Compositional Similarities and Distinctions between Titan's Evaporitic Terrains
Shannon MacKenzie, Jason Barnes

TL;DR
This study investigates the compositional similarities and differences among Titan's evaporitic terrains, revealing multiple types of soluble materials and complex surface processes that suggest a dynamic formation history.
Contribution
It identifies specific spectral features associated with Titan's evaporites and highlights the compositional diversity and complexity of their surface structures.
Findings
Similar absorption features in equatorial and polar deposits suggest common liquid history.
Presence of multiple evaporite types indicates diverse soluble materials.
Surface properties vary, implying complex formation and alteration processes.
Abstract
We document the similarities in composition between the equatorial basins Tui Regio, Hotei Regio, and other 5-m-bright materials, notably the north polar evaporites, by investigating the presence and extent of an absorption feature at 4.92 m. In most observations, Woytchugga Lacuna, Ontario Lacus, MacKay Lacus, deposits near Fensal, some of the lakes and dry lake beds south of Ligeia, and the southern shores of Kraken Mare share the absorption feature at 4.92 \um observed in the spectra of Tui and Hotei. Besides Woytchugga and at Fensal, these 5-m-bright deposits are geomorphologically-substantiated evaporites. Thus, the similarity in composition strengthens the hypothesis that Tui and Hotei once contained liquid. Other evaporite deposits, however, do not show the 4.92 \um absorption, notably Muggel Lacus and the shores of Ligeia Mare at the north pole. This difference in…
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