Exoplanet

HD 10647 b

Orbiting HD 10647

Overview

HD 10647 b is an exoplanet orbiting the star HD 10647, discovered in 2006 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

298.75

Earth masses

0500 M⊕

Orbital Period

989.2

days

0.1d10,000d

Distance

17.3

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

298.75

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Marmier et al. 2013

Orbital Period

989.200+8.1008.100days

Semi-Major Axis

2.0150+0.01100.0110au

M sin(i) (Earth masses)

298.75+25.4325.43

M sin(i) (Jupiter masses)

0.9400+0.08000.0800

Eccentricity

0.1500+0.08000.0800

Epoch of Periastron

2453654.00+99.0099.00days

Argument of Periastron

212.0+39.039.0deg

Radial Velocity Semi-Amplitude

18.10+1.701.70m/s

Distance from Earth

17.3 pc (~57 ly)

Spectral Type

F9 V

Temperature

6218 K

Mass (Solar)

1.11 M☉

Radius (Solar)

1.10 R☉

Luminosity

0.15 log L☉

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

25.6234°, -53.7413°

Discovery Method

Radial Velocity

Discovery Year

2006

Data Sources

Source ID: HD 10647 b

System Context

HD 10647 b orbits HD 10647 and was reported in 2006 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 298.75 Earth masses (M sin i) and an orbital period of 989.2 days.

Catalog data places the system at about 17.3 parsecs from Earth, a host star classified as F9 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 10647