 |bibcode=2002aste.book..485B |ref=CITEREFBrittYeomansHousenConsolmagno2002}}{{·}}{{harvnb|Britt|Yeomans|Housen|Consolmagno|2002|p=486}} |
Atlas {{small|Saturn XV}} |bgcolor=black|File:Atlas color PIA21449.png |align=center |{{val|15.1|0.9}} |align=center |{{val|6.6}} |moon of Saturn |
Ananke {{small|Jupiter XII}} | style="background:#2c2c28;"| File:Ananké.jpg |align=center |{{val|14.55|0.3}} |align=center | |moon of Jupiter |
Albiorix {{small|Saturn XXVI}} |bgcolor=black|File:Albiorix WISE-W4.jpg |align=center |{{val|14.3|2.7}} |align=center | |moon of Saturn |
Pan {{small|Saturn XVIII}} |bgcolor=black|File:Pan by Cassini, March 2017.jpg |align=center |{{val|14.1|1.3}} |align=center |{{val|4.95}} |moon of Saturn {{cite journal |author=Porco, C. C. |title=Saturn's Small Inner Satellites: Clues to Their Origins |journal=Science |date=2007 |volume=318 |issue=5856 |pages=1602–1607 |pmid=18063794 |doi=10.1126/science.1143977 |bibcode=2007Sci...318.1602P |s2cid=2253135 |display-authors=etal |author-link=Carolyn C. Porco }} |
Linus {{small|Kalliope I}} |bgcolor=black| |align=center |{{val|14|1}} |align=center |{{val|60|p=≈ }} |asteroid moon of 22 Kalliope |align=center |{{cite journal|last=Descamps|first=P.|title=New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses|date=2008|journal=Icarus|volume=196|issue=2|pages=578–600|bibcode=2008Icar..196..578D|doi=10.1016/j.icarus.2008.03.014|arxiv=0710.1471|author2=Marchis, F.|last3=Pollock|first3=J.|display-authors=2|last4=Berthier|first4=J|last5=Vachier|first5=F|last6=Birlan|first6=M|last7=Kaasalainen|first7=M|last8=Harris|first8=A|last9=Wong|first9=M|s2cid=118437111}}{{·}}{{cite journal |author=F. Marchis |display-authors=etal |title=A three-dimensional solution for the orbit of the asteroidal satellite of 22 Kalliope |journal=Icarus |date=2003 |volume=165 |issue=1 |pages=112–120 |bibcode=2003Icar..165..112M |doi=10.1016/S0019-1035(03)00195-7}} |
Dioretsa {{small|20461}} |bgcolor=black| |align=center | {{val|14|3}} |align=center | |
Perdita {{small|Uranus XXV}} |bgcolor=black|File:Perditamoon.png |align=center |{{val|13|1}} |align=center | |moon of Uranus |
Telesto {{small|Saturn XIII}} |bgcolor=black|File:Telesto cassini closeup.jpg |align=center | {{val|12.4|0.4}} |align=center | |moon of Saturn; Tethys trojan ({{L4}}) |
Mab {{small|Uranus XXVI}} |bgcolor=black| File:Mabmoon.png |align=center |{{val|12|1}} |align=center | |moon of Uranus |
Phobos {{small|Mars I}} |bgcolor=black| File:Phobos colour 2008.jpg |align=center |{{val|11.1|0.15}} |align=center |{{val|10.659}} |moon of Mars |align=center |{{cite web|date=25 April 2019 |title=Phobos In Depth|publisher=NASA Solar System Exploration |url=https://solarsystem.nasa.gov/moons/mars-moons/phobos/in-depth/|access-date=3 May 2019}}{{·}}{{cite web|date=25 April 2019 |title=Phobos By the Numbers|publisher=NASA Solar System Exploration |url=https://solarsystem.nasa.gov/moons/mars-moons/phobos/by-the-numbers/|access-date=3 May 2019 }} |
Paaliaq {{small|Saturn XX}} |bgcolor=black| File:Paaliaq-CFHT.gif |align=center |{{val|11|p=≈ }} |align=center | |moon of Saturn |
Francisco {{small|Uranus XXII}} |bgcolor=black| |align=center |{{val|11|p=≈ }} |align=center | |moon of Uranus |
Leda {{small|Jupiter XIII}} | style="background:#3c3c3c;"|File:Leda WISE-W3.jpg |align=center |{{val|10.75|0.85}} |align=center | |moon of Jupiter |
Calypso {{small|Saturn XIV}} | style="background:#171717;"|File:Calypso N1644755236 1.jpg |align=center |{{val|10.7|0.7}} |align=center | |moons of Saturn; Tethys trojan ({{L5}}) |
Polymele {{small|15094}} | style="background:#3b3b3b;"|File:15094 Polymele Hubble.jpg |align=center | {{val|10.548|0.068}} |align=center | |Jupiter trojan ({{L4}}) type P |
Margaret {{small|Uranus XXIII}} | style="background:#3c3c3c;"|File:S2003u3acircle.gif |align=center |{{val|10|p=≈ }} |align=center | |moon of Uranus |
Ferdinand {{small|Uranus XXIV}} | style="background:#e9e9e9;"|File:Uranus moon 021002 02.jpg |align=center |{{val|10|p=≈ }} |align=center | |moon of Uranus |
Cupid {{small|Uranus XXVII}} |bgcolor=black|File:Cupidmoon.png |align=center |{{val|9|1}} |align=center | |moon of Uranus |
Ymir {{small|Saturn XIX}} | style="background:#181818;"|File:Ymir-CFHT.gif |align=center |{{val|9|p=≈ }} |align=center | |moon of Saturn |
Trinculo {{small|Uranus XXI}} |bgcolor=black| |align=center |{{val|9|p=≈ }} |align=center | |moon of Uranus |
Eros {{small|433}} |bgcolor=black|File:Eros - PIA02923 (color).jpg |align=center |{{val|8.42|0.02}} |align=center |{{val|6.687|0.003}} |align=center |{{Cite journal |display-authors = 6 |first1 = D. K. |last1 = Yeomans |first2 = P. G. |last2 = Antreasian |first3 = J.-P. |last3 = Barriot |first4 = S. R. |last4 = Chesley |first5 = D. W. |last5 = Dunham |first6 = R. W. |last6 = Farquhar |first7 = J. D. |last7 = Giorgini |first8 = C. E. |last8 = Helfrich |first9 = A. S. |last9 = Konopliv |first10 = J. V. |last10 = McAdams |first11 = J. K. |last11 = Miller |first12 = W. M. |last12 = Owen |first13 = D. J. |last13 = Scheeres |first14 = P. C. |last14 = Thomas |first15 = J. |last15 = Veverka |first16 = B. G. |last16 = Williams |date = September 2000 |title = Radio Science Results During the NEAR-Shoemaker Spacecraft Rendezvous with Eros |journal = Science |volume = 289 |issue = 5487 |pages = 2085–2088 |bibcode = 2000Sci...289.2085Y |doi = 10.1126/science.289.5487.2085 |pmid = 11000104 |
Adrastea {{small|Jupiter XV}} |bgcolor=black|File:Adrastea.jpg |align=center |{{val|8.2|2}} |align=center | |moon of Jupiter |
Kiviuq {{small|Saturn XXIV}} | style="background:#181818;"|File:Kiviuq-CFHT.gif |align=center |{{val|8|p=≈ }} |align=center | |moon of Saturn |
Tarvos {{small|Saturn XXI}} | style="background:#3c3c3c;"|File:Tarvos discovery.gif |align=center |{{val|7.5|p=≈ }} |align=center | |moon of Saturn |
Kerberos {{small|Pluto IV}} |bgcolor=black|File:Kerberos (moon).jpg |align=center |{{val|6.333|p=≈ }} |align=center |{{val|16|9}} |moon of Pluto |align=center |{{cite web|url=https://www.youtube.com/watch?v=ZtoLw0KWzsU?t=7470|title=Special Session: Planet 9 from Outer Space - Pluto Geology and Geochemistry|publisher=Lunar and Planetary Institute|website=YouTube|date=25 March 2016|access-date=27 May 2019}}{{·}}{{cite web|last1=Johnston|first1=Robert|title=(134340) Pluto, Charon, Nix, Hydra, Kerberos, and Styx|url=http://www.johnstonsarchive.net/astro/astmoons/am-pluto.html|access-date=3 May 2019}} |
Gaspra {{small|951}} |bgcolor=black|File:951 Gaspra.jpg |align=center |{{val|6.266}} |align=center |{{val|20 |
30}}
|belt asteroid type S |align=center |{{cite journal | display-authors= 6 | author= P. C. Thomas | author2= J. Veverka | author3= D. Simonelli| author4= P. Helfenstein | author5= B. Carcich| author6= M. J. S. Belton | author7= M. E. Davies| author8= C. Chapman| title= The Shape of Gaspra| journal= Icarus| date= 1994| volume= 107|issue =1 |pages= 23–36|doi =10.1006/icar.1994.1004| bibcode=1994Icar..107...23T| doi-access= free}}{{·}}{{cite journal| author-link= Georgij A. Krasinsky | first=G. A. | last= Krasinsky | author2=Pitjeva, E. V. | author2-link=Elena V. Pitjeva|author3=Vasilyev, M. V.|author4=Yagudina, E. I. | bibcode=2002Icar..158...98K| title=Hidden Mass in the Asteroid Belt| journal=Icarus| volume=158| issue=1| pages=98–105|date=July 2002| doi=10.1006/icar.2002.6837}} |
