HD 1690 b
Orbiting HD 1690
HD 1690 b is an exoplanet orbiting the star HD 1690, discovered in 2010 using the Radial Velocity method.
Minimum Mass (M sin i)
2793.73
Earth masses
Orbital Period
533.0
days
Distance
752.6
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
2793.73
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Stassun et al. 2017
Orbital Period
533.000+1.700−1.700days
Semi-Major Axis
1.3600+0.0900−0.0900au
M sin(i) (Earth masses)
2793.73+1153.72−1153.72
M sin(i) (Jupiter masses)
8.7900+3.6300−3.6300
Eccentricity
0.6400+0.0400−0.0400
Radial Velocity Semi-Amplitude
190.00+29.00−29.00m/s
Distance from Earth
752.6 pc (~2455 ly)
Spectral Type
Unknown
Temperature
4374 K
Mass (Solar)
1.86 M☉
Radius (Solar)
21.66 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
5.3056°, -8.2811°
Discovery Method
Radial Velocity
Discovery Year
2010
Source ID: HD 1690 b
HD 1690 b orbits HD 1690 and was reported in 2010 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 2,793.73 Earth masses (M sin i) and an orbital period of 533 days.
Catalog data places the system at about 752.6 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 1690