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Malliband, C. C.; Rothery, D. A.; Balme, M. R. and Conway, S. J.
(2017).
URL: https://www.hou.usra.edu/meetings/lpsc2017/pdf/147...
Abstract
MESSENGER heralded a new era in our geological understanding of Mercury as a dynamic planet. Geological mapping of surface features is essential in understanding both local and global geology. To this end, we have started mapping the H-10 (Derain) quadrangle to publish at 1:3 million scale to the same standards as other new MESSENGER mapping. This will allow integration into a global geological map. H-10 quadrangle is in the equatorial band of Mercury, located between 0°–72°E and 22N°–22°S. It was not imaged by Mariner 10; therefore this MESSENGER-based work is the first high resolution geological mapping of the quadrangle. Here we present initial observations from the first stages of mapping.
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- Item ORO ID
- 49052
- Item Type
- Conference or Workshop Item
- Academic Unit or School
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Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 2017 The Authors
- Depositing User
- Chris Malliband