1 REVISION 2 2 3 Craters of the Moon National Monument Basalts as Unshocked Compositional and 4 Weathering Analogs for Martian Rocks and Meteorites. 5 6 Christopher T. Adcock1*, Arya Udry1, Elisabeth M. Hausrath1*, and Oliver Tschauner1,2 7 1 Department of Geoscience, University of Nevada, Las Vegas (
[email protected]) 8 2 High Pressure Science and Engineering Center, University of Nevada, Las Vegas 9 10 Short Title: Craters of the Moon National Monument Basalts and Mars 11 12 *Corresponding authors: Christopher T. Adcock (
[email protected]) and 13 Elisabeth M. Hausrath (
[email protected]) 14 1 15 Keywords 16 Mars, Analog, Craters of the Moon, Basalt, Martian Meteorite, Gusev Crater, Weathering, Age 17 correlation 18 Abstract 19 20 The availability of terrestrial sites that are martian analogs allows researchers to 21 investigate Mars using knowledge gained on Earth. Among the terrestrial analog sites for Mars is 22 Craters of the Moon National Monument (COTM) in Idaho, USA. Craters of the Moon National 23 Monument is home to over 60 basalt lava flows, many of which have been dated from 2,050 to 24 18,340 years before present (y.b.p.). Following previous authors, we examined the chemistry and 25 petrogenesis of COTM basalts compared to basaltic martian rocks, martian meteorites, and 26 meteorite clasts, and then examined the results of chemical weathering of the basaltic flows. 27 Results of our comparative chemical analysis suggest COTM basalts are generally more evolved 28 than the martian materials, with a few notable exceptions. Several COTM flow basalts, including 29 rocks of the >18,000 year old Kimama flow, have high FeO, TiO2, and P2O5 contents similar to 30 the Wishstone and Watchtower class rocks analyzed at Gusev Crater, Mars, by the Mars 31 Exploration Rover Spirit.