HD 164595 b
Orbiting HD 164595
HD 164595 b is an exoplanet orbiting the star HD 164595, discovered in 2015 using the Radial Velocity method.
Minimum Mass (M sin i)
16.14
Earth masses
Orbital Period
40.0
days
Distance
28.3
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
16.14
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Courcol et al. 2015
Orbital Period
40.000+0.240−0.240days
Semi-Major Axis
0.2300au
M sin(i) (Earth masses)
16.14+2.72−2.72
M sin(i) (Jupiter masses)
0.0508+0.0086−0.0086
Eccentricity
0.0880+0.1200−0.0660
Epoch of Periastron
2456280.00+12.00−12.00days(BJD)
Argument of Periastron
145.0+160.0−110.0deg
Radial Velocity Semi-Amplitude
3.05+0.41−0.41m/s
Distance from Earth
28.3 pc (~92 ly)
Spectral Type
G2 V
Temperature
5790 K
Mass (Solar)
0.99 M☉
Radius (Solar)
Unknown
Luminosity
Unknown
Planets in System
1
Stars in System
2
Coordinates (RA, Dec)
270.1614°, 29.5727°
Discovery Method
Radial Velocity
Discovery Year
2015
Source ID: HD 164595 b
HD 164595 b orbits HD 164595 and was reported in 2015 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 16.14 Earth masses (M sin i) and an orbital period of 40 days.
Catalog data places the system at about 28.3 parsecs from Earth, a host star classified as G2 V, 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 164595