Published 1994 | Version Published
Book Section - Chapter Open

Oblique impact jetting of geological materials

Abstract

To understand jetting of earth materials, gabbro slabs (5 mm thick) were accelerated to 1.5–2 km/s and impacted inclined gabbro (5–10 mm thick), novaculite (10 mm thick) and porous sandstone (12 mm thick) targets at angles of 30°–60°. The ejecta were collected using a catcher box filled with styrofoam and the particles were extracted using chloroform. The mass of the ejected particles per unit area (∼50 mg/cm^2) remains almost independent of impact velocity, inclination angle, thickness of the target and sample mineralogy and density. Based on this result, we predict that a 500 m diameter asteroid will produce only ∼10^7 gm tektite material. This is negligible comparing to an estimated 2×10^(13) gm in the Ivory Coast tektite strewn field. The recovered ejecta, unlike most tektites, contains both target and impactor materials. Both of the above results suggest that the tektites are not produced by jetting.

Additional Information

© 1994 American Institute of Physics. Published online 10 July 1994. This research is supported by NASA under NAGW 1941. Division of Geological and Planetary Sciences Contribution # 5326.

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Identifiers

Eprint ID
50691
Resolver ID
CaltechAUTHORS:20141022-135113329

Funding

NASA
NAGW 1941

Dates

Created
2014-10-22
Created from EPrint's datestamp field
Updated
2021-11-10
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Caltech Custom Metadata

Series Name
AIP Conference Proceedings
Series Volume or Issue Number
309
Other Numbering System Name
Caltech Division of Geological and Planetary Sciences
Other Numbering System Identifier
5326