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Wright, Jack; Rothery, David; Balme, Matthew and Conway, Susan
(2019).
DOI: https://doi.org/10.1080/17445647.2019.1625821
Abstract
The Hokusai (H05) quadrangle is in Mercury’s northern mid-latitudes (0–90°E, 22.5–65°N) and covers almost 5 million km2, or 6.5%, of the planet’s surface. We have used data from the MESSENGER spacecraft to make the first geological map of H05. Linework was digitized at 1:400,000-scale for final presentation at 1:3,000,000-scale, mainly using a ∼166 m/pixel monochrome basemap. Three major photogeologic units of regional extent were mapped: intercrater, intermediate, and smooth plains. Materials of craters ≥ 20 km in diameter were classified according to their degradation state. Two classification schemes were employed in parallel, one with three classes and the other with five classes, for compatibility with existing MESSENGER-era quadrangle maps and the first global geologic map. This map will provide science context and targets for the ESA-JAXA BepiColombo mission to Mercury.
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About
- Item ORO ID
- 61949
- Item Type
- Journal Item
- ISSN
- 1744-5647
- Project Funding Details
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Funded Project Name Project ID Funding Body Geological mapping of Mercury ST/N50421X/1 STFC Science & Technology Facilities Council - Keywords
- Mercury; planetary geology; Hokusai; quadrangle; impact craters; planetary volcanism
- 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) - Research Group
-
Astronomy
Physics
?? space ?? - Copyright Holders
- © 2019 The Authors
- Depositing User
- Jack Wright