WASP-76 b

WASP-76 b

Planet· orbits the Sun

WASP-76 b — a bloated ultra-hot Jupiter (1.85 Jupiter radii, ~0.9 Jupiter masses) orbiting every 1.8 days with a dayside near 2,400°C. It is famous for IRON RAIN: iron vaporises on the scorching day side, blows to the cooler night side, and — models indicate — condenses and falls as droplets of molten iron. Because it transits with a measured mass, its very low density is real. Its clouds have never been imaged.

Open in 3D viewSee WASP-76 b in the live, interactive 3D map

Key facts

Mass
1.70 × 10²⁷ kg
0.894 M♃ (284 M⊕)
Radius
132,389 km
20.8× wider than Earth
Surface gravity
6.46 m/s²
66% of Earth's
Year
1.81 Earth days
Distance from WASP-76
4,936,730 km

Science

Physical

Mass
1.70 × 10²⁷ kg · 0.894 M♃ (284 M⊕)
Radius
132,389 km · 20.8× wider than Earth
Density
175 kg/m³ · 0.17× water
Surface gravity
6.46 m/s² · 66% of Earth's
Escape velocity
41.4 km/s · 3.7× Earth's

Orbital

Semi-major axis
4,936,730 km
Eccentricity
0
Inclination
0.00 °
Orbital period
43.44 hours
Perihelion
4,936,730 km
Aphelion
4,936,730 km
Mean orbital velocity
198 km/s

Atmosphere

Composition
Hydrogen-dominated with vaporised iron and other metals detected (ESPRESSO, 2020); models indicate iron condenses into rain on the nightside.

Composition

Bulk composition
A bloated ultra-hot Jupiter (1.85 Jupiter radii, ~0.9 Jupiter masses, real density from transit + mass). Its dayside is so hot (~2,400°C) that iron vaporises; in 2020 the ESPRESSO spectrograph traced iron vapour vanishing at the day-night boundary — read as iron condensing and raining down as molten droplets on the cooler night side. One of the most vivid pictures of alien weather. Never imaged.
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 Vision mode; Realism shows a plain spectral colour.

Radiation & temperature

Insolation
4,093 S⊕ · 4,093× the sunlight Earth receives
Equilibrium temperature
2,228 K (1955 °C)

Discovery & history

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

Found transiting in 2016; in 2020 ESPRESSO on the VLT traced iron vapour vanishing at the day-night boundary — read as iron condensing into rain.

Images

Images from open archives · credit shown per image