Geologic Map of Ceres [Dawn Mission] - Global dataset based on the 15 individual quadrangle maps ...
Background: Between 2011 and 2018, the NASA Dawn spacecraft visited asteroid (4) Vesta and dwarf planet (1) Ceres to investigate the surfaces of both protoplanets through optical and hyperspectral imaging and their composition through gamma-ray and neutron spectroscopy from orbit. For both Vesta and...
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| Format: | Dataset |
| Language: | English |
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Zenodo
2023
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| Online Access: | https://dx.doi.org/10.5281/zenodo.7989803 https://zenodo.org/record/7989803 |
| Summary: | Background: Between 2011 and 2018, the NASA Dawn spacecraft visited asteroid (4) Vesta and dwarf planet (1) Ceres to investigate the surfaces of both protoplanets through optical and hyperspectral imaging and their composition through gamma-ray and neutron spectroscopy from orbit. For both Vesta and Ceres, a geologic mapping investigation was realized based on optical and hyperspectral data as well as a photogrammetrically derived digital terrain model. For the global mapping investigation, mappers employed Geographic Information System (GIS) software to map 15 quadrangles. The results were published as individual map sheets alongside research papers discussing the geologic evolution. The style of collaborative mapping to produce a consistent global view represented by individual quadrangle maps is comparably new despite abundantly available mapping experiences. Ongoing data acquisition during mapping created considerable challenges for the coordination and homogenization of mapping results. To handle this ... : {"references": ["Williams, D. et al. (2018) Introduction: The geologic mapping of Ceres. Icarus Vol 316, doi: 10.1016/j.icarus.2017.05.004", "Ruesch, O. et al. (2018) Geology of Ceres' North Pole quadrangle with Dawn FC imaging data. Icarus Vol 316, doi: 10.1016/j.icarus.2017.09.036", "Pasckert, J.H. et al. (2018) Geologic mapping of the Ac-2 Coniraya quadrangle of Ceres from NASA's Dawn mission: Implications for a heterogeneously composed crust. Icarus Vol 316, doi: 10.1016/j.icarus.2017.06.015", "Scully, J. et al. (2018) Ceres' Ezinu quadrangle: a heavily cratered region with evidence for localized subsurface water ice and the context of Occator crater. Icarus Vol. 316, doi: 10.1016/j.icarus.2017.10.038", "Hughson, K.H.G. et al. (2018) The Ac-5 (Fejokoo) quadrangle of Ceres: Geologic map and geomorphological evidence for ground ice mediated surface processes. Icarus Vol. 316, doi: 10.1016/j.icarus.2017.09.035", "Krohn, K. et al. (2018) The unique geomorphology and structural geology of the Haulani crater ... |
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