
"Why do the planets orbit the Sun on a flat plane rather than different paths or levels, much the way electrons orbit the nucleus of an atom?"
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The Planetary Context of Biological Evolution Sub project: Geobiology of Neogene hematitic sedimentary rocks<BR>
Project Investigators: Ariel Anbar, Andrew Knoll
Other Project Members
David Fernández Remolar (Collaborator)Richard Morris (Collaborator)Astrobiology Roadmap Objectives:
- Objective 2.1: Mars exploration
- Objective 7.2: Biosignatures to be sought in nearby planetary systems
Project Progress
We completed laboratory analyses of samples of iron deposits collected along the Rio Tinto basin, southwestern Spain (Fig. 1). Analyses included x-ray diffraction (XRD), Moessbauer, petrological, and paleontological investigations of collected samples. In consequence, we can now show how the primary iron deposits in the Rio Tinto system — hydronium jarrosite, shcwertmannite, and poorly ordered goethite — are transformed through diagenesis to produce iron deposits rich in coarse-grained hematite. Of relevance to Mars, the hematite forms as a stable product of diagenesis over a two million year span, not as an initial precipitate.
We also demonstrated that fossils, including fungal and bacterial microfossils, can be preserved in remarkable detail by goethites in the basin, although subsequent digenetic alteration to hematite commonly obliterates preserved fossils. Finally, we demonstrated that sedimentary features observable with Mars Explorer Rover’s (MER’s) pancam and navcam imagers include features identifiable as biological signatures. Foremost among these are streamers, created by the adherence of iron precipitates to filamentous microorganisms.
The Rio Tinto project provides a terrestrial analog to the Mars Meridiani Planumhematite landing site — indeed the only terrestrial analog in which both initial and diagenetically stabilized deposits have been studied.

Figure 1. Present day iron deposition along the Rio Tinto, Spain
Mission Involvement
Mars MER 2003Cross-Team Collaborations
We collaborated with the Spanish Center for Astrobiology (David Fernandez-Remolar and Ricardo Amils) and with Richard Morris at the Johnson Space Center.
Publications
Javaux, E.J., Knoll, A.H., Marshall, C.P. & Walter, M.R. (Submitted, 2003). Recognizing early life on Earth and Mars [Abstract]. The 3rd European Workshop on Exo/Astrobiology, November 2003, Centro de Astrobiologia, Madrid, Spain.
Squyres, S.W. & the Athena Science Team. (2002). The MER Mission's Athena science investigation [Abstract]. Eos, Transactions of the American Geophysical Union, 83(47, Fall Meeting Supplement). Abstract # P21C-02.
- Environmental changes in the context of biological evolution during Neoproterozoic on the Yangtze Platform, a snowball Earth?
- Evogenomics Focus Group
- Isotopic and molecular approaches to microbial ecology and biogeochemistry (The evolution of organic matter) <BR>
- The Planetary Context of Biological Evolution <BR>Subproject: Carbon Cycle and Climate Dyanamics of Mars
- The Planetary Context of Biological Evolution Sub project: Geobiology of Neogene hematitic sedimentary rocks<BR>
- The Planetary Context of Biological Evolution Subproject: Neoproterozoic-Cambrian Environmental Change and Evolution<BR>
- The Planetary Context of Biological Evolution Subproject: The Proterozoic Oxidiation of the Earth's Surface<BR>
- The Planetary Context of Biological Evolution: Subproject: Permo-Triassic mass extinction and its consequences<BR>
- The use of living plants and fossil chemistry to study the morphological patterns and developmental processes of land plant evolution

