Exoplanet

HD 102329 c

Orbiting HD 102329

Overview

HD 102329 c is an exoplanet orbiting the star HD 102329, discovered in 2016 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

483.10

Earth masses

0500 M⊕

Orbital Period

1123.0

days

0.1d10,000d

Distance

217.1

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

483.10

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Bryan et al. 2016

Orbital Period

1123.000+79.00053.000days

M sin(i) (Earth masses)

483.10+95.3579.46

M sin(i) (Jupiter masses)

1.5200+0.30000.2500

Eccentricity

0.2090+0.23100.2020

Epoch of Periastron

2454736.00+569.00200.00days(JD)

Argument of Periastron

21.0+165.074.0deg

Radial Velocity Semi-Amplitude

27.40+6.804.50m/s

Distance from Earth

217.1 pc (~708 ly)

Spectral Type

Unknown

Temperature

Unknown

Mass (Solar)

1.30 M☉

Radius (Solar)

Unknown

Luminosity

Unknown

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

176.6942°, 3.4742°

Discovery Method

Radial Velocity

Discovery Year

2016

Data Sources

Source ID: HD 102329 c

System Context

HD 102329 c orbits HD 102329 and was reported in 2016 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 483.1 Earth masses (M sin i) and an orbital period of 1,123 days.

Catalog data places the system at about 217.1 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 102329

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