Ultrahot planet hides under a gas blanket ✛

Original: "A Thick Volatile Atmosphere on the Ultrahot Super-Earth TOI-561 b"
arXiv:2509.17231 · 2025-09-21 · CC BY 4.0 · 1 min
The Webb telescope discovered: planet TOI-561 b is wrapped in a dense gas blanket, even as its star scorches relentlessly.

For a long time, planets squeezed right up against their star were thought to be bare rocky spheres. Temperatures in the thousands of degrees strip away any gas envelope. But the James Webb Space Telescope showed: the ultrahot exoplanet TOI-561 b is wrapped in a dense blanket of gases.

The planet completes a full orbit around the star in just 10 hours. It was expected that its dayside would heat up to 3000 °C and glow in infrared light like a furnace. But the spectrum, the splitting of light into colors, revealed a much fainter glow. This means a warm layer of atmosphere, like a blanket, traps the heat near the surface.

Where did it come from? The likely source is an ocean of molten magma.

Molten rock dissolves and traps gases, like soda holds carbon dioxide bubbles.

So the planet acquired a new gas envelope that lasts longer than expected. The surprise is that, at nearly the size of Neptune, this world weighs as much as Mars, a fluffy giant among scorching rocks.

At Neptune's size, TOI-561 b weighs as much as Mars — one of the fluffiest super-Earths.

The magma ocean on TOI-561 b brings to mind Mustafar, the fiery world from Star Wars.

T_{d,max} = T_{irr} (1 - A_b) f^{1/4}
Relates the irradiation temperature, Bond albedo, and heat redistribution factor
Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Concepts
hot jupiter atmospheres terrestrial exoplanet exoplanet atmosphere super earth rocky planet wolf rayet star multi planet systems europa hydrogen atmosphere dayside sub neptune hydrogen envelope ozone layer titanium oxide exoplanets around red dwarfs protoplanetary disk dynamics mercury tess sub neptune formation planetary atmospheric loss