HD 106270 b
Orbiting HD 106270
HD 106270 b is an exoplanet orbiting the star HD 106270, discovered in 2011 using the Radial Velocity method.
Minimum Mass (M sin i)
3219.62
Earth masses
Orbital Period
1888.0
days
Distance
93.8
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
3219.62
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Luhn et al. 2019
Orbital Period
1888.000+16.000−16.000days
Semi-Major Axis
3.3400+0.2000−0.2000au
M sin(i) (Earth masses)
3219.62+85.81−85.81
M sin(i) (Jupiter masses)
10.1300+0.2700−0.2700
Eccentricity
0.1850+0.0270−0.0270
Epoch of Periastron
2456635.00+37.00−37.00days(JD)
Argument of Periastron
3.3+6.1−6.1deg
Radial Velocity Semi-Amplitude
135.40+3.50−3.50m/s
Distance from Earth
93.8 pc (~306 ly)
Spectral Type
Unknown
Temperature
5509 K
Mass (Solar)
1.39 M☉
Radius (Solar)
2.66 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
183.4049°, -9.5136°
Discovery Method
Radial Velocity
Discovery Year
2011
Source ID: HD 106270 b
HD 106270 b orbits HD 106270 and was reported in 2011 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 3,219.62 Earth masses (M sin i) and an orbital period of 1,888 days.
Catalog data places the system at about 93.8 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 106270