Name | Kepler-21 b | ||
Planet Status | Confirmed | ||
Discovered in | 2012 | ||
Mass | 0.01598 ( -0.00541 +0.00541 ) MJ | ![]() |
|
Mass*sin(i) | — | ||
Semi-Major Axis | 0.042717 ( -0.0 +0.0 ) AU | ![]() |
|
Orbital Period | 2.78578 (± 3e-05) day | ![]() |
+ |
Eccentricity | 0.02 ( -0.02 +0.1 ) | ![]() |
+ |
ω | -15.0 ( -79.0 +79.0 ) deg | ![]() |
|
Tperi | 2456797.9 (± 0.7) JD | ![]() |
|
Radius | 0.146 ( -0.001 +0.002 ) RJ | ![]() |
|
Inclination | 83.2 ( -0.26 +0.28 ) deg | ![]() |
|
Update | 2021-02-05 | ||
Detection Method | Primary Transit | ||
Mass Detection Method | — | ||
Radius Detection Method | Primary Transit | ||
Primary transit | 2455093.83716 ( -0.00085 +0.00062 ) JD | ![]() |
+ |
Secondary transit | — | ||
λ | — | ||
Impact Parameter b | 0.584 ( -0.02 +0.018 ) | ![]() |
|
Time Vr=0 | — | ||
Velocity Semiamplitude K | 1.99 (± 0.65) m/s | ![]() |
|
Calculated temperature | 2025.0 K | ![]() |
|
Measured temperature | — | ||
Hottest point longitude | — | ||
Geometric albedo | — | ||
Surface gravity log(g/gH) | — | ||
Alternate Names | Kepler-21 b, 2MASS J19092683+3842505 b, BD+38 3455 b, HD 179070 b, HIP 94112 b, K00975.01, KIC 3632418 b, KOI-975 b, KOI-975.01, Kepler-21 A b, SAO 67891 b, TYC 3120-00963-1 b, WISE J190926.86+384250.7 b |
Name | Kepler-21 | ||
Distance | 108.86 ( -0.38 +0.38 ) pc | ||
Spectral type | F6 IV | ||
Apparent magnitude V | 8.27 | ||
Mass | 1.41 ( -0.03 +0.02 ) MSun | ||
Age | 3.03 ( --0.35 +0.35 ) Gyr | ||
Effective temperature | 6305.0 ( -50.0 +50.0 ) K | ||
Radius | 1.9 ( -0.01 +0.02 ) RSun | ||
Metallicity [Fe/H] | -0.03 ( -0.1 +0.1 ) | ||
Detected Disc | — | ||
Magnetic Field | — | ||
RA2000 | 19:09:26.8 | ||
Dec2000 | +38:42:50 | ||
Alternate Names | Kepler-21, 2MASS J19092683+3842505, BD+38 3455, HD 179070, HIP 94112, KIC 3632418, KOI-975, Kepler-21 A, SAO 67891, TYC 3120-00963-1, WISE J190926.86+384250.7 | ||
Planetary system | 1 planet |
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The Densities of Planets in Multiple Stellar Systems
2017
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Kepler-21b: A rocky planet around a V = 8.25 magnitude star
2016
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2015
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Dynamics of Rotation of Super-Earths
2013
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paper
A Uniformly Derived Catalogue of Exoplanets from Radial Velocities
2012
HOLLIS M., BALAN S., LEVER G. & LAHAV O.
MNRAS, 423, Issue 3, 2800-2814
paper arxiv
An Efficient Automated Validation Procedure for Exoplanet Transit Candidates
2012
MORTON T.
ApJ., 761, 6
paper arxiv
Validation of the Exoplanet Kepler-21b using PAVO/CHARA Long-Baseline Interferometry
2012
HUBER D., IRELAND M., BEDDING T., HOWELL S., MAESTRO V. & 11 additional authors
MNRAS, 423, l16
paper arxiv
The Exoplanet Handbook
2011
PERRYMAN M.
Content
Content and Chapter 5
Kepler-21b: A 1.6REarth Planet Transiting the Bright Oscillating F Subgiant Star HD 179070
2011
HOWEL S., ROWE J., BRYSON S., QUINN S., MARCY G. & 60 additional authors
ApJ.
arxiv
Kepler 21b - Kepler's Brightest Host Star Harbors a 1.6 R_Earth Planet
2011
HOWELL S.