Exoplanet

TOI-2295 c

Orbiting TOI-2295

Overview

TOI-2295 c is an exoplanet orbiting the star TOI-2295, discovered in 2024 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

1783.02

Earth masses

0500 M⊕

Orbital Period

966.5

days

0.1d10,000d

Distance

126.3

parsecs

Nearby10,000 pc

Equilibrium Temp

235

K

150 K3,500 K

Radius (Earth radii)

Unknown

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

1783.02

Radial-velocity minimum

Equilibrium Temperature

235 K

Parameter source: Heidari et al. 2025

Orbital Period

966.500+4.3004.200days

Semi-Major Axis

2.0180+0.04000.0420au

M sin(i) (Earth masses)

1783.02+73.1076.28

M sin(i) (Jupiter masses)

5.6100+0.23000.2400

Eccentricity

0.1940+0.01200.0120

Argument of Periastron

39.5+3.03.0deg

Radial Velocity Semi-Amplitude

105.80+1.101.10m/s

Distance from Earth

126.3 pc (~412 ly)

Spectral Type

Unknown

Temperature

5730 K

Mass (Solar)

1.17 M☉

Radius (Solar)

1.46 R☉

Luminosity

0.31 log L☉

Planets in System

2

Stars in System

1

Coordinates (RA, Dec)

281.5762°, 50.4925°

Discovery Method

Radial Velocity

Discovery Year

2024

Data Sources

Source ID: TOI-2295 c

System Context

TOI-2295 c orbits TOI-2295 and was reported in 2024 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 1,783.02 Earth masses (M sin i), an orbital period of 966.5 days, and an equilibrium temperature near 235 K.

Catalog data places the system at about 126.3 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 TOI-2295

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