Planet Kepler-456 B

Detailed information about planet Kepler-456 B and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

Kepler-456 B

Planet Status

Retracted

Discovered in

2015

Publication Status

Published in a refereed paper

Update

2024-06-09

Mass

—

Mass*sin(i)

313.0 (\begin{matrix} + 44.0 \\ - 68.0 \end{matrix})

M_J

Semi-Major Axis

—

Orbital Period

3378.0 (\pm 10.0)

day 1 publication

Planet Hunters. VIII. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data

Eccentricity

—

Angular distance

—

ω

—

T_peri

—

Radius

0.589 (\begin{matrix} + 2.346 \\ - 0.37 \end{matrix})

R_J 1 publication

Planet Hunters. VIII. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data

Inclination

89.799 (\begin{matrix} + 0.09 \\ - 0.12 \end{matrix})

deg 1 publication

Planet Hunters. VIII. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data

Detection Method

Primary Transit

Mass Meas. Method

—

Radius Meas. Method

Primary Transit

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

3310.0 (\begin{matrix} + 380.0 \\ - 600.0 \end{matrix})

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

—

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

KIC 5951458 b, 2MASS J19155797+4113229 b, WISE J191557.98+411323.0 b

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

10 Jul 2020:
According to Dalba et al. (2020), "For KIC 5951458, we detect a long-term RV trend that suggests the existence of a stellar companion with an orbital period greater than a few thousand days. We also detect an additional signal in the RVs that is possibly caused by a planetary or brown dwarf companion with mass in the range 0.6 - 82 M_J and orbital period below a few thousand days. Curiously, from just the data on hand, it is not possible to determine which object caused the single "transit" event. "
Wang et al. (2015) : confidence level of 0.998

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