Deimos {{small|Mars II}} |bgcolor=black|File:Deimos-MRO.jpg |align=center |{{val|6.2|0.18}} |align=center |{{val|1.476}} |moon of Mars |align=center |{{·}}{{cite web|date=25 April 2019 |title=Deimos By the Numbers|publisher=NASA Solar System Exploration |url=https://solarsystem.nasa.gov/moons/mars-moons/deimos/by-the-numbers/|access-date=3 May 2019}} |
Skamandrios {{small|Hektor I}} |bgcolor=black| |align=center |{{val|6|1.5}} |align=center | |asteroid moon of 624 Hektor |
Ijiraq {{small|Saturn XXII}} | style="background:#181818;"|File:Ijiraq-discovery-CFHT.gif |align=center |{{val|6|p=≈ }} |align=center | |moon of Saturn |
Halley's Comet {{small|1P}} | style="background:#1f0002;"|File:Lspn comet halley.jpg |align=center |{{val|5.75}} |align=center |{{val|0.22}} |align=center |{{cite web |date=1986 |title=What Have We Learned About Halley's Comet? |publisher=Astronomical Society of the Pacific (No. 6 – Fall 1986) |url=http://www.astrosociety.org/education/publications/tnl/06/06.html |access-date=16 December 2008}}{{·}}{{Cite journal|title=Halley, comet's mass loss and age|author1=G. Cevolani |author2=G. Bortolotti |author3=A. Hajduk |date=1987|publisher=Italian Physical Society|journal=Il Nuovo Cimento C|volume=10|issue=5|pages=587–591|doi=10.1007/BF02507255|bibcode = 1987NCimC..10..587C |s2cid=120603847 }} |
Styx {{small|Pluto V}} |bgcolor=black|File:Styx (moon).jpg |align=center |{{val|5.5|p=≈ }} |align=center |{{val|7.65|p=≈ }} |moon of Pluto |
Romulus {{small|Sylvia I}} |bgcolor=black|File:CMSylvia.png |align=center |{{val|5.4|2.8}} |align=center | |asteroid moon of 87 Sylvia |
Masursky {{small|2685}} |bgcolor=black|File:Asteroid 2685Masurky.png |align=center |{{val|5.372|0.085}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2018-05-09 last obs |title=JPL Small-Body Database Browser: 2685 Masursky (1981 JN) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2685 |access-date=5 June 2019}} |
Erriapus {{small|Saturn XXVIII}} | style="background:#181818;"|File:Erriapus-discovery-CFHT.gif |align=center |{{val|5|p=≈ }} |align=center | |moon of Saturn |
Callirrhoe {{small|Jupiter XVII}} |bgcolor=black|File:Callirrhoe - New Horizons.gif |align=center |{{val|4.8|0.65}} |align=center | |moon of Jupiter |
Alexhelios {{small|Kleopatra I}} |bgcolor=black|File:Kleopatra moons - eso2113e.jpg |align=center |{{val|4.45|0.8}} |align=center | |asteroid moon of 216 Kleopatra |align=center |{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (216) Kleopatra, Alexhelios, and Cleoselene |publisher = Johnston's Archive |date = 21 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-00216.html |access-date = 8 June 2019}} |
Esclangona {{small|1509}} |bgcolor=black| |align=center |{{val|4.085|0.3}} |align=center | |inner belt asteroid type S; binary |align=center |{{cite web |type=2019-05-11 last obs |title=JPL Small-Body Database Browser: 1509 Esclangona (1938 YG) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1509 |access-date=5 June 2019}} |
Themisto {{small|Jupiter XVIII}} | style="background:#222342;"| File:S 2000 J 1.jpg |align=center |{{val|4|p=≈ }} |align=center | |moon of Jupiter |
Daphnis {{small|Saturn XXXV}} |bgcolor=black| File:Daphnis (Saturn's Moon).jpg |align=center |{{val|3.8|0.8}} |align=center |{{val|0.077|0.015}} |moon of Saturn |
Petit-Prince {{small|Eugenia I}} |bgcolor=black| |align=center |{{val|3.5|1}} |align=center | |asteroid moon of 45 Eugenia |align=center |{{cite web |date=21 September 2014 |title=(45) Eugenia, Petit-Prince, and S/2004 (45) 1 |publisher=Johnston's Archive |author=Wm. Robert Johnston |url=http://www.johnstonsarchive.net/astro/astmoons/am-00045.html |access-date=12 June 2019}} |
Praxidike {{small|Jupiter XXVII}} |bgcolor=black| File:Praxidike-Jewitt-CFHT-annotated.gif |align=center |{{val|3.5|0.35}} |align=center | |moon of Jupiter |
Bestla {{small|Saturn XXXIX}} | style="background:#3c3c3c;"| File:Bestla-cassini.png |align=center |{{val|3.5|p=≈ }} |align=center | |moon of Saturn |
Remus {{small|Sylvia II}} |bgcolor=black|File:CMSylvia.png |align=center |{{val|3.5|p=≈ }} |align=center | |asteroid moon of 87 Sylvia |
Kalyke {{small|Jupiter XXIII}} | style="background:#181818;"| File:Kalyke-Jewitt-CFHT-annotated.gif |align=center |{{val|3.45|0.65}} |align=center | |moon of Jupiter |
Cleoselene {{small|Kleopatra II}} |bgcolor=black|File:Kleopatra moons - eso2113e.jpg |align=center |{{val|3.45|0.8}} |align=center | |asteroid moon of 216 Kleopatra |
S/2019 (31) 1 {{small|Euphrosyne I}} |bgcolor=black| |align=center |{{val|3.35|1.2}} |align=center | |asteroid moon of 31 Euphrosyne |align=center |{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (31) Euphrosyne |publisher = Johnston's Archive |date = 27 May 2019 |url = http://www.johnstonsarchive.net/astro/astmoons/am-00031.html |access-date = 15 June 2019}} |
Tempel 1 {{small|9P}} |bgcolor=black|File:PIA02127.jpg |align=center |{{val|3|0.1}} |align=center | |Jupiter-family comet; {{small|Deep Impact flyby and impacted}} |align=center |{{cite web |type=2019-01-02 last obs |title=JPL Small-Body Database Browser: 9P/Tempel 1 |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=9P |access-date=8 June 2019}} |
Ireland {{small|5029}} |bgcolor=black| |align=center |{{val|3}} |align=center | |belt asteroid |align=center |https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=5029 |
Phaethon {{small|3200}} | style="background:#3c3c3c;"|File:PIA22185.gif |align=center |{{val|2.9}} |align=center | |
{{mpl-|53319|1999 JM|8}} {{small|53319}} | style="background:#404040;"|File:Asteroid 1999 JM8.gif |align=center |{{val|2.7|0.6}} |align=center | |align=center |{{Cite journal |first1 = Vishnu |last1 = Reddy |first2 = Michael J. |last2 = Gaffey |first3 = Paul A. |last3 = Abell |first4 = Paul S. |last4 = Hardersen |date = May 2012 |title = Constraining albedo, diameter and composition of near-Earth asteroids via near-infrared spectroscopy |journal = Icarus |volume = 219 |issue = 1 |pages = 382–392 |bibcode = 2012Icar..219..382R |doi = 10.1016/j.icarus.2012.03.005}} |
Borrelly {{small|19P}} |bgcolor=black|File:Comet Borrelly Nucleus.jpg |align=center |{{val|2.66}} |align=center | |align=center |{{cite journal |last=Weaver |first=H. A. |author2=Stern, S.A. |author3=Parker, J. Wm. |title=Hubble Space Telescope STIS Observations of Comet 19P/BORRELLY during the Deep Space 1 Encounter |journal=The Astronomical Journal|publisher=The American Astronomical Society |volume=126 |issue=1 |pages=444–451 |date=2003 |doi=10.1086/375752 |bibcode = 2003AJ....126..444W |doi-access=free }} |
Šteins {{small|2867}} |bgcolor=black|File:2867 Šteins by Rosetta (reprocessed).png |align=center |{{val|2.58|0.084}} |align=center | |belt asteroid type E |
Atira {{small|163693}} | style="background:#2c2c2c;"|File:Atira.20jan17.u2.s1p0.gif |align=center |{{val|2.4|0.25}} |align=center | |Atira asteroid type S; binary |align=center |{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (163693) Atira |publisher = Johnston's Archive |date = 19 February 2017 |url = http://www.johnstonsarchive.net/astro/astmoons/am-163693.html |access-date = 8 June 2019}} |
