Surface Energy of the Titan Aerosol Analog "Tholin"
Xinting Yu, Sarah Horst, Chao He, Patricia McGuiggan, Kai Kristiansen,, Xi Zhang

TL;DR
This study measures the surface energy of Titan aerosol analogs ('tholin') produced by different methods, revealing their high cohesiveness and wetting properties, which impact particle growth, cloud formation, and surface interactions on Titan.
Contribution
It provides the first comprehensive measurement of surface energy for Titan aerosol analogs, linking physical properties to atmospheric and surface processes on Titan.
Findings
Tholin surface energy is around 60-70 mJ/m2.
High surface energy indicates high cohesiveness of haze particles.
Haze particles are likely good cloud condensation nuclei.
Abstract
The photochemical haze produced in the upper atmosphere of Titan plays a key role in various atmospheric and surface processes on Titan. The surface energy, one important physical properties of the haze, is crucial for understanding the growth of the haze particles and can be used to predict their wetting behavior with solid and liquid species on Titan. We produced Titan analog haze materials, so-called "tholin", with different energy sources and measured their surface energies through contact angle and direct force measurements. From the contact angle measurement, we found that the tholins produced by cold plasma and UV irradiation have total surface energy around 60-70 mJ/m2. The direct force measurement yields a total surface energy of ~66 mJ/m2 for plasma tholin. The surface energy of tholin is relatively high compared to common polymers, indicating its high cohesiveness. Therefore,…
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