Mineralogic mapping of the Av-9 Numisia quadrangle of Vesta

• Published in: Icarus (New York, N.Y. 1962) Vol. 259; pp. 116 - 128
• Main Authors: Frigeri, A., De Sanctis, M.C., Ammannito, E., Buczkowski, D., Combe, J.P., Tosi, F., Zambon, F., Rocchini, D., Jaumann, R., Raymond, C.A., Russell, C.T.
• Format: Journal Article
• Language: English
• Published: Elsevier Inc 01-10-2015
• Subjects: Asteroid vesta; Basins; Craters; Data reduction techniques; Density; Geological mapping; Geological processes; Mapping; Mathematical models; Mineralogy; Spectra; Vesta asteroid; Data reduction techniques; Geological processes; Asteroid vesta; Mineralogy
• ISSN: 0019-1035; 1090-2643
• DOI: 10.1016/j.icarus.2015.07.029

•We mapped the mineralogy of the Av-9 Numisia quadrangle of Vesta.•We developed a lithologic map of the Av-9 quadrangle.•The OH signature across the study area has been described.•We conclude that Vestalia Terra is composed of howarditic–diogenitic material.
In this manuscript we present the mineralogic mapping of the Av-9 Numisia quadrangle of Vesta using the most up-to-date data from the NASA–Dawn mission.
This quadrangle is located in Vesta’s equatorial zone (22° south to 22° north, 218° to 288° east, in Claudia coordinate system) and takes its name from the impact crater Numisia. The main feature, which dominates the quadrangle, is the Vestalia Terra plateau, a topographic high about 10km above the surrounding areas. To the south, this region fades into the Rheasilvia basin, while to the north it is bounded by the steep scarp of Postumia basin.
The Visible and Infrared mapping spectrometer (VIR) onboard NASA/Dawn provided the main data source for this work, at an unprecedented level of spatial and spectral resolution. In particular we are using spectral parameters to synthesize characteristics of the whole spectra into a single value. Pyroxene-related spectral parameters allow for the detection of lower crust or mantle material (diogenites) and upper crust material (eucrites) in the study area.
The combined analysis of albedo from the Framing Camera, the geologic map and the spectroscopic data offer an interesting opportunity to understand better the surface features of this region of Vesta, and their evolution.
Numisia, Cornelia, Fabia, Teia and Drusilla are the main craters in the study area, rich in bright and dark material outcrops, pitted terrains and OH-rich materials.
Using the spectral parameters we demonstrate that the internal composition of Vestalia Terra is mainly diogenite-rich howardite, as shown by materials excavated by Cornelia and Fabia, and the composition of the slope north of Vestalia Terra. This agrees with the strong positive Bouguer Anomaly observed in the area, indicating a higher density of these features in relation to the surrounding areas.
Besides the recently published works based on gravimetric modeling and geologic interpretation, the mineralogic mapping presented herein gives an additional contribution, in order to depict a more complete geologic history of the Numisia quadrangle of Vesta.