Submicron Magnetite Grains and Carbon Compounds in Martian Meteorite ALH84001: Inorganic, Abiotic Formation by Shock and Thermal Metamorphism
- 1 June 2003
- journal article
- research article
- Published by Mary Ann Liebert Inc in Astrobiology
- Vol. 3 (2) , 369-392
- https://doi.org/10.1089/153110703769016451
Abstract
Purported biogenic features of the ALH84001 Martian meteorite (the carbonate globules, their submicron magnetite grains, and organic matter) have reasonable inorganic origins, and a comprehensive hypothesis is offered here. The carbonate globules were deposited from hydrothermal water, without biological mediation. Thereafter, ALH84001 was affected by an impact shock event, which raised its temperature nearly instantaneously to 500-700K, and induced iron-rich carbonate in the globules to decompose to magnetite and other minerals. The rapidity of the temperature increase caused magnetite grains to nucleate in abundance; hence individual crystals were very small. Nucleation and growth of magnetite crystals were fastest along edges and faces of the precursor carbonate grains, forcing the magnetite grains to be platy or elongated, including the "truncated hexa-octahedra" shape. ALH84001 had formed at some depth within Mars where the lithostatic pressure was significantly above that of Mars' surface. Also, because the rock was at depth, the impact heat dissipated slowly. During this interval, magnetite crystals approached chemical equilibria with surrounding minerals and gas. Their composition, nearly pure Fe3O4, reflects those of equilibria; elements that substitute into magnetite are either absent from iron-rich carbonate (e.g., Ti, Al, Cr), or partitioned into other minerals during magnetite formation (Mg, Mn). Many microstructural imperfections in the magnetite grains would have annealed out as the rock cooled. In this post-shock thermal regime, carbon-bearing gas from the decomposition of iron carbonates reacted with water in the rock (or from its surroundings) to produce organic matter via Fischer-Tropschlike reactions. Formation of such organic compounds like polycyclic aromatic hydrocarbons would have been catalyzed by the magnetite (formation of graphite, the thermochemically stable phase, would be kinetically hindered).Keywords
This publication has 73 references indexed in Scilit:
- Life on Mars: evaluation of the evidence within Martian meteorites ALH84001, Nakhla, and ShergottyPrecambrian Research, 2001
- Abiotic synthesis of polycyclic aromatic hydrocarbons on MarsJournal of Geophysical Research, 1999
- Magnetite whiskers and platelets in the ALH84001 Martian meteorite: Evidence of vapor phase growthPublished by Elsevier ,1999
- An Evaporation Model for Formation of Carbonates in the ALH84001 Martian MeteoriteInternational Geology Review, 1998
- A Search for Endogenous Amino Acids in Martian Meteorite ALH84001Science, 1998
- Isotopic composition of carbonates in the SNC meteorites, Allan Hills 84001 and ZagamiJournal of Geophysical Research, 1997
- Evaluating the Evidence for Past Life on MarsScience, 1996
- A possible high-temperature origin for the carbonates in the martian meteorite ALH84001Nature, 1996
- Record of fluid–rock interactions on Mars from the meteorite ALH84001Nature, 1994
- Hydrocarbon gases and bituminous substances in rocks from the Ilímaussaq alkaline intrusion, South GreenlandLithos, 1970