Exoplanet

Kepler-1655 b

Orbiting Kepler-1655

Overview

Kepler-1655 b is an exoplanet orbiting the star Kepler-1655, discovered in 2018 using the Transit method. It is a Super-Earth world.

Key Measurements

Radius

2.21

Earth radii

015 R⊕

Mass

5.40

Earth masses

0500 M⊕

Orbital Period

11.9

days

0.1d10,000d

Distance

213.3

parsecs

Nearby10,000 pc

Equilibrium Temp

938

K

150 K3,500 K

Radius (Earth radii)

2.21

Mass (Earth masses)

5.40

Measured

Equilibrium Temperature

938 K

Parameter source: Bonomo et al. 2023

Orbital Period

11.873+0.000−0.000days

Semi-Major Axis

0.1029+0.0014−0.0014au

Planet Mass (Earth masses)

5.40+1.70−1.70

Planet Mass (Jupiter masses)

0.0170+0.0053−0.0053

Eccentricity

<0.19

Radial Velocity Semi-Amplitude

1.51+0.48−0.48m/s

Distance from Earth

213.3 pc (~696 ly)

Spectral Type

Unknown

Temperature

6148 K

Mass (Solar)

1.03 M☉

Radius (Solar)

1.03 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

286.6896°, 39.2121°

Discovery Method

Transit

Discovery Year

2018

Data Sources
NASA Exoplanet Archive

Source ID: Kepler-1655 b

System Context

Kepler-1655 b orbits Kepler-1655 and was reported in 2018 and was detected with the Transit method.

Published measurements list a radius of 2.21 Earth radii, a mass of 5.4 Earth masses, an orbital period of 11.87 days, and an equilibrium temperature near 938 K.

Catalog data places the system at about 213.3 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-1655