Published 1988 | Version v1
Report

Debris flows of the Simud-Tiu outflow system of Mars

Creators

Description

It is seen that the magnitude of geologic happenings are commonly quite different between the Earth and Mars because of differences in the makeup and breakup of their crusts. By assessing the differences, and the similarities, between planets, the geologic history of Mars can be more fully understood. The identification of debris-flow deposits in channels of Mars, for example, helps to establish which of several competing explanations for the origin of the channels actually occurred. In turn, the Earth is viewed in new, and commonly enlightening perspectives. By the way, it is fortunate that on Earth, thick sequences of impact ejected are not found that could be transformed into the monstrous debris flows that have devastated the Martian surface

Additional details

Publishing Information

Imprint Title
Nineteenth lunar and planetary science conference. Press abstracts
Journal Page Range
p. 31-33.
Report number
N--88-30473

Conference

Title
19. lunar and planetary science conference.
Dates
14-18 Mar 1988.
Place
Houston, TX (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
20043343
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Numerical Data
Descriptors DEI
EROSION; EXPERIMENTAL DATA; GEOLOGIC HISTORY; GEOLOGIC STRUCTURES; MARS PLANET; SURFACE PROPERTIES
Descriptors DEC
DATA; INFORMATION; NUMERICAL DATA; PLANETS