Exoplanet

HD 147018 c

Orbiting HD 147018

Overview

HD 147018 c is an exoplanet orbiting the star HD 147018, discovered in 2009 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

2080.00

Earth masses

0500 M⊕

Orbital Period

1008.0

days

0.1d10,000d

Distance

40.4

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

2080.00

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Ségransan et al. 2010

Orbital Period

1008.000+18.00018.000days

Semi-Major Axis

1.9220+0.03900.0390au

M sin(i) (Earth masses)

2080.00+100.00100.00

M sin(i) (Jupiter masses)

6.5600+0.32000.3200

Eccentricity

0.1330+0.01100.0110

Epoch of Periastron

2455301.00+22.0022.00days

Argument of Periastron

-133.1+6.96.9deg

Radial Velocity Semi-Amplitude

141.20+4.104.10m/s

Distance from Earth

40.4 pc (~132 ly)

Spectral Type

G9 V

Temperature

5441 K

Mass (Solar)

0.93 M☉

Radius (Solar)

Unknown

Luminosity

Unknown

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

245.7490°, -61.6901°

Discovery Method

Radial Velocity

Discovery Year

2009

Data Sources

Source ID: HD 147018 c

System Context

HD 147018 c orbits HD 147018 and was reported in 2009 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 2,080 Earth masses (M sin i) and an orbital period of 1,008 days.

Catalog data places the system at about 40.4 parsecs from Earth, a host star classified as G9 V, 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 147018

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