Exoplanet

GJ 411 b

Orbiting GJ 411

Overview

GJ 411 b is an exoplanet orbiting the star GJ 411, discovered in 2019 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

2.69

Earth masses

0500 M⊕

Orbital Period

12.9

days

0.1d10,000d

Distance

5.7

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

2.69

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Hurt et al. 2022

Orbital Period

12.939+0.0010.001days

Semi-Major Axis

0.0788+0.00060.0006au

M sin(i) (Earth masses)

2.69+0.190.18

M sin(i) (Jupiter masses)

0.0085+0.00060.0006

Eccentricity

0.0630+0.06100.0430

Epoch of Periastron

2456307.80+2.204.80days(JD)

Argument of Periastron

-30.0+180.0120.0deg

Radial Velocity Semi-Amplitude

1.38+0.090.09m/s

Distance from Earth

5.7 pc (~19 ly)

Spectral Type

Unknown

Temperature

3719 K

Mass (Solar)

0.39 M☉

Radius (Solar)

0.37 R☉

Luminosity

Unknown

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

165.8345°, 35.9723°

Discovery Method

Radial Velocity

Discovery Year

2019

Data Sources

Source ID: GJ 411 b

System Context

GJ 411 b orbits GJ 411 and was reported in 2019 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 2.69 Earth masses (M sin i) and an orbital period of 12.94 days.

Catalog data places the system at about 5.7 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 GJ 411

More planets in this system

GJ 411 b