Kepler-1708b#Potential exomoon
{{short description|Gas giant exoplanet with a potential exomoon}}
{{Infobox planet
| extrasolarplanet = yes
| name = Kepler-1708b
| image =
| image_size =
| image_alt =
| caption =
| discoverer =
| discovery_site =
| discovered = 2019 (candidate)
2021 (confirmed)
| discovery_method = Transit
| alt_names = KIC 7906827.01
| semimajor = {{val|1.64|0.10|ul=AU}}
| eccentricity = <{{val|0.40}}
| period = {{val|737.1131|0.00146|0.00770|ul=d}}
| inclination = {{val|89.92|0.03|0.01|ul=deg}}
| arg_peri =
| satellites = Kepler-1708b I?
| star = Kepler-1708
| mean_radius = {{val|0.8886|0.0535|0.0526|ul=Jupiter radius}})
| mass = <{{val|4.6|ul=Jupiter mass}}
| density =
| surface_grav =
| single_temperature =
}}
Kepler-1708b (previously known as KIC 7906827.01) is a Jupiter-sized exoplanet orbiting the Sun-like star Kepler-1708, located in the constellation of Cygnus approximately 5,600 light years away from Earth. It was first detected in 2011 by NASA's Kepler mission using the transit method, but was not identified as a candidate planet until 2019. In 2021, a candidate Neptune-sized exomoon in orbit around Kepler-1708b was found by astronomer David Kipping and colleagues in an analysis using Kepler transit data. However, subsequent research has raised discrepancies about the possible existence of an exomoon, similar to that of Kepler-1625b, but even more recent research still find the existence of an exomoon likely.
Characteristics
= Mass and radius =
Kepler-1708b is a gas giant planet slightly smaller than Jupiter in size, with a radius of 0.89 Jupiter radii. The mass of the planet remains yet to be measured; precise analysis of its transit timings place a 2-sigma upper limit of <4.6 Jupiter masses. This mass upper limit predicts a maximum radial velocity amplitude of <{{val|98|u=m/s}}—although within reach of the most precise spectrographs available, the faintness of Kepler-1708b's host star would make observations difficult.
= Orbit and temperature =
Kepler-1708b orbits about 1.64 astronomical units from its host star and completes one revolution every {{convert|737.11|d|yr|sigfig=3|disp=or}}, comparable to the orbit of Mars in the Solar System. At this distance, Kepler-1708b lies within the habitable zone of its host star, where it receives an insolation flux {{val|0.561|0.074|0.068}} times that of Earth at a relatively cool equilibrium temperature of {{convert|200–300|K|C F|abbr=out|lk=in}}. The eccentricity of its orbit is unmeasured and is given a 2-sigma upper limit of <0.40.
Host star
Kepler-1708b orbits around the Sun-like star Kepler-1708, located in the constellation of Cygnus {{cvt|1712 ± 75|pc|ly|order=flip}} light years away from Earth. At an apparent magnitude of 16, this star is too faint to be seen by the naked eye. The star's celestial coordinates based on the J2000 epoch are: RA {{RA|19|47|17.79}}, Dec {{DEC|43|37|29.4}}. The European Space Agency's Gaia satellite has measured a stellar parallax of {{val|0.5730|0.0340}} milliarcseconds (mas) and directional proper motion components of RA {{val|-0.770|0.057|u=mas/yr}}, Dec {{val|-5.005|0.059|u=mas/yr}}. Kepler-1708 is known by other designations from various star catalogues including: UCAC4 669-077544, KIC 7906827, TIC 272716898, 2MASS J19471778+4337295, WISE J194717.78+433729.2, and Gaia DR2 2078801971283008128.
Kepler-1708 is slightly larger and more massive than the Sun, with a mass of {{val|1.088|0.072|u=Solar mass}} and radius of {{val|1.117|0.064|u=Solar radius}}. It is also hotter and more luminous than the Sun, with an effective temperature of {{val|6157|231|202|ul=K|fmt=commas}} and a bolometric luminosity of {{val|1.521|ul=Solar luminosity}}.{{efn|Luminosity calculated from the inverse of from Kipping et al. (2022)}} Based on these properties, Kepler-1708 is likely an F-type main sequence star with a Sun-like metallicity of [Fe/H] = {{val|0.0|0.2|ul=Metallicity#Chemical_abundance_ratios{{!}}dex}} and an age of {{val|3.16|2.26}} billion years.{{efn|Age calculated from the inverse of from Kipping et al. (2022)}}
Potential exomoon
File:Kepler-1708b in Celestia.png.]]
