Kepler-41

G-type main sequence star in the constellation Cygnus From Wikipedia, the free encyclopedia

Kepler-41 or KOI-196 is a star in the constellation Cygnus. It is a G-type main-sequence star, like the Sun, and it is located about 3,510 light-years (1,080 parsecs) away.[2] It is fairly similar to the Sun, with 115% of its mass, a radius of 129% times that of the Sun, and a surface temperature of 5,750 K.[5] Search for stellar companions to Kepler-41 in 2013-2014 has yielded inconclusive results, compatible with Kepler-41 being the single star.[7]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Kepler-41
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus[1]
Right ascension 19h 38m 03.1747s[2]
Declination +45° 58 53.877[2]
Apparent magnitude (V) 14.5[3]
Characteristics
Evolutionary stage subgiant[4][2]
Spectral type G2V[5]
Astrometry
Radial velocity (Rv)−27.066±0.008[5] km/s
Proper motion (μ) RA: 3.001(19) mas/yr[2]
Dec.: 2.965(20) mas/yr[2]
Parallax (π)0.9283±0.0156 mas[2]
Distance3,510 ± 60 ly
(1,080 ± 20 pc)
Details
Mass1.15±0.04[5] M
Radius1.36±0.07[4] R
Luminosity1.93[4] L
Surface gravity (log g)4.12[4] cgs
Temperature5,630[4] K
Metallicity [Fe/H]0.38±0.11[5] dex
Rotational velocity (v sin i)6±2[5] km/s
Age4.38+0.85
−0.93
[4] Gyr
Other designations
KIC 9410930, KOI-196, UCAC3 272-156898, 2MASS J19380317+4558539, Gaia DR2 2080061942886335744[6]
Database references
SIMBADdata
KICdata
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Planetary system

In 2011, the planet Kepler-41b was discovered in orbit around the star. The planet orbits extremely close to Kepler-41, completing an orbit once every 1.86 days. Despite it receiving a high amount of radiation from Kepler-41, the radius of the Kepler-41b was initially believed to be less than that of Jupiter making it unusual for a hot Jupiter however later observations showed an inflated radius similar to other hot jupiters.[5] Kepler-41b is also quite reflective, with a geometric albedo of 0.30.[8]

More information Companion (in order from star), Mass ...
The Kepler-41 planetary system[5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.56±0.08 MJ 0.03101±0.0004 1.85555820±0.00000052 0 (fixed) 82.51±0.09° 1.29±0.02 RJ
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References

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