Planet Kepler-60 d

Detailed information about planet Kepler-60 d and its parameters.

Planet parameters Publications Observability Predictor Exo3D

Planet

Name

Kepler-60 d

Planet Status

Confirmed

Discovered in

2012

Publication Status

—

Update

2021-02-05

Mass

0.01309 (\begin{matrix} + 0.00264 \\ - 0.00236 \end{matrix})

M_J 1 publication

Secure Mass Measurements from Transit Timing: 10 Kepler Exoplanets between 3 and 8 M_⊕ with Diverse Densities and Incident Fluxes

Mass*sin(i)

—

Semi-Major Axis

0.10548 AU 1 publication

The Laplace resonance in the Kepler-60 system

Orbital Period

11.8981 (\begin{matrix} + 0.0002 \\ - 0.0002 \end{matrix})

day 1 publication

Secure Mass Measurements from Transit Timing: 10 Kepler Exoplanets between 3 and 8 M_⊕ with Diverse Densities and Incident Fluxes

Eccentricity

—

Angular distance

—

ω

—

T_peri

—

Radius

0.178 (\begin{matrix} + 0.014 \\ - 0.014 \end{matrix})

R_J 2 publications

Secure Mass Measurements from transit timing: 10 Kepler Exoplanets between 3 and 8 Earth Masses with Diverse Densities and Incident Fluxes
Transit Timing Observations from Kepler: VII. Confirmation of 27 planets in 13 multiplanet systems via Transit Timing Variations and orbital stability

Inclination

—

Detection Method

Primary Transit

Mass Meas. Method

TTV

Radius Meas. Method

Primary Transit

Primary transit

2454966.24626 (\pm 0.0063)

JD 1 publication

Transit Timing Observations from Kepler: VII. Confirmation of 27 planets in 13 multiplanet systems via Transit Timing Variations and orbital stability

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 J19155069+4215540 d, K02086.03, KIC 6768394 d, KOI-2086 d, KOI-2086.03, WISE J191550.69+421554.0 d

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-60

Distance

1056.17 (\begin{matrix} + 20.64 \\ - 20.64 \end{matrix})

Spectral type

—

Apparent magnitude V

14.5

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

1.04 (\begin{matrix} + 0.08 \\ - 0.08 \end{matrix})

M_Sun

Age

—

Effective temperature

5905.0 (\begin{matrix} + 144.0 \\ - 144.0 \end{matrix})

Radius

1.26 (\begin{matrix} + 0.09 \\ - 0.09 \end{matrix})

R_Sun

Metallicity [Fe/H]

-0.09 (\begin{matrix} + 0.1 \\ - 0.1 \end{matrix})

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:15:50.7

Dec₂₀₀₀

+42:15:54.0

Alternate Names

2MASS J19155069+4215540, KIC 6768394, KOI-2086, WISE J191550.69+421554.0

Alias KIC 6768394
Alias 2MASS 19155069+4215540

No link

Simbad
Most recent references (ADS)

Planet Kepler-60 d

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-60 d

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

GSF-22 -Resonant Chains on the Scale Manifold: From Kepler Projection to Corridor Capture in Exoplanet Systems

Mean motion resonance capture in the context of type I migration

Architectures of Compact Super-Earth Systems Shaped by Instabilities

Is the orbital distribution of multiplanet systems influenced by pure three-planet resonances?

Resonant Chains of Exoplanets: Libration Centers for Three-body Angles

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

Application of the Shannon entropy in the planar (non-restricted) four-body problem: the long-term stability of the Kepler-60 exoplanetary system

Caught in the Act: Core-powered Mass-loss Predictions for Observing Atmospheric Escape

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

The Laplace resonance in the Kepler-60 system

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

Secure Mass Measurements from Transit Timing: 10 Kepler Exoplanets between 3 and 8 M⊕ with Diverse Densities and Incident Fluxes

Transit Timing Observations from Kepler: VII. Confirmation of 27 planets in 13 multiplanet systems via Transit Timing Variations and orbital stability

Secure Mass Measurements from Transit Timing: 10 Kepler Exoplanets between 3 and 8 M_⊕ with Diverse Densities and Incident Fluxes