Annefrank {{small|5535}} |bgcolor=black|File:Stardust - Annefrank.jpg |align=center |{{val|2.4}} |align=center | |belt asteroid type S |align=center |{{cite web |type=2018-05-24 last obs |title=JPL Small-Body Database Browser: 5535 Annefrank (1942 EM) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=5535 |access-date=8 June 2019}} |
Balam {{small|3749}} |bgcolor=black|File:003749-asteroid shape model (3749) Balam.png |align=center |{{val|2.332|0.107}} |align=center |{{val|0.51|0.02}} |belt asteroid type S; trinary |align=center |{{cite web |type=2019-05-11 last obs |title=JPL Small-Body Database Browser: 3749 Balam (1982 BG1) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3749 |access-date=5 June 2019}}{{·}}{{cite web |date = 2009-01-13 |title = (3749) Balam, S/2002 (3749) 1, and third component |publisher = Johnston's Archive |author = Wm. Robert Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-03749.html |access-date = 15 July 2020}} |
Pallene {{small|Saturn XXXIII}} | style="background:#b5b5b5;"|File:Pallene N1665945513 1.jpg |align=center |{{val|2.22|0.07}} |align=center | |moon of Saturn |align=center |{{cite conference | first = P. C. | last = Thomas |display-authors=4 | author2 = Burns, J. A. |author3=Tiscareno, M. S. |author4=Hedman, M. M. |author5=Helfenstein, P. | title = Saturn's Mysterious Arc-Embedded Moons: Recycled Fluff? | book-title = 44th Lunar and Planetary Science Conference | page = 1598 | date = 2013 | url = http://www.lpi.usra.edu/meetings/lpsc2013/pdf/1598.pdf | access-date = 8 June 2019}} |
Florence {{small|3122}} | style="background:#181818;"|File:Triple asteroid 3122 Florence.gif |align=center |{{val|2.201|0.015}} |align=center |{{val|0.079|0.002}} |Amor asteroid type S; trinary |align=center |{{cite journal |first1 = A. |last1 = Mainzer |first2 = T. |last2 = Grav |first3 = J. |last3 = Masiero |first4 = E. |last4 = Hand |first5 = J. |last5 = Bauer |first6 = D. |last6 = Tholen |date = November 2011 |title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 25 |bibcode = 2011ApJ...741...90M |doi = 10.1088/0004-637X/741/2/90 |arxiv = 1109.6407|s2cid = 118700974 }}{{·}}{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (3122) Florence |publisher = Johnston's Archive |date = 27 May 2019 |url = http://www.johnstonsarchive.net/astro/astmoons/am-03122.html |access-date = 9 June 2019}} |
Wild 2 {{small|81P}} |bgcolor=black|File:Wild2 3.jpg |align=center |{{val|2.133}} |align=center | |align=center |{{cite web |title=Comet 81P/Wild 2 |publisher=The Planetary Society |url=http://www.planetary.org/explore/topics/asteroids_and_comets/wild2.html |access-date=8 June 2019 |archive-url=https://web.archive.org/web/20090106004009/http://planetary.org./explore/topics/asteroids_and_comets/wild2.html |archive-date=6 January 2009 }} |
Litva {{small|2577}} |bgcolor=black| |align=center |{{val|2.115}} |align=center | |Mars-crosser type EU; trinary |align=center |{{cite web |title = LCDB Data for (2577) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=2577%7C |access-date = 11 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040734/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=2577%7C }} |
Churyumov–Gerasimenko {{small|67P}} |bgcolor=black|File:67P Churyumov-Gerasimenko - Rosetta (32755885495).png |align=center |{{val|2}} |align=center |{{val|0.00998|fmt=none}} |align=center |{{cite web |type=2017-04-27 last obs |title=JPL Small-Body Database Browser: 67P/Churyumov-Gerasimenko |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=67P |
Donaldjohanson {{small|52246}} |bgcolor=black|File:Donaldjohanson closest approach.png |align=center |{{val|1.948|0.007}} |align=center | |belt asteroid type C |align=center |{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = J. |last6 = Dailey |first7 = P. R. M. |last7 = Eisenhardt |first8 = R. S. |last8 = McMillan |first9 = T. B. |last9 = Spahr |first10 = M. F. |last10 = Skrutskie |first11 = D. |last11 = Tholen |first12 = R. G. |last12 = Walker |first13 = E. L. |last13 = Wright |first14 = E. |last14 = DeBaun |first15 = D. |last15 = Elsbury |first16 = T. IV |last16 = Gautier |first17 = S. |last17 = Gomillion |first18 = A. |last18 = Wilkins |date = November 2011 |title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 20 |bibcode = 2011ApJ...741...68M |doi = 10.1088/0004-637X/741/2/68 |arxiv = 1109.4096|s2cid = 118745497 }} |
Camelot {{small|9500}} |bgcolor=black| |align=center |{{val|1.9}} |align=center | |belt asteroid |align=center |{{cite web | url=https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=9500 | title=Small-Body Database Lookup }} |
Cuno {{small|4183}} | style="background:#3c3c3c;"|File:4183 cuno.jpg |align=center |{{val|1.826|0.051}} |align=center | |Apollo asteroid type S/type Q |align=center |{{cite web |type=2018-11-06 last obs |title=JPL Small-Body Database Browser: 4183 Cuno (1959 LM) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=4183 |access-date=12 June 2019}} |
{{mpl-|6178|1986 DA}} {{small|6178}} |bgcolor=black| |align=center |{{val|1.575}} |align=center | |align=center |{{Cite journal |first1 = Petr |last1 = Pravec |first2 = Alan W. |last2 = Harris |first3 = Peter |last3 = Kusnirák |first4 = Adrián |last4 = Galád |first5 = Kamil |last5 = Hornoch |date = September 2012 |title = Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations |journal = Icarus |volume = 221 |issue = 1 |pages = 365–387 |bibcode = 2012Icar..221..365P |doi = 10.1016/j.icarus.2012.07.026 }} |
Pichi üñëm {{small|Alauda I}} |bgcolor=black| |align=center |{{val|1.55|0.45}} |align=center | |asteroid moon of 702 Alauda |align=center |{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (702) Alauda and Pichi unem |publisher = Johnston's Archive |date = 21 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-00702.html |access-date = 15 June 2019}} |
Toutatis {{small|4179}} | style="background:#282828;"|File:Toutatis.jpg |align=center |{{val|1.516}} |align=center |{{val|0.0505}} |align=center |{{cite journal |title=The Ginger-shaped Asteroid 4179 Toutatis: New Observations from a Successful Flyby of Chang'e-2 |journal=Scientific Reports |publisher=Nature Research |volume=3 |page=3411 |number=3411 |doi=10.1038/srep03411 |doi-access=free |pmid=24336501 |pmc=3860288 |arxiv=1312.4329 |bibcode=2013NatSR...3.3411H |year=2013 |last1=Huang |first1=Jiangchuan |last2=Ji |first2=Jianghui |last3=Ye |first3=Peijian |last4=Wang |first4=Xiaolei |last5=Yan |first5=Jun |
Methone {{small|Saturn XXXII}} |bgcolor=black|File:Methone PIA14633.jpg |align=center |{{val|1.45|0.03}} |align=center | |moon of Saturn |
Carpo (moon) {{small|Jupiter XLVI}} | |align=center |{{val|1.44}} |align=center | |
{{mpl-|285263|1998 QE|2}} {{small|285263}} |bgcolor=black|File:(285263) 1998 QE2, Goldstone, May 30, 2013.jpg |align=center |{{val|1.375}} |align=center | |align=center |{{cite web |date=28 May 2013 |title=(285263) 1998 QE2 Goldstone Radar Observations Planning |publisher=NASA/JPL Asteroid Radar Research |author=Dr. Lance A. M. Benner |url=http://echo.jpl.nasa.gov/asteroids/1998QE2/1998QE2_planning.html |access-date=7 June 2019}} |
Polydeuces {{small|Saturn XXXIV}} |bgcolor=black|File:Polydeuces.jpg |align=center |{{val|1.3|0.4}} |align=center | |moon of Saturn; Dione trojan ({{L5}}) |
