HIP 74890 b
Orbiting HIP 74890
HIP 74890 b is an exoplanet orbiting the star HIP 74890, discovered in 2016 using the Radial Velocity method.
Minimum Mass (M sin i)
762.79
Earth masses
Orbital Period
822.3
days
Distance
78.7
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
762.79
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Jones et al. 2016
Orbital Period
822.300+16.800−16.800days
Semi-Major Axis
2.1000+0.0900−0.0900au
M sin(i) (Earth masses)
762.79+95.35−95.35
M sin(i) (Jupiter masses)
2.4000+0.3000−0.3000
Eccentricity
0.0700+0.0700−0.0700
Epoch of Periastron
2459820.40+379.80−379.80days(JD)
Argument of Periastron
181.9+93.9−93.9deg
Radial Velocity Semi-Amplitude
36.50+2.70−2.70m/s
Distance from Earth
78.7 pc (~257 ly)
Spectral Type
K1 III
Temperature
4850 K
Mass (Solar)
1.74 M☉
Radius (Solar)
5.77 R☉
Luminosity
1.21 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
229.5715°, -41.4211°
Discovery Method
Radial Velocity
Discovery Year
2016
Source ID: HIP 74890 b
HIP 74890 b orbits HIP 74890 and was reported in 2016 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 762.79 Earth masses (M sin i) and an orbital period of 822.3 days.
Catalog data places the system at about 78.7 parsecs from Earth, a host star classified as K1 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 HIP 74890