Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process
Dawn mission’s second extended phase provided high resolution observations of Occator crater of the dwarf planet Ceres. Here, the authors show stereo imaging and topographic maps of this crater revealing the influence of crustal composition on impact related melt and hydrothermal processes, and comp...
Saved in:
Main Authors: | P. Schenk, J. Scully, D. Buczkowski, H. Sizemore, B. Schmidt, C. Pieters, A. Neesemann, D. O’Brien, S. Marchi, D. Williams, A. Nathues, M. De Sanctis, F. Tosi, C. T. Russell, J. Castillo-Rogez, C. Raymond |
---|---|
Format: | article |
Language: | EN |
Published: |
Nature Portfolio
2020
|
Subjects: | |
Online Access: | https://doaj.org/article/044c971ba7d34351b217f63896b98c6a |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The varied sources of faculae-forming brines in Ceres’ Occator crater emplaced via hydrothermal brine effusion
by: J. E. C. Scully, et al.
Published: (2020) -
The missing large impact craters on Ceres
by: S. Marchi, et al.
Published: (2016) -
Origin of ammoniated phyllosilicates on dwarf planet Ceres and asteroids
by: Santosh K. Singh, et al.
Published: (2021) -
Reconciling safe planetary targets and planetary justice: Why should social scientists engage with planetary targets?
by: J. Gupta, et al.
Published: (2021) -
Dwarf planet (1) Ceres surface bluing due to high porosity resulting from sublimation
by: Stefan E. Schröder, et al.
Published: (2021)