Skip to Main content Skip to Navigation
Journal articles

Radiation damage in diopside and calcite crystals from uranothorianite inclusions.

Abstract : Combining observation and simulation, radiohalos formed around urano-thorianite (UTh) from the Tranomaro granulitic skarns (SE-Madagascar) were studied. These structures consist of UTh grains surrounded by both aluminous diopside (Cpx) and calcite (Cc1) crystals. Optical microscope and Scanning Electron Microscope (SEM) images revealed (1) the presence of radiating cracks around the UTh probably due to swelling of the metamict UTh, (2) a diffuse optical halo at the Cc1/UTh interface, and (3) a wide "reaction zone" at the Cpx/UTh interface, composed of "secondary calcite" (Cc2) with low temperature sheet silicate from the smectite (φ) group. Samples prepared across various interfaces using Focused Ion Beam (FIB) were investigated by Transmission Electron Microscope (TEM). In contrast to SEM observations, there is no direct contact between Cc1 and UTh. From Cc1 to UTh, we found: (1) a large (~200-300 nm) amorphous zone (A), enriched in U, Th and Ca, but without Si; (2) a chain (B) of very small (~20 nm) ThO2 crystals; (3) another amorphous zone (C), which, in contrast to zone A is enriched in Si; and (4) another zone (D) made of small amorphous Si-rich "bubbles". The organization is similar for the UTh-Cc2 interface. The presence of hydrous minerals (smectite) and carbonate (calcite) in reaction zone and in cracks, the presence of Pb-rich inclusions in secondary calcite, the abundance of fluid inclusions in the porous layer in calcite, the dissociation of U and Th in the calcite-uranothorianite layer, and the ThO2 chains along interfaces, are strong indications that low-temperature crystallization was promoted by a fluid phase. SRIM simulation was used to calculate the effect of α and recoil particles of the three decay chains, in Cpx, Cc and UTh. The thickness of the damaged area calculated for α in Cpx and Cc are similar to the widths of the recrystallized areas observed in thin section (~30 µm). Corrected with the ''wandering recoil effect'', the size of the damaged area calculated for recoil nuclei in Cc (~50-60 nm) is ~multiplied by 3 and is in rather good agreement with the thickness of the totally amorphous layer at the Cc-UTh interface (~200 nm). Finally, it is emphasized that radiohalos are a point of chemical and physical weakness in a rock and probably a starting point for alteration.
Document type :
Journal articles
Complete list of metadata

https://hal.archives-ouvertes.fr/hal-00606536
Contributor : Anne-Magali Seydoux-Guillaume Connect in order to contact the contributor
Submitted on : Wednesday, July 6, 2011 - 5:23:28 PM
Last modification on : Tuesday, October 19, 2021 - 11:02:05 PM
Long-term archiving on: : Friday, October 7, 2011 - 2:36:01 AM

Files

Table1.pdf
Files produced by the author(s)

Identifiers

Collections

Citation

Anne-Magali Seydoux-Guillaume, Jean-Marc Montel, Richard Wirth, Bernard Moine. Radiation damage in diopside and calcite crystals from uranothorianite inclusions.. Chemical Geology, Elsevier, 2009, 261 (3-4), pp.318-332. ⟨10.1016/j.chemgeo.2008.04.013⟩. ⟨hal-00606536⟩

Share

Metrics

Record views

619

Files downloads

1447