4754 Panthoos
{{Use dmy dates|date=June 2018}}
{{Infobox planet
| minorplanet = yes
| name = 4754 Panthoos
| background = #C2FFFF
| image =
| image_size =
| caption =
| discoverer = C. J. van Houten
I. van Houten-G.
T. Gehrels
| discovery_site = Palomar Obs.
| discovered = 16 October 1977
| mpc_name = (4754) Panthoos
| alt_names = 5010 T-3{{·}}{{mp|1988 RH|1}}
| adjective = Panthoian
| pronounced = {{IPAc-en|ˈ|p|æ|n|θ|oʊ|ə|s}}]
| named_after = Panthous
{{small|(Greek mythology)}}
| mp_category = Jupiter trojan
{{nowrap|Trojan {{·}}background }}
| epoch = 23 March 2018 (JD 2458200.5)
| uncertainty = 0
| observation_arc = 40.62 yr (14,836 d)
| aphelion = 5.2904 AU
| perihelion = 5.2050 AU
| semimajor = 5.2477 AU
| eccentricity = 0.0081
| period = 12.02 yr (4,391 d)
| mean_anomaly = 187.03°
| mean_motion = {{Deg2DMS|0.0820|sup=ms}} / day
| inclination = 12.318°
| asc_node = 155.06°
| arg_peri = 200.56°
| jupiter_moid = 0.1223 AU
| tisserand = 2.9540
| mean_diameter = {{val|53.02|1.14|ul=km}}
{{val|53.15|4.2|u=km}}
{{val|56.96|2.84|u=km}}
| rotation = {{val|27.68|0.05|ul=h}}
| albedo = {{val|0.051|0.005}}
{{val|0.0571|0.010}}
{{val|0.063|0.011}}
| spectral_type = C {{small|(assumed)}}
}}
4754 Panthoos {{IPAc-en|ˈ|p|æ|n|θ|oʊ|ə|s}} is a Jupiter trojan from the Trojan camp, approximately {{convert|53|km|mi|abbr=off|sigfig=2|sp=us}} in diameter. It was discovered during the third Palomar–Leiden Trojan survey on 16 October 1977, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at the Palomar Observatory in California. It is likely spherical in shape and has a longer-than-average rotation period of 27.68 hours. The assumed C-type asteroid is one of the 80 largest Jupiter trojans. It was named after Panthous (Panthoos) from Greek mythology.
Orbit and classification
Panthoos is a dark Jovian asteroid orbiting in the trailering Trojan camp at Jupiter's {{L5}} Lagrangian point, 60° behind the Gas Giant's orbit in a 1:1 resonance (see Trojans in astronomy). It is also a non-family asteroid of the Jovian background population.
It orbits the Sun at a distance of 5.2–5.3 AU once every 12 years (4,391 days; semi-major axis of 5.25 AU). Its orbit has an eccentricity of 0.01 and an inclination of 12° with respect to the ecliptic. The body's observation arc begins at Palomar on 11 October 1977, just five nights prior to its official discovery observation.
Palomar–Leiden Trojan survey
The survey designation "T-3" stands for the third Palomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar and Leiden Observatory in the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroid discoveries.
Physical characteristics
Panthoos is an assumed C-type asteroid.
= Rotation period =
In February 1994, a rotational lightcurve of Panthoos was obtained from photometric observations over seven consecutive nights by Stefano Mottola and Anders Erikson using the former ESO 1-metre telescope at La Silla Observatory in northern Chile. Lightcurve analysis gave a rotation period of {{val|27.68|0.05}} hours with a brightness variation of 0.09 magnitude ({{small|U=2+}}). While not being a slow rotator, its period is significantly longer than that of most larger Jupiter trojans (see table below). Moreover, the low brightness amplitude measured by Mottola is indicative of a spherical rather than elongated shape.
= Diameter and albedo =
According to the surveys carried out by the Japanese Akari satellite, the Infrared Astronomical Satellite IRAS, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Panthoos measures between 53.02 and 56.96 kilometers in diameter and its surface has an albedo between 0.051 and 0.063. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0624 and a diameter of 53.21 kilometers based on an absolute magnitude of 10.0.
{{Largest Jupiter trojans}}
Naming
This minor planet was named from Greek mythology after Panthous (Panthoos), a priest and member of the Trojan senate who warned of the imminent destruction of Troy. The official naming citation was published by the Minor Planet Center on 28 May 1991 ({{small|M.P.C. 18308}}).
