Exoplanet

HD 125595 b

Orbiting HD 125595

Overview

HD 125595 b is an exoplanet orbiting the star HD 125595, discovered in 2011 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

6.36

Earth masses

0500 M⊕

Orbital Period

9.7

days

0.1d10,000d

Distance

28.2

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

6.36

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Stassun et al. 2017

Orbital Period

9.674+0.0040.004days

Semi-Major Axis

0.0800+0.00000.0000au

M sin(i) (Earth masses)

6.36+3.183.18

M sin(i) (Jupiter masses)

0.0200+0.01000.0100

Eccentricity

0.0000

Radial Velocity Semi-Amplitude

4.80+0.500.50m/s

Distance from Earth

28.2 pc (~92 ly)

Spectral Type

Unknown

Temperature

4691 K

Mass (Solar)

0.29 M☉

Radius (Solar)

0.74 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

215.3434°, -40.3942°

Discovery Method

Radial Velocity

Discovery Year

2011

Data Sources

Source ID: HD 125595 b

System Context

HD 125595 b orbits HD 125595 and was reported in 2011 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 6.36 Earth masses (M sin i) and an orbital period of 9.67 days.

Catalog data places the system at about 28.2 parsecs from Earth 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 125595