Kepler-421

Kepler-421 is a star. Kepler-421 has an exoplanet orbiting it (Kepler-421b), which is notable for its position near the snow line.

Kepler-421
Observation data
Epoch J2000      Equinox J2000
Constellation Lyra
Right ascension  18h 53m 01.6406s[1]
Declination 45° 5 15.9725[1]
Apparent magnitude (V) 13.56±0.04[2]
Characteristics
Evolutionary stage Dwarf
Spectral type G9/K0[2]
Astrometry
Proper motion (μ) RA: −4.010±0.032[1] mas/yr
Dec.: −20.398±0.037[1] mas/yr
Parallax (π)2.8401 ± 0.0166[1] mas
Distance1,148 ± 7 ly
(352 ± 2 pc)
Details
Mass0.76[3] M
Radius0.84[3] R
Luminosity0.451[1] L
Surface gravity (log g)4.54[3] cgs
Temperature5,308±50[2] K
Metallicity [Fe/H]−0.25±0.08[2] dex
Rotation28.5±0.3 d[2]
Rotational velocity (v sin i)1.5±0.5[3] km/s
Age14.38[3] Gyr
Other designations
KOI-1274, KIC 8800954, 2MASS J18530163+4505159 [4]
Database references
SIMBADdata
KICdata

References

  1. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. Kipping, D. M.; Torres, G.; Buchhave, L. A.; Kenyon, S. J.; Henze, C.; Isaacson, H.; Kolbl, R.; Marcy, G. W.; Bryson, S. T.; Stassun, K.; Bastien, F. (9 October 2014). "Discovery of a Transiting Planet Near the Snow-Line". The Astrophysical Journal. 795 (1): 25. arXiv:1407.4807. Bibcode:2014ApJ...795...25K. doi:10.1088/0004-637X/795/1/25.
  3. Brewer, John M.; Fischer, Debra A. (2018). "Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest". The Astrophysical Journal Supplement Series. 237 (2): 38. arXiv:1804.00673. Bibcode:2018ApJS..237...38B. doi:10.3847/1538-4365/aad501.
  4. "Kepler-421". SIMBAD. Centre de données astronomiques de Strasbourg.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.