subject predicate object context
6180 Creator 96fdb8f74aad60e762b1aef18d80ab45
6180 Creator 970b917038a425943ae594e993a37e66
6180 Date 2006-10-29
6180 Is Part Of repository
6180 Is Part Of p14712970
6180 abstract One of the goals of the present Martian exploration is to search for evidence of extinct (or even extant) life. This could be redefined as a search for carbon. The carbon cycle (or, more properly, cycles) on Earth is a complex interaction among three reservoirs: the atmosphere; the hydrosphere; and the lithosphere. Superimposed on this is the biosphere, and its presence influences the fixing and release of carbon in these reservoirs over different time-scales. The overall carbon balance is kept at equilibrium on the surface by a combination of tectonic processes (which bury carbon), volcanism (which releases it) and biology (which mediates it). In contrast to Earth, Mars presently has no active tectonic system; neither does it possess a significant biosphere. However, these observations might not necessarily have held in the past. By looking at how Earth's carbon cycles have changed with time, as both the Earth's tectonic structure and a more sophisticated biology have evolved, and also by constructing a carbon cycle for Mars based on the carbon chemistry of Martian meteorites, we investigate whether or not there is evidence for a Martian biosphere.
6180 authorList authors
6180 issue 1474
6180 status peerReviewed
6180 volume 361
6180 type AcademicArticle
6180 type Article
6180 label Grady, Monica M. and Wright, Ian (2006). The carbon cycle on early Earth—and on Mars? Philosophical Transactions of the Royal Society B: Biological Sciences, 361(1474) 1703 -1713.
6180 label Grady, Monica M. and Wright, Ian (2006). The carbon cycle on early Earth—and on Mars? Philosophical Transactions of the Royal Society B: Biological Sciences, 361(1474) 1703 -1713.
6180 Title The carbon cycle on early Earth—and on Mars?
6180 in dataset oro