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Kepler-371

From Wikipedia, the free encyclopedia
Star in the constellation Cygnus
Kepler-371
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus[1]
Right ascension19h 29m 18.3513s[2]
Declination+38° 39′ 27.273″[2]
Apparent magnitude (V)14.0[3]
Characteristics
Evolutionary stagesubgiant[2]
Spectral typeG4V[4]
Astrometry
Proper motion (μ)RA: 3.560(12)mas/yr[2]
Dec.: −7.358(14)mas/yr[2]
Parallax (π)1.2177±0.0121 mas[2]
Distance2,680 ± 30 ly
(821 ± 8 pc)
Details
Mass0.93±0.05[5] M
Radius1.3[6] R
Luminosity1.6[6] L
Surface gravity (log g)4.20[6] cgs
Temperature5,759+70
−87
[5] K
Metallicity[Fe/H]−0.25[6] dex
Rotation149 days[7]
Rotational velocity (v sin i)2.0[7] km/s
Age5.5[5] Gyr
Other designations
Gaia DR2 2052702348375966208,KOI-2194,KIC 3548044,2MASS J19291835+3839273[8]
Database references
SIMBADdata
Exoplanet Archivedata

Kepler-371 (also known asKOI-2194 orKIC 3548044) is astar some 2,680 ly away from theEarth.[2] It hosts a multi planetary system consisting of 2 confirmedSuper-Earths, as well as 1 unconfirmed Near-Earth sized exoplanet in itshabitable zone.[9]

The Kepler-371 planetary system
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b0.234.763278±0.000351089.95°1.89 R🜨
c0.31367.968015089.95°1.78 R🜨
d(unconfirmed)

References

[edit]
  1. ^Roman, 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. ^abcdefVallenari, 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. ^Ostberg, Colby; Kane, Stephen R.; Li, Zhexing; Schwieterman, Edward W.; Hill, Michelle L.; Bott, Kimberly; Dalba, Paul A.; Fetherolf, Tara; Head, James W.; Unterborn, Cayman T. (2023)."The Demographics of Terrestrial Planets in the Venus Zone".The Astronomical Journal.165 (4): 168.arXiv:2302.03055.Bibcode:2023AJ....165..168O.doi:10.3847/1538-3881/acbfaf.
  4. ^Gray, R. O.; Corbally, C. J.; Cat, P. De; Fu, J. N.; Ren, A. B.; Shi, J. R.; Luo, A. L.; Zhang, H. T.; Wu, Y.; Cao, Z.; Li, G.; Zhang, Y.; Hou, Y.; Wang, Y. (2016)."Lamost Observations in the Kepler Field: Spectral Classification with the Mkclass Code".The Astronomical Journal.151 (1): 13.Bibcode:2016AJ....151...13G.doi:10.3847/0004-6256/151/1/13.
  5. ^abcMorton, Timothy D.; et al. (2016)."False Positive Probabilities for All Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives".The Astrophysical Journal.822 (2): 86.arXiv:1605.02825.Bibcode:2016ApJ...822...86M.doi:10.3847/0004-637X/822/2/86.S2CID 20832201.
  6. ^abcdYu, Jie; Khanna, Shourya; Themessl, Nathalie; Hekker, Saskia; Dréau, Guillaume; Gizon, Laurent; Bi, Shaolan (2023)."Revised Extinctions and Radii for 1.5 Million Stars Observed by APOGEE, GALAH, and RAVE".The Astrophysical Journal Supplement Series.264 (2): 41.arXiv:2206.00046.Bibcode:2023ApJS..264...41Y.doi:10.3847/1538-4365/acabc8.
  7. ^abTejada Arevalo, Roberto A.; Winn, Joshua N.; Anderson, Kassandra R. (2021)."Further Evidence for Tidal Spin-up of Hot Jupiter Host Stars".The Astrophysical Journal.919 (2): 138.arXiv:2107.05759.Bibcode:2021ApJ...919..138T.doi:10.3847/1538-4357/ac1429.
  8. ^"Kepler-371".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-08-21.
  9. ^"Kepler Host Overview Page".
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