Είμαστε μόνοι στο συμπάν; Οι μετεωρίτες δίνουν απαντήσεις;


Published: Dec 2, 2013
Keywords:
Tissint Mars planetology life
Ι. Μπαζιώτης
L. A. Taylor
Abstract

The humankind, despite the recent technological achievements, does not yet have the ability to carry out routine trips to nearby celestial bodies. However, space science is a reality. The “Apollo” missions, that took place during the period 1969-1972, included the moon landing, the walk of astronauts and collection of valuable samples. Since then, no similar space journey has been carried out. The possibility for future missions such as the return to the Moon or Mars, or to an asteroid (e.g., Vesta), seems small enough to be implemented in the next decades. Nevertheless, nature has the mechanism and procedures to resolve this problem by sending extra-terrestrial rocks in earth in the form of meteorites. Meteorite fall on Earth is a major event, as it reveals important information about the primordial stages of formation of our solar system, or the creation processes of other planets. However, the big question still remains; whether these rocks host or have traces of past life in turn employs researchers in the last twenty years. McKay et al. (1996) studied the meteorite ALH 84001 originating from Mars, claimed for important discoveries such as structures corresponding to nanobacteria. In the current paper, we focus on the origin of Martian meteorites, presenting their complete geological history; from the genesis of their protoliths till their falling to the earth. We attempt to shade light in the understanding of meteorite formation using mineralogical-petrological-geochemical data, and the assignment of timing for each event based upon contemporary geochronological data. Recently, studies of the Martian meteorite Tissint, allegedly discovered structures rich in carbon and oxygen. Furthermore, recent field observations from Curiosity rover, indicates the existence of surface water that flowed once in the past at the Martian surface. We conclude that the planet Mars might not be a "dead" planet. But it turns out that many of the meteorites that reach the Earth, have undergone a complex history which is associated with the development of very high pressures and temperatures on the surface of the planet (e.g., Mars) from which they originate, able to destroy any trace of life before them. After all, we should be very sceptic and evaluate all the possibilities before the acceptance for the existence of life out there. 

