Kepler-71

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

Kepler-71 is a yellow main sequence star in the constellation of Cygnus.

Quick facts Constellation, Right ascension ...
Kepler-71
Observation data
Epoch J2000      Equinox ICRS
Constellation Cygnus[1]
Right ascension 19h 37m 27.716s[2]
Declination 46° 17 08.941[2]
Apparent magnitude (V) 15.06[citation needed]
Characteristics
Evolutionary stage main sequence[citation needed]
Spectral type G8V[3]
V−R color index −0.29
R−I color index 0.46
J−H color index 0.377
J−K color index 0.457
Variable type ROT[4]
Astrometry
Radial velocity (Rv)−23.88±0.02[5] km/s
Proper motion (μ) RA: −2.379±0.021 mas/yr[2]
Dec.: −0.983±0.022 mas/yr[2]
Parallax (π)1.0647±0.0204 mas[2]
Distance3,060 ± 60 ly
(940 ± 20 pc)
Details[6][3][7]
Mass0.923 M
Radius0.816 R
Surface gravity (log g)4.54±0.01 cgs
Temperature5,545 K
Metallicity [Fe/H]0.22 dex
Rotationperiod 20 days
Age2.5-4 Gyr
Other designations
KOI-217, BOKS 40959, KIC 9595827, 2MASS J19392772+4617090, Gaia DR2 2080095679848047872[8]
Database references
SIMBADdata
Close

Star characteristics

Kepler-71 is enriched by heavy elements at 170% of Sun metallicity, young and has a very prominent starspot activity. Starspots are covering about 40% of star surface at transit latitudes, each planetary transit passing over an average six starspots.[6] The bright facula regions are even more extensive.[9] Unlike Sun, the photosphere of Kepler-71 rotates nearly like rigid body, with differential rotation not exceeding 2%.[7]

Planetary system

The "Hot Jupiter" class planet Kepler-71b was discovered around Kepler-71 in 2010.[3]

More information Companion (in order from star), Mass ...
The Kepler-71 planetary system[6][7]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b 0.05029+0.00002
0.00006
3.905079476+0.000008
0.000009
0 89.8+0.2
0.4
1.1987±0.0044 RJ
Close

References

Related Articles

Wikiwand AI