Exoplanet

Kepler-68 e

Orbiting Kepler-68

Overview

Kepler-68 e is an exoplanet orbiting the star Kepler-68, discovered in 2023 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

86.45

Earth masses

0500 M⊕

Orbital Period

3455.0

days

0.1d10,000d

Distance

144.2

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

86.45

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Bonomo et al. 2023

Orbital Period

3455.000+348.000169.000days

Semi-Major Axis

4.6000+0.32000.1600au

M sin(i) (Earth masses)

86.45+10.1710.17

M sin(i) (Jupiter masses)

0.2720+0.03200.0320

Eccentricity

0.3300+0.11000.1100

Argument of Periastron

196.0+17.020.0deg

Radial Velocity Semi-Amplitude

3.73+0.390.39m/s

Distance from Earth

144.2 pc (~470 ly)

Spectral Type

Unknown

Temperature

5847 K

Mass (Solar)

1.06 M☉

Radius (Solar)

1.26 R☉

Luminosity

Unknown

Planets in System

4

Stars in System

2

Coordinates (RA, Dec)

291.0323°, 49.0402°

Discovery Method

Radial Velocity

Discovery Year

2023

Data Sources

Source ID: Kepler-68 e

System Context

Kepler-68 e orbits Kepler-68 and was reported in 2023 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 86.45 Earth masses (M sin i) and an orbital period of 3,455 days.

Catalog data places the system at about 144.2 parsecs from Earth and 4 known planets in the system.

Host star

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

Open Kepler-68

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