Other
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufm.v41d2206c&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #V41D-2206
Other
[1115] Geochronology / Radioisotope Geochronology, [1140] Geochronology / Thermochronology, [1160] Geochronology / Planetary And Lunar Geochronology
Scientific paper
A common feature observed in 40Ar/39Ar age spectra of extraterrestrial (ET) rocks is a conspicuous decrease in the ages of high temperature extractions relative to lower temperature steps and a correlated increase in Ca/K, often succeeded by a monotonic increase in ages. This feature is routinely attributed to recoil-implanted 39Ar from a potassium (K)-rich donor phase into a K-poor receptor phase (e.g., 1,2). While 39Ar recoil redistribution is undoubtedly manifested in many terrestrial and ET 40Ar/39Ar whole-rock age spectra, it cannot easily explain the magnitude of high release temperature 40Ar*/39ArK anomalies observed in Martian meteorites ALH 84001 and Nakhla, as well as other course-grained meteorites and lunar rocks. Depending on the aliquot and sample, 50 - 100% of the pyroxene release spectra in ALH 84001 and Nakhla appear strongly perturbed to lower ages. As the mean recoil distance of 39Ar ~0.1 µm, the recoil hypothesis demands that a high-K phase be ubiquitously distributed amongst sub-micron to micron sized pyroxene crystals to account for the observed pyroxene age spectra. However, in both Nakhla and ALH 84001, pyroxene is often completely isolated from high-K phases and individual grains commonly exceed 100 µm in diameter. 40Ar/39Ar analyses of pyroxene-bearing terrestrial basalts, wherein fine-grained pyroxene and plagioclase are intimately adjoined, show that recoil-implanted 39Ar into pyroxene produces much less precipitous anomalies in 40Ar*/39ArK, as predicted by the recoil lengthscale. An alternative hypothesis is that whole-rock age spectra of ET samples with anomalously low ages at high temperatures may reflect diffusive 40Ar distributions within considerably degassed pyroxene grains. Owing to apparent differences in activation energies between glass and/or plagioclase and pyroxene, 40Ar may diffuse more rapidly from pyroxene under certain high-temperature conditions (i.e., above the temperature at which the extrapolated Ar Arrhenius relationships intersect). Thus, very brief, high-temperature shock-heating events may preferentially degas pyroxene without significantly resetting glass and plagioclase 40Ar/39Ar age spectra. This effect would be enhanced by highly localized shock-heating focused along pyroxene (sub)grain boundaries, as has been inferred in other cases (e.g., 3). The shock and impact origin of this feature may explain its frequent appearance in ET samples, regardless of grain size, as well as the general absence of terrestrial analogs. We will present new 40Ar/39Ar data from Martian meteorites and physical models to distinguish between these competing hypotheses. References Cited: 1. Turner & Cadogan, 1974, Possible effects of 39Ar recoil in 40Ar-39Ar dating. Proc. 5th LPSC, 1601- 1615. 2. Huneke & Smith, 1976, The realities of recoil: 39Ar recoil out of small grains and anomalous age patterns in 40Ar-39Ar dating. Proc. 7th LPSC, 1987-2008. 3. Min et al., 2003, Single grain (U-Th)/He ages from phosphates in Acapulco meteorite and implications for thermal history. EPSL 209, 323-336.
Cassata William S.
Renne Paul R.
Shuster David L.
Weiss Benjamin P.
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