Exoplanet

HD 96127 b

Orbiting HD 96127

Overview

HD 96127 b is an exoplanet orbiting the star HD 96127, discovered in 2011 using the Radial Velocity method.

Key Measurements

Mass

1207.75

Earth masses

0500 M⊕

Orbital Period

638.9

days

0.1d10,000d

Distance

587.7

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

Mass (Earth masses)

1207.75

Measured

Equilibrium Temperature

Unknown

Parameter source: Piccinini et al. 2026

Orbital Period

638.900+17.00016.700days

Semi-Major Axis

1.4100+0.13000.1300au

Planet Mass (Earth masses)

1207.75+413.18381.39

Planet Mass (Jupiter masses)

3.8000+1.30001.2000

Eccentricity

0.3000+0.10000.1000

Epoch of Periastron

2458441.00+27.0024.00days(BJD)

Argument of Periastron

163.1+15.915.6deg

Radial Velocity Semi-Amplitude

100.70+19.5014.40m/s

Distance from Earth

587.7 pc (~1917 ly)

Spectral Type

K2 III

Temperature

3943 K

Mass (Solar)

0.91 M☉

Radius (Solar)

35.00 R☉

Luminosity

Unknown

Planets in System

1

Stars in System

1

Coordinates (RA, Dec)

166.4415°, 44.3015°

Discovery Method

Radial Velocity

Discovery Year

2011

Data Sources

Source ID: HD 96127 b

System Context

HD 96127 b orbits HD 96127 and was reported in 2011 and was detected with the Radial Velocity method.

Published measurements list a mass of 1,207.75 Earth masses and an orbital period of 638.9 days.

Catalog data places the system at about 587.7 parsecs from Earth, a host star classified as K2 III, 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 96127