Planet Kepler-102 d

Name Kepler-102 d
Planet Status Confirmed
Discovered in 2014
Mass 0.0082 ( -0.0035 +0.0041 ) MJ
Mass*sin(i)
Semi-Major Axis
Orbital Period 10.3117 day
Eccentricity
ω
Tperi 2454972.9875 (± 0.0032) JD
Radius 0.104 ( -0.006 +0.004 ) RJ
Inclination
Update 2015-12-09
Detection Method Primary Transit
Mass Detection Method
Radius Detection Method
Primary transit
Secondary transit
λ
Impact Parameter b 0.22 (± 0.05)
Time Vr=0
Velocity Semiamplitude K 1.37 (± 0.6) m/s
Calculated temperature
Measured temperature
Hottest point longitude
Geometric albedo
Surface gravity log(g/gH)
Alternate Names KOI 82.02

Star

Kepler-102
Name Kepler-102
Distance
Spectral type
Apparent magnitude V 11.492
Mass 0.81 ( -0.09 +0.04 ) MSun
Age 1.41 Gyr
Effective temperature 4809.0 (± 41.0) K
Radius 0.76 (± 0.07) RSun
Metallicity [Fe/H] 0.18 ( -0.47 +0.42 )
Detected Disc
Magnetic Field
RA2000 18:45:55.9
Dec2000 +47:12:29
Alternate Names KOI-82, KIC 10187017
Planetary system
5 planets

More data

Observability Predictor

Remarks

The KOI number of the planets of this system, ordered following Kepler photometric capability, are not in order of decreasing orbital period (the criterion followed for giving Kepler letters).


Related publications

Densities and Eccentricities of 139 Kepler Planets from Transit Time Variations
2014 HADDEN S. & LITHWICK Y.
ApJ, 787, 80
paper   arxiv   ADS  

The Mass-Radius Relation Between 65 Exoplanets Smaller than 4 Earth Radii
2014 WEISS L. & MARCY G.
ApJ Letters, 783, L6
paper   arxiv   ADS  

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets
2014 MARCY G., ISAACSON H., HOWARD A., ROWE J., JENKINS J. et al.
ApJ Suppl, 210, 20
paper   arxiv   ADS  

Influence of Stellar Multiplicity On Planet Formation. I. An Insight From $Kepler$ Multiple Planet Candidate Systems
2014 WANG J., XIE J.-W., BARCLAY Th. & FISCHER D.
ApJ, 783, id. 4, 15 pp
paper   arxiv   ADS