{{mpl-|153591|2001 SN|263}} {{small|153591}} |bgcolor=black|File:2001sn263 arecibo.png |align=center |{{val|1.315|0.2}} |align=center |{{val|0.00951|0.00013|fmt=none}} |Amor asteroid type C; trinary |align=center |{{Cite journal |first1 = Julia |last1 = Fang |first2 = Jean-Luc |last2 = Margot |first3 = Marina |last3 = Brozovic |first4 = Michael C. |last4 = Nolan |first5 = Lance A. M. |last5 = Benner |first6 = Patrick A. |last6 = Taylor |date = May 2011 |title = Orbits of Near-Earth Asteroid Triples 2001 SN263 and 1994 CC: Properties, Origin, and Evolution |journal = The Astronomical Journal |volume = 141 |issue = 5 |page = 15 |bibcode = 2011AJ....141..154F |doi = 10.1088/0004-6256/141/5/154 |arxiv = 1012.2154 |s2cid = 119193346 }}{{·}}{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (153591) 2001 SN263, "Beta", and "Gamma" |publisher = Johnston's Archive |date = 21 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-153591.html |access-date = 9 June 2019}} |
S/2003 (1509) 1 {{small|Esclangona I}} |bgcolor=black| |align=center |{{val|1.285}} |align=center | |asteroid moon of 1509 Esclangona |align=center |{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (1509) Esclangona and S/2003 (1509) 1 |publisher = Johnston's Archive |date = 21 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-01509.html |access-date = 5 June 2019}} |
APL {{small|132524}} |bgcolor=black|File:132524 APL New Horizons.jpg |align=center |{{val|1.25|p=≈ }} |align=center | |belt asteroid type S |align=center |{{Cite news |title = New Horizons Mission to Pluto |date = 18 July 2015 |work = Technology Org |url = https://www.technology.org/2015/07/18/new-horizons-mission-to-pluto/ |access-date = 4 December 2018}} |
Camillo {{small|3752}} | style="background:#282828;"|File:3752 Camillo Radar.jpg |align=center |{{val|1.153|0.044}} |align=center | |
Cruithne {{small|3753}} | style="background:#2c2c2c;"|File:Cruithne.jpg |align=center |{{val|1.036|0.053}} |align=center | |Aten asteroid type Q; quasi-satellite of Earth |align=center |{{cite web |type=2019-05-12 last obs |title=JPL Small-Body Database Browser: 3753 Cruithne (1986 TO) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3753 |access-date=8 June 2019}} |
= Below 1 km =
{{See also|Satellite|Space debris}}
This list contains examples of objects below 1 km in radius. That means that irregular bodies can have a longer chord in some directions, hence the mean radius averages out.
In the asteroid belt alone there are estimated to be between 1.1 and 1.9 million objects with a radius above 0.5 km,{{cite press release
|first=Edward
|last=Tedesco
|author2=Metcalfe, Leo
|title=New study reveals twice as many asteroids as previously believed
|publisher=European Space Agency
|date=4 April 2002
|url=http://www.spaceref.com/news/viewpr.html?pid=7925
|access-date=20 October 2012
|archive-date=6 March 2023
|archive-url=https://web.archive.org/web/20230306222828/https://spaceref.com/press-release/new-study-reveals-twice-as-many-asteroids-as-previously-believed/
|url-status=dead
}} many of which are in the range 0.5–1.0 km. Countless more have a radius below 0.5 km.
Very few objects in this size range have been explored or even imaged. The exceptions are objects that have been visited by a probe, or have passed close enough to Earth to be imaged. Radius is by mean geometric radius. Number of digits not an endorsement of significant figures. Mass scale shifts from × 1015 to 109 kg, which is equivalent to one billion kg or 1012 grams (Teragram – Tg).
Currently most of the objects of mass between 109 kg to 1012 kg (less than 1000 teragrams (Tg)) listed here are near-Earth asteroids (NEAs). The Aten asteroid {{mp|1994 WR|12}} has less mass than the Great Pyramid of Giza, 5.9 × 109 kg.
For more about very small objects in the Solar System, see meteoroid, micrometeoroid, cosmic dust, and interplanetary dust cloud. (See also Visited/imaged bodies.)
class="wikitable sortable sticky-header-multi" |
style="font-weight:normal; width:130px;"| Body{{notetag|name=A}}
! class="unsortable" | Image ! data-sort- type="number" style="width:85px; font-weight:normal;"| Radius{{notetag|name=B}} ! data-sort- type="number" style="width:75px;"| Mass ! Type – notes ! class="unsortable" style="font-weight: normal; width: 3.8em; text-align: center;" | Refs{{notetag|name=Refs|text=Reference column specifically for radius (r) and mass (M) citations}} |
---|
Ra-Shalom {{small|2100}} |bgcolor=black|File:2100Ra-Shalom (Lightcurve Inversion).png |align=center |{{val|990|25}} |align=center | |
Geographos {{small|1620}} |bgcolor=black|File:Geographos.jpg |align=center |{{val|980|30}} |align=center | |
Midas {{small|1981}} |bgcolor=black| |align=center |{{val|975|35}} |align=center | |Apollo asteroid type S |
Mithra {{small|4486}} |bgcolor=black| |align=center |{{val|924.5|11}} |align=center | |Apollo asteroid type S |
{{mpl-|12538|1998 OH}} {{small|12538}} |bgcolor=black| |align=center |{{val|831.5|164.5}} |align=center | |
Tantalus {{small|2102}} |bgcolor=black|File:1862Apollo (Lightcurve Inversion).png |align=center |{{val|824.5|22.5}} |align=center | |align=center |{{cite web |type=2017-06-28 last obs |title=JPL Small-Body Database Browser: 2102 Tantalus (1975 YA) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2102 |access-date=8 June 2019}} |
Braille {{small|9969}} |bgcolor=black|File:Braille3.jpg |align=center |{{val|820}} |align=center | |align=center |{{cite web |title = LCDB Data for (9969) Braille |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=9969%7CBraille |access-date = 8 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040737/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=9969%7CBraille }} |
{{mpl-|308242|2005 GO|21}} {{small|308242}} | style="background:#282828;"| File:2005GO21-20120617.jpg |align=center |{{val|780}} |align=center | |align=center |{{cite web |title = LCDB Data for (308242) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=308242%7C |access-date = 9 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040737/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=308242%7C }} |
Apollo {{small|1862}} |bgcolor=black|File:1862Apollo (Lightcurve Inversion).png |align=center |{{val|750|p=≈ }} |align=center | |align=center |{{cite web |type=2018-04-27 last obs |title=JPL Small-Body Database Browser: 1862 Apollo (1932 HA) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1862 |access-date=8 June 2019}} |
{{mpl-|85989|1999 JD|6}} {{small|85989}} | style="background:#646464;"|File:Asteroid 1999 JD6.jpg |align=center |{{val|731|10.5}} |align=center | |Aten asteroid type K; contact binary |align=center |{{cite web |type=2019-06-08 last obs |title=JPL Small-Body Database Browser: 85989 (1999 JD6) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=85989 |access-date=12 June 2019}} |
Icarus {{small|1566}} | style="background:#010658;"| File:Icarus Goldstone radar Jun17.jpg |align=center |{{val|730}} |align=center | |align=center |{{Cite journal |display-authors = 6 |first1 = Adam H. |last1 = Greenberg |first2 = Jean-Luc |last2 = Margot |first3 = Ashok K. |last3 = Verma |first4 = Patrick A. |last4 = Taylor |first5 = Shantanu P. |last5 = Naidu |first6 = Marina. |last6 = Brozovic |first7 = Lance A. M. |last7 = Benner |date = March 2017 |title = Asteroid 1566 Icarus's Size, Shape, Orbit, and Yarkovsky Drift from Radar Observations |journal = The Astronomical Journal |volume = 153 |issue = 3 |page = 16 |bibcode = 2017AJ....153..108G |doi = 10.3847/1538-3881/153/3/108 |arxiv = 1612.07434|s2cid = 28388555 |doi-access = free }} |
