Exoplanet

HD 180617 b

Orbiting HD 180617

Overview

HD 180617 b is an exoplanet orbiting the star HD 180617, discovered in 2018 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

12.21

Earth masses

0500 M⊕

Orbital Period

105.9

days

0.1d10,000d

Distance

5.9

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

12.21

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Burt et al. 2021

Orbital Period

105.911+0.1090.109days

Semi-Major Axis

0.3430+0.00400.0040au

M sin(i) (Earth masses)

12.21+1.051.05

M sin(i) (Jupiter masses)

0.0384+0.00330.0033

Eccentricity

0.1010+0.05300.0530

Argument of Periastron

257.4+51.351.3deg

Radial Velocity Semi-Amplitude

2.70+0.220.22m/s

Distance from Earth

5.9 pc (~19 ly)

Spectral Type

Unknown

Temperature

3534 K

Mass (Solar)

0.48 M☉

Radius (Solar)

0.48 R☉

Luminosity

-1.49 log L☉

Planets in System

1

Stars in System

2

Coordinates (RA, Dec)

289.2277°, 5.1632°

Discovery Method

Radial Velocity

Discovery Year

2018

Data Sources

Source ID: HD 180617 b

System Context

HD 180617 b orbits HD 180617 and was reported in 2018 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 12.21 Earth masses (M sin i) and an orbital period of 105.91 days.

Catalog data places the system at about 5.9 parsecs from Earth 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 180617