Planet Kepler-89 b
| Name | Kepler-89 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2012 | ||
| Mass | 0.033 ( -0.014 +0.014 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.05 AU | |
|
| Orbital Period | 3.7432451 (± 3.1e-05) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 0.153 ( -0.014 +0.014 ) RJ | |
+ |
| Inclination | — | ||
| Update | 2013-11-05 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| Primary transit | 2454965.74047 (± 0.00019) JD | |
|
| 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-89| Name | Kepler-89 | ||
| Distance | — | ||
| Spectral type | |||
| Apparent magnitude V | 12.4 | ||
| Mass | 1.25 (± 0.04) MSun | |
|
| Age | 3.9 (± 0.3) Gyr | |
|
| Effective temperature | 6116.0 (± 30.0) K | |
|
| Radius | 1.656 RSun | ||
| Metallicity [Fe/H] | -0.01 (± 0.04) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 19:49:20.0 | ||
| Dec2000 | +41:53:28 | ||
| Alternate Names | KOI-94 | ||
| Planetary system | 4 planets |
Observability Predictor 
Remarks
Alias KOI-94.04.The candidate KOI-94.04 is labelled here as KOI-94b according to the convention that increasing periods label planets b, c, d etc.
21 Sep 2012: The KOI-94 system is likely a planetary system given the measured Rossiter-McLaughlin effect for the candidate KOI-94 d (alias KOI-94.01) and the probable planet-planet eclipse for KOI-94 d and KOI-94 e (Hirano et al. 2012).
Related publications
The Planetary Mass-Radius Relation and its Dependence on Orbital Period as Measured by Transit Timing Variations and Radial Velocities
2017
MILLS S. & MAZEH T.
ApJ. Letters, 839, L8
paper arxiv ADS
Warm Jupiters are less lonely than hot Jupiters: close neighbours
2016
HUANG Ch., WU Y. & TRIAUD A.
ApJ, 825, 98
paper arxiv ADS
Asteroseismology of Exoplanet Host Stars
2015
HUBER D.
in "Focus Meeting 17 - IAU General Assembly in Hawaii, August 2015"
arxiv
The Mass-Radius Relation Between 65 Exoplanets Smaller than 4 Earth Radii
2014
WEISS L. & MARCY G.
ApJ Letters, 783, L6
paper arxiv ADS
A Discovery of a Candidate Companion to a Transiting System KOI-94: A Direct Imaging Study for a Possibility of a False Positive
2013
TAKABAYASHI Y., NARITA N., HIRANO T., KUZUHARA M., TAMURA M. & 48 additional authors
ApJ Letters, submitted
arxiv
Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse
2013
MASUDA K., HIRANO T., TAUYA A., NAGASAWA M. & SUTO Y.
ApJ, 778, 185
paper arxiv
Planet-Planet Eclipse and the Rossiter-McLaughlin Effect of a Multiple Transiting System: Joint Analysis of the Subaru Spectroscopy and the Kepler Photometry
2012
HIRANO T., NARITA N., SATO B., TAKAHASHI Y., MASUDA K. & 4 additional athors
ApJ Letters, 759, L36
paper arxiv
