Exoplanet

Gl 725 B c

Orbiting Gl 725 B

Overview

Gl 725 B c is an exoplanet orbiting the star Gl 725 B, discovered in 2026 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

3.40

Earth masses

0500 M⊕

Orbital Period

37.9

days

0.1d10,000d

Distance

6.8

parsecs

Nearby10,000 pc

Equilibrium Temp

215

K

150 K3,500 K

What these measurements mean

These comparisons use the reported catalog values. They are interpretations and calculations, not additional observations.

A year on this world
A 365.25-day Earth year spans about 9.64 of these orbits. This comparison uses the reported orbital period. It does not measure the planet's rotation or the length of its day.
What the mass can tell you
M sin i is a lower bound on the true mass because the viewing angle affects the radial-velocity measurement. Do not treat it as an exact mass or use it to claim a measured density.
Temperature has limits
Equilibrium temperature describes a model of absorbed and emitted energy, not a measured surface temperature. Atmosphere and reflectivity affect the interpretation. This value alone cannot establish liquid water, a habitable surface, or life.

Radius (Earth radii)

Unknown

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

3.40

Radial-velocity minimum

Equilibrium Temperature

215 K

Parameter source: Ould-Elhkim et al. 2026

Orbital Period

37.900+0.170−0.170days

Semi-Major Axis

0.1390+0.0040−0.0040au

M sin(i) (Earth masses)

3.40+0.70−0.70

M sin(i) (Jupiter masses)

0.0107+0.0022−0.0022

Radial Velocity Semi-Amplitude

1.70+0.30−0.30m/s

Distance from Earth

6.8 pc (~22 ly)

Spectral Type

Unknown

Temperature

3379 K

Mass (Solar)

0.25 M☉

Radius (Solar)

0.28 R☉

Luminosity

-2.04 log L☉

Planets in System

2

Stars in System

2

Coordinates (RA, Dec)

280.6954°, 59.6271°

Discovery Method

Radial Velocity

Discovery Year

2026

Data Sources

Source ID: Gl 725 B c

System Context

Gl 725 B c orbits Gl 725 B and was reported in 2026 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 3.4 Earth masses (M sin i), an orbital period of 37.9 days, and an equilibrium temperature near 215 K.

Catalog data places the system at about 6.8 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 Gl 725 B