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A Cross-laboratory Comparison Study of Titan Haze Analogs: Surface Energy II

  • Authors: Eric C. Austin, Xinting Yu, 馨婷 余, Chao He, Cara Pesciotta, Ella Sciamma-O'Brien, Joshua A. Sebree, Jose Raul Montes-Bojorquez, Adis Husić, Erik White, Christopher R. Bond, Sarah M. Hörst, Farid Salama, Patricia McGuiggan

Eric C. Austin et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 4.

Surface energies of pristine and air-exposed tholins produced from 5% CH4 in N2 on glass, quartz, and mica: (a) ARC/COSmIC plasma, (b) JHU/PHAZER plasma, (c) JHU/PHAZER UV, and (d) UNI/PAC UV. Colored bars show total surface energy and identify the substrate; silver and gray segments show the dispersive and polar components, respectively. Black, blue, and red error bars denote 1σ uncertainties in the total, dispersive, and polar values, respectively.

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