Exoplanet

Kepler-1650 b

Orbiting Kepler-1650

Overview

Kepler-1650 b is an exoplanet orbiting the star Kepler-1650, discovered in 2017 using the Transit method. It is a Earth-sized world.

Key Measurements

Radius

0.96

Earth radii

015 R⊕

Mass (est.)

0.84

Earth masses

0500 M⊕

Orbital Period

1.5

days

0.1d10,000d

Distance

134.4

parsecs

Nearby10,000 pc

Radius (Earth radii)

0.96

Mass (Earth masses)

0.84

Estimated

Equilibrium Temperature

Unknown

Parameter source: Mann et al. 2017

Orbital Period

1.538+0.0000.000days

Eccentricity

0.0100+0.15000.0100

Distance from Earth

134.4 pc (~438 ly)

Spectral Type

Unknown

Temperature

3410 K

Mass (Solar)

0.33 M☉

Radius (Solar)

0.33 R☉

Luminosity

-1.87 log L☉

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

297.7292°, 42.8667°

Discovery Method

Transit

Discovery Year

2017

Data Sources

Source ID: Kepler-1650 b

System Context

Kepler-1650 b orbits Kepler-1650 and was reported in 2017 and was detected with the Transit method.

Published measurements list a radius of 0.96 Earth radii, a mass of 0.84 Earth masses (estimated), and an orbital period of 1.54 days.

Catalog data places the system at about 134.4 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-1650