Geologic map of the Noachis Quadrangle of Mars
January 9, 2023
The Noachis quadrangle is in the ancient cratered highlands of Mars. Craters dominate the surface of the planet in this area; most are of impact origin, some are of volcanic origin, and some are of undetermined origin. Impact craters in the Noachis quadrangle are classified into four groups based on their morphologic characteristics, each group representing a relative age range. Where applicable, superposition relations support relative age determinations based on crater morphology.
Citation Information
Publication Year | 2023 |
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Title | Geologic map of the Noachis Quadrangle of Mars |
DOI | 10.5066/P9YTJ1MC |
Authors | J. E. Peterson |
Product Type | Data Release |
Record Source | USGS Digital Object Identifier Catalog |
USGS Organization | Astrogeology Science Center |
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Geologic map of the Noachis Quadrangle of Mars
The Noachis quadrangle is in the ancient cratered highlands of Mars. Craters dominate the surface of the planet in this area; most are of impact origin, some are of volcanic, origin, and some are of undetermined origin. Martian craters are I general similar in morphology of lunar craters but are more degraded. Analogous morphologies and size-frequency distributions of lunar and Martian craters ind
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Geologic map of the Noachis Quadrangle of Mars
The Noachis quadrangle is in the ancient cratered highlands of Mars. Craters dominate the surface of the planet in this area; most are of impact origin, some are of volcanic, origin, and some are of undetermined origin. Martian craters are I general similar in morphology of lunar craters but are more degraded. Analogous morphologies and size-frequency distributions of lunar and Martian craters ind