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Abstract
Individual Martian equatorial troughs are described, and their stratigraphy, geomorphology and structure are discussed. Possible origins and the overall sequence of events are addressed. Wall rock, interior layered deposits, irregular floor deposits, fractured floor material, and surficial deposits are examined. Chasma walls, wall stability, pits and pit chains, tributary canyons, and the transition from troughs to channels are also discussed.
| Publication type | Book chapter |
|---|---|
| Publication Subtype | Book Chapter |
| Title | The canyon system on Mars |
| Year Published | 1992 |
| Language | English |
| Contributing office(s) | Astrogeology Science Center |
| Description | 40 p. |
| Larger Work Type | Book chapter |
| Larger Work Subtype | Book Chapter |
| Larger Work Title | Mars |
| First page | 453 |
| Last page | 492 |
| Google Analytic Metrics | Metrics page |