Planet KOI-332.02

Detailed information about planet KOI-332.02 and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

KOI-332.02

Planet Status

Candidate

Discovered in

2017

Publication Status

Announced on a website

Update

2025-03-01

Mass

—

Mass*sin(i)

—

Semi-Major Axis

0.0745 AU 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Orbital Period

6.86674226 (\pm 9.996e-05)

day 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Eccentricity

0.0 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Angular distance

—

ω

—

T_peri

—

Radius

0.0705 (\begin{matrix} + 0.0107 \\ - 0.0054 \end{matrix})

R_J 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Inclination

87.98 deg 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Detection Method

Primary Transit

Mass Meas. Method

—

Radius Meas. Method

Primary Transit

Primary transit

2454968.347 (\begin{matrix} + 2454833.014 \\ - 2454832.986 \end{matrix})

Secondary transit

—

λ

—

Impact Parameter b

0.405 (\begin{matrix} + 0.05 \\ - 0.405 \end{matrix})

1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

1043.0 K 1 publication

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

—

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

Star

Name

Kepler-526 A

Distance

504.0 pc

Spectral type

G1V

Apparent magnitude V

—

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

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

M_Sun

Age

2.14 (\begin{matrix} + 1.31 \\ - -0.832 \end{matrix})

Gyr

Effective temperature

5894.0 (\begin{matrix} + 80.86 \\ - 84.44 \end{matrix})

Radius

1.14 (\begin{matrix} + 0.07 \\ - 0.06 \end{matrix})

R_Sun

Metallicity [Fe/H]

0.34 (\begin{matrix} + 0.07 \\ - 0.069 \end{matrix})

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:50:36.2

Dec₂₀₀₀

+47:23:46.7

Alternate Names

2MASS J19503622+4723466, KIC 10290666, KOI-332, WISE J195036.22+472346.4

Sullivan et al. (2024): A K dwarf companion star is detected 0.13 arcseconds away (65.5 AUs at 504 pc).

No link

Simbad
Most recent references (ADS)

Planet KOI-332.02

Planet

Basic informations 30 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 1 planet

Remarks Some remarks

Other web pages No page

More data 2 references

Planet KOI-332.02

Planet

Basic informations 30 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 1 planet

Remarks Some remarks

Other web pages No page

More data 2 references

Related publications

Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems is Dependent on Stellar Separation

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25

Planetary Candidates Observed by Kepler IV: Planet Sample From Q1-Q8 (22 Months)