Planet Kepler-130 Ac

Detailed information about planet Kepler-130 Ac and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

Kepler-130 Ac

Planet Status

Confirmed

Discovered in

2014

Publication Status

—

Update

2024-08-03

Mass

—

Mass*sin(i)

—

Semi-Major Axis

0.1739 AU 2 publications

The Kepler Giant Planet Search. I. A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory
Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates

Orbital Period

27.50868 (\begin{matrix} + 6e-05 \\ - 7e-05 \end{matrix})

day 1 publication

Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates

Eccentricity

0.0 2 publications

The Kepler Giant Planet Search. I. A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory
Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates

Angular distance

—

ω

0.0 (\begin{matrix} + 10.89 \\ - 0.0 \end{matrix})

deg

T_peri

—

Radius

0.25667 (\pm 0.00642)

R_J 2 publications

The Kepler Giant Planet Search. I. A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory
Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates

Inclination

89.34 (\begin{matrix} + 0.66 \\ - 0.31 \end{matrix})

deg 1 publication

Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates

Detection Method

Primary Transit

Mass Meas. Method

—

Radius Meas. Method

Primary Transit

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

0.38 (\begin{matrix} + 0.14 \\ - 0.38 \end{matrix})

1 publication

Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

683.0 (\begin{matrix} + 29.0 \\ - 29.0 \end{matrix})

K 1 publication

Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

Kepler-130 c, KOI-282 c, KOI-282.01, K00282.01, KIC 5088536 c, 2MASS J19134816+4014431 c, WISE J191348.14+401442.7 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-130 A

Distance

316.663 (\begin{matrix} + 2.353 \\ - 2.319 \end{matrix})

pc 1 publication

The Revised TESS Input Catalog and Candidate Target List

Spectral type

G0V

Apparent magnitude V

—

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

1.091 (\begin{matrix} + 0.167 \\ - 0.113 \end{matrix})

M_Sun 1 publication

The Revised TESS Input Catalog and Candidate Target List

Age

5.89 (\begin{matrix} + 0.98 \\ - 0.9 \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

5958.0 (\begin{matrix} + 116.6 \\ - 97.52 \end{matrix})

K 1 publication

The Revised TESS Input Catalog and Candidate Target List

Radius

1.179 (\begin{matrix} + 0.062 \\ - 0.047 \end{matrix})

R_Sun 1 publication

The Revised TESS Input Catalog and Candidate Target List

Metallicity [Fe/H]

-0.199 (\pm 0.005)

1 publication

The Revised TESS Input Catalog and Candidate Target List

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:13:48.2

Dec₂₀₀₀

+40:14:43.1

Alternate Names

WISE J191348.14+401442.7, Kepler-130, KOI-282, KIC 5088536, 2MASS J19134816+4014431

Michel & Mugrauer (2024): An M dwarf companion star lies 1326 AUs away.

No link

Simbad
Most recent references (ADS)

Planet Kepler-130 Ac

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-130 Ac

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

A high stellar multiplicity rate amongst TESS planet candidates in the Neptunian desert using Gaia DR3 astrometry

The Kepler Giant Planet Search. I. A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory

Gaia Search for (sub)stellar Companions of Exoplanet Hosts

TESS Observations of Kepler Systems with Transit Timing Variations

Testing exoplanet evaporation with multi-transiting systems

The Revised TESS Input Catalog and Candidate Target List

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

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

Validation of Kepler's Multiple Planet Candidates. III: Light Curve Analysis & Announcement of Hundreds of New Multi-planet Systems

Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation due to Stellar Companions within 20 AU and Validation of Four Planets from the Kepler Multiple Planet Candidates