Planet Kepler-50 b

Detailed information about planet Kepler-50 b and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

Kepler-50 b

Planet Status

Confirmed

Discovered in

2012

Update

2021-02-05

Mass

0.1 (\begin{matrix} + 0.0 \\ - 0.1 \end{matrix})

M_J 1 publication

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

Mass*sin(i)

—

Semi-Major Axis

0.077 (\begin{matrix} + 0.012 \\ - 0.02 \end{matrix})

AU 1 publication

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65

Orbital Period

7.81254 (\begin{matrix} + 0.0001 \\ - 0.0001 \end{matrix})

day 1 publication

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65

Eccentricity

—

ω

—

T_peri

—

Radius

0.153 (\begin{matrix} + 0.004 \\ - 0.009 \end{matrix})

R_J 1 publication

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65

Inclination

—

Detection Method

Primary Transit

Mass Meas. Method

—

Radius Meas. Method

—

Primary transit

2455005.63186 (\pm 0.0022)

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

0.74 (\begin{matrix} + 0.07 \\ - 0.36 \end{matrix})

1 publication

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65

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 J19122420+5002013 b, K00262.01, KIC 11807274 b, KOI-262 b, KOI-262.01, WISE J191224.21+500201.2  b

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-50

Distance

251.91 (\begin{matrix} + 1.87 \\ - 1.87 \end{matrix})

Spectral type

—

Apparent magnitude V

11.0

Mass

1.24 (\pm 0.05)

M_Sun 1 publication

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65

Age

3.8 (\pm 0.8)

Gyr 1 publication

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65

Effective temperature

6225.0 (\pm 66.0)

K 1 publication

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65

Radius

1.58 (\pm 0.02)

R_Sun 1 publication

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65

Metallicity [Fe/H]

0.03 (\begin{matrix} + 0.06 \\ - 0.06 \end{matrix})

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

19:12:24.2

Dec₂₀₀₀

+50:02:01.4

Alternate Names

2MASS J19122420+5002013, KIC 11807274, KOI-262, WISE J191224.21+500201.2

Alias KIC 11807274
Alias 2MASS 19122420+5002013

No link

Simbad
Most recent references (ADS)

Planet Kepler-50 b

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 2 planets

Remarks Some remarks

Other web pages No page

More data 2 references

Planet Kepler-50 b

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 2 planets

Remarks Some remarks

Other web pages No page

More data 2 references

Related publications

Spin-orbit alignment of exoplanet systems: ensemble analysis using asteroseismology

Asteroseismology of Exoplanet Host Stars

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

Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65