Exoplanet

HD 25912 c

Orbiting HD 25912

Overview

HD 25912 c is an exoplanet orbiting the star HD 25912, discovered in 2022 using the Radial Velocity method.

Key Measurements

Mass

5252.75

Earth masses

0500 M⊕

Orbital Period

26308.7

days

0.1d10,000d

Distance

49.2

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

Mass (Earth masses)

5252.75

Measured

Equilibrium Temperature

Unknown

Parameter source: Feng et al. 2022

Orbital Period

26308.656+2095.1742794.644days

Semi-Major Axis

17.8480+1.14701.4840au

Planet Mass (Earth masses)

5252.75+437.33444.64

Planet Mass (Jupiter masses)

16.5270+1.37601.3990

Eccentricity

0.0510+0.04800.0250

Epoch of Periastron

2443594.24+2887.242605.59days(BJD)

Argument of Periastron

51.9+21.619.8deg

Radial Velocity Semi-Amplitude

106.31+2.122.09m/s

Distance from Earth

49.2 pc (~160 ly)

Spectral Type

Unknown

Temperature

Unknown

Mass (Solar)

1.08 M☉

Radius (Solar)

Unknown

Luminosity

Unknown

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

60.9075°, -51.9315°

Discovery Method

Radial Velocity

Discovery Year

2022

Data Sources

Source ID: HD 25912 c

System Context

HD 25912 c orbits HD 25912 and was reported in 2022 and was detected with the Radial Velocity method.

Published measurements list a mass of 5,252.75 Earth masses and an orbital period of 26,308.66 days.

Catalog data places the system at about 49.2 parsecs from Earth 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 25912

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