This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: Neptune's moon and ring system stand out among the giant planets because of the strange imbalance between its one very large moon and its many tiny moons. Its largest moon, Triton, makes up more than 99% of the mass of all satellites orbiting the planet while orbiting retrograde compared with Neptune's rotation.
The predominant theory is that Triton is a captured Kuiper Belt object that caused a major disruption in Neptune's early moon system. Now, a new study published in Science Advances provides spectroscopic evidence to support this theory. When a group of researchers recently analyzed data from the James Webb Space Telescope's (JWST) near-infrared spectrograph (NIRSpec), they found something they didn't expect: signs of clay-like minerals on two of Neptune's small moons and its rings.
The team says no similar feature has ever been detected on any outer solar system bodies beyond Jupiter. The finding is odd because these magnesium-rich phyllosilicates indicate extensive alteration caused by liquid water. Yet the two moons in question, Larissa and Galatea, and the rings are far too cold for liquid water near the surface.
The team also did not detect any water ice there, meaning the magnesium-rich phyllosilicates formed somewhere else, such as the warmer interior of a larger body. The study authors write, "The advanced degree of aqueous alteration experienced by these bodies may be related to their size, with larger objects allowing convection of interior melt during (partial) internal differentiation, which effectively increases the water-rock ratio. The phyllosilicate component of the inner Neptunian moons is broadly consistent with Ceres and the largest main-belt asteroids, perhaps suggesting that they formed in differentiated parent bodies that are much larger than the moons' current sizes." The researchers think the most likely explanation is that the small moons re-formed from the exposed interior debris of larger ancient moons that were destroyed during Triton's violent capture.
This would mean that at least one of Neptune's primordial moons was large enough to contain a differentiated, heated core where the phyllosilicates formed. The early system may have been more like other moon systems and only became the unbalanced enigma it is today after the gravitational capture of Triton, which likely tore apart the primordial moons. The study authors write, "The inner Neptunian moons are therefore the only place in the solar system where we can directly probe the interior of an icy satellite or possibly a dwarf planet if the aqueous alteration occurred before the formation of Neptune's original system.
In either case, the presence of CM2-like phyllosilicates on Neptune's inner moons demonstrates that when heated sufficiently, outer solar system materials undergo a mineralogical evolution nearly identical to that observed in main-belt asteroids." Although the team thinks the most likely explanation is that these tiny moons are made up of primordial moon remnants, they note another possibility. They say another large Kuiper Belt object could have been torn apart near Neptune and delivered phyllosilicate-bearing interior material to the system. However, a previous study on another of Neptune's moons suggests otherwise.
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