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