Planet Kepler-223 d

Detailed information about planet Kepler-223 d and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

Kepler-223 d

Planet Status

Confirmed

Discovered in

2014

Update

2021-02-05

Mass

0.02517 (\begin{matrix} + 0.00472 \\ - 0.00409 \end{matrix})

M_J 1 publication

A resonant chain of four transiting, sub-Neptune planets

Mass*sin(i)

—

Semi-Major Axis

0.116

AU 1 publication

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

Orbital Period

14.78869 (\begin{matrix} + 0.0003 \\ - 0.00027 \end{matrix})

day 1 publication

A resonant chain of four transiting, sub-Neptune planets

Eccentricity

0.037 (\begin{matrix} + 0.018 \\ - 0.017 \end{matrix})

1 publication

A resonant chain of four transiting, sub-Neptune planets

ω

—

T_peri

—

Radius

0.467 (\begin{matrix} + 0.023 \\ - 0.04 \end{matrix})

R_J 1 publication

A resonant chain of four transiting, sub-Neptune planets

Inclination

87.94 (\begin{matrix} + 0.32 \\ - 0.26 \end{matrix})

deg 1 publication

A resonant chain of four transiting, sub-Neptune planets

Detection Method

Primary Transit

Mass Meas. Method

—

Radius Meas. Method

—

Primary transit

—

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 J19531640+4716461 d, K00730.01, KIC 10227020 d, KOI-730 d, KOI-730.01, WISE J195316.39+471645.8  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-223

Distance

1960.49 (\begin{matrix} + 120.21 \\ - 120.21 \end{matrix})

Spectral type

—

Apparent magnitude V

—

Mass

1.12 (\begin{matrix} + 0.09 \\ - 0.07 \end{matrix})

M_Sun

Age

— 1 publication

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

Effective temperature

5829.0 (\pm 200.0)

K 1 publication

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

Radius

1.72 (\begin{matrix} + 0.07 \\ - 0.14 \end{matrix})

R_Sun

Metallicity [Fe/H]

-0.211

1 publication

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

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:53:16.4

Dec₂₀₀₀

+47:16:46.2

Alternate Names

2MASS J19531640+4716461, KIC 10227020, KOI-730, WISE J195316.39+471645.8

No remarks

No link

Simbad
Most recent references (ADS)

Planet Kepler-223 d

Planet

Basic informations 28 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks No remark

Other web pages No page

Star

Basic informations 13 parameters

Planetary system 4 planets

Remarks No remark

Other web pages No page

More data 2 references

Planet Kepler-223 d

Planet

Basic informations 28 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks No remark

Other web pages No page

Star

Basic informations 13 parameters

Planetary system 4 planets

Remarks No remark

Other web pages No page

More data 2 references

Related publications

Resonant Chains and the Convergent Migration of Planets in Protoplanetary Disks

Spin Dynamics of Planets in Resonant Chains

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes

Mean motion resonance capture in the context of type I migration

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

Conditions for Convergent Migration of N-Planet Systems

A Criterion for the Stability of Planets in Chains of Resonances

Architectures of Compact Super-Earth Systems Shaped by Instabilities

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

Kepler-223 resonance holds information on turbulence during the gas disk phase

Sculpting the sub-Saturn Occurrence Rate via Atmospheric Mass Loss

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

Chains of Planets in Mean Motion Resonances Arising from Oligarchic Growth

Deflating Super-Puffs: Impact of Photochemical Hazes on the Observed Mass-Radius Relationship of Low Mass Planets

The nature and origins of sub-Neptune size planets

Analytical model of multi-planetary resonant chains and constraints on migration scenarios

A resonant chain of four transiting, sub-Neptune planets

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

On the structural law of exoplanetary systems