Planet Kepler-29 c

Detailed information about planet Kepler-29 c and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

Kepler-29 c

Planet Status

Confirmed

Discovered in

2011

Update

2021-02-05

Mass

0.01416 (\begin{matrix} + 0.00346 \\ - 0.00346 \end{matrix})

M_J 1 publication

Diffuser-assisted Infrared Transit Photometry for Four Dynamically Interacting Kepler Systems

Mass*sin(i)

—

Semi-Major Axis

0.11 AU 1 publication

Transit Timing Observations from Kepler: IV. Confirmation of 4 Multiple Planet Systems by Simple Physical Models

Orbital Period

13.28613 (\begin{matrix} + 0.00026 \\ - 0.00021 \end{matrix})

day 1 publication

Diffuser-assisted Infrared Transit Photometry for Four Dynamically Interacting Kepler Systems

Eccentricity

— 1 publication

Diffuser-assisted Infrared Transit Photometry for Four Dynamically Interacting Kepler Systems

ω

—

T_peri

—

Radius

0.209 (\begin{matrix} + 0.011 \\ - 0.01 \end{matrix})

R_J 1 publication

Diffuser-assisted Infrared Transit Photometry for Four Dynamically Interacting Kepler Systems

Inclination

—

Detection Method

Primary Transit

Mass Meas. Method

TTV

Radius Meas. Method

Primary Transit

Primary transit

2454978.471 (\pm 0.016)

JD 1 publication

Transit Timing Observations from Kepler: IV. Confirmation of 4 Multiple Planet Systems by Simple Physical Models

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

2MASS J19532359+4729284 c, K00738.02, KIC 10358759 c, KOI-738 c, KOI-738.02, WISE J195323.60+472928.3  c

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

28 Jan 2012: The upper mass limit is inferred from tranist time variations, simple planet models and dynamical stability (Fabrycky et al; 2012)

No link

Star

Name

Kepler-29

Distance

851.9 (\begin{matrix} + 27.37 \\ - 27.37 \end{matrix})

Spectral type

—

Apparent magnitude V

15.5

Mass

0.76 (\begin{matrix} + 0.02 \\ - 0.03 \end{matrix})

M_Sun

Age

—

Effective temperature

5378.0 (\begin{matrix} + 60.0 \\ - 60.0 \end{matrix})

Radius

0.73 (\begin{matrix} + 0.03 \\ - 0.03 \end{matrix})

R_Sun

Metallicity [Fe/H]

-0.44 (\begin{matrix} + 0.04 \\ - 0.04 \end{matrix})

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:53:23.6

Dec₂₀₀₀

+47:29:28.4

Alternate Names

2MASS J19532359+4729284, KIC 10358759, KOI-738, WISE J195323.60+472928.3

Alias KOI 738
Alias KIC 10358759
Alias 2MASS 19532359+4729284

No link

Simbad
Most recent references (ADS)

Planet Kepler-29 c

Planet

Basic informations 28 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks Some remarks

Other web pages No page

Star

Basic informations 13 parameters

Planetary system 2 planets

Remarks Some remarks

Other web pages No page

More data 2 references

Planet Kepler-29 c

Planet

Basic informations 28 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks Some remarks

Other web pages No page

Star

Basic informations 13 parameters

Planetary system 2 planets

Remarks Some remarks

Other web pages No page

More data 2 references

Related publications

Diffuser-assisted Infrared Transit Photometry for Four Dynamically Interacting Kepler Systems

The Reversibility Error Method (REM): a new, dynamical fast indicator for planetary dynamics

The origin and 9:7 MMR dynamics of the Kepler-29 system

Secure Mass Measurements from transit timing: 10 Kepler Exoplanets between 3 and 8 Earth Masses with Diverse Densities and Incident Fluxes

Evolutionary outcomes for pairs of planets undergoing orbital migration and circularization: second order resonances and observed period ratios in Kepler's planetary systems

Transit Timing Observations from Kepler: IV. Confirmation of 4 Multiple Planet Systems by Simple Physical Models

The Exoplanet Handbook