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Molecular parameters of post impact cooling in the Boltysh impact structure

Watson, J.S.; Gilmour, I.; Jolley, D.W.; Kelley, S.P.; Gilmour, M.A. and Gurov, E.P. (2010). Molecular parameters of post impact cooling in the Boltysh impact structure. In: 41st Lunar and Planetary Science Conference, 1-5 March 2010, Houston.

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Impact events have the potential to generate a number of long-term sources of heat that can lead to the initiation of hydrothermal systems when the impact occurs on a water- or ice-rich target. Such hydrothermal systems have been postulated as promising locations to search for evidence of past biological processes on Mars due to the prevalence of impact cratering as a surface process in Mars’s early history. In this study, we have used molecular parameters of the thermal maturity of organic matter combined with palynology and carbon isotope stratigraphy to study the post impact thermal history of crater fill sediments from the Boltysh crater, Ukraine.

Item Type: Conference Item
Copyright Holders: 2010 The Authors
Academic Unit/Department: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 21166
Depositing User: Jonathan Watson
Date Deposited: 14 Apr 2010 10:54
Last Modified: 05 Oct 2016 01:16
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