Exoplanet

Kepler-1432 b

Orbiting Kepler-1432

Overview

Kepler-1432 b is an exoplanet orbiting the star Kepler-1432, discovered in 2016 using the Transit method. It is a Super-Earth world.

Key Measurements

Radius

2.22

Earth radii

015 R⊕

Mass (est.)

5.92

Earth masses

0500 M⊕

Orbital Period

23.9

days

0.1d10,000d

Distance

2171.9

parsecs

Nearby10,000 pc

Radius (Earth radii)

2.22

Mass (Earth masses)

5.92

Estimated

Equilibrium Temperature

Unknown

Parameter source: Morton et al. 2016

Orbital Period

23.911+0.000−0.000days

Distance from Earth

2171.9 pc (~7084 ly)

Spectral Type

Unknown

Temperature

6031 K

Mass (Solar)

1.09 M☉

Radius (Solar)

1.13 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

295.5241°, 49.8295°

Discovery Method

Transit

Discovery Year

2016

Data Sources
NASA Exoplanet Archive

Source ID: Kepler-1432 b

System Context

Kepler-1432 b orbits Kepler-1432 and was reported in 2016 and was detected with the Transit method.

Published measurements list a radius of 2.22 Earth radii, a mass of 5.92 Earth masses (estimated), and an orbital period of 23.91 days.

Catalog data places the system at about 2,171.9 parsecs from Earth and 1 known planet in the system.

Host star

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

Open Kepler-1432