Exoplanet

HD 125612 c

Orbiting HD 125612

Overview

HD 125612 c is an exoplanet orbiting the star HD 125612, discovered in 2009 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

15.57

Earth masses

0500 M⊕

Orbital Period

4.2

days

0.1d10,000d

Distance

57.6

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

15.57

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Feng et al. 2022

Orbital Period

4.155+0.0000.000days

Semi-Major Axis

0.0510+0.00200.0020au

M sin(i) (Earth masses)

15.57+2.542.86

M sin(i) (Jupiter masses)

0.0490+0.00800.0090

Eccentricity

0.1490+0.14100.0930

Epoch of Periastron

2453187.02+3.460.10days(BJD)

Argument of Periastron

149.7+64.761.2deg

Radial Velocity Semi-Amplitude

6.00+0.900.86m/s

Distance from Earth

57.6 pc (~188 ly)

Spectral Type

Unknown

Temperature

Unknown

Mass (Solar)

1.05 M☉

Radius (Solar)

Unknown

Luminosity

Unknown

Planets in System

3

Stars in System

2

Coordinates (RA, Dec)

215.2227°, -17.4818°

Discovery Method

Radial Velocity

Discovery Year

2009

Data Sources

Source ID: HD 125612 c

System Context

HD 125612 c orbits HD 125612 and was reported in 2009 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 15.57 Earth masses (M sin i) and an orbital period of 4.15 days.

Catalog data places the system at about 57.6 parsecs from Earth and 3 known planets in the system.

Host star

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

Open HD 125612

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