Lithologic Mapping of HED Terrains on Vesta using Dawn Framing Camera Color Data
Guneshwar Thangjam, Vishnu Reddy, Lucille Le Corre, Andreas Nathues,, Holger Sierks, Harald Hiesinger, Jian-Yang Li, Juan A. Sanchez, Christopher, T. Russell, Robert Gaskell, Carol Raymond

TL;DR
This study uses Dawn Framing Camera color data to map HED lithologies on Vesta, revealing its magmatic differentiation, impact history, and hemispherical compositional dichotomy, with diogenite-rich material indicating a differentiated crust.
Contribution
It introduces a novel application of lunar color parameters to identify and map HED terrains on Vesta, providing new insights into its petrologic evolution.
Findings
Identification of HED terrains using color parameters
Confirmation of hemispherical compositional dichotomy
Detection of diogenite-rich material in southern hemisphere
Abstract
The surface composition of Vesta, the most massive intact basaltic object in the asteroid belt, is interesting because it provides us with an insight into magmatic differentiation of planetesimals that eventually coalesced to form the terrestrial planets. The distribution of lithologic and compositional units on the surface of Vesta provides important constraints on its petrologic evolution, impact history and its relationship with Vestoids and howardite-eucrite-diogenite (HED) meteorites. Using color parameters (band tilt and band curvature) originally developed for analyzing lunar data, we have identified and mapped HED terrains on Vesta in Dawn Framing Camera (FC) color data. The average color spectrum of Vesta is identical to that of howardite regions, suggesting an extensive mixing of surface regolith due to impact gardening over the course of solar system history. Our results…
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