Kepler-102

Star in the constellation Lyra From Wikipedia, the free encyclopedia

Kepler-102 is a star 353 light-years (108 parsecs) away in the constellation of Lyra. Kepler-102 is less luminous than the Sun.[6] The star system does not contain any observable amount of dust.[7] Kepler-102 is suspected to be orbited by a binary consisting of two red dwarf stars, at projected separations of 591 and 627 AU.[8]

Right ascension18h 45m 55.85599s[2]
Declination+47° 12 28.8453[2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Kepler-102
Observation data
Epoch J2000      Equinox J2000
Constellation Lyra[1]
Right ascension 18h 45m 55.85599s[2]
Declination +47° 12 28.8453[2]
Apparent magnitude (V) 12.07[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type K3V[3]
Astrometry
Radial velocity (Rv)−28.51±0.37[2] km/s
Proper motion (μ) RA: −41.044 mas/yr[2]
Dec.: −43.267 mas/yr[2]
Parallax (π)9.2517±0.0102 mas[2]
Distance352.5 ± 0.4 ly
(108.1 ± 0.1 pc)
Details
Mass0.803±0.021[4] M
Radius0.724±0.018[4] R
Temperature4909±98[4] K
Metallicity [Fe/H]0.11±0.04[4] dex
Rotation26.572±0.153 d[5]
Age1.1+3.6
−0.5
[4] Gyr
Other designations
KOI-82, KIC 10187017, TYC 3544-1383-1, 2MASS J18455585+4712289, Gaia DR2 2119583201145735808
Database references
SIMBADdata
Exoplanet Archivedata
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Planetary system

In January 2014, a system of five planets around the star was announced, three of them being smaller than Earth. While 3 of the transit signals were discovered during the first year of the Kepler mission, their small size made them hard to confirm as possibilities of these being false positives were needed to be removed. Later, two other signals were detected. Follow-up radial velocity data helped to determine the mass of the two largest planets (Kepler-102d and Kepler-102e).[9]

By 2017, the search for additional planets utilizing the transit-timing variation method had yielded zero results,[10] although the presence of planets with semimajor axis beyond 10 AU cannot be excluded.[11]

More information Companion (in order from star), Mass ...
The Kepler-102 planetary system[4]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b <1.1 M🜨 0.05521±0.00049 5.286965(12) <0.100 89.78±0.22° 0.460±0.026 R🜨
c <1.7 M🜨 0.06702±0.00059 7.071392(22) <0.094 89.82±0.15° 0.567±0.028 R🜨
d 3.0±1.3 M🜨 0.08618±0.00076 10.3117670(41) <0.092 89.49±0.11° 1.154±0.058 R🜨
e 4.7±1.8 M🜨 0.1162±0.0010 16.1456994(22) <0.089 89.488±0.051° 2.17±0.11 R🜨
f <4.3 M🜨 0.1656±0.0015 27.453592(60) <0.10 89.320±0.037° 0.861±0.022 R🜨
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See also

References

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