TOI-1759 b
Orbiting TOI-1759
TOI-1759 b is an exoplanet orbiting the star TOI-1759, discovered in 2022 using the Transit method. It is a Mini-Neptune world.
Radius
3.14
Earth radii
Mass
10.80
Earth masses
Orbital Period
18.9
days
Distance
40.1
parsecs
Equilibrium Temp
443
K
Radius (Earth radii)
3.14
Mass (Earth masses)
10.80
Measured
Equilibrium Temperature
443 K
Parameter source: Espinoza et al. 2022
Orbital Period
18.850+0.000−0.000days
Semi-Major Axis
0.1177+0.0038−0.0038au
Planet Mass (Earth masses)
10.80+1.50−1.50
Planet Mass (Jupiter masses)
0.0340+0.0047−0.0047
Eccentricity
0.0000
Argument of Periastron
90.0deg
Radial Velocity Semi-Amplitude
3.64+0.50−0.51m/s
Distance from Earth
40.1 pc (~131 ly)
Spectral Type
M0.0 V
Temperature
4065 K
Mass (Solar)
0.61 M☉
Radius (Solar)
0.60 R☉
Luminosity
-1.06 log L☉
Planets in System
1
Stars in System
1
Coordinates (RA, Dec)
326.8517°, 62.7538°
Discovery Method
Transit
Discovery Year
2022
Source ID: TOI-1759 b
TOI-1759 b orbits TOI-1759 and was reported in 2022 and was detected with the Transit method.
Published measurements list a radius of 3.14 Earth radii, a mass of 10.8 Earth masses, an orbital period of 18.85 days, and an equilibrium temperature near 443 K.
Catalog data places the system at about 40.1 parsecs from Earth, a host star classified as M0.0 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 TOI-1759