Planet Kepler-80 g

Detailed information about planet Kepler-80 g and its parameters.

Planet parameters Publications Observability Predictor Exo3D

Planet

Name

Kepler-80 g

Planet Status

Confirmed

Discovered in

2017

Publication Status

—

Update

2021-02-05

Mass

—

Mass*sin(i)

—

Semi-Major Axis

0.14 AU 1 publication

Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90

Orbital Period

14.64558 (\pm 0.00012)

day 1 publication

Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90

Eccentricity

—

Angular distance

—

ω

—

T_peri

—

Radius

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

R_J 1 publication

Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90

Inclination

89.35 (\begin{matrix} + 0.98 \\ - 0.47 \end{matrix})

deg 1 publication

Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90

Detection Method

Primary Transit

Mass Meas. Method

—

Radius Meas. Method

Primary Transit

Primary transit

2455658.0073 (\pm 0.0037)

Secondary transit

—

λ

—

Impact Parameter b

0.52 (\pm 0.28)

1 publication

Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

418.0 (\pm 36.0)

K 1 publication

Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

2MASS J19442701+3958436 g, KIC 4852528 g, KOI-500 g, WISE J194427.01+395843.5 g

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-80

Distance

357.0 pc

Spectral type

Apparent magnitude V

15.0

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

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

M_Sun

Age

2.0 (\begin{matrix} + 1.0 \\ - -1.0 \end{matrix})

Gyr

Effective temperature

4540.0 (\begin{matrix} + 100.0 \\ - 100.0 \end{matrix})

Radius

0.68 (\begin{matrix} + 0.02 \\ - 0.02 \end{matrix})

R_Sun

Metallicity [Fe/H]

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

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:44:27.0

Dec₂₀₀₀

+39:58:43.6

Alternate Names

KOI-500, 2MASS J19442701+3958436, KIC 4852528, WISE J194427.01+395843.5

Alias KIC 4852528
Alias 2MASS 19442701+3958436

No link

Simbad
Most recent references (ADS)

Planet Kepler-80 g

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 6 planets

Remarks Some remarks

Other web pages No page

More data 2 references

Planet Kepler-80 g

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 6 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

Resonant Chains and the Convergent Migration of Planets in Protoplanetary Disks

Tidal interactions' shape period ratios in planetary systems with three-body resonant chains

Mean motion resonance capture in the context of type I migration

exoMMR: a New Python Package to Confirm and Characterize Mean Motion Resonances

Kepler-80 Revisited: Assessing the Participation of a Newly Discovered Planet in the Resonant Chain

Architectures of Compact Super-Earth Systems Shaped by Instabilities

A Criterion for the Stability of Planets in Chains of Resonances

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

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

A Five-Planet Resonant Chain: Reevaluation of the Kepler-80 System

Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90