TOI-791 b

Planet· orbits TOI-791

TOI-791 b — a planet as wide as Jupiter that weighs about nine and a half Earths, which makes it about a twentieth as dense as water: a tenth of Saturn, and far thinner than cork. It circles its star every 139 days, at about two-thirds the Earth-Sun distance, where the sunlight leaves it near 434 K. Both its size and its weight are measured, so the density is a real number rather than an inference — which is what makes it hard to explain.

Open in 3D viewSee TOI-791 b in the live, interactive 3D map

Key facts

Mass
5.67 × 10²⁵ kg
9.5 M⊕
Radius
70,913 km
11.1× wider than Earth
Surface gravity
0.753 m/s²
8% of Earth's gravity
Year
139 Earth days
Distance from TOI-791
0.602 AU

Science

Physical

Mass
5.67 × 10²⁵ kg · 9.5 M⊕
NASA Exoplanet Archive (Dransfield et al. 2026, MNRAS) — adopted transit + mass solution, read 2026-09-23
Radius
70,913 km · 11.1× wider than Earth
NASA Exoplanet Archive (Dransfield et al. 2026, MNRAS) — adopted transit + mass solution, read 2026-09-23
Density
38 kg/m³ · 0.038× water
Computed from mass and radius
Surface gravity
0.753 m/s² · 8% of Earth's gravity
Computed from mass and radius
Escape velocity
10.3 km/s · 92% of Earth's escape velocity
Computed from mass and radius

Orbital

Semi-major axis
0.602 AU
From the NASA Exoplanet Archive (transit + orbit fit)
Eccentricity
0.032
From the NASA Exoplanet Archive (transit + orbit fit)
Inclination
0.00 °
From the NASA Exoplanet Archive (transit + orbit fit)
Orbital period
139.3 days
From the NASA Exoplanet Archive (transit + orbit fit)
Perihelion
0.583 AU
Computed from the orbital elements
Aphelion
0.621 AU
Computed from the orbital elements
Mean orbital velocity
47 km/s
Computed from the orbital elements

Composition

Bulk composition
A transiting giant of 11.13 ± 0.37 Earth radii and 9.50 (+1.64/−1.81) Earth masses (Dransfield et al. 2026) — a measured density roughly a tenth of Saturn's and a twentieth of water's. Nothing is known of its composition beyond that: no atmospheric spectrum has been taken. A density this low normally implies an enormous, hot, extended envelope, which is straightforward for the young super-puffs that orbit close in and is not yet explained for a world this cool.
Cloud appearance
Appearance based on NASA/JPL-Caltech's artist's concept. No spacecraft has imaged this world, so its real appearance is unknown — The banded clouds shown are a representation of its class, shown only in Visual mode; Realism shows a plain spectral colour.

Radiation & temperature

Insolation
8.48 S⊕ · 8.48× the sunlight Earth receives
Computed from TOI-791's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).
Equilibrium temperature
434 K (161 °C)
The archive's computed equilibrium value — not measured.

Discovery & history

Method
Transit detection
Name
Designated 'b' under the IAU convention that letters a star's planets 'b', 'c', 'd'… in the order found (the star is the unwritten 'a'); no IAU proper name has been assigned.

Flagged by TESS in 2019 as candidate 791.01 and confirmed in 2026, when follow-up measurements weighed it and found a Jupiter-sized world with barely a Neptune's mass.

Images

No telescope has imaged this world — it is known only from the tiny dip it makes crossing its star. Only its host system has been pictured (see the system view); its true surface appearance is unknown.