Exoplanet

Kepler-432 c

Orbiting Kepler-432

Overview

Kepler-432 c is an exoplanet orbiting the star Kepler-432, discovered in 2015 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

772.33

Earth masses

0500 M⊕

Orbital Period

406.2

days

0.1d10,000d

Distance

848.0

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

Minimum Mass, M sin(i) (Earth masses)

772.33

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Quinn et al. 2015

Orbital Period

406.200+3.9002.500days

M sin(i) (Earth masses)

772.33+69.9276.28

M sin(i) (Jupiter masses)

2.4300+0.22000.2400

Eccentricity

0.4980+0.02900.0590

Argument of Periastron

60.8+7.011.2deg

Radial Velocity Semi-Amplitude

62.10+6.105.80m/s

Distance from Earth

848.0 pc (~2766 ly)

Spectral Type

Unknown

Temperature

4995 K

Mass (Solar)

1.32 M☉

Radius (Solar)

4.06 R☉

Luminosity

Unknown

Planets in System

2

Stars in System

2

Coordinates (RA, Dec)

293.2822°, 48.2859°

Discovery Method

Radial Velocity

Discovery Year

2015

Data Sources

Source ID: Kepler-432 c

System Context

Kepler-432 c orbits Kepler-432 and was reported in 2015 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 772.33 Earth masses (M sin i) and an orbital period of 406.2 days.

Catalog data places the system at about 848 parsecs from Earth and 2 known planets in the system.

Host star

Explore the stellar record for this system to compare temperature, spectral type, and known planets.

Open Kepler-432

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