Kepler-410

Kepler-410
Observation data
Epoch J2000      Equinox J2000
Constellation Lyra
Right ascension 18h 52m 36.1606s[1]
Declination +45° 08′ 23.343″[1]
Apparent magnitude (V) 9.50[1]
Characteristics
Kepler-410A
Evolutionary stage Subgiant
Spectral type F6IV[2]
Kepler-410B
Spectral type K2[3]
Astrometry
A
Radial velocity (Rv)−40.6±0.7[4] km/s
Proper motion (μ) RA: 61.683[4] mas/yr
Dec.: 61.673[4] mas/yr
Parallax (π)6.7933 ± 0.0109 mas[4]
Distance480.1 ± 0.8 ly
(147.2 ± 0.2 pc)
B
Proper motion (μ) RA: 61.679[4] mas/yr
Dec.: 60.937[5] mas/yr
Parallax (π)6.8007 ± 0.0260 mas[5]
Distance480 ± 2 ly
(147.0 ± 0.6 pc)
Position (relative to Kepler-410A)[6]
ComponentKepler-410B
Angular distance1.6672±0.0015″
Position angle35.975±0.052°
Projected separation245 AU
Details
Kepler-410A
Mass1.223±0.054[7] M☉
Radius1.357±0.022[7] R☉
Luminosity2.66±0.16[7] L☉
Surface gravity (log g)4.28±0.02[8] cgs
Temperature6325±75[8] K
Metallicity [Fe/H]0.01±0.10[8] dex
Rotation20.3+2.2
−1.3 d[9]
Age1.81±0.27[7] Gyr
Kepler-410B
Mass0.728[3] M☉
Radius0.89+0.09
−0.03[3] R☉
Other designations
BD+44 3008, Kepler-410, KOI-42, KIC 8866102, TYC 3540-760-1, GSC 03540-00760, 2MASS J18523616+4508233[1]
Kepler-410A: Gaia EDR3 2106904148451706752
Kepler-410B: Gaia EDR3 2106904148449360000
Database references
SIMBADdata
B

Kepler-410 is a binary star system. Its primary star, also known as Kepler-410A, is a F-type subgiant star, orbited by the orange dwarf star Kepler-410B on a wide orbit. The companion star was discovered in 2012.[6]

The primary star's surface temperature is 6325±75 K.[8] HD 175289 is similar to the Sun in its concentration of heavy elements, with a metallicity Fe/H index of 0.01±0.10,[8] but is much younger at an age of 1.81±0.27 billion years.[7]

  1. ^ a b c d "HD 175289". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-24.
  2. ^ Molenda-Żakowicz, J.; Sousa, S. G.; Frasca, A.; Uytterhoeven, K.; Briquet, M.; Van Winckel, H.; Drobek, D.; Niemczura, E.; Lampens, P.; Lykke, J.; Bloemen, S.; Gameiro, J. F.; Jean, C.; Volpi, D.; Gorlova, N.; Mortier, A.; Tsantaki, M.; Raskin, G. (2013). "Atmospheric parameters of 169 F-, G-, K- and M-type stars in the Kepler field". Monthly Notices of the Royal Astronomical Society. 434 (2): 1422. arXiv:1306.6011. Bibcode:2013MNRAS.434.1422M. doi:10.1093/mnras/stt1095. S2CID 59269553.
  3. ^ a b c Ziegler, Carl; Law, Nicholas M.; Baranec, Christoph; Howard, Ward; Morton, Tim; Riddle, Reed; Duev, Dmitry A.; Salama, Maïssa; Jensen-Clem, Rebecca; Kulkarni, S. R. (2018). "Robo-AO Kepler Survey. V. The Effect of Physically Associated Stellar Companions on Planetary Systems". The Astronomical Journal. 156 (2): 83. arXiv:1804.10208. Bibcode:2018AJ....156...83Z. doi:10.3847/1538-3881/aace59. S2CID 96459123.
  4. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  5. ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  6. ^ a b 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.
  7. ^ a b c d e Bellinger, E. P.; Hekker, S.; Angelou, G. C.; Stokholm, A.; Basu, S. (2020). "Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy". Astronomy & Astrophysics. 622: A130. arXiv:1812.06979. doi:10.1051/0004-6361/201834461. S2CID 119293351.
  8. ^ a b c d e Cite error: The named reference Kayhan2019 was invoked but never defined (see the help page).
  9. ^ Suto, Yasushi; Kamiaka, Shoya; Benomar, Othman (2019). "Asteroseismic Determination of the Stellar Rotation Period of the Kepler Transiting Planetary Systems and its Implications for the Spin–Orbit Architecture". The Astronomical Journal. 157 (5): 172. arXiv:1903.04669. Bibcode:2019AJ....157..172S. doi:10.3847/1538-3881/ab0f33. S2CID 119120529.