Exoplanet

HD 116029 b

Orbiting HD 116029

Overview

HD 116029 b is an exoplanet orbiting the star HD 116029, discovered in 2011 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

444.96

Earth masses

0500 M⊕

Orbital Period

670.0

days

0.1d10,000d

Distance

123.2

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

444.96

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Stassun et al. 2017

Orbital Period

670.000+11.00011.000days

Semi-Major Axis

1.6500+0.05000.0500au

M sin(i) (Earth masses)

444.96+92.1792.17

M sin(i) (Jupiter masses)

1.4000+0.29000.2900

Eccentricity

0.0000

Radial Velocity Semi-Amplitude

36.60+3.103.10m/s

Distance from Earth

123.2 pc (~402 ly)

Spectral Type

Unknown

Temperature

4819 K

Mass (Solar)

0.83 M☉

Radius (Solar)

4.89 R☉

Luminosity

Unknown

Planets in System

2

Stars in System

2

Coordinates (RA, Dec)

200.1647°, 24.6485°

Discovery Method

Radial Velocity

Discovery Year

2011

Data Sources

Source ID: HD 116029 b

System Context

HD 116029 b orbits HD 116029 and was reported in 2011 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 444.96 Earth masses (M sin i) and an orbital period of 670 days.

Catalog data places the system at about 123.2 parsecs from Earth and 2 known planets in the system.

Host star

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

Open HD 116029

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