TOI-969 c
Orbiting TOI-969
TOI-969 c is an exoplanet orbiting the star TOI-969, discovered in 2022 using the Radial Velocity method.
Minimum Mass (M sin i)
3591.46
Earth masses
Orbital Period
1700.0
days
Distance
77.3
parsecs
Equilibrium Temp
96
K
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
3591.46
Radial-velocity minimum
Equilibrium Temperature
96 K
Parameter source: Lillo-Box et al. 2023
Orbital Period
1700.000+290.000−280.000days
Semi-Major Axis
2.5200+0.2700−0.2900au
M sin(i) (Earth masses)
3591.46+349.61−286.05
M sin(i) (Jupiter masses)
11.3000+1.1000−0.9000
Eccentricity
0.6280+0.0430−0.0360
Argument of Periastron
208.5+7.8−7.3deg
Distance from Earth
77.3 pc (~252 ly)
Spectral Type
K V
Temperature
4435 K
Mass (Solar)
0.73 M☉
Radius (Solar)
0.67 R☉
Luminosity
Unknown
Planets in System
2
Stars in System
1
Coordinates (RA, Dec)
115.1367°, 2.0986°
Discovery Method
Radial Velocity
Discovery Year
2022
Source ID: TOI-969 c
TOI-969 c orbits TOI-969 and was reported in 2022 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 3,591.46 Earth masses (M sin i), an orbital period of 1,700 days, and an equilibrium temperature near 96 K.
Catalog data places the system at about 77.3 parsecs from Earth, a host star classified as K V, 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-969More planets in this system