Article Details
  • Section
  • Opening Lectures
Downloads
Download data is not yet available.
References
Baziotis I.P., Liu Y., Mc Sween H.Y., Bodnar R.J. and Taylor L.A. 2012. Tissint Meteorite: A fresh piece of Martian lava with new discoveries, 75th Annual Meeting Met. Soc., August 12-17, 2012 in Cairns, Australia, #5250.
Baziotis I.P., Liu Y., DeCarli P.S., Melosh H.J., Mc Sween H.Y., Bodnar R.J. and Taylor L.A. 2013. The Tissint Martian meteorite as evidence for the largest impact excavation, Nature Comm., 4, 1404, doi: 10.1038/ncomms2414.
Baziotis I.P., Liu Y. and Taylor L.A. 2013. Detailed Raman Spectroscopic Study of the Tissint Meteorite: Extraordinary Occurrence of High Pressure Polymorphs in a Single Fresh Piece of Martian Shergottite, Geoph. Res. Abs., 15, EGU2013-5463.
Bianciardi G., Miller J.D., Straat P.A. and Levin G.V. 2012. Complexity analysis of the Viking labeled release experiments, Int. J. Aeronautical Space Sci., 13(1), 14-26.
Bischoff A. 2001. Meteorite classification and the definition of new chondrite classes as a result of successful meteorite search in hot and cold deserts, Planet. Space Sci., 49 (8), 769-776.
Blinova A. and Herd C.D.K. 2009. Experimental study of polybaric REE partitioning between olivine, pyroxene and melt of the Y 980459 composition: insights into the petrogenesis of depleted shergottites, Geochim. Cosmochim. Acta, 73, 3471 – 3492.
Brennecka G.A., Borg L.E. and Wadhwa M. 2012. The age of Tissint: Sm-Nd & Rb-Sr isotope systematics, 75th Annual Meeting Met. Soc., August 12-17, 2012 in Cairns, Australia, #5157.
Chennaoui Aoudjehane H. et al. 2012. Tissint Martian Meteorite: A fresh look at the interior, Surface, and Atmosphere of Mars, Science, 338, 785-788.
DeCarli P.S. 2013. Meteorites from Mars via a Natural Two-stage Gas Gun, Procedia Engineering, 58, 570-573.
El Goresy, A., Gillet, P., Miyahara, M., Ohtani, L., Ozawa, S., Lin, Y., Feng, L., Escerig, S., 2013. Multiple shock events and diamond formation on Mars, 44th LPSC, The Woodlands, Texas, #1037.
Ferrière L., Brandstätter F., Topa D., Schula T., Baziotis I.P., Münker C. and Koeberl C. 2013. The complex history of Tissint inferred from different types of melt inclusions and isotopic systems, 76th Annual Meeting Met. Soc., July 29th - August 2nd, 2013 in Edmonton, Canada,
Fritz J., Artemieva N. and Greshake A. 2005. Ejection of Martian meteorites, Meteorit. Planet. Sci., 40, 1393-1411.
Grosshans T.E., Lapen T.J., Andreasen R. and Irving A.J. 2013. Lu-Hf and Sm-Nd ages and source compositions for depleted shergottite Tissint, 44th LPSC, The Woodlands, Texas, #2872.
Head J.N., Melosh H.J. and Ivanov B.A. 2002. Martian meteorite launch: high-speed ejecta from small craters, Science, 298, 1752–1756.
Herd C.D.K., Borg L E., Jones J.H. and Papike J.J. 2002. Oxygen fugacity and geochemical variations in the martian basalts: implications for martian basalt petrogenesis and the oxidation state of the upper mantle of Mars, Geochim. Cosmochim. Acta, 66, 2025–2036.
Irving A.J., Kuehner S.M., Tanaka R., Herd C.D.K., Chen G. and Lapen T.J. 2012. The Tissint depleted permafic olivine-phyric shergottite: petrologic, elemental and isotopic characterization of a recent Martian fall in Morocco, 43rd LPSC, The Woodlands, Texas, #2510.
Levin G. V. and Straat P.A. 1976. Viking labeled release biology experiment: interim results, Science, 194(4271), 1322-1329.
Lin Y. et al. 2013. NanoSims analysis of organic carbon from Mars: evidence for a biogenetic origin, 44th LPSC, The Woodlands, Texas, #1476.
Liu Y., Taylor L.A., Baziotis I.P., Mc Sween H.Y., Bodnar R.J., DeCarli P.S. and Melosh H.J. 2013. Impact excavation of Martian meteorites: index from shock formed minerals, 44th LPSC, The Woodlands, Texas, #1371.
McKay D.S., Gibson E.K., Thomas-Keprta K.L., Vali H., Romanek C.S., Clemett S.J., Chillier X.D.F., Maechling C.R. and Zare R.N., 1996. Search for life on Mars: possible relic biogenic activity in martian meteorite ALH84001, Science, 273, 924–930.
Moser D.E., Chamberlain K.R., Tait K.T., Schmitt A.K., Darling J.R., Barker I.R. and Hyde B.C. 2013. Solving the Martian meteorite age conundrum using micro-baddeleyite and lauchgenerated zircon, Nature, 499, 454-457, doi: 10.1038/nature12341.
Sharp T.G. and DeCarli P.S. 2006. Shock effects in meteorites, Meteorites and the early solar system II, 653-677.
Shaw C.S.J. and Walton E. 2013. Thermal modeling of shock melts in Martian meteorites: Implications for preserving Martian atmospheric signatures and crystallization of high-pressure minerals from shock melts, Meteorit. Planet. Sci., 1-13, doi: 10.1111/maps.12100.
Shearer C.K., Burger P.V., Papike J.J., Borg L.E., Irving A.J. and Herd C. 2008. Petrogenetic linkages among martian basalts. Implications based on trace element chemistry of olivine, Meteorit. Planet. Sci., 43, 1241–1258.
Steele A. et al. 2012. A reduced organic carbon component in Martian basalts, Science, 337, 212-215.
Symes S.J.K., Borg L.E., Shearer C.K. and Irving A.J. 2008. The age of martian meteorite NWA 1195 and the differentiation history of the shergottites, Geochim. Cosmochim. Acta, 72, 1696 – 1710.
Wallis J., Wickramasinghe C., Wallis D., Miyake N., Wallis M., Di Gregorio B. and Al Mufti S. 2012. Discovery of biological structures in the Tissint Mars meteorite, J Cosmology, 18, 8500-8505.
Williams R.M.E. et al. 2013. Martian fluvial conglomerates at Gale Crater, Science, 340, 1068-1072.