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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 8.

Best-fitting Voigt parameters as a function of temperature (solid black circles). Polynomial fits to the parameters using Equation (7) and the values in Table 1 (black line). A Voigt function and these polynomials reproduce the HDO band at any temperature between 150 and 10 K.

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