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Impact flows and crater scaling on the moon

O'Keefe, John D. and Ahrens, Thomas J. (1978) Impact flows and crater scaling on the moon. Physics of the Earth and Planetary Interiors, 16 (4). pp. 341-351. ISSN 0031-9201. https://resolver.caltech.edu/CaltechAUTHORS:20141222-135223089

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Abstract

The axisymmetric distribution of stress, internal energy and particle velocity resulting from the impact of an iron meteoroid with a gabbroic anorthosite lunar crust has been calculated for the regime in which shock-induced melting and vaporization takes place. Comparison of impact flow fields, with phase changes in silicates taken into account, with earlier results demonstrate that in the phase change case when the 15-km/s projectile has penetrated some two projectile radii into the moon, the peak stress in the flow is ∼0.66 Mbar at a depth of 66 km, and the stress has decayed to ∼66 kbar at a depth of 47 km. Rapid attenuation occurs because of the high rarefaction velocity of the high-pressure phases associated with a 35% (zero-pressure) density increase. This feature of the phase-change flow tends to strongly concentrate the maximum shock pressures along the meteoroid trajectory (axis) and makes the conical zone along which high internal energy deposition occurs, both shallow and narrow. Examination of the gravitational energies required to excavate larger craters on the moon indicates the importance of gravity forces acting during the excavation of craters having radii in the range greater than ∼2 – ∼140 km. It is observed that the “hydrodynamic” energy vs. crater radius relation approaches those for various “gravitational” energy vs. radius relations at the radii values corresponding to the larger mare basins. Cratering energy values in the range of (1.0 – 9.4) • 10^(32) erg are inferred on this basis for the Imbrium crater. Using these values and the criteria that all rocks exposed to ∼100 kbar or greater shock pressures are included in the ejecta (some of which falls back) implies that the maximum depth of sampling expected to be represented within the Apollo collection lies in the range 148–328 km.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/0031-9201(78)90072-9DOIArticle
http://www.sciencedirect.com/science/article/pii/0031920178900729PublisherArticle
Additional Information:© 1977 Elsevier Scientific Publishing Company. Received May 3, 1975; accepted for publication August 16, 1977. This research was supported under NASA Grant NSG-7129. We have profited from the reviewers comments.
Funders:
Funding AgencyGrant Number
NASANSG-7129
Issue or Number:4
Record Number:CaltechAUTHORS:20141222-135223089
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20141222-135223089
Official Citation:John D. O'Keefe, Thomas J. Ahrens, Impact flows and crater scaling on the moon, Physics of the Earth and Planetary Interiors, Volume 16, Issue 4, May 1978, Pages 341-351, ISSN 0031-9201, http://dx.doi.org/10.1016/0031-9201(78)90072-9. (http://www.sciencedirect.com/science/article/pii/0031920178900729)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:53106
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:22 Dec 2014 22:04
Last Modified:03 Oct 2019 07:47

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