Exoplanet

HIP 41378 g

Orbiting HIP 41378

Overview

HIP 41378 g is an exoplanet orbiting the star HIP 41378, discovered in 2025 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

5.75

Earth masses

0500 M⊕

Orbital Period

63.2

days

0.1d10,000d

Distance

106.3

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

5.75

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Grouffal et al. 2026

Orbital Period

63.190+0.1200.120days

M sin(i) (Earth masses)

5.75+0.760.83

M sin(i) (Jupiter masses)

0.0181+0.00240.0026

Eccentricity

0.0550+0.02400.0540

Distance from Earth

106.3 pc (~347 ly)

Spectral Type

Unknown

Temperature

6290 K

Mass (Solar)

1.22 M☉

Radius (Solar)

1.30 R☉

Luminosity

Unknown

Planets in System

6

Stars in System

1

Coordinates (RA, Dec)

126.6158°, 10.0804°

Discovery Method

Radial Velocity

Discovery Year

2025

Data Sources

Source ID: HIP 41378 g

System Context

HIP 41378 g orbits HIP 41378 and was reported in 2025 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 5.75 Earth masses (M sin i) and an orbital period of 63.19 days.

Catalog data places the system at about 106.3 parsecs from Earth and 6 known planets in the system.

Host star

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

Open HIP 41378
HIP 41378 g