Exoplanet

TOI-1203 e

Orbiting TOI-1203

Overview

TOI-1203 e is an exoplanet orbiting the star TOI-1203, discovered in 2025 using the Radial Velocity method.

Key Measurements

Minimum Mass (M sin i)

42.10

Earth masses

0500 M⊕

Orbital Period

204.6

days

0.1d10,000d

Distance

65.0

parsecs

Nearby10,000 pc

Radius (Earth radii)

Unknown

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

42.10

Radial-velocity minimum

Equilibrium Temperature

Unknown

Parameter source: Gandolfi et al. 2025

Orbital Period

204.590+0.6700.630days

M sin(i) (Earth masses)

42.10+1.831.78

M sin(i) (Jupiter masses)

0.1325+0.00580.0056

Eccentricity

0.1520+0.02900.0290

Epoch of Periastron

2458962.29+6.385.89days(BJD-TDB)

Argument of Periastron

189.7+11.410.8deg

Radial Velocity Semi-Amplitude

5.02+0.170.16m/s

Distance from Earth

65.0 pc (~212 ly)

Spectral Type

G3 V

Temperature

5737 K

Mass (Solar)

0.89 M☉

Radius (Solar)

1.18 R☉

Luminosity

Unknown

Planets in System

4

Stars in System

1

Coordinates (RA, Dec)

168.2267°, -34.4069°

Discovery Method

Radial Velocity

Discovery Year

2025

Data Sources

Source ID: TOI-1203 e

System Context

TOI-1203 e orbits TOI-1203 and was reported in 2025 and was detected with the Radial Velocity method.

Published measurements list a minimum mass of 42.1 Earth masses (M sin i) and an orbital period of 204.59 days.

Catalog data places the system at about 65 parsecs from Earth, a host star classified as G3 V, and 4 known planets in the system.

Host star

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

Open TOI-1203