We use 1.4-4.6 micron multi-band photometry of the small inner Uranian and Neptunian satellites obtained with the James Webb Space Telescope’s near-infrared imager NIRCam to characterize their surface compositions.
We find that the satellites of the ice giants have, to first-order, similar compositions to one another, with a 3.0 micron absorption feature possibly associated with an O-H stretch, indicative of water ice or hydrated minerals.
Additionally, the spectrophotometry for the small ice giant satellites matches spectra of some Neptune Trojans and excited Kuiper belt objects, suggesting shared properties. Future spectroscopy of these small satellites is necessary to identify and better constrain their specific surface compositions.
Matthew Belyakov, M. Ryleigh Davis, Zachariah Milby, Ian Wong, Michael E. Brown
Comments: 14 pages, 5 figures, Accepted to the Planetary Science Journal Subjects: Earth and Planetary Astrophysics (astro-ph.EP) Cite as: arXiv:2404.06660 [astro-ph.EP] (or arXiv:2404.06660v1 [astro-ph.EP] for this version) Submission history From: Matthew Belyakov [v1] Wed, 10 Apr 2024 00:02:41 UTC (9,984 KB) https://arxiv.org/abs/2404.06660 Astrobiology,
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