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  • 1980-1984  (6)
  • 1
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    Structural geology of the Montgomery Mountains and the northern half of the Nopah and Resting Spring Ranges, Nevada and California (1983)
    Geological Society of America
    Details
    Publication Date: 1983-01-01
    Print ISSN: 0016-7606
    Electronic ISSN: 1943-2674
    Topics: Geosciences
    Published by Geological Society of America
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    PAPER CURRENT
  • 2
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    The Borealis Basin of Mars (1984)
    In:  CASI
    Details
    Publication Date: 2006-04-06
    Description: Why the lowlands of Mars are concentrated in the Northern Hemisphere and the highlands in the Southern Hemisphere is probably the most fundamental unsolved problem in martian geology. No explanation that accounts both for this asymmetric distribution and for the isostatic equilibrium across the scarp or sloping transition zone dividing the two provinces has been generally accepted; thinning of the lithosphere in the northern hemisphere by internal processes has been suggested. Because other lowland-highland distributions on Mars, Moon, and Mercury are controlled by impact basins, it is proposed that a giant basin formed early in Mars' history has caused the martian hemispheric dichotomy as well.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA. Washington Rept. of Planetary Geol. Program, 1983; p 110-112
    Format: text
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    NASA TECHNICAL REPORTS
  • 3
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    Moon (1984)
    In:  CASI
    Details
    Publication Date: 2014-09-18
    Description: The present state and evolution of the physical features which are visible on the Moon's surface are emphasized herein. Lunar craters, their distribution and stratigraphy, and the cratering processes are addressed. Homologous material is presented for lunar basins. Terra breccias, maria, and mare basalts are discussed. Lunar geologic history is also considered.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: JPL The Geol. of the Terrest. Planets; p 107-206
    Format: text
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    NASA TECHNICAL REPORTS
  • 4
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    The martian hemispheric dichotomy may be due to a giant impact (1984)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: Of the two approximately hemispherical, fundamentally different geological provinces into which Mars is divided, the more southerly province is heavily cratered, while the northern is lightly cratered and contains younger geological units. Lowlands occupy about one-third of Mars, and these are separated from the highlands by a distinct scarp or by a sloping transitional zone which is characterized by a variety of landforms that are unknown on other planets. It is presently proposed that the largest expanse of lowlands is substantially due to the formation of a large impact basin early in the planet's history, which has markedly influenced the character of the Martian surface.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Nature (ISSN 0028-0836); 309; 138-140
    Format: text
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    NASA TECHNICAL REPORTS
  • 5
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    The Geology of the Terrestrial Planets (1984)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: The geologic history of the terrestrial planets is outlined in light of recent exploration and the revolution in geologic thinking. Among the topics considered are planet formation; planetary craters, basins, and general surface characteristics; tectonics; planetary atmospheres; and volcanism.
    Keywords: SPACE SCIENCES (GENERAL)
    Type: NASA-SP-469 , NAS 1.21:469
    Format: application/pdf
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    NASA TECHNICAL REPORTS
  • 6
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    The geology of Ganymede (1982)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: A broad outline of the geologic history of Ganymede is presented, obtained from a first attempt to map the geology on a global scale and to interpret the characteristics of the observed geologic units. Features of the ancient cratered terrain such as craters and palimpsests, furrows and troughs, are discussed. The grooved terrain is described, including its sulci and cells, and the age relation of these units is considered along with the structure and origin of this terrain. The Gilgamesh Basin and Western Equatorial Basin in the post grooved terrain are treated, as are the bright and dark ray craters and the regolith. The development of all these regions and features is discussed in context. For the regolith, this includes the effect of water migration, sputtering, and thermal annealing. The histories of the ancient cratered terrain, the grooved terrain, and the post grooved terrain are presented.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Format: text
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    NASA TECHNICAL REPORTS
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