TOI-771 c
Orbiting TOI-771
TOI-771 c is an exoplanet orbiting the star TOI-771, discovered in 2025 using the Radial Velocity method.
Minimum Mass (M sin i)
2.87
Earth masses
Orbital Period
7.6
days
Distance
25.3
parsecs
Equilibrium Temp
365
K
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
2.87
Radial-velocity minimum
Equilibrium Temperature
365 K
Parameter source: Lacedelli et al. 2025
Orbital Period
7.610+0.030−0.030days
Semi-Major Axis
0.0460+0.0020−0.0020au
M sin(i) (Earth masses)
2.87+0.41−0.38
M sin(i) (Jupiter masses)
0.0090+0.0013−0.0012
Eccentricity
0.0650+0.0620−0.0450
Epoch of Periastron
2458573.80+2.50−2.50days(BJD)
Argument of Periastron
-82.0+88.0−84.0deg
Radial Velocity Semi-Amplitude
2.58+0.27−0.25m/s
Distance from Earth
25.3 pc (~82 ly)
Spectral Type
M3
Temperature
3370 K
Mass (Solar)
0.22 M☉
Radius (Solar)
0.23 R☉
Luminosity
-2.20 log L☉
Planets in System
2
Stars in System
1
Coordinates (RA, Dec)
164.1139°, -72.9852°
Discovery Method
Radial Velocity
Discovery Year
2025
Source ID: TOI-771 c
TOI-771 c orbits TOI-771 and was reported in 2025 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 2.87 Earth masses (M sin i), an orbital period of 7.61 days, and an equilibrium temperature near 365 K.
Catalog data places the system at about 25.3 parsecs from Earth, a host star classified as M3, 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-771More planets in this system