Exoplanet

HD 30669 b

Orbiting HD 30669

Overview

HD 30669 b is an exoplanet orbiting the star HD 30669, discovered in 2014 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

149.37

Earth masses

0500 M⊕

Orbital Period

1684.0

days

0.1d10,000d

Distance

58.1

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

149.37

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Moutou et al. 2015

Orbital Period

1684.000+61.00061.000days

Semi-Major Axis

2.6900+0.08000.0800au

M sin(i) (Earth masses)

149.37+19.0719.07

M sin(i) (Jupiter masses)

0.4700+0.06000.0600

Eccentricity

0.1800+0.15000.1500

Epoch of Periastron

2457181.00+101.001395.00days

Argument of Periastron

82.0+43.036.0deg

Radial Velocity Semi-Amplitude

8.60+1.101.10m/s

Distance from Earth

58.1 pc (~189 ly)

Spectral Type

G9 V

Temperature

5400 K

Mass (Solar)

0.92 M☉

Radius (Solar)

0.91 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

72.1199°, -28.4191°

Discovery Method

Radial Velocity

Discovery Year

2014

Data Sources

Source ID: HD 30669 b

System Context

HD 30669 b orbits HD 30669 and was reported in 2014 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 149.37 Earth masses (M sin i) and an orbital period of 1,684 days.

Catalog data places the system at about 58.1 parsecs from Earth, a host star classified as G9 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 30669