NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The origin of the moon: Further studies of the giant impactA number of technical improvements in the calculations which simulate the most violent event that has occurred to the earth during its history: its collision with the next largest body which was present in its region of accumulation in the early solar system, are discussed. This body was a planet in its own right, an object a little more massive than the planet Mars. The collision created a disk of molten and gaseous debris in orbit around the protoearth, and it is believed that the dissipation of this disk resulted in the formation of the moon. Also discussed is the serendipitous discovery that has emerged from the simulations: the role played by a huge, hot, rotating bar of rock and iron, which is formed immediately after the collision, in transferring angular momentum to much of the rock that is put into orbit, and in robbing the iron of angular momentum so that it falls promptly into the protoearth.
Document ID
19880021090
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Benz, W.
(Harvard-Smithsonian Center for Astrophysics Amado, AZ., United States)
Cameron, A. G. W.
(Harvard-Smithsonian Center for Astrophysics Amado, AZ., United States)
Melosh, H. J.
(Arizona Univ. Tucson., United States)
Benz, W.
(Harvard-Smithsonian Center for Astrophysics, Amado AZ., United States)
Date Acquired
September 5, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Lunar and Planetary Inst., Nineteenth Lunar and Planetary Science Conference. Press abstracts
Subject Category
Lunar And Planetary Exploration
Accession Number
88N30474
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Document Inquiry

Available Downloads

There are no available downloads for this record.
No Preview Available