HATS-59 c
Orbiting HATS-59
HATS-59 c is an exoplanet orbiting the star HATS-59, discovered in 2018 using the Radial Velocity method.
Minimum Mass (M sin i)
4036.44
Earth masses
Orbital Period
1422.0
days
Distance
642.9
parsecs
Equilibrium Temp
176
K
Radius (Earth radii)
Unknown
Minimum Mass, M sin(i) (Earth masses)
4036.44
Radial-velocity minimum
Equilibrium Temperature
176 K
Parameter source: Sarkis et al. 2018
Orbital Period
1422.000+14.000−14.000days
Semi-Major Axis
2.5040+0.0350−0.0350au
M sin(i) (Earth masses)
4036.44+276.51−276.51
M sin(i) (Jupiter masses)
12.7000+0.8700−0.8700
Eccentricity
<0.083
Radial Velocity Semi-Amplitude
224.00+14.00−14.00m/s
Distance from Earth
642.9 pc (~2097 ly)
Spectral Type
Unknown
Temperature
5670 K
Mass (Solar)
1.04 M☉
Radius (Solar)
1.04 R☉
Luminosity
-0.00 log L☉
Planets in System
2
Stars in System
1
Coordinates (RA, Dec)
170.3243°, -22.3882°
Discovery Method
Radial Velocity
Discovery Year
2018
Source ID: HATS-59 c
HATS-59 c orbits HATS-59 and was reported in 2018 and was detected with the Radial Velocity method.
Published measurements list a minimum mass of 4,036.44 Earth masses (M sin i), an orbital period of 1,422 days, and an equilibrium temperature near 176 K.
Catalog data places the system at about 642.9 parsecs from Earth and 2 known planets in the system.
Host star
Explore the stellar record for this system to compare temperature, spectral type, and known planets.
Open HATS-59More planets in this system