Geologic map of Tooting crater, Amazonis Planitia region of Mars
Links
- More information: USGS Index Page
- Document: Pamphlet (10.4 MB pdf)
- Plate: Map sheet (134 MB pdf)
- Additional Report Piece: Interactive map - Geologic Map of Tooting Crater, Amazonis Planitia Region, Mars, 1:200K. Mouginis-Mark (2015)
- Data Release: USGS data release - Interactive Map: USGS SIM 3297 Geologic Map of Tooting Crater, Amazonis Planitia Region of Mars
- Metadata: Metadata (13 kB pdf)
- Read Me: Read Me (txt)
- Spatial Data: GIS data (100 MB pdf) Contains: geospatial database. Refer to the Readme and Metadata files for more information.
- Download citation as: RIS | Dublin Core
Abstract
Tooting crater has a diameter of 27.2 km, and formed on virtually flat lava flows within Amazonis Planitia ~1,300 km west of the summit of Olympus Mons volcano, where there appear to have been no other major topographic features prior to the impact. The crater formed in an area ~185 x 135 km that is at an elevation between −3,870 m and −3,874 m relative to the Mars Orbiter Laser Altimeter (MOLA) Mars datum. This fortuitous situation (for example, a bland, horizontal target) allows the geometry of the crater and the thickness of the ejecta blanket to be accurately determined by subtracting the appropriate elevation of the surrounding landscape (−3,872 m) from the individual MOLA measurements across the crater. Thus, for the first time, it is possible to determine the radial decrease of ejecta thickness as a function of distance away from the rim crest. On the basis of the four discrete ejecta layers surrounding the crater cavity, Tooting crater is classified as a Multiple-Layered Ejecta (MLE) crater. By virtue of the asymmetric distribution of secondary craters and the greater thickness of ejecta to the northeast, Morris and others (2010) proposed that Tooting crater formed by an oblique impact from the southwest. The maximum range of blocks that produced identifiable secondary craters is ~500 km (~36.0 crater radii) from the northeast rim crest. In contrast, secondary craters are only identifiable ~215 km (15.8 radii) to the southeast and 225 km (16.5 radii) to the west.
| Publication type | Report |
|---|---|
| Publication Subtype | USGS Numbered Series |
| Title | Geologic map of Tooting crater, Amazonis Planitia region of Mars |
| Series title | Scientific Investigations Map |
| Series number | 3297 |
| DOI | 10.3133/sim3297 |
| Year Published | 2015 |
| Language | English |
| Publisher | U.S. Geological Survey |
| Publisher location | Reston, VA |
| Contributing office(s) | Astrogeology Science Center |
| Description | Pamphlet: i, 4 p.; Map sheet: 44.61 x 37.35 inches; GIS data; Metadata; Readme |
| Other Geospatial | Amazonis Planitia Region, Mars |
| Projection | Transverse Mercator Projection |
| Scale | 200000 |
| Online Only (Y/N) | N |
| Additional Online Files (Y/N) | Y |
| Google Analytic Metrics | Metrics page |