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Kepler-1708b

(Redirected from Draft:Kepler-1708b I)

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.[1] 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.[2][3] 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.[1][4] However, subsequent research has raised discrepancies about the possible existence of an exomoon, similar to that of Kepler-1625b.[5]

Kepler-1708b
Discovery[1]
Discovery date2019 (candidate)[2][3]
2021 (confirmed)[1][4]
Transit
Designations
KIC 7906827.01
Orbital characteristics[1]
1.64±0.10 AU
Eccentricity<0.40
737.1131+0.00146
−0.00770 d
Inclination89.92°+0.03°
−0.01°
StarKepler-1708
Physical characteristics[1]
0.8886+0.0535
−0.0526 RJ)[4]
Mass<4.6 MJ

Characteristics

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Mass and radius

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Kepler-1708b is a gas giant planet slightly smaller than Jupiter in size, with a radius of 0.89 Jupiter radii.[6][4] 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 <98 m/s—although within reach of the most precise spectrographs available, the faintness of Kepler-1708b's host star would make observations difficult.[1][7]

Orbit and temperature

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Kepler-1708b orbits about 1.64 astronomical units from its host star and completes one revolution every 737.11 days or 2.02 years, comparable to the orbit of Mars in the Solar System.[8] At this distance, Kepler-1708b lies within the habitable zone of its host star, where it receives an insolation flux 0.561+0.074
−0.068 times that of Earth at a relatively cool equilibrium temperature of 200–300 kelvins (−73–27 °C; −100–80 °F).[1][9] The eccentricity of its orbit is unmeasured and is given a 2-sigma upper limit of <0.40.[1]

Host star

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Kepler-1708b orbits around the Sun-like star Kepler-1708, located in the constellation of Cygnus 5,580 ± 240 ly (1,712 ± 75 pc) light years away from Earth.[1] At an apparent magnitude of 16, this star is too faint to be seen by the naked eye.[10] The star's celestial coordinates based on the J2000 epoch are: RA 19h 47m 17.79s, Dec 43° 37′ 29.4″.[10] The European Space Agency's Gaia satellite has measured a stellar parallax of 0.5730±0.0340 milliarcseconds (mas) and directional proper motion components of RA −0.770±0.057 mas/yr, Dec −5.005±0.059 mas/yr.[10] 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.[10]

Kepler-1708 is slightly larger and more massive than the Sun, with a mass of 1.088±0.072 M☉ and radius of 1.117±0.064 R☉. It is also hotter and more luminous than the Sun, with an effective temperature of 6,157+231
−202 K and a bolometric luminosity of 1.521 L☉.[a] Based on these properties, Kepler-1708 is likely an F-type main sequence star with a Sun-like metallicity of [Fe/H] = 0.0±0.2 dex and an age of 3.16±2.26 billion years.[b][6][1]

Potential exomoon

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Kepler-1708b and its possible exomoon, rendered in Celestia.

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.[11] 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.[1][12] 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.[1]

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.[13]

In 2024, a paper was published disputing both 1625b I and 1708b I’s existences.[5]

See also

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Notes

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  1. ^ Luminosity calculated from the inverse of   from Kipping et al. (2022)[1]
  2. ^ Age calculated from the inverse of   from Kipping et al. (2022)[1]

References

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  1. ^ a b c d e f g h i j k l m n o Kipping, David; Bryson, Steve; Burke, Chris; Christiansen, Jessie; Hardegree-Ullman, Kevin; Quarles, Billy; Hansen, Brad; Szulágyi, Judit; Teachey, Alex (January 2022). "An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i" (PDF). Nature Astronomy. 6 (3): 367–380. arXiv:2201.04643. Bibcode:2022NatAs...6..367K. doi:10.1038/s41550-021-01539-1. PMC 8938273. PMID 35399159. S2CID 245906142.
  2. ^ a b Herman, Miranda K.; Zhu, Wei; Wu, Yanqin (June 2019). "Revisiting the Long-period Transiting Planets from Kepler". The Astronomical Journal. 157 (6): 15. arXiv:1901.01974. Bibcode:2019AJ....157..248H. doi:10.3847/1538-3881/ab1f70. S2CID 119550672. 248.
  3. ^ a b Kawahara, Hajime; Masuda, Kento (June 2019). "Transiting Planets Near the Snow Line from Kepler. I. Catalog". The Astronomical Journal. 157 (6): 27. arXiv:1904.04980. Bibcode:2019AJ....157..218K. doi:10.3847/1538-3881/ab18ab. S2CID 119099510. 218.
  4. ^ a b c d "Kepler-1708 Overview". NASA Exoplanet Archive. Infrared Processing and Analysis Center. Retrieved 16 January 2022.
  5. ^ a b Heller, René; Hippke, Michael (2024). "Large exomoons unlikely around Kepler-1625 b and Kepler-1708 B". Nature Astronomy. 8: 193. arXiv:2312.03786. Bibcode:2024NatAs...8..193H. doi:10.1038/s41550-023-02148-w.
  6. ^ a b "Kepler-1708 b". NASA Exoplanet Exploration. NASA. Retrieved 16 January 2022.
  7. ^ Timmermann, Anina; Heller, René; Reiners, Ansgar; Zechmeister, Mathias (March 2020). "Radial velocity constraints on the long-period transiting planet Kepler-1625 b with CARMENES" (PDF). Astronomy & Astrophysics. 635: 2. arXiv:2001.10867. Bibcode:2020A&A...635A..59T. doi:10.1051/0004-6361/201937325. S2CID 210942758. A59.
  8. ^ Skuse, Ben (14 January 2022). "Needle in the Haystack: New Exomoon Candidate Found". Sky & Telescope. Retrieved 16 January 2022.
  9. ^ Kane, Stephen; Gelino, Dawn. "Habitable Zone Gallery". Retrieved 16 January 2022.
  10. ^ a b c d "UCAC4 669-077544 -- Star". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 January 2022.
  11. ^ "Scientists think they've found a big, weird moon in a far-off star system". NPR.org. Retrieved 2022-03-28.
  12. ^ O'Callaghan, Jonathan (13 January 2022). "Astronomers Have Found Another Possible 'Exomoon' beyond Our Solar System". Scientific American. Retrieved 16 January 2022.
  13. ^ Cassese, Ben; Kipping, David (2022-03-24). "Kepler-1708 b-i is likely undetectable with HST". Monthly Notices of the Royal Astronomical Society. 516 (3): 3701–3708. arXiv:2203.13290. doi:10.1093/mnras/stac2090.
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