Dactyl {{small|Ida I}} |bgcolor=black|File:Dactyl-HiRes.jpg |align=center |{{val|700}} |align=center | |asteroid moon of 243 Ida |
Castalia {{small|4769}} |bgcolor=black| |align=center |{{val|700}} |align=center | |Apollo asteroid type S; contact binary |align=center |{{cite web |type=2016-06-17 last obs |title=JPL Small-Body Database Browser: 4769 Castalia (1989 PB) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=4769 |access-date=8 June 2019}} |
{{mpl-|214869|2007 PA|8}} {{small|214869}} | style="background:#181818;"| File:Pa8radar.jpg |align=center |{{val|675|70}} |align=center | |align=center |{{Cite journal |first1 = Marina |last1 = Brozovic |first2 = Lance A. M. |last2 = Benner |first3 = Christopher |last3 = Magri |first4 = Daniel J. |last4 = Scheeres |first5 = Michael W. |last5 = Busch |first6 = Jon D. |last6 = Giorgini |date = April 2017 |title = Goldstone radar evidence for short-axis mode non-principal-axis rotation of near-Earth asteroid (214869) 2007 PA8 |journal = Icarus |volume = 286 |pages = 314–329 |bibcode = 2017Icar..286..314B |doi = 10.1016/j.icarus.2016.10.016}} |
Moshup {{small|66391}} |bgcolor=black|File:1999kw4 vlt-eso1910.jpg |align=center |{{val|658.5|20}} |align=center |{{val|2490|54}} |Aten asteroid type S; binary |align=center |{{cite web |type=2019-06-04 last obs |title=JPL Small-Body Database Browser: 66391 Moshup (1999 KW4) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=66391 |access-date=8 June 2019}}{{·}}{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (66391) Moshup and Squannit |publisher = Johnston's Archive |date = 20 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-66391.html |access-date = 8 June 2019}} |
{{mpl-|29075|1950 DA}} {{small|29075}} |bgcolor=black|File:1950 DA (color).png |align=center |{{val|653}} |align=center |{{val|2000|p=≈ }} |Apollo asteroid type S |align=center |{{Cite journal |first1 = Michael W. |last1 = Busch |first2 = Jon D. |last2 = Giorgini |first3 = Steven J. |last3 = Ostro |first4 = Lance A. M. |last4 = Benner |first5 = Raymond F. |last5 = Jurgens |first6 = Randy |last6 = Rose |date = October 2007 |title = Physical modeling of near-Earth Asteroid (29075) 1950 DA |url = https://echo.jpl.nasa.gov/asteroids/29075_1950DA/busch.etal.2007.1950da.pdf |journal = Icarus |volume = 190 |issue = 2 |pages = 608–621 |bibcode = 2007Icar..190..608B |doi = 10.1016/j.icarus.2007.03.032}}{{·}}{{cite web |title = Earth Impact Risk Summary: 29075 |publisher = NASA/JPL Near-Earth Object Program Office |url = https://cneos.jpl.nasa.gov/sentry/details.html#?des=29075 |archive-url = https://web.archive.org/web/20190305035418/https://cneos.jpl.nasa.gov/sentry/details.html#?des=29075 |archive-date = 5 March 2019 |url-status = live |access-date = 14 June 2019 |df = dmy-all}} |
{{mpl-|394130|2006 HY|51}} {{small|394130}} |bgcolor=black| |align=center |{{val|609|114}} |align=center | |align=center |{{cite web |type=2019-06-01 last obs |title=JPL Small-Body Database Browser: 394130 (2006 HY51) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=394130 |access-date=12 June 2019}} |
Hartley 2 {{small|103P}} |bgcolor=black|File:Comet Hartley 2 (super crop).jpg |align=center |{{val|570|80}} |align=center |{{val|300|p=≈ }} |align=center |{{cite journal |last=Lisse |first=C. M. |author2=Fernandez |author3=Reach |author4=Bauer |author5=A'Hearn |author6=Farnham |display-authors= etal |title=Spitzer Space Telescope Observations of the Nucleus of Comet 103P/Hartley 2 |journal=Publications of the Astronomical Society of the Pacific |volume=121 |issue=883 |pages=968–975 |date=2009 |doi=10.1086/605546 |jstor=10.1086/605546 |bibcode=2009PASP..121..968L |arxiv = 0906.4733|s2cid=17318657 |
{{mpl-|163899|2003 SD|220}} {{small|163899}} | style="background:#525252;"|File:PIA20279.jpg |align=center |{{val|515}} |align=center | |align=center |{{cite web |title = LCDB Data for (163899) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=163899%7C |access-date = 9 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040738/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=163899%7C }} |
Nyx {{small|3908}} |bgcolor=black|File:3908 nyx-s02.jpg |align=center |{{val|500|75}} |align=center | |align=center |{{cite web |type=2019-04-25 last obs |title=JPL Small-Body Database Browser: 3908 Nyx (1980 PA) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3908 |access-date=8 June 2019}} |
{{mpl-|153814|2001 WN|5}} {{small|153814}} |bgcolor=black| |align=center |{{val|466|5.5}} |align=center | |align=center |{{cite web |type=2019-06-02 last obs |title=JPL Small-Body Database Browser: 153814 (2001 WN5) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=153814 |access-date=10 June 2019}} |
{{mpl|2017 YE|5}}
| style="background:#181818;"| File:PIA22559.gif |align=center |{{val|450|25}} |align=center | |Apollo asteroid type S; binary |align=center |{{cite web |title = LCDB Data for 2017 YE5 |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0%7C2017+YE5 |access-date = 9 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040736/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0%7C2017+YE5 }} |
Ryugu {{small|162173}} |bgcolor=black|File:Ryugu colored.jpg |align=center |{{val|432.5|7.5}} |align=center |{{val|450|p=≈ }} |align=center |{{cite journal |first1 = T. G. |last1 = Müller |first2 = J. |last2 = Durech |first3 = M. |last3 = Ishiguro |first4 = M. |last4 = Mueller |first5 = T. |last5 = Krühler |first6 = H. |last6 = Yang |date = March 2017 |title = Hayabusa-2 mission target asteroid 162173 Ryugu (1999 JU3): Searching for the object's spin-axis orientation |journal = Astronomy and Astrophysics |volume = 599 |page = 25 |bibcode = 2017A&A...599A.103M |doi = 10.1051/0004-6361/201629134 |arxiv = 1611.05625 |s2cid = 73519172 |
{{mpl-|162058|1997 AE|12}} {{small|162058}} |bgcolor=black| |align=center |{{val|423.5|6.5}} |align=center | |align=center |{{cite journal |display-authors = 6 |first1 = C. R. |last1 = Nugent |first2 = A. |last2 = Mainzer |first3 = J. |last3 = Bauer |first4 = R. M. |last4 = Cutri |first5 = E. A. |last5 = Kramer |first6 = T. |last6 = Grav |first7 = J. |last7 = Masiero |first8 = S. |last8 = Sonnett |first9 = E. L. |last9 = Wright |date = September 2016 |title = NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos |journal = The Astronomical Journal |volume = 152 |issue = 3 |page = 12 |bibcode = 2016AJ....152...63N |doi = 10.3847/0004-6256/152/3/63 |arxiv = 1606.08923 |s2cid = 119289027 |doi-access = free }} |
{{mpl|2014 JO|25}}
| style="background:#282828;"|File:PIA21597 - New Radar Images of Asteroid 2014 JO25 (cropped).gif |align=center |{{val|409}} |align=center | |Apollo asteroid type S; contact binary |align=center |{{cite web |title = LCDB Data for 2014 JO25 |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0%7C2014+JO25 |access-date = 9 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040733/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0%7C2014+JO25 }} |
