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Kepler-1658

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(Redirected fromKepler-1658b)
Triple star system in the constellation Cygnus
Kepler-1658
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus[1]
Right ascension18h 46m 22.24188s[2]
Declination+75° 26′ 02.2400″[2]
Apparent magnitude (V)11.556±0.100[3]
Characteristics
A
Evolutionary stageSubgiant[4]
Spectral typeF5[5]
BC
Evolutionary stagemain sequence[6]
Spectral typeKV + MV[6]
Variable typeeclipsing binary[6]
Astrometry
Radial velocity (Rv)−21.815±0.053[7] km/s
Proper motion (μ)RA: +0.100mas/yr[2]
Dec.: −5.542mas/yr[2]
Parallax (π)1.2260±0.0173 mas[2]
Distance2,660 ± 40 ly
(820 ± 10 pc)
Orbit[6]
PrimaryA
CompanionBC
Semi-major axis (a)50 AU
Orbit[6]
PrimaryB
CompanionC
Period (P)3.849363145 days
Details[8]
Kepler-1658 A
Mass1.45±0.03 M
Radius3.26±0.14 R
Surface gravity (log g)4.13±0.05 cgs
Temperature5,948±100 K
Metallicity[Fe/H]−0.27±0.06 dex
Rotational velocity (v sin i)38 km/s
Age2.0±0.1 Gyr
Kepler-1658 B
Mass0.75[6] M
Kepler-1658 C
Mass0.19[6] M
Radius0.23[6] R
Other designations
KOI-4,KIC 3861595,TIC 377873569,TYC 3135-652-1[9]
Database references
SIMBADdata

Kepler-1658 is atriple star system located in the constellationCygnus.[1] Based onparallax measurements by theGaia spacecraft,[2] it is located at a distance of 2,660light-years (820parsecs).

This is an hierarchical triple system whose primary is anF-typesubgiant star with 1.45 times theSun's mass and 3.26 times theSun's radius.[8] The outer system, 50astronomical units away from the primary, is aneclipsing binary whose components have an orbital period of 3.8 days: star B is probably aK-type dwarf with 0.8 times the Sun's mass, and star C ared dwarf with 0.19 times the mass of the Sun and 0.23 times the radius.[6]

Search for planets

[edit]

In 2009, ahot Jupiter planet candidate (KOI-4.01, now known as Kepler-1658b) was identified around Kepler-1658 by theKepler space telescope via thetransit method. Initially ruled out as a false alarm, a 2019 study re-claimed its nature as a planet. This would be the first planet ever detected by Kepler.[4] Analysis of theTransiting Exoplanet Survey Satellite (TESS) data in 2022 showed that it is gradually spiraling into its star, with its orbit decaying.[10] However, in 2025 it was demonstrated that Kepler-1658b is afalse positive planet.[6] In reality, all the data that supported the detection of a planet with physical orbital decay were caused by the eclipsing outer system, whoselight travel time effect is responsible for the supposed orbital decay.[6]

References

[edit]
  1. ^abRoman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  2. ^abcdeVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^Zacharias, N.; Finch, C. T.; Girard, T. M.; Henden, A.; Bartlett, J. L.; Monet, D. G.; Zacharias, M. I. (2013-01-14). "The Fourth Us Naval Observatory CCD Astrograph Catalog (Ucac4)".The Astronomical Journal.145 (2): 44.arXiv:1212.6182.Bibcode:2013AJ....145...44Z.doi:10.1088/0004-6256/145/2/44.ISSN 0004-6256.
  4. ^abChontos, Ashley; Huber, Daniel; Latham, David W.; Bieryla, Allyson; Eylen, Vincent Van; Bedding, Timothy R.; Berger, Travis; Buchhave, Lars A.; Campante, Tiago L.; Chaplin, William J.; Colman, Isabel L.; Coughlin, Jeff L.; Davies, Guy; Hirano, Teruyuki; Howard, Andrew W. (2019)."The Curious Case of KOI 4: Confirming Kepler ' s First Exoplanet Detection".The Astronomical Journal.157 (5): 192.arXiv:1903.01591.Bibcode:2019AJ....157..192C.doi:10.3847/1538-3881/ab0e8e.ISSN 1538-3881.S2CID 119240124.
  5. ^Su, Tianhao; Zhang, Li-yun; Long, Liu; Han, Xianming L.; Misra, Prabhakar; Meng, Gang; Pi, Qingfeng; Yang, ZiLu; Yang, Jiawei (2022-07-27)."Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys".The Astrophysical Journal Supplement Series.261 (2): 26.Bibcode:2022ApJS..261...26S.doi:10.3847/1538-4365/ac7151.ISSN 0067-0049.
  6. ^abcdefghijkWinn, Joshua N.; Stefánsson, Guđmundur (2025-12-01)."Orbital Decay Candidates Reconsidered: WASP-4 b Is Not Decaying and Kepler-1658 b Is Not a Planet".The Planetary Science Journal.6 (12): 300.arXiv:2510.05229.doi:10.3847/PSJ/ae21db.ISSN 2632-3338.
  7. ^Jönsson, Henrik; Holtzman, Jon A.; Prieto, Carlos Allende; Cunha, Katia; García-Hernández, D. A.; Hasselquist, Sten; Masseron, Thomas; Osorio, Yeisson; Shetrone, Matthew; Smith, Verne; Stringfellow, Guy S.; Bizyaev, Dmitry; Edvardsson, Bengt; Majewski, Steven R.; Mészáros, Szabolcs (2020-08-17)."APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South".The Astronomical Journal.160 (3): 120.arXiv:2007.05537.Bibcode:2020AJ....160..120J.doi:10.3847/1538-3881/aba592.ISSN 0004-6256.
  8. ^abPetigura, Erik A.; Rogers, James G.; Isaacson, Howard; Owen, James E.; Kraus, Adam L.; Winn, Joshua N.; MacDougall, Mason G.; Howard, Andrew W.; Fulton, Benjamin; Kosiarek, Molly R.; Weiss, Lauren M.; Behmard, Aida; Blunt, Sarah (April 2022)."The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age".The Astronomical Journal.163 (4): 179.arXiv:2201.10020.Bibcode:2022AJ....163..179P.doi:10.3847/1538-3881/ac51e3.ISSN 0004-6256.
  9. ^"Kepler-1658".SIMBAD.Centre de données astronomiques de Strasbourg.
  10. ^Vissapragada, Shreyas; Chontos, Ashley; Greklek-McKeon, Michael; Knutson, Heather A.; Dai, Fei; González, Jorge Pérez; Grunblatt, Sam; Huber, Daniel; Saunders, Nicholas (2022)."The Possible Tidal Demise of Kepler's First Planetary System".The Astrophysical Journal Letters.941 (2): L31.arXiv:2212.09752.Bibcode:2022ApJ...941L..31V.doi:10.3847/2041-8213/aca47e.ISSN 2041-8205.S2CID 254875671.
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