Kepler-385

Kepler-385
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus[1]
Right ascension 19h 37m 21.23819s[2]
Declination +50° 20′ 11.5477″[2]
Apparent magnitude (V) 15.76[3]
Astrometry
Proper motion (μ) RA: 2.738 mas/yr[2]
Dec.: -5.398 mas/yr[2]
Parallax (π)0.6597 ± 0.0183 mas[2]
Distance4,900 ± 100 ly
(1,520 ± 40 pc)
Details[4]
Mass0.99±0.03 M☉
Radius1.09±0.05 R☉
Surface gravity (log g)4.19±0.10 cgs
Temperature5835±64 K
Metallicity [Fe/H]0.010±0.037 dex
Other designations
Kepler-385, KOI-2433, KIC 11968463, TIC 27082352, 2MASS J19372123+5020115[5]
Database references
SIMBADdata

Kepler-385 (also designated KOI-2433) is an F-type main-sequence star located about 4,900 light-years (1,500 parsecs) away from Earth in the constellation of Cygnus. The star is 10% larger and 5% hotter than the Sun. The star has at least three, and potentially up to seven, exoplanets discovered orbiting it.[6][7]

The star has a mass of 1.05 solar masses, a radius of 1.157 solar radii, a temperature of 5829 Kelvin and a luminosity of 1.39 times the solar luminosity.[3]

  1. ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
  2. ^ a b c d Cite error: The named reference GaiaDR3 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference NASAExoplanetArchive was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference Lissauer2023 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference NASA-20231102 was invoked but never defined (see the help page).
  7. ^ Anderson, Natali (2023-11-06). "Kepler-385 Hosts Seven Large Exoplanets, Astronomers Say | Sci.News". Sci.News: Breaking Science News. Retrieved 2023-11-07.