Rogue Moons: Warmth Without a Star ✎ express

Original: "Habitability of Tidally Heated H$$_2$$-Dominated Exomoons around Free-Floating Planets"
arXiv:2602.05378 · 2026-02-05 · arXiv non-exclusive · independent analysis · 1 min
Moons of rogue planets can retain liquid water for billions of years thanks to tidal heat and a hydrogen atmosphere that acts like a warm blanket.

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Rogue planets, ejected from star systems, may harbor life on their moons. A moon of such a planet can preserve heat and liquid water for billions of years. The whole secret lies in a reliable "blanket" and an internal "stove."

The stove is tidal forces: they squeeze and stretch the moon's interior, heating it up like kneading clay.

But without a blanket, heat escapes. Carbon dioxide is a poor insulator: it freezes out too easily. A dense hydrogen envelope acts like a down comforter, trapping heat. This allows liquid water to exist for up to 4.3 billion years.

A surprising bonus: tides create wet-dry cycles, which, as it turns out, help assemble RNA chains — the first step toward life.

Add a bit of carbon, nitrogen, and ammonia to the atmosphere, and you get an alkaline environment, perfect for the chemistry of life. Even in the pitch darkness of interstellar space, warm worlds can bloom.

The hydrogen "fur coat" of such a moon can weigh as much as several Earth oceans, yet remain transparent — on the surface, eternal twilight, but warm.

Scientists
Charles-Augustin de CoulombJohannes RydbergTheodore LymanDaniel BernoulliLeonhard EulerArchimedes
Concepts
hydrogen atmosphere habitability hot jupiter atmospheres exoplanet atmospheres tidal heating habitable zone terrestrial exoplanet europa marine heatwave titan exomoon red dwarf habitability free-floating planet exoplanets around red dwarfs tidal migration sulfur dioxide ocean-atmosphere coupling water vapor sub neptune formation planetary atmospheric loss