Planet Kepler-452 b
| Name | Kepler-452 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2015 | ||
| Mass | — | ||
| Mass*sin(i) | — | ||
| Semi-Major Axis | 1.046 ( -0.015 +0.019 ) AU |  |
|
| Orbital Period | 384.843 ( -0.012 +0.007 ) day | |
|
| Eccentricity | 0.035 (± 0.75) | |
|
| ω | — | ||
| Tperi | — | ||
| Radius | 0.145 ( -0.02 +0.021 ) RJ | |
|
| Inclination | 89.806 ( -0.049 +0.134 ) deg | |
|
| Update | 2021-02-05 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | — | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2455147.9788 (± 0.0135) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.69 ( -0.16 +0.45 ) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | 265.0 K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | 2MASS J19440088+4416392 b, K07016.01, KIC 8311864 b, KOI-7016 b, KOI-7016.01, WISE J194400.89+441639.2 b |
Star
Kepler-452| Name | Kepler-452 | ||
| Distance | 560.62 ( -5.32 +5.32 ) pc | ||
| Spectral type | G2 | ||
| Apparent magnitude V | 13.7 | ||
| Mass | 1.04 ( -0.05 +0.05 ) MSun | ||
| Age | 6.0 (± 2.0) Gyr | |
|
| Effective temperature | 5757.0 (± 85.0) K | |
|
| Radius | 1.11 ( -0.09 +0.15 ) RSun | |
|
| Metallicity [Fe/H] | 0.21 (± 0.09) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 19:44:00.9 | ||
| Dec2000 | +44:16:39 | ||
| Alternate Names | 2MASS J19440088+4416392, KIC 8311864, KOI-7016, WISE J194400.89+441639.2 | ||
| Planetary system | 1 planet |
Observability Predictor 
Remarks
2 Apr 2018: Kepler-452 b is still to be confirmed (Mullally et al. 2018)Related publications
A New Definition of Exoplanet Habitability: Introducing the Photosynthetic Habitable Zone
2023
HALL C., STANCIL P., TERRY J. & ELLISON C.
ApJ. Letters, 948, L26
paper arxiv
Continuous Habitable Zones: Using Bayesian Methods to Prioritize Characterization of Potentially Habitable Worlds
2022
WARE A., YOUNG P., TRUITT A. & SPACEK A.
ApJ, 929, 143
paper arxiv
Habitability of exoplanet waterworlds
2018
KITE E. & FORD E.
ApJ, 864, 75
arxiv
paper
Kepler's Earth-like Planets Should Not Be Confirmed Without Independent Detection: The Case of Kepler-452b
2018
MULLALY F., THOMPSON S., COUGHLIN J., BURKE Ch. & ROWE J.
Astron J., 155, 210
arxiv
article
Probabilistic Forecasting of the Masses and Radii of Other Worlds
2017
CHEN J. & KIPPING D.
ApJ, 834, 17
paper arxiv
ADS
Climate and Habitability of Kepler 452b Simulated with a Fully Coupled Atmosphere–Ocean General Circulation Model
2017
HU Y., WANG Y., LIU Y. & YANG J.
ApJ Lett, L6
paper
Quantitative estimates of the surface habitability of Kepler-452b
2017
SILVA L., VIADILO G., MURANTE G. & PROVENZALE A.
MNRAS, 470, 2270
paper arxiv
How alien can alien worlds be?
2017
ADIBEKYAN F., FIGUEIRA P. & SANTOS N.
in EWASS Special Session 4 (2017): Star-planet interactions
arxiv
Discovery and Validation of Kepler-452b: A 1.6 R⨁ Super Earth Exoplanet in the Habitable Zone of a G2 Star
2015
JENKINS J., TWICKEN J., BATALHA N., CALDWELL D., COCHRAN W. et al.
Astron. J., 150, 56
paper
Discovery and Validation of Kepler-452b: A 1.6 R ⨁ Super Earth Exoplanet in the Habitable Zone of a G2 Star
2015
JENKINS J. M., TWICKEN J. D., BATALHA N. M., CALDWELL D. A., COCHRAN W. D. et al.
The Astronomical Journal, 150, 56
ADS
