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Super-Earth

TOI-5789 b

Orbiting TOI-5789 | 20.5 parsecs away

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TOI-5789 b is a Super-Earth exoplanet (a planet larger than Earth but smaller than Neptune) with a mass of 2.1 Earth masses. Its scorching equilibrium temperature of 1201 K (928°C) makes it far too hot for liquid water. Despite its name, Super-Earths are not necessarily habitable; the term refers only to size. The planet completes one orbit around its star every 2.8 Earth days. It was discovered in 2026 using the radial velocity method. It orbits the K-type star TOI-5789, located approximately 20 parsecs (67 light-years) from Earth.

2026

Discovered

2.1

Earth Masses

1201

Temperature (K)

Discovery Information

Discovery MethodRadial Velocity
Discovery Year2,026
Discovery FacilityMultiple Observatories

Orbital Properties

Orbital Period2.7637 days
Semi-Major Axis0.0361 AU
Eccentricity0

Physical Properties

Mass (Jupiter)0.0067 MJ
Mass (Earth)2.12 M⊕
Eq. Temperature1,201 K
Planetary Extremes

Where TOI-5789 b sits on the spectrum of all known exoplanets.

Mass2.1 M⊕
FeatherweightColossus
Temperature1201 K
FrozenInferno
Year Length2.8 days
LightningGlacial
Star Distance0.036 AU
ScorchedFrozen exile
Star System View
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Orbit Comparison
EarthTOI-5789 b
Earth: 365.25 days (1 AU)TOI-5789 b: 2.8 Earth days (0.036 AU)
Host Star: TOI-5789

Spectral TypeK1 V
Effective Temperature5,185 K
Mass0.821 M☉
Radius0.833 R☉
Size vs Sun1.20x smaller
Luminosity0.469 L☉
Luminosity vs Sun2.1x dimmer
Metallicity [Fe/H]-0.12
Distance (pc)20.4581 pc
Distance (ly)66.7 light-years

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