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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 7.

Comparison of the best-fitting Gaussian (dashed–dotted line), Lorentzian (dotted line), and Voigt (dashed line) band profiles to the HDO band measured at 80 K (red line). The Voigt profile provides a closer match to the HDO band than the Gaussian or Lorentzian profile, thereby enabling us to provide analytical expressions for HDO effective optical constants using Equations (3)–(7) and Table 1.

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