Planet KOI-1894 b

Detailed information about planet KOI-1894 b and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

KOI-1894 b

Planet Status

Candidate

Discovered in

2015

Publication Status

Published in a refereed paper

Update

2021-10-05

Mass

0.1 (\begin{matrix} + 0.08 \\ - 0.07 \end{matrix})

M_J

Mass*sin(i)

0.1 (\begin{matrix} + 0.07 \\ - 0.07 \end{matrix})

M_J 1 publication

Precise Radial Velocity Measurements for Kepler Giants Hosting Planetary Candidates: Kepler-91 and KOI-1894

Semi-Major Axis

—

Orbital Period

5.2880157 (\pm 4.47e-05)

day

Eccentricity

0.186 (\begin{matrix} + 0.097 \\ - 0.15 \end{matrix})

1 publication

Precise Radial Velocity Measurements for Kepler Giants Hosting Planetary Candidates: Kepler-91 and KOI-1894

Angular distance

—

ω

65.0 (\begin{matrix} + 70.0 \\ - 74.0 \end{matrix})

deg 1 publication

Precise Radial Velocity Measurements for Kepler Giants Hosting Planetary Candidates: Kepler-91 and KOI-1894

T_peri

—

Radius

0.66 (\begin{matrix} + 0.05 \\ - 0.05 \end{matrix})

R_J 1 publication

Precise Radial Velocity Measurements for Kepler Giants Hosting Planetary Candidates: Kepler-91 and KOI-1894

Inclination

76.2 (\begin{matrix} + 10.0 \\ - 4.0 \end{matrix})

deg 1 publication

Precise Radial Velocity Measurements for Kepler Giants Hosting Planetary Candidates: Kepler-91 and KOI-1894

Detection Method

Other

Mass Meas. Method

Radial Velocity

Radius Meas. Method

Primary Transit

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

—

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

—

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

23 Jan 2015: The planet is provisionally classified as "to be confirmed" since " the radial velocities and light curves with 2–3σ confidence level which could be explained as a reflex motion and ellipsoidal variation of the star." (Sato et al. 2015).

No link