Exoplanet

HD 60532 c

Orbiting HD 60532

Overview

HD 60532 c is an exoplanet orbiting the star HD 60532, discovered in 2008 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

797.75

Earth masses

0500 M⊕

Orbital Period

600.1

days

0.1d10,000d

Distance

26.0

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

797.75

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Borgniet et al. 2017

Orbital Period

600.100+2.4002.400days

Semi-Major Axis

1.6000+0.04000.0400au

M sin(i) (Earth masses)

797.75+50.8550.85

M sin(i) (Jupiter masses)

2.5100+0.16000.1600

Eccentricity

0.0300+0.02000.0200

Epoch of Periastron

2454973.00+100.10100.10days(BJD)

Argument of Periastron

179.8+58.758.7deg

Radial Velocity Semi-Amplitude

46.10+1.001.00m/s

Distance from Earth

26.0 pc (~85 ly)

Spectral Type

Unknown

Temperature

6245 K

Mass (Solar)

1.50 M☉

Radius (Solar)

2.57 R☉

Luminosity

Unknown

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

113.5131°, -22.2959°

Discovery Method

Radial Velocity

Discovery Year

2008

Data Sources

Source ID: HD 60532 c

System Context

HD 60532 c orbits HD 60532 and was reported in 2008 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 797.75 Earth masses (M sin i) and an orbital period of 600.1 days.

Catalog data places the system at about 26 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 60532

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