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TOI-5210 b

Hot Jupiter Vulpecula

TOI-5210 b is a hot Jupiter orbiting TOI-5210 in the constellation Vulpecula. It lies about 985 light-years from Earth and was discovered in 2025 using the transit method.

10.73×Earth radius
82.0×Earth mass
4.6 dOrbital period
1,286 KEquilibrium temp.
985 lyDistance
2025Discovered

How Big Is TOI-5210 b?

Earth1.00 R⊕TOI-5210 b10.73 R⊕Jupiter11.21 R⊕
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TOI-5210 b has a radius of 10.73 times that of Earth, or 0.96 times the radius of Jupiter. Its mass is 82.0 times that of Earth, giving it a density of 0.36 g/cm³ — closer to gas planets like Jupiter (1.33 g/cm³).

Is TOI-5210 b in the Habitable Zone?

TOI-5210 b orbits inside the inner edge of the habitable zone of TOI-5210. So close to its star, surface conditions are far too hot for liquid water.

TOI-5210 b
Too hot Optimistic habitable zone Conservative habitable zone Too cold

Habitable zone of TOI-5210: 0.897–2.117 AU (conservative: 1.136–2.007 AU), per Kopparapu et al. (2014). Earth orbits the Sun at 1 AU.

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Temperature on TOI-5210 b

The equilibrium temperature of TOI-5210 b is about 1,286 K (1,013 °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 456 times the stellar energy that Earth gets from the Sun.

Orbit and Year Length

A year on TOI-5210 b — one full orbit around TOI-5210 — lasts 4.57 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. Its orbit is mildly elliptical (eccentricity 0.07).

How Was TOI-5210 b Discovered?

TOI-5210 b was discovered in 2025 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-5210 b?

TOI-5210 b is 985.3 light-years (302.1 parsecs) from Earth. Light arriving here tonight left the planet around the year 1041. A probe traveling at the speed of Voyager 1 — about 17 km/s, the fastest outbound spacecraft ever launched — would need roughly 17,341,280 years to make the journey.

The Host Star: TOI-5210

TOI-5210

Surface temperature
5,723 K (Sun: 5,772 K)
Mass
1.11 M☉
Radius
1.21 R☉
Luminosity
1.4200 L☉
Age
5.3 billion years (Sun: 4.6)

Planetary System

TOI-5210 b is the only planet known to orbit TOI-5210 so far.

TOI-5210 b — Complete Data

Radius10.727 Earth radii (0.957 Jupiter radii)
Mass82.00 Earth masses (0.258 Jupiter masses)
Density0.36 g/cm³ (Earth: 5.51)
Orbital period4.57 days
Orbital distance0.056 AU
Eccentricity0.066
Equilibrium temperature1,286 K (1,013 °C)
Stellar irradiation456.00× Earth
Distance from Earth985.3 light-years (302.1 parsecs)
ConstellationVulpecula
Discovery methodTransit
Discovery facilityTransiting Exoplanet Survey Satellite (TESS)
Discovery year2025

Data: NASA Exoplanet Archive, last updated 2025-07-29. Earth Similarity Index: PHL @ UPR Arecibo.

Frequently Asked Questions About TOI-5210 b

Is TOI-5210 b habitable?

No — TOI-5210 b orbits too close to its star and is too hot for liquid water to exist on its surface.

How far away is TOI-5210 b?

TOI-5210 b is about 985 light-years from Earth in the constellation Vulpecula. A spacecraft traveling as fast as Voyager 1 (about 17 km/s) would need roughly 17,341,280 years to get there.

How big is TOI-5210 b compared to Earth?

TOI-5210 b has 10.73 times the radius of Earth and about 82.0 times its mass.

How long is a year on TOI-5210 b?

One orbit around TOI-5210 takes 4.6 Earth days — short enough that 80 of its years would fit into one Earth year.

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