References
{{reflist|30em|refs=
|type = 2018-05-25 last obs.
|title = JPL Small-Body Database Browser: 4754 Panthoos (5010 T-3)
|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004754
|publisher = Jet Propulsion Laboratory
|access-date = 16 June 2018}}
|title = 4754 Panthoos (5010 T-3)
|work = Minor Planet Center
|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=4754
|access-date = 16 June 2018}}
|title = List of Jupiter Trojans
|work = Minor Planet Center
|first3 = V. |last3 = Carruba
|date = 1 June 2018
|url = https://www.minorplanetcenter.net/iau/lists/JupiterTrojans.html
|access-date = 16 June 2018}}
|title = Minor Planet Discoverers (by number)
|work = Minor Planet Center
|url = https://www.minorplanetcenter.net/iau/lists/MPDiscsNum.html
|date = 31 May 2018
|access-date = 16 June 2018}}
|title = MPC/MPO/MPS Archive
|work = Minor Planet Center
|url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
|access-date = 16 June 2018}}
|first1 = T. |last1 = Grav
|first2 = A. K. |last2 = Mainzer
|first3 = J. M. |last3 = Bauer
|first4 = J. R. |last4 = Masiero
|first5 = C. R. |last5 = Nugent
|date = November 2012
|title = WISE/NEOWISE Observations of the Jovian Trojan Population: Taxonomy
|journal = The Astrophysical Journal
|volume = 759
|issue = 1
|page = 10
|bibcode = 2012ApJ...759...49G
|doi = 10.1088/0004-637X/759/1/49
|arxiv = 1209.1549
|s2cid = 119101711
}} ([http://vizier.cfa.harvard.edu/viz-bin/VizieR-6?-source=J/ApJ/759/49/table1&MPC=04754 online catalog])
|title = Asteroid (4754) Panthoos – Proper Elements
|publisher = AstDyS-2, Asteroids – Dynamic Site
|url = https://newton.spacedys.com/astdys/index.php?n=4754&pc=1.1.6
|access-date= 16 June 2018}}
|first1 = E. F. |last1 = Tedesco
|first2 = P. V. |last2 = Noah
|first3 = M. |last3 = Noah
|first4 = S. D. |last4 = Price
|date = October 2004
|title = IRAS Minor Planet Survey V6.0
|url = https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab
|journal = NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0
|volume = 12
|pages = IRAS-A-FPA-3-RDR-IMPS-V6.0
|bibcode = 2004PDSS...12.....T
|access-date = 16 June 2018}}
|title = LCDB Data for (4754) Panthoos
|publisher = Asteroid Lightcurve Database (LCDB)
|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=4754%7CPanthoos
|access-date = 16 June 2018}}
|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=
}} ([http://vizier.cfa.harvard.edu/viz-bin/VizieR-5?-source=J/PASJ/63/1117/acua_v1&Num=4754 online], [https://core.ac.uk/download/pdf/43545172.pdf AcuA catalog p. 153])
|display-authors = 6
|first1 = Stefano |last1 = Mottola
|first2 = Mario |last2 = Di Martino
|first3 = Anders |last3 = Erikson
|first4 = Maria |last4 = Gonano-Beurer
|first5 = Albino |last5 = Carbognani
|first6 = Uri |last6 = Carsenty
|first7 = Gerhard |last7 = Hahn
|first8 = Hans-Josef |last8 = Schober
|first9 = Felix |last9 = Lahulla
|first10 = Marco |last10 = Delbò
|first11 = Claes-Ingvar |last11 = Lagerkvist
|date = May 2011
|title = Rotational Properties of Jupiter Trojans. I. Light Curves of 80 Objects
|journal = The Astronomical Journal
|volume = 141
|issue = 5
|page = 32
|bibcode = 2011AJ....141..170M
|doi = 10.1088/0004-6256/141/5/170
|doi-access= free
}}
}}
External links
- [http://www.minorplanet.info/PHP/lcdbsummaryquery.php Asteroid Lightcurve Database (LCDB)], query form ([http://www.minorplanet.info/lightcurvedatabase.html info] {{Webarchive|url=https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html |date=16 December 2017 }})
- [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
- [https://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html Discovery Circumstances: Numbered Minor Planets (1)-(5000)] – Minor Planet Center
- [https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=4754+Panthoos Asteroid 4754 Panthoos] at the Small Bodies Data Ferret
- {{AstDys|4754}}
- {{JPL small body}}
{{Minor planets navigator |4753 Phidias |number=4754 |4755 Nicky}}
{{Small Solar System bodies}}
{{Authority control}}
{{DEFAULTSORT:Panthoos}}
Category:Discoveries by Cornelis Johannes van Houten
Category:Discoveries by Ingrid van Houten-Groeneveld