Planet Kepler-296 c

Name Kepler-296 c
Planet Status Confirmed
Discovered in 2014
Mass
Mass*sin(i)
Semi-Major Axis 0.054 AU
Orbital Period 5.841648 ( -1.5e-05 +1.5e-05 ) day
Eccentricity
ω
Tperi
Radius 0.192 ( -0.009 +0.009 ) RJ
Inclination
Update 2014-03-06
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-296
Name Kepler-296
Distance
Spectral type
Apparent magnitude V
Mass
Age
Effective temperature 4249.0 (± 100.0) K
Radius 0.56 (± 0.02) RSun
Metallicity [Fe/H] 0.168
Detected Disc
Magnetic Field
RA2000 19:06:09.6
Dec2000 +49:26:14
Alternate Names
Planetary system
5 planets

More data


Related publications

The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis
2015 BARCLAY Th., QUINTANA E., ADAMS F., CIARDI D., HUBER D. et al.
ApJ, 809, 7
arxiv   paper   ADS  

Hubble Space Telescope High Resolution Imaging of Kepler Small and Cool Exoplanet Host Stars
2015 GILLILAND R., CARTIER K., ADAMS E., CIARDI D., KALAS P. et al.
Astron. J., 149, 24
paper  arxiv  

Validation of Twelve Small Kepler Transiting Planets in the Habitable Zone
2015 TORRES G., KIPPING D., FRESSIN F., CALSDWELL D., TWICKEN J. et al.
ApJ, accepted
arxiv  

Revision of Earth-sized Kepler Planet Candidate Properties with High-resolution Imaging by the Hubble Space Telescope
2015 CARTIER K., GILLILAND R., WRIGHT J. & CIARDI D.
ApJ, 804, 97
paper  arxiv  ADS  

Validation of Kepler's Multiple Planet Candidates. III: Light Curve Analysis & Announcement of Hundreds of New Multi-planet Systems
2014 ROWE J., BRYSON T., MARCY G., LISSAUER J., JONTOF-HUTTER D. et al.
ApJ, 784, 45
paper  arxiv  

Revision of Earth-sized Kepler Planet Candidate Properties with High Resolution Imaging by Hubble Space Telescope
2014 STAR K., GILLILAND R., WRIGHT J. & CIARDI D.
ApJ, submitted
arxiv