HD 167768 b
Orbiting HD 167768
HD 167768 b is an exoplanet orbiting the star HD 167768, discovered in 2022 using the Radial Velocity method.
Minimum Mass (M sin i)
270.15
Earth masses
Orbital Period
20.7
days
Distance
107.2
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
270.15
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Teng et al. 2023
Orbital Period
20.653+0.003−0.004days
Semi-Major Axis
0.1512+0.0058−0.0063au
M sin(i) (Earth masses)
270.15+38.14−34.96
M sin(i) (Jupiter masses)
0.8500+0.1200−0.1100
Eccentricity
0.1490+0.1010−0.0960
Epoch of Periastron
2454594.07+3.10−2.25days(BJD)
Argument of Periastron
58.7+49.6−45.3deg
Radial Velocity Semi-Amplitude
61.06+6.74−6.96m/s
Distance from Earth
107.2 pc (~350 ly)
Spectral Type
G8 III
Temperature
4851 K
Mass (Solar)
1.08 M☉
Radius (Solar)
9.70 R☉
Luminosity
1.67 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
274.2213°, -3.0086°
Discovery Method
Radial Velocity
Discovery Year
2022
Source ID: HD 167768 b
HD 167768 b orbits HD 167768 and was reported in 2022 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 270.15 Earth masses (M sin i) and an orbital period of 20.65 days.
Catalog data places the system at about 107.2 parsecs from Earth, a host star classified as G8 III, 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 167768