Synthesis of the special issue: The formation and evolution of Ceres’ Occator crater

Author:

Scully Jennifer E.C.,Bowling Timothy,Bu CaixiaORCID,Buczkowski Debra L.,Longobardo AndreaORCID,Nathues Andreas,Neesemann AdrianORCID,Palomba ErnestoORCID,Quick Lynnae C.ORCID,Raponi AndreaORCID,Ruesch Ottaviano,Schenk Paul M.,Stein Nathan T.,Thomas E.C.,Russell Christopher T.ORCID,Castillo-Rogez Julie C.,Raymond Carol A.,Jaumann Ralf

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference56 articles.

1. Why is Ceres so lumpy? Surface deformation induced by solid-state subsurface flow;Bland,2018

2. Post-impact thermal structure and cooling timescales of Occator crater on asteroid 1 Ceres;Bowling;Icarus,2018

3. Ganymede crater dimensions – Implications for central peak and central pit formation and development;Bray;Icarus,2012

4. Stability of hydrated carbonates on Ceres;Bu;Icarus,2018

5. Tectonic analysis of fracturing associated with Occator crater;Buczkowski;Icarus,2018

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