Hermes {{small|69230}} | style="background:#646464;"|File:Hermes planetoid.jpg |align=center |{{val|400|50}} |align=center | |Apollo asteroid type Sq |align=center |{{cite journal |display-authors = etal |first1 = F. |last1 = Marchis |first2 = J. E. |last2 = Enriquez |first3 = J. P. |last3 = Emery |first4 = M. |last4 = Mueller |first5 = M. |last5 = Baek |first6 = J. |last6 = Pollock |date = November 2012 |title = Multiple asteroid systems: Dimensions and thermal properties from Spitzer Space Telescope and ground-based observations |journal = Icarus |volume = 221 |issue = 2 |pages = 1130–1161 |bibcode = 2012Icar..221.1130M |doi = 10.1016/j.icarus.2012.09.013 |arxiv = 1604.05384 |s2cid = 161887 }} |
Didymos {{small|65803}} |bgcolor=black|File:Didymos-Dimorphos 0401929889 03770 crop.png |align=center |{{val|390|4}} |align=center |{{val|527}} |Apollo asteroid type Xk; binary |align=center |{{cite web |type=2018-04-24 last obs |title=JPL Small-Body Database Browser: 65803 Didymos (1996 GT) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=65803 |access-date=8 June 2019}}{{·}}{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (65803) Didymos |publisher = Johnston's Archive |date = 20 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-65803.html |access-date = 8 June 2019}} |
Aten {{small|2062}} |bgcolor=black| |align=center |{{val|365|15}} |align=center | |
Aegaeon {{small|Saturn LIII}} |bgcolor=black|File:N1643264379 1.jpg |align=center |{{val|330|60}} |align=center | |
{{mpl|2015 TB|145}}
| style="background:#282828;"|File:Skull2015-TB145.jpg |align=center |{{val|325|15}} |align=center | |align=center |{{cite journal | url=https://www.aanda.org/articles/aa/pdf/2017/02/aa29584-16.pdf | title=Large Halloween asteroid at lunar distance | last1=Müller|first1=T. G. | last2=Marciniak|first2=A. | last3=Butkiewicz-Bąk|first3=M. | last4=Duffard|first4=R. | last5=Oszkiewicz|first5=D. | last6=Käufl|first6=H. U. | last7=Szakáts|first7=R. | last8=Santana-Ros|first8=T. | last9=Kiss|first9=C. | last10=Santos-Sanz|first10=P. | journal=Astronomy & Astrophysics | volume=598 | pages=A63 | doi=10.1051/0004-6361/201629584 | arxiv=1610.08267 | bibcode=2017A&A...598A..63M | date=February 2017 | s2cid=119162848 | access-date=9 June 2019}} |
{{mpl-|136617|1994 CC}} {{small|136617}} |bgcolor=black|File:1994CC-with-moons.gif |align=center |{{val|310|30}} |align=center |{{val|266|32.9}} |Apollo asteroid type Sq; trinary |align=center |{{cite journal |first1 = Marina |last1 = Brozovic |first2 = Lance A. M. |last2 = Benner |first3 = Patrick A. |last3 = Taylor |first4 = Michael C. |last4 = Nolan |first5 = Ellen S. |last5 = Howell|author5-link=Ellen Howell |first6 = Christopher |last6 = Magri |date = November 2011 |title = Radar and optical observations and physical modeling of triple near-Earth Asteroid (136617) 1994 CC |journal = Icarus |volume = 216 |issue = 1 |pages = 241–256 |bibcode = 2011Icar..216..241B |doi = 10.1016/j.icarus.2011.09.002 |arxiv = 1310.2000 }}{{·}}{{cite web |first1 = Wm. Robert |last1 = Johnston |title = (136617) 1994 CC, "Beta", and "Gamma" |publisher = Johnston's Archive |date = 21 September 2014 |url = http://www.johnstonsarchive.net/astro/astmoons/am-136617.html |access-date = 9 June 2019}} |
{{mpl-|172034|2001 WR|1}} {{small|172034}} |bgcolor=black| |align=center |{{val|315.5|9}} |align=center | |align=center |{{cite web |type=2019-05-21 last obs |title=JPL Small-Body Database Browser: 172034 (2001 WR1) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=172034 |access-date=8 June 2019}} |
Golevka {{small|6489}} |bgcolor=black|File:Asteroid-golevka.jpeg |align=center |{{val|265|15}} |align=center | |align=center |{{cite web |type=2015-11-03 last obs |title=JPL Small-Body Database Browser: 6489 Golevka (1991 JX) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=6489 |access-date=8 June 2019}} |
Bennu {{small|101955}} |bgcolor=black|File:Bennu mosaic OSIRIS-REx (square).png |align=center |{{val|262.5|37.5}} |align=center |{{val|78|9}} |Apollo asteroid type B |align=center |{{cite journal |last1=Nolan |first1=M. C. |last2=Magri |first2=C. |last3=Howell |first3=E. S.|author3-link=Ellen Howell |last4=Benner |first4=L. A. M. |last5=Giorgini |first5=J. D. |last6=Hergenrother|first6=C. W. |last7=Hudson |first7=R. S. |last8=Lauretta |first8=D. S. |last9=Margot |first9=J. L. |last10=Ostro |first10=S. J. |last11=Scheeres |first11=D. J. |title=Shape model and surface properties of the OSIRIS-REx target Asteroid (101955) Bennu from radar and lightcurve observations |journal=Icarus|volume=226|issue=1|year=2013|pages=629–640 |issn=0019-1035|doi=10.1016/j.icarus.2013.05.028|bibcode=2013Icar..226..629N |url=http://www.escholarship.org/uc/item/6mh8b2t5}}{{·}}{{cite journal |last1=Chesley|first1=Steven R.|last2=Farnocchia|first2=Davide|last3=Nolan|first3=Michael C.|last4=Vokrouhlický|first4=David|last5=Chodas|first5=Paul W.|last6=Milani|first6=Andrea|last7=Spoto|first7=Federica|last8=Rozitis|first8=Benjamin|last9=Benner|first9=Lance A.M.|last10=Bottke|first10=William F.|last11=Busch|first11=Michael W.|last12=Emery|first12=Joshua P.|last13=Howell|first13=Ellen S.|author13-link=Ellen Howell|last14=Lauretta|first14=Dante S.|last15=Margot|first15=Jean-Luc|last16=Taylor|first16=Patrick A.|title=Orbit and bulk density of the OSIRIS-REx target Asteroid (101955) Bennu|journal=Icarus|volume=235|date=2014|pages=5–22|issn=0019-1035|doi=10.1016/j.icarus.2014.02.020 | bibcode=2014Icar..235....5C|arxiv=1402.5573|s2cid=30979660}} |
{{mpl-|153201|2000 WO|107}} {{small|153201}} |bgcolor=black|File:2000WO107-20201128.jpg |align=center |{{val|255|41.5}} |align=center | |align=center |{{cite web |type=2018-10-13 last obs |title=JPL Small-Body Database Browser: 153201 (2000 WO107) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=153201 |access-date=12 June 2019}} |
{{mpl-|163132|2002 CU|11}} {{small|163132}} |bgcolor=black| |align=center |{{val|230|8.5}} |align=center | |align=center |{{cite web |type=2018-09-09 last obs |title=JPL Small-Body Database Browser: 163132 (2002 CU11) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=163132 |access-date=8 June 2019}} |
|Squannit {{small|Moshup I}} |bgcolor=black|File:1999kw4 vlt-eso1910.jpg |align=center |{{val|225.5|13.5}} |align=center | |asteroid moon of 66391 Moshup |
{{mpl|2014 HQ|124}}
| style="background:#646464;"| File:PIA17829-Asteroid-2013YP139-20131229.jpg |align=center |{{val|204.5|84}} |align=center | |Aten asteroid type S |
{{mpl|2013 YP|139}}
|bgcolor=black|File:PIA18412-Asteroid2014HQ124-20140608.jpg |align=center |{{val|201|13}} |align=center | |
{{mpl-|341843|2008 EV|5}} {{small|341843}} |bgcolor=black|File:Asteroid-2008EV5-ShapeModel-20111006.gif |align=center |{{val|200|7}} |align=center | |
{{mpl-|388188|2006 DP|14}} {{small|388188}} | style="background:#333;"|File:Asteroid2006DP14.jpg |align=center |{{val|200|p=≈ }} |align=center | |Apollo asteroid type S; contact binary |align=center |{{cite web |title = Radar Images of near-Earth Asteroid 2006 DP14 |url = https://www.jpl.nasa.gov/news/news.php?release=2014-060 |publisher = Jet Propulsion Laboratory |date = 25 February 2014 |access-date = 9 June 2019}} |
