Published 1987
| Version v1
Report
Mars: a water-rich planet
Creators
Description
Good geomorphic evidence is presented for a planet that was once water rich, and that a lower limit on the amount of water available for a given Martian watershed may be estimated by assuming that the volume of material eroded was equal to the volume of water available. This estimate, coupled with high latitude water estimates of 50 to 100 m gives a global inventory of about 500 m total water in the subsurface. It was emphasized that this is a lower limit as considerable water may be bound in weathered debris and in primary minerals
Additional details
Publishing Information
- Imprint Title
- MECA symposium on Mars: Evolution of its climate and atmosphere
- Journal Page Range
- p. 23-25.
- Report number
- N--89-10780
Conference
- Title
- the evolution of its climate and atmosphere.
- Acronym
- MECA conference on mars
- Dates
- 18 Jul 1986.
- Place
- Washington, DC (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20027995
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- GEOMORPHOLOGY; MARS PLANET; MINERALS; SOLAR SYSTEM EVOLUTION; SURFACE WATERS; WATER
- Descriptors DEC
- GEOLOGY; HYDROGEN COMPOUNDS; OXYGEN COMPOUNDS; PLANETS; POLAR SOLVENTS; SOLVENTS