Sustainability 2010, 2(7), 1969-1990; doi:10.3390/su2071969

The Search for Sustainable Subsurface Habitats on Mars, and the Sampling of Impact Ejecta

1,* email and 2email
Received: 20 May 2010; Accepted: 22 June 2010 / Published: 5 July 2010
(This article belongs to the Special Issue Astrobiology and Sustainability)
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Abstract: On Earth, the deep subsurface biosphere of both the oceanic and the continental crust is well known for surviving harsh conditions and environments characterized by high temperatures, high pressures, extreme pHs, and the absence of sunlight. The microorganisms of the terrestrial deep biosphere have an excellent capacity for adapting to changing geochemistry, as the alteration of the crust proceeds and the conditions of their habitats slowly change. Despite an almost complete isolation from surface conditions and the surface biosphere, the deep biosphere of the crustal rocks has endured over geologic time. This indicates that the deep biosphere is a self-sufficient system, independent of the global events that occur at the surface, such as impacts, glaciations, sea level fluctuations, and climate changes. With our sustainable terrestrial subsurface biosphere in mind, the subsurface on Mars has often been suggested as the most plausible place to search for fossil Martian life, or even present Martian life. Since the Martian surface is more or less sterile, subsurface settings are the only place on Mars where life could have been sustained over geologic time. To detect a deep biosphere in the Martian basement, drilling is a requirement. However, near future Mars sample return missions are limited by the mission’s payload, which excludes heavy drilling equipment and restrict the missions to only dig the topmost meter of the Martian soil. Therefore, the sampling and analysis of Martian impact ejecta has been suggested as a way of accessing the deeper Martian subsurface without using heavy drilling equipment. Impact cratering is a natural geological process capable of excavating and exposing large amounts of rock material from great depths up to the surface. Several studies of terrestrial impact deposits show the preservation of pre-impact biosignatures, such as fossilized organisms and chemical biological markers. Therefore, if the Martian subsurface contains a record of life, it is reasonable to assume that biosignatures derived from the Martian subsurface could also be preserved in the Martian impact ejecta.
Keywords: subsurface biosphere; hydrothermal systems; impact ejecta; life on Mars
PDF Full-text Download PDF Full-Text [310 KB, uploaded 5 July 2010 10:28 CEST]

Export to BibTeX |

MDPI and ACS Style

Ivarsson, M.; Lindgren, P. The Search for Sustainable Subsurface Habitats on Mars, and the Sampling of Impact Ejecta. Sustainability 2010, 2, 1969-1990.

AMA Style

Ivarsson M, Lindgren P. The Search for Sustainable Subsurface Habitats on Mars, and the Sampling of Impact Ejecta. Sustainability. 2010; 2(7):1969-1990.

Chicago/Turabian Style

Ivarsson, Magnus; Lindgren, Paula. 2010. "The Search for Sustainable Subsurface Habitats on Mars, and the Sampling of Impact Ejecta." Sustainability 2, no. 7: 1969-1990.

Sustainability EISSN 2071-1050 Published by MDPI AG, Basel, Switzerland RSS E-Mail Table of Contents Alert