In 2021, David Kipping and colleagues performed a search for exomoons around cool, long-period gas giant exoplanets using Kepler photometric data. Out of a sample of 70 exoplanets analyzed, only Kepler-1708b exhibited signs of an orbiting exomoon manifesting as faint, secondary transits accompanying the planet's transits.{{Cite news |title=Scientists think they've found a big, weird moon in a far-off star system |language=en |work=NPR.org |url=https://www.npr.org/2022/01/13/1072570125/kepler-large-exomoon |access-date=2022-03-28}} This possible exomoon, designated Kepler-1708b I, appears to measure below the size of Neptune at 2.6 times Earth's radius. It likely orbits coplanar to its host planet from a distance up to 12 planetary radii—comparable to the distance between Jupiter and its moon Europa, or twice the Earth–Moon distance. The extraordinarily large size of Kepler-1708b I is reminiscent of Kepler-1625b I, another Neptune-sized exomoon candidate previously reported by Kipping et al. in 2017.
Additional observations are necessary to confirm or refute the exomoon's existence—only two transits by Kepler-1708b and its possible exomoon have been observed, and no transit timing variations can be determined as of yet. Kipping et al. determine that the probability of detecting one false positive exomoon in the studied sample of 70 exoplanets was <50%. A follow-up study suggested Kepler-1708b I is likely undetectable with the Hubble Space Telescope, but the James Webb Space Telescope should be able to confirm or refute its existence.{{cite journal |last1=Cassese |first1=Ben |last2=Kipping |first2=David |date=2022-03-24 |title=Kepler-1708 b-i is likely undetectable with HST |journal=Monthly Notices of the Royal Astronomical Society |volume=516 |issue=3 |pages=3701–3708 |doi=10.1093/mnras/stac2090 |doi-access=free |arxiv=2203.13290 }}
In 2024, a paper was published disputing both 1625b I and 1708b I’s existences,{{cite journal | url=https://ui.adsabs.harvard.edu/abs/2024NatAs...8..193H/abstract | bibcode=2024NatAs...8..193H | title=Large exomoons unlikely around Kepler-1625 b and Kepler-1708 B | last1=Heller | first1=René | last2=Hippke | first2=Michael | journal=Nature Astronomy | date=2024 | volume=8 | issue=2 | page=193 | doi=10.1038/s41550-023-02148-w | arxiv=2312.03786 }} but a reply to this paper refute most claims given, and conclude that the existence of an exomoon is likely but need additional observations.{{cite arXiv |eprint=2401.10333 |last1=Kipping |first1=David |last2=Teachey |first2=Alex |last3=Yahalomi |first3=Daniel A. |last4=Cassese |first4=Ben |last5=Quarles |first5=Billy |last6=Bryson |first6=Steve |last7=Hansen |first7=Brad |last8=Szulágyi |first8=Judit |last9=Burke |first9=Chris |last10=Hardegree-Ullman |first10=Kevin |title=A Reply to: Large Exomoons unlikely around Kepler-1625 b and Kepler-1708 B |date=2024 |class=astro-ph.EP }}
See also
Notes
{{notelist}}
References
{{reflist|refs=
|title = UCAC4 669-077544 -- Star
|url = https://simbad.u-strasbg.fr/simbad/sim-basic?Ident=KIC+7906827&submit=SIMBAD+search
|work = SIMBAD
|publisher = Centre de données astronomiques de Strasbourg
|accessdate = 16 January 2022}}
|title = Kepler-1708 Overview
|url = https://exoplanetarchive.ipac.caltech.edu/overview/Kepler-1708
|work = NASA Exoplanet Archive
|publisher = Infrared Processing and Analysis Center
|accessdate = 16 January 2022}}
|title = Kepler-1708 b
|url = https://exoplanets.nasa.gov/exoplanet-catalog/8358/kepler-1708-b/
|work = NASA Exoplanet Exploration
|date = 13 January 2022
|publisher = NASA
