Westfälische Wilhelms-Universität Münster: Forschungsbericht 2003-2004 - Institut für Planetologie

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Institut für Planetologie

Tel. (0251) 83-33492
Fax: (0251) 83-36301
e-mail: ifp@uni-muenster.de
www: http://ifp.uni-muenster.de/
Wilhelm-Klemm-Str. 10
48149 Münster
Geschäftsführender Direktor: HDoz. Dr. Thomas Stephan

Forschungsschwerpunkte 2003 - 2004  
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Experimentelle und Analytische Planetologie
Der Einfluss von Mikrostrukturen auf die geologische Signifikanz radiometrischer Alter von Datierungsmineralen: Beispiel Monazit

 
Dating with the U-(Th)-Pb, Rb-Sr, and K-Ar decay systems is one of the most fundamental techniques in geoscience. Yet frequently disturbances in the isotope systems of the dated minerals hamper an assessment of the geologic relevance of the measured data ("ages"). Such disturbances include partial loss of radiogenic isotopes, and parent-daughter element fractionation. These effects are explained by diffusion along lattice defects, re-crystallization, dissolution - precipitation processes, and most popular, by volume diffusion. The latter process stood in the center of most experimental and theoretical studies in the field of "opening and resetting of isotope systems", whereas, the essential role of the mineral's micro-structures is persistently underestimated. - We have studied the micro-structure of monazite using scanning electron microscopy (SEM), electron microprobe analysis (EMP), X-ray diffraction patterns (XRD) and transmission electron microscopy (TEM). Four well-characterized monazites were investigated, with concordant U-Pb ages ranging from 24 to 1928 Ma, and up to ~15 wt.% ThO2, and ~0.94 wt.% UO2. The single crystal fragments lack significant chemical zoning. The monazites are not metamict, despite their old ages, very high abundances of radionuclides, and hence, high time-integrated radiation doses. Except for the youngest one, the monazite crystals are composed of a mosaic of crystalline but slightly distorted domains. This structure is responsible for the presence of (1) mottled diffraction contrasts on the TEM, and (2) a second structural phase (B), with very broad XRD reflection patterns. For the 1928 Ma monazite, XRD reveals only the broad reflections of phase B, implying that the whole monazite was affected by radiation damage that resulted in total distortion of the lattice. It is concluded that radiation damage in the form of amorphous domains does not accumulate in monazite because self-annealing heals the defects as they are produced by a-decay damage. The only memory of irradiation-induced defects is the presence of distorted domains. As the diffusion rate of Pb in an undisturbed monazite lattice is extremely low, Pb loss due to volume diffusion out of the monazite lattice is virtually impossible. This is the basic reason why almost all monazites have concordant U-Th-Pb ages. Moreover, as long-term self-irradiation effects are limited in monazite, we consider this phase as good candidate for the storage of high-level nuclear waste under the aspect of its high resistance to irradiation.

Drittmittelgeber:

Deutsche Forschungsgemeinschaft

Beteiligte Wissenschaftler:

Deutsch A. (Leiter), Schärer U. (Univ. Nice), Seydoux-Guillaume A.-M., Wirth R. (GFZ-Potsdam)

Veröffentlichungen:

Seydoux-Guillaume A.-M., Goncalves Ph., Wirth R. and Deutsch A. (2003) Transmission electron microscope study of polyphase and discordant monazites: Site-specific specimen preparation using the focused ion beam technique. Geology 31, 973-976.

Seydoux-Guillaume A.-M., Wirth R., Deutsch A. and Schärer U. (2004) Microstructure of 24 - 1928 Ma concordant monazites; implications for geochronology and nuclear waste deposits. Geochim. Cosmochim. Acta 68, 2517-2527.

 

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