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How Hydrogen and Magma Create Water Deep Inside Planets ⚡ экспресс

Original: "Building Wet Planets through High-Pressure Magma-Hydrogen Reactions"
arXiv:2511.06507 · 2025-11-09 · CC BY 4.0 · ⏱ 1 min · Exoplanets
Experiment: Hot hydrogen steals oxygen from molten rock, producing water — up to 10% of the planet's mass.
Abstract

Experiments show that deep inside sub-Neptunes (mid-size planets), scorching, dense hydrogen mingles with magma and squeezes out water—up to tens of percent by weight, way more than old models ever predicted. That means a planet born brimming with hydrogen can turn into a water world without ever drifting toward its star. So spotting water-rich atmospheres on exoplanets isn't automatically a clue they were born on the frigid fringes. This insight shakes up how we connect a planet's makeup to where it formed.

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Sub-Neptunes — worlds slightly smaller than Neptune — are common among exoplanets. They are detected using the transit method (by the dimming of a star), pioneered by William Borucki. Previously, it was thought that such planets were either dry and surrounded by hydrogen, or wet, with large amounts of water. The wet ones supposedly formed far out, where ice gathers, and then migrated closer to their stars. A new experiment breaks this mold.

In the lab, a mixture of hydrogen and silicate melt (magma) was compressed at thousands of degrees. The planet’s depths acted like an alchemical furnace: hydrogen aggressively ripped oxygen from minerals, and from the scorching rock, water was born. This reaction runs to completion: silicon goes into a metallic alloy, and every kilogram of magma yields up to a hundred grams of water — nearly half a cup. The mass fraction of water reached tens of percent, far higher than old estimates based on ideal gas models.

This means a planet with a hydrogen atmosphere and a magma ocean can transform into a water world without leaving its orbit. Atmospheric analysis using spectroscopy (breaking down light) is now unreliable for determining a planet’s place of birth. Detecting water doesn’t prove migration — the planet could have flooded itself. Astronomers studying exoplanets will have to rewrite their biographies.

🎯 One kilogram of silicate magma, after reacting with hydrogen, can yield up to 100 grams of water — that’s nearly half a cup of liquid born right in the planet’s interior.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Tags
exoplanet hydrogen Water transit method spectroscopy
Laws
Doppler effectKepler's third lawCoulomb's lawMaxwell's equationsPlanck's lawPlanck–Einstein relation
Original: arXiv:2511.06507 · CC BY 4.0 · bridge42worlds