HD 126525 b
Orbiting HD 126525
HD 126525 b is an exoplanet orbiting the star HD 126525, discovered in 2018 using the Radial Velocity method.
Minimum Mass (M sin i)
75.33
Earth masses
Orbital Period
960.4
days
Distance
37.7
parsecs
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
75.33
Radial-velocity minimum
Equilibrium Temperature
Unknown
Parameter source: Barbato et al. 2018
Orbital Period
960.410+6.190−6.330days
Semi-Major Axis
1.8370+0.0100−0.0100au
M sin(i) (Earth masses)
75.33+0.64−0.64
M sin(i) (Jupiter masses)
0.2370+0.0020−0.0020
Eccentricity
0.0350+0.0390−0.0240
Epoch of Periastron
2456161.70+534.80−215.70days(BJD)
Argument of Periastron
247.5+76.2−184.1deg
Radial Velocity Semi-Amplitude
5.26+0.25−0.25m/s
Distance from Earth
37.7 pc (~123 ly)
Spectral Type
Unknown
Temperature
5638 K
Mass (Solar)
0.90 M☉
Radius (Solar)
0.98 R☉
Luminosity
Unknown
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
216.8853°, -51.9329°
Discovery Method
Radial Velocity
Discovery Year
2018
Source ID: HD 126525 b
HD 126525 b orbits HD 126525 and was reported in 2018 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 75.33 Earth masses (M sin i) and an orbital period of 960.41 days.
Catalog data places the system at about 37.7 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 126525