Name | Kepler-1229 b | ||
Planet Status | Confirmed | ||
Discovered in | 2016 | ||
Mass | — | ||
Mass*sin(i) | — | ||
Semi-Major Axis | — | ||
Orbital Period | 86.828989 ( -0.001069 +0.001069 ) day | ||
Eccentricity | — | ||
ω | — | ||
Tperi | — | ||
Radius | 0.125 ( -0.012 +0.01 ) RJ | ||
Inclination | — | ||
Update | 2021-02-05 | ||
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 | 2MASS J19495680+4659481 b, K02418.01, KIC 10027247 b, KOI-2418 b, KOI-2418.01, WISE J194956.83+465948.1 b |
Name | Kepler-1229 | ||
Distance | 236.0 pc | ||
Spectral type | — | ||
Apparent magnitude V | — | ||
Mass | 0.54 ( -0.04 +0.03 ) MSun | ||
Age | 3.72 ( --2.07 +5.32 ) Gyr | ||
Effective temperature | 3784.0 ( -38.61 +38.88 ) K | ||
Radius | 0.51 ( -0.03 +0.03 ) RSun | ||
Metallicity [Fe/H] | -0.06 ( -0.109 +0.086 ) | ||
Detected Disc | — | ||
Magnetic Field | — | ||
RA2000 | 19:49:56.8 | ||
Dec2000 | +46:59:48 | ||
Alternate Names | 2MASS J19495680+4659481, KIC 10027247, KOI-2418, WISE J194956.83+465948.1 | ||
Planetary system | 1 planet |
Revising Properties of Planet-host Binary Systems II: Apparent Near-Earth Analog Planets in Binaries Are Often Sub-Neptunes
2022
SULLIVAN K. & KRAUS A.
Astron. & Astrophys., 164, 138
paper arxiv
Liquid water on cold exo-Earths via basal melting of ice sheets
2022
OJHA L., TRONCONE B., BUFFO J., JOURNAUX B. & McDONALD G.
Nature Communications, 13, 7521
paper arxiv
Habitability of exoplanet waterworlds
2018
KITE E. & FORD E.
ApJ, 864, 75
arxiv
paper
False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives
2016
MORTON T., BRYSON S., COUGHLIN J., ROWE J., RAVICHANDRAN G. et al.
ApJ, 822, 86
paper arxiv
ADS