{{mpl-|6037|1988 EG}} {{small|6037}} |bgcolor=black| |align=center |{{val|199.5|1.35}} |align=center | |Apollo asteroid type S |align=center |{{cite journal |display-authors = 6 |first1 = D. E. |last1 = Trilling |first2 = M. |last2 = Mueller |first3 = J. L. |last3 = Hora |first4 = G. |last4 = Fazio |first5 = T. |last5 = Spahr |first6 = J. A. |last6 = Stansberry |first7 = H. A. |last7 = Smith |first8 = S. R. |last8 = Chesley |first9 = A. K. |last9 = Mainzer |date = August 2008 |title = Diameters and Albedos of Three Subkilometer Near-Earth Objects Derived from Spitzer Observations |journal = The Astrophysical Journal Letters |volume = 683 |issue = 2 |pages = L199–L202 |bibcode = 2008ApJ...683L.199T |doi = 10.1086/591668 |arxiv = 0807.1717 |s2cid = 14319204 }} |
{{mpl|2010 TK|7}}
|bgcolor=black|File:PIA14405-full crop.jpg |align=center |{{val|189.5|61.5}} |align=center | |Aten asteroid; Earth trojan ({{L4}}) |align=center |{{cite web |type=2017-10-30 last obs |title=JPL Small-Body Database Browser: (2010 TK7) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3548081 |access-date=8 June 2019}} |
{{mpl-|292220|2006 SU|49}} {{small|292220}} |bgcolor=black| |align=center |{{val|188.5|p=≈ }} |align=center |{{val|73|p=≈ }} |Apollo asteroid |align=center |{{cite web |title = 2006 SU49 Impact Risk |publisher = NASA/JPL Near-Earth Object Program Office |url = http://neo.jpl.nasa.gov/risk/2006su49.html |archive-url = https://web.archive.org/web/20060928234147/http://neo.jpl.nasa.gov/risk/2006su49.html |
{{mpl-|308635|2005 YU|55}} {{small|308635}} |bgcolor=black|File:2005YU55-20111107.jpg |align=center |{{val|180|20}} |align=center | |Apollo asteroid type C |align=center |{{cite web |date=31 March 2012 |title=Shape and Spin of Near-Earth Asteroid 308635 (2005 YU55) From Radar Images and Speckle Tracking |publisher=Lunar and Planetary Institute |author=M.W. Busch |display-authors=etal |url=http://www.lpi.usra.edu/meetings/acm2012/pdf/6179.pdf |access-date=9 April 2012}} |
{{mpl-|419624|2010 SO|16}}
|bgcolor=black| |align=center |{{val|178.5|63}} |align=center | |Apollo asteroid; co-orbital with Earth |align=center |{{cite journal |display-authors = 6 |first1 = C. R. |last1 = Nugent |first2 = A. |last2 = Mainzer |first3 = J. |last3 = Masiero |first4 = J. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = T. |last6 = Grav |first7 = E. |last7 = Kramer |first8 = S. |last8 = Sonnett |first9 = R. |last9 = Stevenson |first10 = E. L. |last10 = Wright |date = December 2015 |title = NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos |journal = The Astrophysical Journal |volume = 814 |issue = 2 |page = 13 |bibcode = 2015ApJ...814..117N |doi = 10.1088/0004-637X/814/2/117 |arxiv = 1509.02522 |s2cid = 9341381 }} |
Itokawa {{small|25143}} |bgcolor=black| File:Itokawa06 hayabusa.jpg |align=center |{{val|173}} |align=center |{{val|35.1|1.05}} |Apollo asteroid type S |align=center |{{cite journal |first1 = A. |last1 = Fujiwara |first2 = J. |last2 = Kawaguchi |first3 = D. K. |last3 = Yeomans |first4 = M. |last4 = Abe |first5 = T. |last5 = Mukai |first6 = T. |last6 = Okada |date = June 2006 |title = The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa |url = https://www.researchgate.net/publication/7042075 |journal = Science |volume = 312 |issue = 5778 |pages = 1330–1334 |bibcode = 2006Sci...312.1330F |doi = 10.1126/science.1125841 |pmid = 16741107 |s2cid = 206508294 |
Apophis {{small|99942}} |bgcolor=black|File:99942 Apophis shape.png |align=center |{{val|162.5|7.5}} |align=center |{{val|61|p=≈ }} |align=center |{{cite web |type=2015-01-03 last obs |title=JPL Small-Body Database Browser: 99942 Apophis (2004 MN4) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=99942 |access-date=8 June 2019}}{{·}}{{cite web |title = Earth Impact Risk Summary: 99942 |publisher = NASA/JPL Near-Earth Object Program Office |url = https://cneos.jpl.nasa.gov/sentry/details.html#?des=99942 |archive-url = https://web.archive.org/web/20190305035418/https://cneos.jpl.nasa.gov/sentry/details.html#?des=99942 |archive-date = 5 March 2019 |url-status = live |access-date = 14 June 2019 |df = dmy-all}} |
S/2009 S 1
| style="background:#868686;"|File:PIA11665 moonlet in B Ring cropped.jpg |align=center |{{val|150|p=≈ }} |align=center | |align=center |{{cite web | title = A Small Find Near Equinox | date = 7 August 2009 | work = Cassini Solstice Mission | publisher = Jet Propulsion Laboratory | url = http://saturn.jpl.nasa.gov/photos/imagedetails/index.cfm?imageId=3617 | access-date = 8 June 2019 | archive-url = https://web.archive.org/web/20091010124459/http://saturn.jpl.nasa.gov/photos/imagedetails/index.cfm?imageId=3617 | archive-date = 10 October 2009 }} |
{{mpl|277475|2005 WK|4}}
|bgcolor=black|File:Pia17406-full.jpg |align=center |{{val|142}} |align=center | |align=center |{{cite web |title = LCDB Data for (277475) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=277475%7C |access-date = 11 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040734/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=277475%7C }} |
{{mpl-|357439|2004 BL|86}} {{small|357439}} |bgcolor=black|File:Radar images of 2004 BL86 and its moon 2.gif |align=center |{{val|131.5|13}} |align=center | |Apollo asteroid type V; binary |align=center |{{cite journal |first1 = Vishnu |last1 = Reddy |first2 = Bruce L. |last2 = Gary |first3 = Juan A. |last3 = Sanchez |first4 = Driss |last4 = Takir |first5 = Cristina A. |last5 = Thomas |first6 = Paul S. |last6 = Hardersen |date = September 2015 |title = The Physical Characterization of the Potentially Hazardous Asteroid 2004 BL86: A Fragment of a Differentiated Asteroid |journal = The Astrophysical Journal |volume = 811 |issue = 1 |page = 10 |bibcode = 2015ApJ...811...65R |doi = 10.1088/0004-637X/811/1/65 |arxiv = 1509.07122|s2cid = 119260041 }} |
{{mpl|2007 TU|24}}
|bgcolor=black|File:2007 TU24 radar image 20080128.jpg |align=center |{{val|125}} |align=center | |Apollo asteroid type S |align=center |{{cite web |title=NASA Scientists Get First Images of Earth Flyby Asteroid |publisher=Jet Propulsion Laboratory |date=25 January 2008 |url=http://www.jpl.nasa.gov/news/news.cfm?release=2008-014 |access-date=6 March 2009 |archive-date=29 January 2008 |archive-url=https://web.archive.org/web/20080129062350/http://www.jpl.nasa.gov/news/news.cfm?release=2008-014 }} |
Zoozve {{small|524522}} |bgcolor=black| |align=center |{{val|118|p=≈ }} |align=center | |Aten asteroid type X; co-orbital with Venus |align=center |{{cite web |title = LCDB Data for 2002 VE68 |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0%7C2002+VE68 |access-date = 12 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040735/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0%7C2002+VE68 }} |
{{mpl-|436724|2011 UW|158}} {{small|436724}} | style="background:#181818;"|File:2011UW158.jul14.p05us.p27Hz(1).gif |align=center |{{val|110|20}} |align=center | |Apollo asteroid type S |align=center |{{cite journal |first = Gary |last = Bruce L. |date = January 2016 |title = Unusual Properties for the NEA (436724) 2011 UW158 |journal = The Minor Planet Bulletin |volume = 43 |issue = 1 |pages = 33–38 |issn = 1052-8091 |bibcode = 2016MPBu...43...33G }} |
Dimorphos {{small|Didymos I}} |bgcolor=black| |align=center |{{val|85|15}} |align=center | |asteroid moon of 65803 Didymos |
{{mpl|2017 BQ|6}}
