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Titania’s Deuterium Abundance and the Origin of Its Water

  • Authors: Stephen C. Tegler, Richard J. Cartwright, William M. Grundy, Bryan J. Holler, William A. Burris, Mark J. Loeffler, Christopher R. Glein, Ryan D. Wochner, Samantha H. Hemmelgarn

Stephen C. Tegler et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 1.

Spectrum of Titania’s leading hemisphere taken with JWST and NIRSpec (R. J. Cartwright 2026). Peak absorptions of the weak HDO and CO2 bands are observed at 4.14 and 4.27 μm, respectively. An artifact (A) of the data reduction process appears at 4.05 μm. The HDO band is distinct from the artifact and CO2 band. The feature at 3.1 μm is the H2O Fresnel peak.

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