|accessdate = 16 January 2022}}
|title = Habitable Zone Gallery
|url = http://www.hzgallery.org/table.html
|first1 = Stephen |last1 = Kane
|first2 = Dawn |last2 = Gelino
|accessdate = 16 January 2022}}
|title = Astronomers Have Found Another Possible 'Exomoon' beyond Our Solar System
|url = https://www.scientificamerican.com/article/astronomers-have-found-another-possible-exomoon-beyond-our-solar-system/
|first = Jonathan |last = O'Callaghan
|work = Scientific American
|date = 13 January 2022
|accessdate = 16 January 2022}}
|title = Needle in the Haystack: New Exomoon Candidate Found
|url = https://skyandtelescope.org/astronomy-news/needle-in-the-haystack-new-exomoon-candidate-found/
|first = Ben |last = Skuse
|work = Sky & Telescope
|date = 14 January 2022
|accessdate = 16 January 2022}}
|first1 = Miranda K. |last1 = Herman
|first2 = Wei |last2 = Zhu
|first3 = Yanqin |last3 = Wu | author3-link = Yanqin Wu
|title = Revisiting the Long-period Transiting Planets from Kepler
|journal = The Astronomical Journal
|date = June 2019
|volume = 157
|issue = 6
|id = 248
|pages = 15
|doi-access = free
|doi = 10.3847/1538-3881/ab1f70
|arxiv = 1901.01974
|bibcode = 2019AJ....157..248H
|s2cid = 119550672}}
|first1 = Hajime |last1 = Kawahara
|first2 = Kento |last2 = Masuda
|title = Transiting Planets Near the Snow Line from Kepler. I. Catalog
|journal = The Astronomical Journal
|date = June 2019
|volume = 157
|issue = 6
|id = 218
|pages = 27
|doi-access = free
|doi = 10.3847/1538-3881/ab18ab
|arxiv = 1904.04980
|bibcode = 2019AJ....157..218K
|s2cid = 119099510}}
|first1 = Anina |last1 = Timmermann
|first2 = René |last2 = Heller
|first3 = Ansgar |last3 = Reiners
|first4 = Mathias |last4 = Zechmeister
|title = Radial velocity constraints on the long-period transiting planet Kepler-1625 b with CARMENES
|url = https://www.aanda.org/articles/aa/pdf/2020/03/aa37325-19.pdf
|journal = Astronomy & Astrophysics
|date = March 2020
|volume = 635
|id = A59
|page = 2
|doi-access = free
|doi = 10.1051/0004-6361/201937325
|arxiv = 2001.10867
|bibcode = 2020A&A...635A..59T
|s2cid = 210942758}}
|first1 = David |last1 = Kipping
|first2 = Steve |last2 = Bryson
|first3 = Chris |last3 = Burke
|first4 = Jessie |last4 = Christiansen
|first5 = Kevin |last5 = Hardegree-Ullman
|first6 = Billy |last6 = Quarles
|first7 = Brad |last7 = Hansen
|first8 = Judit |last8 = Szulágyi
|first9 = Alex |last9 = Teachey
|title = An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i
|url = https://www.nature.com/articles/s41550-021-01539-1.pdf
|journal = Nature Astronomy
|date = January 2022
|volume = 6
|issue = 3
|pages = 367–380
|doi-access = free
|doi = 10.1038/s41550-021-01539-1
|pmid = 35399159
|pmc = 8938273
|arxiv = 2201.04643
|bibcode = 2022NatAs...6..367K
|s2cid = 245906142}}
}}
External links
- [https://news.columbia.edu/news/astronomers-find-evidence-second-exomoon Astronomers Find Evidence for a Second Supermoon Beyond Our Solar System], Kim Martineau, Columbia News, Columbia University, 13 January 2022
- [https://exoplanetarchive.ipac.caltech.edu/cgi-bin/ICETimeSeriesViewer/nph-ICEtimeseriesviewer?idtype=source&inventory_mode=id_single&id=7906827&dataset=KeplerDV KIC 7906827 – Kepler Time Series Visualizer] NASA Exoplanet Archive, Infrared Processing and Analysis Center
- [https://exoplanet.eu/catalog/kepler_1708_b--8058/ Planet Kepler-1708 b], The Extrasolar Planets Encyclopaedia, last updated 14 January 2022
{{cygnus (constellation)}}
{{2022 in space}}
Category:Exoplanets discovered in 2022
Category:Exoplanets discovered by the Kepler space telescope