HD 10975 b
Orbiting HD 10975
HD 10975 b is an exoplanet orbiting the star HD 10975, discovered in 2021 using the Radial Velocity method.
Minimum Mass (M sin i)
143.02
Earth masses
Orbital Period
283.8
days
Distance
116.5
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
143.02
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Teng et al. 2022
Orbital Period
283.800+12.700−0.100days
Semi-Major Axis
0.9500+0.0600−0.0800au
M sin(i) (Earth masses)
143.02+19.07−47.67
M sin(i) (Jupiter masses)
0.4500+0.0600−0.1500
Eccentricity
0.4420+0.0400−0.3890
Epoch of Periastron
2455450.70+29.10−182.90days(JD)
Argument of Periastron
135.0+153.0−35.0deg
Radial Velocity Semi-Amplitude
12.30+0.20−3.50m/s
Distance from Earth
116.5 pc (~380 ly)
Spectral Type
K0 III
Temperature
4840 K
Mass (Solar)
1.41 M☉
Radius (Solar)
11.16 R☉
Luminosity
1.79 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
27.1628°, 37.9528°
Discovery Method
Radial Velocity
Discovery Year
2021
Source ID: HD 10975 b
HD 10975 b orbits HD 10975 and was reported in 2021 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 143.02 Earth masses (M sin i) and an orbital period of 283.8 days.
Catalog data places the system at about 116.5 parsecs from Earth, a host star classified as K0 III, and 1 known planet in the system.
Host star
Explore the stellar record for this system to compare temperature, spectral type, and known planets.
Open HD 10975