Exoplanet

HD 147379 b

Orbiting HD 147379

Overview

HD 147379 b is an exoplanet orbiting the star HD 147379, discovered in 2017 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

21.60

Earth masses

0500 M⊕

Orbital Period

86.6

days

0.1d10,000d

Distance

10.8

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

21.60

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Stalport et al. 2023

Orbital Period

86.580+0.1400.140days

M sin(i) (Earth masses)

21.60+1.101.10

M sin(i) (Jupiter masses)

0.0680+0.00350.0035

Eccentricity

0.0630+0.04700.0380

Argument of Periastron

130.1+58.348.1deg

Radial Velocity Semi-Amplitude

4.49+0.220.22m/s

Distance from Earth

10.8 pc (~35 ly)

Spectral Type

M0.0 V

Temperature

4090 K

Mass (Solar)

0.58 M☉

Radius (Solar)

Unknown

Luminosity

Unknown

Planets in System

1

Stars in System

2

Coordinates (RA, Dec)

244.1726°, 67.2392°

Discovery Method

Radial Velocity

Discovery Year

2017

Data Sources

Source ID: HD 147379 b

System Context

HD 147379 b orbits HD 147379 and was reported in 2017 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 21.6 Earth masses (M sin i) and an orbital period of 86.58 days.

Catalog data places the system at about 10.8 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 147379