Origin of the Olympus Mons Aureole and Perimeter Scarp
Abstract
The aureole materials that form an annulus of corrugated terrain surrounding Olympus Mons are considered to be the product of mass movement. The scarp at the mountain's foot formed as a result of this massive removal of material from the volcano's outer flanks. This interpretation is supported by a comparison of the amount of material originally available before scarp formation, and the present volume of aureole materials. On the basis of distribution, surface textures and theoretical considerations it is considered that the aureole was produced by a series of megaslides, rather than by a flow mechanism. Production of the megaslides may have been assisted by a period of widespread melting of permafrost.
- Publication:
-
Moon and Planets
- Pub Date:
- April 1980
- DOI:
- 10.1007/BF00898433
- Bibcode:
- 1980M&P....22..221L
- Keywords:
-
- Escarpments;
- Mars Surface;
- Planetary Evolution;
- Volcanoes;
- Landslides;
- Melting;
- Permafrost;
- Surface Properties;
- Terrain;
- Lunar and Planetary Exploration;
- MARS;
- OLYMPUS MONS;
- AUREOLES;
- SCARPS;
- FORMATION;
- VOLCANOES;
- MAPS;
- DISTRIBUTION;
- TEXTURES;
- SURFACE;
- THEORETICAL STUDIES;
- PHOTOGRAPHS;
- ORIGIN;
- GEOLOGY;
- TOPOGRAPHY;
- VOLUME;
- COMPARISONS;
- LANDSLIDES;
- GRAVITATIONAL POTENTIAL;
- FLOWS;
- LAVAS;
- FEATURES;
- GRABENS;
- GRAVITY;
- HYPOTHESES;
- VELOCITY;
- FRICTION;
- FLOODS;
- VOLCANISM;
- Mars