HIP 19976 b
Orbiting HIP 19976
HIP 19976 b is an exoplanet orbiting the star HIP 19976, discovered in 2022 using the Radial Velocity method.
Minimum Mass (M sin i)
21.61
Earth masses
Orbital Period
50.7
days
Distance
40.3
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
21.61
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Feng et al. 2022
Orbital Period
50.659+0.063−0.078days
Semi-Major Axis
0.2340+0.0090−0.0100au
M sin(i) (Earth masses)
21.61+2.86−5.09
M sin(i) (Jupiter masses)
0.0680+0.0090−0.0160
Eccentricity
0.3040+0.2000−0.1450
Epoch of Periastron
2455579.02+1.56−40.78days(BJD)
Argument of Periastron
188.9+26.7−44.1deg
Radial Velocity Semi-Amplitude
5.12+0.81−1.01m/s
Distance from Earth
40.3 pc (~131 ly)
Spectral Type
Unknown
Temperature
Unknown
Mass (Solar)
0.67 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
2
Coordinates (RA, Dec)
64.2598°, -40.7985°
Discovery Method
Radial Velocity
Discovery Year
2022
Source ID: HIP 19976 b
HIP 19976 b orbits HIP 19976 and was reported in 2022 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 21.61 Earth masses (M sin i) and an orbital period of 50.66 days.
Catalog data places the system at about 40.3 parsecs from Earth 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 19976