subject predicate object context
62333 Creator 34150f2f89a55de66712a0576f106400
62333 Creator 7c9060b8651fa54e11ffd46d3aba6da8
62333 Creator bd12e480200a0e58504d6106bfed3c8a
62333 Creator 0519c7e3d5b481315278655a3c8c63cf
62333 Creator 95f68b10fb49eec7b7d3b7db9817decc
62333 Date 2017
62333 Is Part Of repository
62333 abstract There is evidence that water may exist on Mars in the form of brines. The chemistries of these brines will be greatly influenced by the local lithologies, which would, in turn, impact on the organisms that could survive there . Four geological analogues were developed based on four broad martian lithologies: a global composition, an early and unaltered basaltic composition, a sulfur rich composition and a haematite rich composition (see talk by Ramkissoon et al., this conference, for further details). These analogues, and the brines derived from them, will be used to simulate the martian environment and will be inoculated with three species of methanogenic archaea to examine the impacts on their growth and metabolism. Methanogenic archaea represent model organisms for attempting to characterize martian life. A hydrogenotrophic metabolism enables them to survive through autotrophic growth on carbon dioxide. Three species of methanogenic archaea were selected to be used in a series of simulation experiments to evaluate the potential habitability of potential aqueous subsurface environments on Mars. Of the selected species, all have been shown to have a robust temperature and pH tolerance. Furthermore, Methanosarcina soligelidi SMA-21 is highly resistant to desiccation, starvation and ultraviolet radiation and has been shown to grow under martian simulation conditions; Methanobacterium arcticum M2 is able to tolerate high concentrations of perchlorate. In this poster, we will present details of how these organisms will be inoculated into brines derived from the martian regolith analogues and how survivability, growth and alterations in metabolism of these species will be assessed following incubation.
62333 authorList authors
62333 presentedAt ext-f508e728033eb387ed73e0677278d556
62333 status peerReviewed
62333 type AcademicArticle
62333 type Article
62333 label Macey, Michael C. ; Ramkissoon, Nisha K. ; Schwenzer, Susanne P. ; Pearson, Victoria K. and Olsson-Francis, Karen (2017). The impact of martian chemistry on the metabolism of methanogenic archaea. In: 7th Astrobiology Society of Britain Conference, 13-14 Sep 2017, The Open University, Milton Keynes, UK.
62333 label Macey, Michael C. ; Ramkissoon, Nisha K. ; Schwenzer, Susanne P. ; Pearson, Victoria K. and Olsson-Francis, Karen (2017). The impact of martian chemistry on the metabolism of methanogenic archaea. In: 7th Astrobiology Society of Britain Conference, 13-14 Sep 2017, The Open University, Milton Keynes, UK.
62333 Title The impact of martian chemistry on the metabolism of methanogenic archaea
62333 in dataset oro