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Impact Crater Formation, Shock Metamorphism, and Distribution of Impact Ejecta

  • Billy P. Glass
  • Bruce M. SimonsonEmail author
Chapter
Part of the Impact Studies book series (IMPACTSTUD)

Abstract

As previously mentioned, an integral part of the cratering process is the formation and widespread distribution of ejecta. In order to comprehend how the distribution, thickness, and nature of an impact ejecta layer varies with distance from its source crater, one needs to understand the cratering process. Thus, we begin this chapter with a brief review of cratering mechanics. This leads into a discussion of shock metamorphism, which occurs during the cratering process and which is important in the identification of impact craters and distal ejecta layers. At the end of the chapter we briefly discuss some theoretical and experimental data on how ejecta, including the degree of shock metamorphism of the ejecta, vary with distance from the source crater. This last subject is addressed again in  Chap. 10, but in  Chap. 10 we compare observations on how distal ejecta vary with distance from source craters with theoretical and experimental data of how the thickness and nature of distal ejecta should vary with distance from the source crater.

Keywords

Shock Pressure Kink Band Impact Structure Vapor Plume Shock Metamorphism 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© Springer-Verlag Berlin Heidelberg 2013

Authors and Affiliations

  1. 1.Department of GeologyUniversity of DelawareNewarkUSA
  2. 2.Department of GeologyOberlin CollegeOberlinUSA

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