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

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Conditions for Convergent Migration of N-Planet Systems

Architectures of Compact Super-Earth Systems Shaped by Instabilities

A Criterion for the Stability of Planets in Chains of Resonances

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

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

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

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The nature and origins of sub-Neptune size planets

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

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