Planet Kepler-65 b

Name Kepler-65 b
Planet Status Confirmed
Discovered in 2013
Mass
Mass*sin(i)
Semi-Major Axis 0.035 ( -0.001 +0.002 ) AU
Orbital Period 2.1549156 (± 2.5e-06) day +
Eccentricity 0.02 ( -0.02 +0.17 )
ω
Tperi
Radius 0.1257 ( -0.0015 +0.0015 ) RJ
Inclination
Update 2015-12-02
Detection Method Primary Transit
Mass Detection Method
Radius Detection Method
Primary transit
Secondary transit
λ
Impact Parameter b
Time Vr=0
Velocity Semiamplitude K
Calculated temperature
Measured temperature
Hottest point longitude
Geometric albedo
Surface gravity log(g/gH)
Alternate Names

Star

Kepler-65
Name Kepler-65
Distance 312.43 (± 9.75) pc
Spectral type B
Apparent magnitude V 11.018
Mass 1.199 ( -0.03 +0.029 ) MSun +
Age 3.89 ( -0.48 +0.59 ) Gyr +
Effective temperature 6211.0 (± 66.0) K
Radius 1.399 (± 0.012) RSun +
Metallicity [Fe/H] 0.17 (± 0.06)
Detected Disc
Magnetic Field
RA2000 19:14:45.0
Dec2000 +41:09:04
Alternate Names
Planetary system
3 planets

More data


Related publications

Spin-orbit alignment of exoplanet systems: ensemble analysis using asteroseismology
2016 CAMPANTE T., LUND M., KUSZLEWICZ J., DAVIES G., CHAPLIN W. et al;
ApJ, 819, 85
paper  arxiv  ADS  

Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities
2015 VAN EYLEN V. & ALBRECHT S.
ApJ, 808, 126
paper   arxiv   ADS  

Asteroseismology of Exoplanet Host Stars
2015 HUBER D.
in "Focus Meeting 17 - IAU General Assembly in Hawaii, August 2015"
arxiv  

Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology
2015 SILVA AGUIRRE V., DAVIES G., BASU S., CHRISTENSEN-DALSGAARD J., CREEVY O. et al.
MNRAS, 452, 2127
paper   arxiv   ADS  

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65
2013 CHAPLIN W., SANCHIS-OJEDA R., CAMPANTE T., HANDBERG R., STELLO D. & 24 additional authors
ApJ, 766, 101
paper   arxiv   ADS