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Tracing the Source of Carbon Oxides on the Large Moons of Uranus

  • Authors: Richard J. Cartwright, Sasha Cryan, Rosario Brunetto, Apolline Leclef, Eric Quirico, Bryan J. Holler, William M. Grundy, Tom A. Nordheim, Ujjwal Raut, Matthew M. Hedman, Riley A. DeColibus, Chloe B. Beddingfield, Marc Neveu, Christopher R. Glein, Sara Faggi, Geronimo L. Villanueva, Noemi Pinilla-Alonso, Stephanie M. Menten

Richard J. Cartwright et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 1.

NIRSpec IFU (G395M/F290LP) reflectance spectra and 1σ uncertainties for the leading and trailing hemispheres of Ariel, Umbriel, Titania, and Oberon, normalized to 1 at 3.59 μm and vertically offset for clarity. The spectra of Ariel, originally reported in R. J. Cartwright et al. (2024a), were rereduced here using an updated version of the calibration pipeline, revealing additional spectral structure between 5.1 and 5.25 μm that was not previously presented.

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