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Television observations of Mercury by Mariner 10The morphology and optical properties of the surface of Mercury resemble those of the Moon in remarkable detail, recording a very similar sequence of events; chemical and mineralogical similarity of the outer layers is implied. Mercury is probably a differentiated planet with an iron-rich core. Differentiation is inferred to have occurred very early. No evidence of atmospheric modification of any landform is found. Large-scale scarps and ridges unlike lunar or Martian features may reflect a unique period of planetary compression near the end of heavy bombardment, perhaps related to contraction of the core.
Document ID
19780005042
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Murray, B. C.
(California Inst. of Tech. Pasadena, CA, United States)
Belton, M. J. S.
(Arizona Univ. Tucson, Ariz., United States)
Danielson, E. G.
(Jet Propulsion Lab Pasadena, Calif., United States)
Davies, M. E.
(Rand Corp. Santa Monica, Calif., United States)
Gault, D. E.
(Ames Research Center Moffett Field, Calif., United States)
Hapke, B.
(Pittsburgh Univ. Pa., United States)
Oleary, B.
(Hampshire Coll. Amherst, Mass., United States)
Strom, R. G.
(California Inst. of Tech. Pasadena, CA, United States)
Suomi, V.
(Wisconsin Univ. Madison, United States)
Trask, N.
(U.S. Geological Survey Reston, Va., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1977
Publication Information
Publication: NASA, Washington The Soviet-Am. Conf. on Cosmochem. of the Moon and Planets, Pt. 2
Subject Category
Astrophysics
Accession Number
78N12985
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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