Why is this a Water World?Your planet has abundant oxygen (27.8%) and hydrogen (12.2%), creating extensive water coverage while in the habitable temperature zone.
Water worlds have deep global oceans covering most or all of their surface. They form when planets have high water content and orbit in the habitable zone.
Matched on physical properties only — but pulsar planets are real: the first exoplanets ever confirmed (PSR B1257+12, 1992) orbit a neutron star.Discovered 2024 via radial velocity · 12 light-years awaySource: NASA Exoplanet Archive
Tidal braking locked the planet to its moon: one face forever moonward.
Tidal flexing melts its interior: an actively volcanic surface (Io-like).
Moon 2merged0.010% - 9.1 radii
Merged with an adjacent moon: too close for both to hold a stable orbit.
Moon 3merged0.0032% - 9.3 radii
Merged with an adjacent moon: too close for both to hold a stable orbit.
Moon 4stableCarbon-rich0.010% - 23.5 radii
Small and distant: a quiet, stable companion.
Moon 5stableSulfur-rich0.00022% - 7.4 radii
Small and distant: a quiet, stable companion.
Moon 6stableNitrogen ices lost: water ice0.010% - 11.2 radii
Small and distant: a quiet, stable companion.
Too warm for nitrogen and methane frost and too small to hold them as an atmosphere: those ices escaped to space, leaving water ice.
+4 chemistry: tidal pools cycle wet and dry - a boost for prebiotic chemistry
Habitability
✓ Conditions could support lifeThis planet’s modelled conditions could support biological processes: stable temperatures, liquid water and the chemistry life as we know it needs. That makes life possible, not present.