Traces – burrows, borings, footprints – are major evidences of biological behaviour on Earth, yet they received little attention in the field of astrobiology. This study aims to discuss the application of ichnology (i.e. the study of life activity traces) to the search for past and modern life beyond Earth (i.e. herein called Astroichnology). Why to look for traces is a central question, given that organisms (and their body fossils) apparently represent a more direct evidence of life in present and past times. The reason is fourfold. First, the Earth’s ichnological record shows that traces record accurately the activity of soft-bodied organisms – from annelids to bacteria – that are comparatively underrepresented in the fossil record but that constitute the most part of the benthic biomass. Second, trace fossils are commonly preserved in sediments that are otherwise unfossiliferous. Third, bioturbation and bioerosion change permanently the physico-chemical properties of the substrate and leave geochemical, petrographic and geotechnical signals that enable to relate with the presence of life. In addition, the bioturbating activity of organisms commonly results in structures that are far more abundant and more visible than their tracemakers (e.g. several arthropod taxa produce km-scale mounded topographies in aquatic and continental environments; ectomycorrhizal fungi are responsible for soil microbioturbation; cm-sized organisms shaped the geochemistry of the Earth’s benthic ecosystem during the Cambrian Agronomic revolution). With increasing availability of high-resolution imagery, the search for past and modern traces is possible for several terrestrial bodies, among which the Moon, Mars, Venus, Titan and Mercury. Nevertheless, finding ichnological evidences beyond Earth is still a significant challenge because of (a) resolution issues, (b) relative paucity of bedding-plane imagery, (c) lack of core data, (d) lack of method-specific instrumentation. For these reasons, there is a great potential for developing tools that incorporate ichnology into an astrobiological framework. Specifically, tools for the analysis of sediment and/or rock cores are needed for observing biogenically-produced sedimentary fabrics (ichnofabrics) beyond Earth. Applied ichnology provides a vast set of practical tools (i.e. CT-scanning, borehole imagery) for studying ichnofabrics. Finally, a question might arise: What to expect? Models of bioturbation beyond Earth are extremely complex and variable due to the variety of geodynamical conditions existing on exoplanets. Nevertheless, burrowing and boring behaviours are expected to be a general pattern for life because they allow to face harsh surficial physico-chemical conditions (e.g. cosmic rays) and/or evolutionary pressures, both for mineralized or soft-bodied organisms. Identifying more precisely the forms and variation of Earth’s traces in extreme environments and their evolutionary paths is likely to provide a more robust predictive model for bioturbation beyond Earth.
Bioturbation beyond Earth: potential, methods and models of Astroichnology / A. Baucon, C.N. Carvalho, F. Felletti. ((Intervento presentato al convegno EANA15 tenutosi a Noordwijk nel 2015.
|Titolo:||Bioturbation beyond Earth: potential, methods and models of Astroichnology|
FELLETTI, FABRIZIO (Ultimo)
|Data di pubblicazione:||ott-2015|
|Settore Scientifico Disciplinare:||Settore GEO/01 - Paleontologia e Paleoecologia|
Settore GEO/02 - Geologia Stratigrafica e Sedimentologica
|Citazione:||Bioturbation beyond Earth: potential, methods and models of Astroichnology / A. Baucon, C.N. Carvalho, F. Felletti. ((Intervento presentato al convegno EANA15 tenutosi a Noordwijk nel 2015.|
|Appare nelle tipologie:||14 - Intervento a convegno non pubblicato|