HIP 71135 b
Orbiting HIP 71135
HIP 71135 b is an exoplanet orbiting the star HIP 71135, discovered in 2019 using the Radial Velocity method.
Minimum Mass (M sin i)
18.80
Earth masses
Orbital Period
87.2
days
Distance
32.3
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
18.80
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Feng et al. 2019
Orbital Period
87.190+0.381−0.381days
Semi-Major Axis
0.3350+0.0070−0.0070au
M sin(i) (Earth masses)
18.80+4.10−4.10
M sin(i) (Jupiter masses)
0.0592+0.0129−0.0129
Eccentricity
0.2100+0.1300−0.1300
Argument of Periastron
115.6+71.7−71.7deg
Radial Velocity Semi-Amplitude
3.71+0.79−0.79m/s
Distance from Earth
32.3 pc (~105 ly)
Spectral Type
M1
Temperature
4146 K
Mass (Solar)
0.66 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
218.2158°, -52.6465°
Discovery Method
Radial Velocity
Discovery Year
2019
Source ID: HIP 71135 b
HIP 71135 b orbits HIP 71135 and was reported in 2019 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 18.8 Earth masses (M sin i) and an orbital period of 87.19 days.
Catalog data places the system at about 32.3 parsecs from Earth, a host star classified as M1, 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 HIP 71135