Exoplanet

HD 216770 b

Orbiting HD 216770

Overview

HD 216770 b is an exoplanet orbiting the star HD 216770, discovered in 2003 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

181.16

Earth masses

0500 M⊕

Orbital Period

118.5

days

0.1d10,000d

Distance

36.7

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

181.16

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Stassun et al. 2017

Orbital Period

118.450+0.5500.550days

Semi-Major Axis

0.4600+0.01000.0100au

M sin(i) (Earth masses)

181.16+15.8915.89

M sin(i) (Jupiter masses)

0.5700+0.05000.0500

Eccentricity

0.3700+0.06000.0600

Radial Velocity Semi-Amplitude

30.90+1.901.90m/s

Distance from Earth

36.7 pc (~120 ly)

Spectral Type

Unknown

Temperature

5399 K

Mass (Solar)

0.74 M☉

Radius (Solar)

0.93 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

343.9749°, -26.6595°

Discovery Method

Radial Velocity

Discovery Year

2003

Data Sources

Source ID: HD 216770 b

System Context

HD 216770 b orbits HD 216770 and was reported in 2003 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 181.16 Earth masses (M sin i) and an orbital period of 118.45 days.

Catalog data places the system at about 36.7 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 216770