Webb Detects 2.72-Micron Clay Signature in Neptune's Inner Moons and Rings
Updated
Updated · Astrobiology News · Aug 17
Webb Detects 2.72-Micron Clay Signature in Neptune's Inner Moons and Rings
3 articles · Updated · Astrobiology News · Aug 17
Summary
James Webb observations found Neptune’s rings and three inner moons—Larissa, Galatea and Proteus—carry unusual spectra, including a 2.72-micron absorption band tied to magnesium-rich phyllosilicates.
Those moons and rings also show deep 3-micron OH absorption but no evidence of water ice, making their composition distinct from other known outer solar system objects.
The clay-like minerals point to extensive aqueous alteration and likely formed inside primordial satellites later destroyed during Triton’s capture, or inside a tidally shredded dwarf planet.
That scenario suggests Neptune’s present inner moons and rings reaccreted from exposed deep-interior material, giving scientists a rare window into the makeup of differentiated icy bodies.