The effects of meteorite impacts on the availability of bioessential elements for endolithic organisms
(2012) In Meteoritics and Planetary Science 47(10). p.1681-1691- Abstract
Meteorite impacts, one of the most ubiquitous processes in the solar system, have the ability to destroy as well as create habitats for life. The impact process can increase the translucency and porosity of the target substrate, as well as mobilize biologically relevant elements within the substrate. For endolithic organisms, this process has important implications, especially in extreme environments where they are forced to seek refuge in the interior of rocks. Here, we show that unshocked target rocks and rocks that have experienced pressures up to about 80GPa from the Haughton impact structure, Devon Island, Canada, possess a small, but discernible change in bulk chemistry within the major oxide analysis. However, changes in the... (More)
Meteorite impacts, one of the most ubiquitous processes in the solar system, have the ability to destroy as well as create habitats for life. The impact process can increase the translucency and porosity of the target substrate, as well as mobilize biologically relevant elements within the substrate. For endolithic organisms, this process has important implications, especially in extreme environments where they are forced to seek refuge in the interior of rocks. Here, we show that unshocked target rocks and rocks that have experienced pressures up to about 80GPa from the Haughton impact structure, Devon Island, Canada, possess a small, but discernible change in bulk chemistry within the major oxide analysis. However, changes in the distribution of elements did occur with increasing shock level for both the sedimentary and crystalline target. Both the crystalline and sedimentary target rocks contain significant amounts of glasses at higher shock levels (up to about 95% by volume), which would improve the availability of these elements to potential microbial endoliths as glasses are more easily dissolved by organic acids. The implication that impact events do not impoverish their capacity to serve as a "substrate" through volatilization is important with respect to analogous impact structures on Mars. After the deleterious effects of the direct meteorite impact, any microorganisms on Mars would have benefited from the input of heat, the mobilization of a possible frozen groundwater system, as well as increased translucency, porosity, and trace nutrient availability of the target substrate.
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- author
- Pontefract, Alexandra ; Osinski, Gordon R. ; Lindgren, Paula LU ; Parnell, John ; Cockell, Charles S. and Southam, Gordon
- publishing date
- 2012-10
- type
- Contribution to journal
- publication status
- published
- subject
- in
- Meteoritics and Planetary Science
- volume
- 47
- issue
- 10
- pages
- 11 pages
- publisher
- Wiley-Blackwell
- external identifiers
-
- scopus:84869015738
- ISSN
- 1086-9379
- DOI
- 10.1111/maps.12004
- language
- English
- LU publication?
- no
- id
- 3a5b981e-524b-4765-9994-769f3bc3d5f8
- date added to LUP
- 2017-06-16 15:58:44
- date last changed
- 2022-02-14 20:07:46
@article{3a5b981e-524b-4765-9994-769f3bc3d5f8,
abstract = {{<p>Meteorite impacts, one of the most ubiquitous processes in the solar system, have the ability to destroy as well as create habitats for life. The impact process can increase the translucency and porosity of the target substrate, as well as mobilize biologically relevant elements within the substrate. For endolithic organisms, this process has important implications, especially in extreme environments where they are forced to seek refuge in the interior of rocks. Here, we show that unshocked target rocks and rocks that have experienced pressures up to about 80GPa from the Haughton impact structure, Devon Island, Canada, possess a small, but discernible change in bulk chemistry within the major oxide analysis. However, changes in the distribution of elements did occur with increasing shock level for both the sedimentary and crystalline target. Both the crystalline and sedimentary target rocks contain significant amounts of glasses at higher shock levels (up to about 95% by volume), which would improve the availability of these elements to potential microbial endoliths as glasses are more easily dissolved by organic acids. The implication that impact events do not impoverish their capacity to serve as a "substrate" through volatilization is important with respect to analogous impact structures on Mars. After the deleterious effects of the direct meteorite impact, any microorganisms on Mars would have benefited from the input of heat, the mobilization of a possible frozen groundwater system, as well as increased translucency, porosity, and trace nutrient availability of the target substrate.</p>}},
author = {{Pontefract, Alexandra and Osinski, Gordon R. and Lindgren, Paula and Parnell, John and Cockell, Charles S. and Southam, Gordon}},
issn = {{1086-9379}},
language = {{eng}},
number = {{10}},
pages = {{1681--1691}},
publisher = {{Wiley-Blackwell}},
series = {{Meteoritics and Planetary Science}},
title = {{The effects of meteorite impacts on the availability of bioessential elements for endolithic organisms}},
url = {{http://dx.doi.org/10.1111/maps.12004}},
doi = {{10.1111/maps.12004}},
volume = {{47}},
year = {{2012}},
}