Planet Kepler-23 b

Detailed information about planet Kepler-23 b and its parameters.

Planet parameters Publications Observability Predictor Exo3D

Planet

Name

Kepler-23 b

Mass

0.8 (\begin{matrix} + 0.0 \\ - 0.75 \end{matrix})

M_J 1 publication

Transit Timing Observations from Kepler: II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis

Mass*sin(i)

—

Semi-Major Axis

0.075 AU 1 publication

Transit Timing Observations from Kepler: II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis

Orbital Period

7.1073 day 1 publication

Transit Timing Observations from Kepler: II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis

Eccentricity

0.06 (\begin{matrix} + 0.26 \\ - 0.06 \end{matrix})

1 publication

Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities

ω

—

T_peri

—

Radius

0.17

R_J 1 publication

Transit Timing Observations from Kepler: II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis

Inclination

—

Primary transit

2454971.3022 JD 1 publication

Transit Timing Observations from Kepler: II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

—

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

No remarks

No link

Star

Name

Kepler-23

Distance

856.34 (\begin{matrix} + 11.79 \\ - 11.79 \end{matrix})

Spectral type

—

Apparent magnitude V

14.0

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

1.11

M_Sun 1 publication

Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations

Age

—

Effective temperature

5828.0 (\begin{matrix} + 100.0 \\ - 100.0 \end{matrix})

Radius

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

R_Sun

Metallicity [Fe/H]

—

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:36:52.5

Dec₂₀₀₀

+49:28:45.2

Alternate Names

2MASS J19365254+4928452, GSC 03564-01806, KIC 11512246, KOI-168, WISE J193652.53+492845.3

View all in the catalogue :

AMD-Stability Calculator for the System :

Exo3D (1 star, 3 simulable planets)

Alias KOI-168
Alias KIC 11512246
Alias 2MASS 19365254+4928452

No link

Simbad
Most recent references (ADS)

Planet Kepler-23 b

Planet

Basic informations 20 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks No remark

Other web pages No page

Star

Basic informations 17 parameters

Planetary system 3 planets

Remarks Some remarks

Other web pages No page

More data 2 references

Planet Kepler-23 b

Planet

Basic informations 20 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks No remark

Other web pages No page

Star

Basic informations 17 parameters

Planetary system 3 planets

Remarks Some remarks

Other web pages No page

More data 2 references

Related publications

Stability Constrained Characterization of Multiplanet Systems

How Close are Compact Multi-Planet Systems to the Stability Limit?

Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities

The destruction of inner planetary systems during high-eccentricity migration of gas giants

Densities and Eccentricities of 139 Kepler Planets from Transit Time Variations

A Correlation Between the Eclipse Depths of Kepler Gas Giant Candidates and the Metallicities of their Parent Stars

Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations

Transit Timing Observations from Kepler: II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis

The Exoplanet Handbook