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Kepler-107

Summary

Kepler-107 is a star about 1,694 light-years (519 parsecs) away in the constellation Cygnus. It is a spectral type G2 star. An imaging survey in 2016 failed to find any stellar companions to it.[4]

Kepler-107
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 48m 06.77346s[1]
Declination +48° 12′ 30.9642″[1]
Apparent magnitude (V) 12.70
Characteristics
Spectral type G2V[2]
Apparent magnitude (B) 13.34[2]
Apparent magnitude (V) 12.70[2]
Apparent magnitude (J) 11.39[2]
Apparent magnitude (K) 11.06[2]
Astrometry
Radial velocity (Rv)5.64423 ± 4.5 × 10–4[2] km/s
Proper motion (μ) RA: −9.393 mas/yr[1]
Dec.: 0.158 mas/yr[1]
Parallax (π)1.9259 ± 0.0092 mas[1]
Distance1,694 ± 8 ly
(519 ± 2 pc)
Details
Mass1.238±0.029[2] M☉
Radius1.447±0.014[2] R☉
Surface gravity (log g)(Spectroscopic) 4.28 ± 0.10 cgs
(Asteroseismic) 4.210 ± 0.013[2] cgs
Temperature5854±61[2] K
Metallicity [Fe/H]0.321±0.065[2] dex
Rotational velocity (v sin i)3.6±0.5[2] km/s
Age4.29+0.70
−0.56[2] Gyr
Other designations
Kepler-107, KOI-117, Gaia DR2 2086625752425381632, KIC 10875245, 2MASS J19480677+4812309[3]
Database references
SIMBADdata

Planetary system edit

Kepler-107 has four known planets discovered in 2014.[5][6][7][8] A giant impact is the likely origin of two planets in the system.[2] Kepler-107 c is more than twice as dense (about 12.6 g cm−3) as the innermost exoplanet Kepler-107 b (about 5.3 g  cm−3).[2]

The Kepler-107 planetary system[9]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 3.8+1.8
−1.7 M🜨 		0.04544±0.00036 3.1800218±0.0000029 <0.10 89.05±0.67° 1.536±0.025 R🜨
c 10.0±2.0 M🜨 0.06064±0.00048 4.901452±0.0 <0.080 89.49+0.34
−0.44° 		1.597±0.026 R🜨
d <7.7 M🜨 0.08377±0.00065 7.95839±0.00012 <0.11 87.55+0.64
−0.48° 		0.860±0.060 R🜨
e 14.1±3.3 M🜨 0.12638±0.00099 14.749143±0.000019 <0.10 89.67±0.22° 2.903±0.035 R🜨

References edit

  1. ^ a b c d Vallenari, 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 at VizieR.
  2. ^ a b c d e f g h i j k l m n o Bonomo, Aldo S.; Zeng, Li; Damasso, Mario; Leinhardt, Zoë M.; Justesen, Anders B.; Lopez, Eric; Lund, Mikkel N.; Malavolta, Luca; Silva Aguirre, Victor; Buchhave, Lars A.; Corsaro, Enrico; Denman, Thomas; Lopez-Morales, Mercedes; Mills, Sean M.; Mortier, Annelies; Rice, Ken; Sozzetti, Alessandro; Vanderburg, Andrew; Affer, Laura; Arentoft, Torben; Benbakoura, Mansour; Bouchy, François; Christensen-Dalsgaard, Jørgen; Collier Cameron, Andrew; Cosentino, Rosario; Dressing, Courtney D.; Dumusque, Xavier; Figueira, Pedro; Fiorenzano, Aldo F. M.; García, Rafael A.; Handberg, Rasmus; Harutyunyan, Avet; Johnson, John A.; Kjeldsen, Hans; Latham, David W.; Lovis, Christophe; Lundkvist, Mia S.; Mathur, Savita; Mayor, Michel; Micela, Giusi; Molinari, Emilio; Motalebi, Fatemeh; Nascimbeni, Valerio; Nava, Chantanelle; Pepe, Francesco; Phillips, David F.; Piotto, Giampaolo; Poretti, Ennio; Sasselov, Dimitar; Ségransan, Damien; Udry, Stéphane; Watson, Chris (May 2019). "A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system". Nature Astronomy. 3 (5): 416–423. arXiv:1902.01316. Bibcode:2019NatAs...3..416B. doi:10.1038/s41550-018-0684-9. S2CID 89604609.
  3. ^ Kepler-107 -- Rotationally variable Star
  4. ^ Kraus, Adam L.; Ireland, Michael J.; Huber, Daniel; Mann, Andrew W.; Dupuy, Trent J. (2016), "The Impact of Stellar Multiplicity on Planetary Systems. I. The Ruinous Influence of Close Binary Companions", The Astronomical Journal, 152 (1): 8, arXiv:1604.05744, Bibcode:2016AJ....152....8K, doi:10.3847/0004-6256/152/1/8, S2CID 119110229
  5. ^ "Exoplanets Data Explorer | Exoplanets - Detail View". exoplanets.org. Retrieved 5 May 2017.
  6. ^ "Exoplanets Data Explorer | Exoplanets - Detail View". exoplanets.org. Retrieved 5 May 2017.
  7. ^ "Exoplanets Data Explorer | Exoplanets - Detail View". exoplanets.org. Retrieved 5 May 2017.
  8. ^ "Exoplanets Data Explorer | Exoplanets - Detail View". exoplanets.org. Retrieved 5 May 2017.
  9. ^ Bonomo, A. S.; Dumusque, X.; et al. (April 2023). "Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems". Astronomy & Astrophysics. arXiv:2304.05773. doi:10.1051/0004-6361/202346211. S2CID 258078829.