TY - JOUR
T1 - Quantifying the martian geochemical reservoirs
T2 - An interdisciplinary perspective
AU - Toplis, Michael J.
AU - Bell, James
AU - Chassefière, Eric
AU - Sotin, Christophe
AU - Spohn, Tilman
AU - Blanc, Michel
PY - 2013/1
Y1 - 2013/1
N2 - The Special Issue of Space Science Review 2013 discusses the ISSI-Europlanet Workshop entitled 'Quantifying the Martian Geochemical Reservoirs', organized in April 2011 at Bern with the objective to create a diverse interdisciplinary forum composed of scientists directly involved in space-based exploration of the Martian surface, meteoriticists studying SNC meteorites, and planetary and/or Earth scientists simulating, numerically or experimentally, the physical and chemical processes occurring on or within Mars. The special volume begins with a paper by Brasser, describing current thoughts on the formation of Mars, the reasons for its relatively small size, the composition of its building blocks and its accretion time-scale. The second contribution by Mezger and co-researchers is largely based on isotopic studies of the SNC meteorites, which can be used to constrain the extent and time-scales of planet-wide differentiation into a core, mantle, and crust. Lasue focuses on the Martian hydrosphere/crusher, considering the morphological evidence for the presence of water, both at the present time and in the past.
AB - The Special Issue of Space Science Review 2013 discusses the ISSI-Europlanet Workshop entitled 'Quantifying the Martian Geochemical Reservoirs', organized in April 2011 at Bern with the objective to create a diverse interdisciplinary forum composed of scientists directly involved in space-based exploration of the Martian surface, meteoriticists studying SNC meteorites, and planetary and/or Earth scientists simulating, numerically or experimentally, the physical and chemical processes occurring on or within Mars. The special volume begins with a paper by Brasser, describing current thoughts on the formation of Mars, the reasons for its relatively small size, the composition of its building blocks and its accretion time-scale. The second contribution by Mezger and co-researchers is largely based on isotopic studies of the SNC meteorites, which can be used to constrain the extent and time-scales of planet-wide differentiation into a core, mantle, and crust. Lasue focuses on the Martian hydrosphere/crusher, considering the morphological evidence for the presence of water, both at the present time and in the past.
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U2 - 10.1007/s11214-012-9951-8
DO - 10.1007/s11214-012-9951-8
M3 - Article
AN - SCOPUS:84872683149
SN - 0038-6308
VL - 174
SP - 5
EP - 9
JO - Space Science Reviews
JF - Space Science Reviews
IS - 1-4
ER -