| style="background:#181818;"|File:2017 BQ6 radar rotation.gif |align=center |{{val|78}} |align=center | |align=center |{{cite web |title = LCDB Data for 2017 BQ6 |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0%7C2017+BQ6 |access-date = 9 June 2019 |archive-date = 10 July 2021 |archive-url = https://web.archive.org/web/20210710040733/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0%7C2017+BQ6 }} |
YORP {{small|54509}} |bgcolor=black|File:54509 YORP image radar and 3D model.gif |align=center |{{val|61.8}} |align=center | |align=center |{{cite journal |title = Spin Rate of Asteroid (54509) 2000 PH5 Increasing Due to the YORP Effect |display-authors = etal |last = Taylor |first = Patrick A. |date = 13 April 2007 |journal = Science |volume = 316 |issue = 5822 |pages = 274–277 |doi = 10.1126/science.1139038 |url = http://www.astro.cornell.edu/~jlm/publications/Taylor07.science316.yorp.pdf |pmid = 17347415 |bibcode = 2007Sci...316..274T|s2cid = 29191700 }} |
Kamoʻoalewa {{small|469219}} |bgcolor=black| |align=center |{{val|41}} |align=center | |Apollo asteroid type S; quasi-satellite of Earth |align=center |{{cite web |title = LCDB Data for (469219) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=469219%7C |access-date = 8 June 2019 |archive-date = 13 June 2020 |archive-url = https://web.archive.org/web/20200613003629/http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=469219%7C }} |
Duende {{small|367943}} |bgcolor=black|File:Radar-2012DA14-Goldstone.jpg |align=center |{{val|23.75}} |align=center | |align=center |{{cite web |date=13 January 2013 |title={{mp|2012 DA|14}} Goldstone Radar Observations Planning |publisher=NASA/JPL Asteroid Radar Research |author=Dr. Lance A. M. Benner |url=http://echo.jpl.nasa.gov/asteroids/2012DA14/2012DA14_planning.html |access-date=15 January 2013}} |
{{mpl|1998 KY|26}}
|bgcolor=black|File:Asteroid 1998 KY26.faces model.jpg |align=center |{{val|15|p=≈ }} |align=center | |align=center |{{cite journal |first1 = Steven J. |last1 = Ostro |first2 = Petr |last2 = Pravec |first3 = Lance A. M. |last3 = Benner |first4 = R. Scott |last4 = Hudson |first5 = Lenka |last5 = Sarounová |first6 = Michael D. |last6 = Hicks |date = June 1999 |title = Radar and Optical Observations of Asteroid 1998 KY26 |journal = Science |volume = 285 |issue = 5427 |pages = 557–559 (SciHomepage) |bibcode = 1999Sci...285..557O |doi = 10.1126/science.285.5427.557 |pmid = 10417379|s2cid = 5728247 }} |
{{mpl|2012 TC|4}}
|bgcolor=black|File:2012 TC4 radar animation before closest approach.gif |align=center |{{val|11.5}} |align=center | |Apollo asteroid type E/type Xe |align=center |{{cite web |title =The 2012 TC4 Observing Campaign – Radar observations UPDATE October 12, 2017 |publisher = University of Maryland |url = http://2012tc4.astro.umd.edu/References/TC4RadarUpdate.txt |access-date = 10 June 2019}} |
2014 RC
|bgcolor=black| |align=center |{{val|11|p=≈ }} |align=center | |align=center |{{cite web |title=Reports of Meteorite Strike in Nicaragua and Update on Asteroid 2014 RC |publisher=NASA/JPL Near-Earth Object Program Office |url=http://neo.jpl.nasa.gov/news/news185.html |access-date=10 June 2019 |archive-url=https://web.archive.org/web/20141011215227/http://neo.jpl.nasa.gov/news/news185.html |archive-date=11 October 2014}} |
{{mpl|2010 RF|12}}
|bgcolor=black| |align=center |{{val|3.5|p=≈ }} |align=center |{{val|0.0005|p=≈ }} |Apollo asteroid |align=center |{{cite web |title = Earth Impact Risk Summary: 2010 RF12 |publisher = NASA/JPL Near-Earth Object Program Office |url = https://cneos.jpl.nasa.gov/sentry/details.html#?des=2010%20RF12 |archive-url = https://web.archive.org/web/20170122151206/http://neo.jpl.nasa.gov/risk/2010rf12.html#?des=2010%20RF12 |archive-date = 22 January 2017 |url-status = live |access-date = 12 June 2019 |df = dmy-all}} |
2011 MD
| style="background:#300409;"|File:PIA18453-Asteroid2011MD-SpitzerSpaceTelescope-IRAC-Feb2014.jpg |align=center |{{val|3|2|1}} |align=center | |Apollo asteroid/Amor asteroid type S |align=center |{{cite journal |title=Physical properties of near-earth asteroid 2011 MD |last=Mommert |first=M. |display-authors=etal |date=19 June 2014 |journal=The Astrophysical Journal Letters |volume=789 |issue=1 |page=L22 |arxiv=1406.5253 |bibcode=2014ApJ...789L..22M |doi=10.1088/2041-8205/789/1/L22|s2cid=67851874 }} |
{{mpl|2008 TC|3}}
|bgcolor=black|File:2008 TC3 Tumbling (reduced).gif |align=center |{{val|2.05}} |align=center |{{val|0.00008|fmt=none}} |Apollo asteroid type F/type M |align=center |{{cite journal |last=Jenniskens |first=P. |date=2009 |volume=458 |issue=7237 |pages=485–488 |title=The impact and recovery of asteroid 2008 TC3 |journal=Nature |bibcode=2009Natur.458..485J |doi=10.1038/nature07920 |pmid=19325630 |s2cid=7976525 |
2023 BU
|bgcolor=black| |align=center |{{val|1.5|p=}} | |
{{mpl|2008 TS|26}}
|bgcolor=black| |align=center |{{val|0.49|p=≈ }} |align=center | |align=center |{{cite web |title = Asteroid 2008 TS26 |publisher = Asteroids Near Earth |url = https://www.asteroidsnear.com/asteroid-2008-ts26-1490 |access-date = 22 June 2019 |archive-date = 22 June 2019 |archive-url = https://web.archive.org/web/20190622130639/https://www.asteroidsnear.com/asteroid-2008-ts26-1490 }} |
2015 FF415
|bgcolor=black| |align=center |{{val|0.25|p=≈ }} |align=center | |align=center |{{Cite web |date=2025-01-01 |title=Small-Body Database Query |url=https://ssd.jpl.nasa.gov/tools/sbdb_query.html |access-date=2025-04-16 |archive-url=https://web.archive.org/web/20250101171802/https://ssd.jpl.nasa.gov/tools/sbdb_query.html |archive-date=1 January 2025 }}{{Cite web |date=2025-01-01 |title=Asteroid Size Estimator |url=https://cneos.jpl.nasa.gov/tools/ast_size_est.html |access-date=2025-04-16 |archive-url=https://web.archive.org/web/20250101175034/https://cneos.jpl.nasa.gov/tools/ast_size_est.html |archive-date=1 January 2025 }} |
Gallery
See also
Notes
{{notelist}}
{{reflist|group=note}}
References
{{reflist|refs=
}}
Further reading
- [http://www.psi.edu/pds/ NASA Planetary Data System (PDS)]
- [http://www.johnstonsarchive.net/astro/asteroidmoons.html Asteroids with Satellites]
- [http://www.cfa.harvard.edu/iau/lists/NumberedMPs.txt Minor Planet discovery circumstances]
- Supplemental IRAS Minor Planet Survey (SIMPS) and IRAS Minor Planet Survey (IMPS)
- [https://web.archive.org/web/20090817051318/http://www.psi.edu/pds/resource/imps.html SIMPS & IMPS] ([http://www.psi.edu/pds/asteroid/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab V6], [http://www.psi.edu/pds/asteroid/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/addl.tab additional], [http://www.psi.edu/pds/asteroid/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/ from here])
- [https://archive.today/20060623213811/http://www.psi.edu/pds/archive/astdata04/simps04/diamalb.tab Asteroid Data Archive ] [https://web.archive.org/web/20041226203709/http://www.psi.edu/pds/archive/astdata04/simps04/diamalb.tab Archive] Planetary Science Institute
External links
- [http://nssdc.gsfc.nasa.gov/planetary/planetfact.html Planetary fact sheets]
- [http://nssdc.gsfc.nasa.gov/planetary/factsheet/asteroidfact.html Asteroid fact sheet]
{{Solar System}}
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{{DEFAULTSORT:List Of Solar System Objects By Size}}