omi UMa b
Orbiting omi UMa
omi UMa b is an exoplanet orbiting the star omi UMa, discovered in 2012 using the Radial Velocity method.
Minimum Mass (M sin i)
1160.39
Earth masses
Orbital Period
1569.8
days
Distance
54.9
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
1160.39
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Teng et al. 2023
Orbital Period
1569.810+12.760−13.590days
Semi-Major Axis
3.6910+0.0200−0.0210au
M sin(i) (Earth masses)
1160.39+55.94−94.71
M sin(i) (Jupiter masses)
3.6510+0.1760−0.2980
Eccentricity
0.1490+0.0440−0.0790
Epoch of Periastron
2453348.80+132.60−84.10days(JD)
Argument of Periastron
40.8+30.9−21.4deg
Radial Velocity Semi-Amplitude
33.11+1.64−2.77m/s
Distance from Earth
54.9 pc (~179 ly)
Spectral Type
G4 II-III
Temperature
5075 K
Mass (Solar)
2.72 M☉
Radius (Solar)
13.84 R☉
Luminosity
2.06 log L☉
Planets in System
1
Stars in System
2
Coordinates (RA, Dec)
127.5650°, 60.7177°
Discovery Method
Radial Velocity
Discovery Year
2012
Source ID: omi UMa b
omi UMa b orbits omi UMa and was reported in 2012 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 1,160.39 Earth masses (M sin i) and an orbital period of 1,569.81 days.
Catalog data places the system at about 54.9 parsecs from Earth, a host star classified as G4 II-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 omi UMa