Running Head: Komatiites: geological settings to astrobiological contexts Review Komatiites: From Earth’s Geological Settings to Planetary and Astrobiological Contexts Delphine Nna-Mvondo1 and Jesus Martinez-Frias1 1 Planetary Geology Laboratory, Centro de Astrobiologia (CSIC/INTA), associated to NASA Astrobiology Institute, Ctra. De Ajalvir, km 4. 28850 Torrejon de Ardoz, Madrid, Spain. Correspondence: Laboratorio de Geología Planetaria, Centro de Astrobiología (CSIC/INTA), associated to NASA Astrobiology Institute, Instituto Nacional de Técnica Aeroespacial, Ctra. De Ajalvir, km 4. 28850 Torrejón de Ardoz, Madrid, Spain. Phone: +34 915206434 Fax: +34 915201074 E-mail:
[email protected] 1 ABSTRACT Komatiites are fascinating volcanic rocks. They are among the most ancient lavas of the Earth following the 3.8 Ga pillow basalts at Isua and they represent some of the oldest ultramafic magmatic rocks preserved in the Earth’s crust at 3.5 Ga. This fact, linked to their particular features (high magnesium content, high melting temperatures, low dynamic viscosities, etc.), has attracted the community of geoscientists since their discovery in the early sixties, who have tried to determine their origin and understand their meaning in the context of terrestrial mantle evolution. In addition, it has been proposed that komatiites are not restricted to our planet, but they could be found in other extraterrestrial settings in our Solar System (particularly on Mars and Io). It is important to note that komatiites may be extremely significant in the study of the origins and evolution of Life on Earth. They not only preserve essential geochemical clues of the interaction between the pristine Earth rocks and atmosphere, but also may have been potential suitable sites for biological processes to develop.