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A. Longobardo

As seen in: Color Research & Application
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Articles

Evidence for the Interior Evolution of Ceres from Geologic Analysis of Fractures

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By D. L. Buczkowski, N. Schmedemann, C. A. Raymond, A. I. Ermakov, D. O'Brien, S. Marchi, A. Longobardo, C. T. Russell, R. Fu, J. C. Castillo-Rogez, S. D. King, M. T. Bland, M. Neveu
| Color Research & Application Verified
Ceres is the largest asteroid belt object, and the Dawn spacecraft observed Ceres since 2015. Dawn observed two morphologically distinct linear features on Ceres's surface: secondary crater chains and pit chains. Pit chains provide unique insights into Ceres's interior evolution. We interpret pit chains called the Samhain Catenae as the surface expression of subsurface fractures.
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Spectral Analysis of Ahuna Mons from Dawn mission's Visible-Infrared Spectrometer

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By A. Raponi, M. Ciarniello, K. Stephan, E. Ammannito, C. T. Russell, C. A. Raymond, F. Zambon, F. Tosi, L. A. McFadden, F. G. Carrozzo, A. Longobardo, K. Krhon, E. Palomba, C. M. Pieters
| Color Research & Application Verified
Ahuna Mons is the highest mountain on Ceres. A unique complex in terms of size, shape, and morphology, Ahuna is bordered by flanks of the talus around its summit. Recent work by Ruesch et al. [2016] based on Dawn's Framing Camera images shed light on the possible origin of Ahuna Mons. According to Ruesch et al. [2016], Ahuna Mons is formed by a volcanic process involving the ascent of cryomagma and extrusion onto the surface followed by dome development and subsequent spreading.
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