HD 14787 b
Orbiting HD 14787
HD 14787 b is an exoplanet orbiting the star HD 14787, discovered in 2018 using the Radial Velocity method.
Minimum Mass (M sin i)
356.29
Earth masses
Orbital Period
676.6
days
Distance
119.1
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
356.29
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Luhn et al. 2019
Orbital Period
676.600+8.100−8.100days
Semi-Major Axis
1.7000+0.1900−0.1900au
M sin(i) (Earth masses)
356.29+21.93−21.93
M sin(i) (Jupiter masses)
1.1210+0.0690−0.0690
Eccentricity
0.1550+0.0730−0.0730
Epoch of Periastron
2455555.00+49.00−49.00days(JD)
Argument of Periastron
343.0+28.0−28.0deg
Radial Velocity Semi-Amplitude
20.70+1.30−1.30m/s
Distance from Earth
119.1 pc (~389 ly)
Spectral Type
Unknown
Temperature
4946 K
Mass (Solar)
1.43 M☉
Radius (Solar)
5.01 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
35.8085°, 10.8368°
Discovery Method
Radial Velocity
Discovery Year
2018
Source ID: HD 14787 b
HD 14787 b orbits HD 14787 and was reported in 2018 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 356.29 Earth masses (M sin i) and an orbital period of 676.6 days.
Catalog data places the system at about 119.1 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 HD 14787