Planet Kepler-1063 Ab

Detailed information about planet Kepler-1063 Ab and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

Kepler-1063 Ab

Planet Status

Confirmed

Discovered in

2016

Publication Status

Announced on a website

Update

2025-02-11

Mass

—

Mass*sin(i)

—

Semi-Major Axis

0.1176 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

14.07969236 (\pm 3.103e-05)

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

Angular distance

—

ω

—

T_peri

—

Radius

0.1856 (\begin{matrix} + 0.0321 \\ - 0.0491 \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

89.53 deg 1 publication

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

Detection Method

Primary Transit

Mass Meas. Method

—

Radius Meas. Method

Primary Transit

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

0.544 (\begin{matrix} + 0.396 \\ - 0.334 \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

931.0 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

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

WISE J192206.41+380834.5 b, Kepler-1063 b, KOI-2032 b, KOI-2032.01, K02032.01, KIC 2985767 b, 2MASS J19220642+3808347 b

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

Star

Name

Kepler-1063 A

Distance

365.0 pc 1 publication

False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives

Spectral type

G0V

Apparent magnitude V

13.04

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

1.09 (\begin{matrix} + 0.11 \\ - 0.07 \end{matrix})

M_Sun 1 publication

False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives

Age

3.39 (\begin{matrix} + 2.2 \\ - -1.68 \end{matrix})

Gyr 1 publication

False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives

Effective temperature

5945.0 (\begin{matrix} + 188.84 \\ - 155.38 \end{matrix})

K 1 publication

False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives

Radius

1.14 (\begin{matrix} + 0.3 \\ - 0.14 \end{matrix})

R_Sun 1 publication

False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives

Metallicity [Fe/H]

0.09 (\begin{matrix} + 0.146 \\ - 0.133 \end{matrix})

1 publication

False Positive Probabilities for all Kepler Objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:22:06.4

Dec₂₀₀₀

+38:08:34.7

Alternate Names

WISE J192206.41+380834.5, Kepler-1063, KOI-2032, KIC 2985767, 2MASS J19220642+3808347

Furlan et al. (2017) report three visual companions 0.063, 1.085 and 1.147 arcseconds away (23, 396 and 418 AUs at 365 pc). Michel & Mugrauer (2024) confirm the outermost companion star, a Solar-type G dwarf, providing a separation of 576 AUs. The candidate innermost companion, if it too gravitationally bound, is likely similar.

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