HIP 4845 b
Orbiting HIP 4845
HIP 4845 b is an exoplanet orbiting the star HIP 4845, discovered in 2020 using the Radial Velocity method.
Minimum Mass (M sin i)
14.40
Earth masses
Orbital Period
34.1
days
Distance
21.1
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
14.40
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Feng et al. 2020
Orbital Period
34.150+0.046−0.046days
Semi-Major Axis
0.1760+0.0070−0.0070au
M sin(i) (Earth masses)
14.40+3.00−3.00
M sin(i) (Jupiter masses)
0.0453+0.0094−0.0094
Eccentricity
0.2500+0.1400−0.1400
Epoch of Periastron
2454702.00+5.60−5.60days(JD)
Argument of Periastron
108.0+72.0−72.0deg
Radial Velocity Semi-Amplitude
4.05+0.86−0.86m/s
Distance from Earth
21.1 pc (~69 ly)
Spectral Type
Unknown
Temperature
Unknown
Mass (Solar)
0.62 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
15.5882°, -10.4246°
Discovery Method
Radial Velocity
Discovery Year
2020
Source ID: HIP 4845 b
HIP 4845 b orbits HIP 4845 and was reported in 2020 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 14.4 Earth masses (M sin i) and an orbital period of 34.15 days.
Catalog data places the system at about 21.1 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 4845