Planet Kepler-114 c

Detailed information about planet Kepler-114 c and its parameters.

Planet parameters Publications Observability Predictor Exo3D

Planet

Name

Kepler-114 c

Planet Status

Confirmed

Discovered in

2013

Publication Status

—

Update

2021-02-05

Mass

0.009 (\begin{matrix} + 0.002 \\ - 0.002 \end{matrix})

M_J 1 publication

Transit Timing Variation of Near-resonance Planetary Pairs. II. Confirmation of 30 Planets in 15 Multiple-planet Systems

Mass*sin(i)

—

Semi-Major Axis

0.07 AU 1 publication

Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data

Orbital Period

8.041 day 2 publications

Transit Timing Variation of Near-resonance Planetary Pairs. II. Confirmation of 30 Planets in 15 Multiple-planet Systems
Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data

Eccentricity

—

Angular distance

—

ω

—

T_peri

—

Radius

0.143 (\begin{matrix} + 0.016 \\ - 0.016 \end{matrix})

R_J 1 publication

Transit Timing Variation of Near-resonance Planetary Pairs. II. Confirmation of 30 Planets in 15 Multiple-planet Systems

Inclination

88.24 deg 1 publication

Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data

Detection Method

Primary Transit

Mass Meas. Method

TTV

Radius Meas. Method

—

Primary transit

2454976.039 (\pm 0.0015)

JD 1 publication

Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

623.0 K 1 publication

Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

2MASS J19362914+4820582 c, K00156.01, KIC 10925104 c, KOI-156 c, KOI-156.01, WISE J193629.11+482058.9 c

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-114

Distance

261.49 (\begin{matrix} + 1.32 \\ - 1.32 \end{matrix})

Spectral type

M0 V

Apparent magnitude V

13.7

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

0.71 (\begin{matrix} + 0.15 \\ - 0.2 \end{matrix})

M_Sun 1 publication

Transit Timing Variation of Near-resonance Planetary Pairs. II. Confirmation of 30 Planets in 15 Multiple-planet Systems

Age

—

Effective temperature

4605.0 (\begin{matrix} + 100.0 \\ - 100.0 \end{matrix})

Radius

0.67 (\begin{matrix} + 0.04 \\ - 0.04 \end{matrix})

R_Sun

Metallicity [Fe/H]

-0.003

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:36:29.1

Dec₂₀₀₀

+48:20:58.3

Alternate Names

2MASS J19362914+4820582, KIC 10925104, KOI-156, WISE J193629.11+482058.9

Alias 2MASS 19362914+4820582

No link

Simbad
Most recent references (ADS)

Planet Kepler-114 c

Planet

Basic informations 30 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-114 c

Planet

Basic informations 30 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

The Orbital Eccentricity Distribution of Planets Orbiting M dwarfs

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

The role of dissipative evolution for three-planet, near-resonant extrasolar systems

Transit Timing Variation of Near-resonance Planetary Pairs. II. Confirmation of 30 Planets in 15 Multiple-planet Systems

Densities and Eccentricities of 139 Kepler Planets from Transit Time Variations

Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data