Planet Kepler-1632 b

Detailed information about planet Kepler-1632 b and its parameters.

Planet parameters Publications Observability Predictor Exo3D

Planet

Name

Kepler-1632 b

Mass

—

Mass*sin(i)

—

Semi-Major Axis

0.6762 AU 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Orbital Period

224.150923 (\pm 0.001794)

day 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Eccentricity

0.0 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

ω

—

T_peri

—

Radius

0.215 (\begin{matrix} + 0.0428 \\ - 0.0633 \end{matrix})

R_J 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Inclination

89.99 deg 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

0.019 (\begin{matrix} + 0.404 \\ - 0.019 \end{matrix})

1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

369.0 K 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Measured temperature

—

Hottest point longitude

—

Surface gravity log(g/g_H)

—

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

Thompson et al. (2018) provide a different orbital solution with a shorter orbital period (P = 224.15 d), smaller separation (a = 0.676 AUs) but nearly equal radius (r = 2.41 R_E) in respect with original solution by Morton et al. (2016) (P = 448.3 d).

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