Lava Oceans of Exoplanets express

Original: "Magma Ocean Waves and Thermal Variability on Lava Worlds"
· Mohammad Farhat, Eugene Chiang
arXiv:2601.07080v2 · 2026-01-11 · CC BY 4.0 · 1 min
Tidal forces melt entire planets, forging lava oceans with waves kilometers high.

A planet whose orbit is a little stretched dives closer to its star each pass, then backs away. The varying gravity heats it up, solid rocks melt, becoming an ocean of lava.

If a year on such a planet is shorter than a day, even its core becomes liquid.

On the night side, a frozen crust acts as a shore. Tidal waves crash against it, collide, and spawn wandering hot spots. As a result, the planet’s glow flickers erratically, like a candle flame. Waves can rise several kilometers high — slow-moving stone ridges crawling across the scorching expanse.

The temperature of these lava oceans is higher than in a smelting furnace: around 3000°C.

Lava worlds like Mustafar from Star Wars turn out even more turbulent than in fiction, thanks to tides.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Concepts
magma ocean marine heatwave tidal heating tidal migration terrestrial exoplanet mantle dayside hydrogen atmosphere ocean current Kelvin wave hot jupiter tropical cyclone rocky planet protoplanetary disk dynamics plasma wave sea surface temperature sea surface temperature anomaly protoplanetary disk winds galactic winds gravitational waves