Exoplanet

HD 191939 e

Orbiting HD 191939

Overview

HD 191939 e is an exoplanet orbiting the star HD 191939, discovered in 2022 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

112.20

Earth masses

0500 M⊕

Orbital Period

101.1

days

0.1d10,000d

Distance

53.6

parsecs

Nearby10,000 pc

Equilibrium Temp

390

K

150 K3,500 K

Radius (Earth radii)

Unknown

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

112.20

Radial-velocity minimum

Equilibrium Temperature

390 K

Parameter source: Orell-Miquel et al. 2023

Orbital Period

101.120+0.1300.130days

Semi-Major Axis

0.4070+0.01200.0120au

M sin(i) (Earth masses)

112.20+4.004.00

M sin(i) (Jupiter masses)

0.3530+0.01260.0126

Eccentricity

0.0310+0.00800.0160

Argument of Periastron

-130.0+180.016.0deg

Radial Velocity Semi-Amplitude

17.73+0.140.16m/s

Distance from Earth

53.6 pc (~175 ly)

Spectral Type

G9 V

Temperature

5348 K

Mass (Solar)

0.81 M☉

Radius (Solar)

0.94 R☉

Luminosity

-0.19 log L☉

Planets in System

6

Stars in System

1

Coordinates (RA, Dec)

302.0256°, 66.8503°

Discovery Method

Radial Velocity

Discovery Year

2022

Data Sources

Source ID: HD 191939 e

System Context

HD 191939 e orbits HD 191939 and was reported in 2022 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 112.2 Earth masses (M sin i), an orbital period of 101.12 days, and an equilibrium temperature near 390 K.

Catalog data places the system at about 53.6 parsecs from Earth, a host star classified as G9 V, and 6 known planets in the system.

Host star

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

Open HD 191939