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TOI-4791 b

Hot Jupiter Canis Major

TOI-4791 b is a hot Jupiter orbiting TOI-4791 in the constellation Canis Major. It lies about 1,072 light-years from Earth and was discovered in 2023 using the transit method.

12.44×Earth radius
734×Earth mass
4.3 dOrbital period
1,472 KEquilibrium temp.
0.07Earth similarity
1,072 lyDistance
2023Discovered

How Big Is TOI-4791 b?

Earth1.00 R⊕TOI-4791 b12.44 R⊕Jupiter11.21 R⊕
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TOI-4791 b has a radius of 12.44 times that of Earth, or 1.11 times the radius of Jupiter. Its mass is 734 times that of Earth, giving it a density of 2.09 g/cm³ — between that of rocky and gaseous planets.

Is TOI-4791 b in the Habitable Zone?

TOI-4791 b orbits inside the inner edge of the habitable zone of TOI-4791. So close to its star, surface conditions are far too hot for liquid water.

TOI-4791 b
Too hot Optimistic habitable zone Conservative habitable zone Too cold

Habitable zone of TOI-4791: 1.143–2.675 AU (conservative: 1.448–2.536 AU), per Kopparapu et al. (2014). Earth orbits the Sun at 1 AU.

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Temperature on TOI-4791 b

The equilibrium temperature of TOI-4791 b is about 1,472 K (1,199 °C) — hot enough to melt many metals. This estimate ignores any atmosphere, which could change surface temperatures dramatically — Earth's greenhouse effect adds about 33 °C. It receives 783 times the stellar energy that Earth gets from the Sun.

Orbit and Year Length

A year on TOI-4791 b — one full orbit around TOI-4791 — lasts 4.28 Earth days, shorter than Mercury's 88-day year. It orbits at an average distance of 0.056 AU — closer to its star than Mercury is to the Sun.

How Was TOI-4791 b Discovered?

TOI-4791 b was discovered in 2023 using the transit method, with observations from Transiting Exoplanet Survey Satellite (TESS).

The transit method watches a star for the tiny, regular dip in brightness that occurs when a planet crosses in front of it. The depth and timing of these dips reveal the planet's size and orbital period.

How Far Away Is TOI-4791 b?

TOI-4791 b is 1,072.4 light-years (328.8 parsecs) from Earth. Light arriving here tonight left the planet about 1,072 years ago. A probe traveling at the speed of Voyager 1 — about 17 km/s, the fastest outbound spacecraft ever launched — would need roughly 18,874,240 years to make the journey.

Earth Similarity Index

The Earth Similarity Index (ESI) scores how physically similar a planet is to Earth, from 0 to 1, based on radius, density, escape velocity and surface temperature. TOI-4791 b scores 0.07, ranking #4,866 of 5,568 planets with a known ESI. For reference, Mars scores about 0.70.

The Host Star: TOI-4791

TOI-4791

Surface temperature
6,058 K (Sun: 5,772 K)
Mass
1.24 M☉
Radius
1.41 R☉
Luminosity
2.4000 L☉
Age
3.3 billion years (Sun: 4.6)

Planetary System

TOI-4791 b is the only planet known to orbit TOI-4791 so far.

TOI-4791 b — Complete Data

Radius12.442 Earth radii (1.110 Jupiter radii)
Mass734.18 Earth masses (2.310 Jupiter masses)
Density2.09 g/cm³ (Earth: 5.51)
Orbital period4.28 days
Orbital distance0.056 AU
Equilibrium temperature1,472 K (1,199 °C)
Stellar irradiation783.20× Earth
Earth Similarity Index0.07
Distance from Earth1,072.4 light-years (328.8 parsecs)
ConstellationCanis Major
Discovery methodTransit
Discovery facilityTransiting Exoplanet Survey Satellite (TESS)
Discovery year2023

Data: NASA Exoplanet Archive, last updated 2023-02-27. Earth Similarity Index: PHL @ UPR Arecibo.

Frequently Asked Questions About TOI-4791 b

Is TOI-4791 b habitable?

No — TOI-4791 b orbits too close to its star and is too hot for liquid water to exist on its surface.

How far away is TOI-4791 b?

TOI-4791 b is about 1,072 light-years from Earth in the constellation Canis Major. A spacecraft traveling as fast as Voyager 1 (about 17 km/s) would need roughly 18,874,240 years to get there.

How big is TOI-4791 b compared to Earth?

TOI-4791 b has 12.44 times the radius of Earth and about 734 times its mass.

How long is a year on TOI-4791 b?

One orbit around TOI-4791 takes 4.3 Earth days — short enough that 85 of its years would fit into one Earth year.

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