The second-largest Mars rock in private hands.
It’s quite moving to hold a piece of Mars in your hands… to reflect on its incredible interplanetary journey, and the science that gives confidence as to the origin of this unusual piece of rock.
This is the main mass of DaG 1037, an igneous Martian shergottite meteorite discovered in 1999 in the Dar al Gani desert of Libya. Meteorites are often found in North West Africa, not because they land there more often, but because they are easy to spot as peculiar objects in the desert sands. (It’s like searching for your car keys where the streetlight shines bright).
From the geochemistry and various isotopes, we can deduce the origin and transit time of interstellar objects (a bit like Carbon-14 dating for formerly living artifacts on Earth). The 133 meteorites from Mars exhibit precise elemental and isotopic compositions similar to rocks and atmosphere gases analyzed by spacecraft on Mars, starting with the Viking lander in 1976. Compared to other meteorites, the Martians have younger formation ages, unique oxygen isotopic composition (consistent for Mars and not for Earth http://tinyurl.com/MARS1037 ), and the presence of aqueous weathering products. A trapped gas analysis concluded that their origin was Mars quite recently, in the year 2000.
More from NASA JPL: http://www2.jpl.nasa.gov/snc/dag1037.html
It is the latest addition to http://tinyurl.com/FVspace Museum
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