Detecting crater ejecta-blanket boundaries and constraining source crater regions for boulder tracks and elongated secondary craters on Eros
Version of Record online: 9 JUL 2012
© The Meteoritical Society, 2012
Meteoritics & Planetary Science
Volume 47, Issue 6, pages 1087–1097, June 2012
How to Cite
DURDA, D. D., CHAPMAN, C. R., MERLINE, W. J. and ENKE, B. L. (2012), Detecting crater ejecta-blanket boundaries and constraining source crater regions for boulder tracks and elongated secondary craters on Eros. Meteoritics & Planetary Science, 47: 1087–1097. doi: 10.1111/j.1945-5100.2012.01380.x
- Issue online: 9 JUL 2012
- Version of Record online: 9 JUL 2012
- (Received 02 May 2011; revision accepted 21 May 2012)
Video S1. Animation showing a model of a hypothetical equatorial impact on Eros. This example shows the evolution of ejecta leading to the deposition of a markedly asymmetric ejecta blanket with very sharp boundaries, caused by the combination of impact location on the asteroid and the asteroid’s rotation ‘out from under’ the leading edge of the expanding ejecta curtain.
|MAPS_1380_sm_eros-equatorial.avi||6007K||Supporting info item|
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