HD 12484 b
Orbiting HD 12484
HD 12484 b is an exoplanet orbiting the star HD 12484, discovered in 2016 using the Radial Velocity method.
Minimum Mass (M sin i)
947.13
Earth masses
Orbital Period
58.8
days
Distance
48.3
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
947.13
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Hébrard et al. 2016
Orbital Period
58.830+0.080−0.080days
Semi-Major Axis
0.2970+0.0050−0.0050au
M sin(i) (Earth masses)
947.13+44.50−44.50
M sin(i) (Jupiter masses)
2.9800+0.1400−0.1400
Eccentricity
0.0700+0.0300−0.0300
Epoch of Periastron
2456699.00+5.00−5.00days(BJD)
Argument of Periastron
-35.0+40.0−40.0deg
Radial Velocity Semi-Amplitude
155.00+5.00−5.00m/s
Distance from Earth
48.3 pc (~158 ly)
Spectral Type
F8
Temperature
5920 K
Mass (Solar)
1.01 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
30.6115°, 2.8158°
Discovery Method
Radial Velocity
Discovery Year
2016
Source ID: HD 12484 b
HD 12484 b orbits HD 12484 and was reported in 2016 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 947.13 Earth masses (M sin i) and an orbital period of 58.83 days.
Catalog data places the system at about 48.3 parsecs from Earth, a host star classified as F8, 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 HD 12484