Planet Kepler-102 d

Detailed information about planet Kepler-102 d and its parameters.

Planet parameters Publications Observability Predictor Exo3D

Planet

Name

Kepler-102 d

Mass

0.012 (\begin{matrix} + 0.006 \\ - 0.006 \end{matrix})

M_J 1 publication

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

Mass*sin(i)

—

Semi-Major Axis

—

Orbital Period

10.3117 day 1 publication

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

Eccentricity

—

ω

—

T_peri

2454972.9875 (\pm 0.0032)

Radius

0.105 (\begin{matrix} + 0.004 \\ - 0.004 \end{matrix})

R_J 1 publication

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

Inclination

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

0.22 (\pm 0.05)

1 publication

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

Time V_r=0

—

Velocity Semiamplitude K

1.37 (\pm 0.6)

m/s 1 publication

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

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

The KOI number of the planets of this system, ordered following Kepler photometric capability, are not in order of decreasing orbital period (the criterion followed for giving Kepler letters).

No link

Star

Name

Kepler-102

Distance

108.13 (\begin{matrix} + 0.22 \\ - 0.22 \end{matrix})

Spectral type

—

Apparent magnitude V

11.492

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

0.81 (\begin{matrix} + 0.04 \\ - 0.09 \end{matrix})

M_Sun 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

Age

1.41 Gyr 1 publication

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

Effective temperature

4909.0 (\begin{matrix} + 41.0 \\ - 41.0 \end{matrix})

Radius

0.76 (\pm 0.07)

R_Sun 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

Metallicity [Fe/H]

0.18 (\begin{matrix} + 0.42 \\ - 0.47 \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

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

18:45:55.9

Dec₂₀₀₀

+47:12:28.9

Alternate Names

KOI-82, KIC 10187017, 2MASS J18455585+4712289, WISE J184555.80+471228.4

No remarks

No link

Simbad
Most recent references (ADS)

Planet Kepler-102 d

Planet

Basic informations 20 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks Some remarks

Other web pages No page

Star

Basic informations 17 parameters

Planetary system 5 planets

Remarks No remark

Other web pages No page

More data 2 references

Planet Kepler-102 d

Planet

Basic informations 20 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks Some remarks

Other web pages No page

Star

Basic informations 17 parameters

Planetary system 5 planets

Remarks No remark

Other web pages No page

More data 2 references

Related publications

Kepler-102: Masses and Compositions for a Super-Earth and Sub-Neptune Orbiting an Active Star

TESS Observations of Kepler Systems with Transit Timing Variations

Dynamical instabilities in systems of multiple short-period planets are likely driven by secular chaos: a case study of Kepler-102

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

The Mass-Radius Relation Between 65 Exoplanets Smaller than 4 Earth Radii

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

Densities and Eccentricities of 139 Kepler Planets from Transit Time Variations