Exoplanet

HD 238090 b

Orbiting HD 238090

Overview

HD 238090 b is an exoplanet orbiting the star HD 238090, discovered in 2020 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

6.89

Earth masses

0500 M⊕

Orbital Period

13.7

days

0.1d10,000d

Distance

15.2

parsecs

Nearby10,000 pc

Equilibrium Temp

470

K

150 K3,500 K

Radius (Earth radii)

Unknown

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

6.89

Radial-velocity minimum

Equilibrium Temperature

470 K

Parameter source: Stock et al. 2020

Orbital Period

13.671+0.0110.010days

Semi-Major Axis

0.0932+0.00110.0011au

M sin(i) (Earth masses)

6.89+0.920.95

M sin(i) (Jupiter masses)

0.0217+0.00290.0030

Eccentricity

0.3000+0.16000.1700

Argument of Periastron

119.3+22.824.8deg

Radial Velocity Semi-Amplitude

2.85+0.380.39m/s

Distance from Earth

15.2 pc (~50 ly)

Spectral Type

M0.0 V

Temperature

3933 K

Mass (Solar)

0.58 M☉

Radius (Solar)

0.57 R☉

Luminosity

-1.15 log L☉

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

183.0886°, 54.4862°

Discovery Method

Radial Velocity

Discovery Year

2020

Data Sources

Source ID: HD 238090 b

System Context

HD 238090 b orbits HD 238090 and was reported in 2020 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 6.89 Earth masses (M sin i), an orbital period of 13.67 days, and an equilibrium temperature near 470 K.

Catalog data places the system at about 15.2 parsecs from Earth, a host star classified as M0.0 V, 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 HD 238090