Meteoritics & Planetary Science 1–18 (2013) doi: 10.1111/maps.12172 Opaque minerals, magnetic properties, and paleomagnetism of the Tissint Martian meteorite Jerome^ GATTACCECA1,2*, Roger H. HEWINS3, Jean-Pierre LORAND4, Pierre ROCHETTE1, France LAGROIX5,Cecile COURNEDE 1, Minoru UEHARA1, Sylvain PONT3, Violaine SAUTTER3, Rosa. B. SCORZELLI6, Chrystel HOMBOURGER7, Pablo MUNAYCO6, Brigitte ZANDA3,8, Hasnaa CHENNAOUI9, and Ludovic FERRIERE 10 1CNRS, Aix-Marseille Universite, CEREGE UM34, Aix-en-Provence, France 2Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA 3Laboratoire de Mineralogie et Cosmochimie du Museum, MNHN, UMR 7202 Paris, France 4Laboratoire de planetologie et geodynamique de Nantes, UMR 6112, Universite de Nantes, Faculte des Sciences, Nantes, France 5Institut de Physique du Globe de Paris, Paris, France 6Centro Brasileiro de Pesquisas Fısicas, Rio de Janeiro, Brazil 7CAMECA SAS, Gennevilliers, France 8Department of Earth and Planetary Sciences, Rutgers University, Piscataway, New Jersey 08854, USA 9Department of Geochemistry of Earth Sciences, Hassan II University, Casablanca, Morocco 10Natural History Museum, Vienna, Austria *Corresponding author. E-mail:
[email protected] (Received 19 December 2012; revision accepted 24 June 2013) Abstract–We present a description of opaque minerals, opaque mineral compositions, magnetic properties, and paleomagnetic record of the Tissint heavily shocked olivine-phyric shergottite that fell to Earth in 2011. The magnetic mineralogy of Tissint consists of about 0.6 wt% of pyrrhotite and 0.1 wt% of low-Ti titanomagnetite (in the range ulvospinel€ 3–15 magnetite 85–97). The titanomagnetite formed on Mars by oxidation-exsolution of ulvospinel€ grains during deuteric alteration. Pyrrhotite is unusual, with respect to other shergottites, for its higher Ni content and lower Fe content.