Tissint Martian Meteorite: A Fresh Look at the Interior, Surface, and Atmosphere of Mars

A New Rock from Mars On 18 July 2011 a meteorite originating from Mars fell on the moroccan desert. Chennaoui Aoudjehane et al. (p. 785, published online 11 October) show that this meteorite was ejected from the surface of Mars 700,000 years ago and contains components derived from the interior, surface, and atmosphere of the red planet. Previous to this fall, only four other martian meteorites have been collected after being witnessed falling to Earth. All the other martian meteorites that are represented in collections around the world, have been found long after their arrival on Earth, and thus have suffered from exposure to the terrestrial environment. A meteorite that fell in Morocco in July 2011 provides a sample to study processes that operated on Mars 700,000 years ago. Tissint (Morocco) is the fifth martian meteorite collected after it was witnessed falling to Earth. Our integrated mineralogical, petrological, and geochemical study shows that it is a depleted picritic shergottite similar to EETA79001A. Highly magnesian olivine and abundant glass containing martian atmosphere are present in Tissint. Refractory trace element, sulfur, and fluorine data for the matrix and glass veins in the meteorite indicate the presence of a martian surface component. Thus, the influence of in situ martian weathering can be unambiguously distinguished from terrestrial contamination in this meteorite. Martian weathering features in Tissint are compatible with the results of spacecraft observations of Mars. Tissint has a cosmic-ray exposure age of 0.7 ± 0.3 million years, consistent with those of many other shergottites, notably EETA79001, suggesting that they were ejected from Mars during the same event.

[1]  J. Blichert‐Toft,et al.  Bulk chemistry of Saharan shergottite Dar al Gani 476 , 2001 .

[2]  V. Sautter,et al.  A new Martian meteorite from Morocco: the nakhlite North West Africa 817 , 2002 .

[3]  C. Herd,et al.  Martian regolith in Elephant Moraine 79001 shock melts? Evidence from major element composition and sulfur speciation , 2010 .

[4]  A. Jambon,et al.  Petrology and mineralogy of the angrite Northwest Africa 1670 , 2008 .

[5]  J. Carignan,et al.  Routine Analyses of Trace Elements in Geological Samples using Flow Injection and Low Pressure On-Line Liquid Chromatography Coupled to ICP-MS: A Study of Geochemical Reference Materials BR, DR-N, UB-N, AN-G and GH , 2001 .

[6]  C. Pillinger,et al.  C, N, and noble gas isotopes in grain size separates of presolar diamonds from Efremovka. , 1998, Science.

[7]  L. Taylor,et al.  Detailed Geochemistry of New Shergottite, Dhofar 019 , 2001 .

[8]  M. Funaki,et al.  Matching Martian crustal magnetization and magnetic properties of Martian meteorites , 2005 .

[9]  M. Lindstrom,et al.  Geochemistry of eucrites: genesis of basaltic eucrites, and Hf and Ta as petrogenetic indicators for altered antarctic eucrites , 2003 .

[10]  A. Nier,et al.  Composition and structure of Mars' Upper atmosphere: Results from the neutral mass spectrometers on Viking 1 and 2 , 1977 .

[11]  D. Bogard,et al.  Martian Gases in an Antarctic Meteorite? , 1983, Science.

[12]  J. Vuilleumier,et al.  The “La Vue-des-Alpes” underground laboratory , 2003 .

[13]  Martian soil component in impact glasses in a Martian meteorite , 1999, Geophysical research letters.

[14]  B. Reynard,et al.  Silica as a shock index in shergottites: A cathodoluminescence study , 2005 .

[15]  G. Castagnoli,et al.  Measurement of cosmogenic radionuclides in meteorites with a sensitive gamma-ray spectrometer , 1992 .

[16]  D. Ming,et al.  Water alteration of rocks and soils on Mars at the Spirit rover site in Gusev crater , 2005, Nature.

[17]  B. Reynard,et al.  Petrography and geochemistry of the chassignite Northwest Africa 2737 (NWA 2737) , 2006 .

[18]  A. Simonetti,et al.  Trace element and Pb isotope provenance analyses of native copper in northwestern North America: results of a recent pilot study using INAA, ICP-MS, and LA-MC-ICP-MS , 2008 .

[19]  A. Treiman,et al.  The SNC meteorites are from Mars , 2000 .

[20]  K. Keil,et al.  Signatures of the martian atmosphere in glass of the Zagami meteorite. , 1995, Science.

[21]  C. Pillinger,et al.  The oxygen‐isotopic composition of Earth and Mars , 1999 .

[22]  Raymond E. Arvidson,et al.  The Martian surface as imaged, sampled, and analyzed by the Viking landers , 1989 .

[23]  J. Ashby References and Notes , 1999 .

[24]  M. Wadhwa,et al.  The terrestrial alteration of saharan shergottites dar al gani 476 and 489: a case study of weathering in a hot desert environment , 2001 .

[25]  F. Albarède,et al.  The Lu–Hf isotope geochemistry of shergottites and the evolution of the Martian mantle–crust system , 1999 .

[26]  Robert O. Pepin,et al.  The case for a martian origin of the shergottites: nitrogen and noble gases in EETA 79001 , 1984 .

[27]  D. R. Rushneck,et al.  The composition of the atmosphere at the surface of Mars , 1977 .

[28]  C. Arpesella A low background counting facility at laboratori nazionali del Gran Sasso , 1996 .

[29]  D. Britt,et al.  Density, porosity, and magnetic susceptibility of achondritic meteorites , 2011 .

[30]  F. Moynier,et al.  Geochemistry of CI chondrites: Major and trace elements, and Cu and Zn Isotopes , 2012 .

[31]  B. Marty,et al.  Nitrogen and noble gases in micrometeorites , 2005 .

[32]  V. Sautter,et al.  Petrology and chemistry of the Picritic Shergottite North West Africa 1068 (NWA 1068) , 2002 .

[33]  Jean-Pierre Bibring,et al.  Sulfates in Martian Layered Terrains: The OMEGA/Mars Express View , 2005, Science.