Worlds with Eternal Magma Oceans express

Original: "Most Rocky Sub-Neptunes are Molten: Mapping the Solidification Shoreline for Gas Dwarf Exoplanets"
arXiv:2512.05816 · 2025-12-05 · CC BY 4.0 · 1 min
Beneath the hydrogen envelope of most known sub-Neptunes, an eternal ocean of liquid magma likely churns.

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A star warms its planet like an oven warms a kettle. For most sub-Neptunes (worlds larger than Earth but smaller than Neptune), the heat is enough to keep an ocean of molten rock eternally churning beneath a hydrogen sky. A computer model revealed that 98% of such known planets remain molten inside — provided they truly resemble gas dwarfs with a light atmosphere of hydrogen.

This heat leaves distinctive chemical fingerprints. We can spot them with spectroscopy — breaking a distant planet’s light into a rainbow to read its makeup. These fingerprints will provide direct evidence of hidden magma oceans.

If a planet has a lot of oxygen inside and carbon outside, its atmosphere gets heavier and cools faster. But for most worlds, the internal fire hasn’t gone out. This flips our understanding upside down: we used to think such bodies freeze solid over billions of years, but it turns out their interiors are still blazing.

Sub-Neptunes are the most common planet type in our galaxy, yet none exist in our Solar System.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Concepts
sub neptune formation sub neptune exoplanets around red dwarfs super earth hydrogen atmosphere rocky planet red dwarf planets gas giant hot jupiter atmospheres magma ocean terrestrial exoplanet sulfur dioxide exoplanet atmospheres subsurface ocean crust gas exotic neutron star interior snow line protoplanetary disk dynamics planetary composition formation