R. Kyle Guimon
University of Arkansas
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Geochimica et Cosmochimica Acta | 1985
R. Kyle Guimon; Bradly D. Keck; Karen S. Weeks; John Milton Dehart; Derek W. G. Sears
Abstract Samples of a type 3.4 chondrite have been annealed at 400–1000°C for 1–200 hours, their thermoluminescence properties determined and analyzed for K, Na, Mn, Sc and Ca by instrumental neutron activation analysis. After annealing at ⩽900°C, the samples showed a 50% decrease in TL sensitivity, while after annealing at 1000°C it fell to 0.1-0.01 times its unannealed value and loss of Na and K occurred. The TL and compositional changes resemble those observed for the equilibrated Kernouve chondrite after similar annealing treatments, except that the sharp TL decrease, and element loss, occurred at ~ 1100°C; this difference is presumably due to petrographic differences in the feldspar of the two meteorites. The temperature and the width of the TL peak showed a discontinuous increase after annealing at 800°C; peak temperature jumped from 130 to 200°C and peak width increased from 90 to 150°C. The activation energies for these TL changes are 7–10 kcal/mole. Similar increases in the TL peak temperature have been reported in TL studies of Amelia, VA, albite, where they were associated with the low to high-temperature transformation. However, the activation energy for the transformation is ~80 kcal/mole. These changes in TL emission characteristics resemble trends observed in type 3 ordinary chondrites and it is suggested that type 3.3–3.5 chondrites have a low-feldspar as TL phosphor and > 3.5 have high-feldspar as the phosphor. Thermoluminescence therefore provides a means of palaeothermometry for type 3 ordinary chondrites.
Geochimica et Cosmochimica Acta | 1988
R. Kyle Guimon; Gary E. Lofgren; Derek W. G. Sears
Samples of four type 3 chondrites have been annealed at 400–850°C and 0.77–1 kbar for 10–500 h in the presence of various amounts of water (0–10 wt.%) and sodium disilicate (0–2 molal) and their thermoluminescence properties measured. After annealing for >20 h at temperatures >600°C, the TL sensitivity of the samples increased by factors of up to 40. After annealing at 800°C. When both high and low forms were present originally, the low-form was destroyed preferentially. We suggest that these data are consistent with the TL-metamorphism trends observed in type >3.2 chondrites, being due to the formation of feldspar (with structural details being dependent on formation temperature) by the devitrification of chondrule glass during metamorphism. For types <3.2, the TL data are equally consistent with these types experiencing lower levels of metamorphism than the higher types, or with type 3.0 being produced from higher types by aqueous alteration. The presence of water with non-terrestrial D/H ratios, and petrographic evidence for aqueous alteration in Semarkona, lead us to favour the aqueous alteration hypothesis.
Earth and Planetary Science Letters | 1986
Bradly D. Keck; R. Kyle Guimon; Derek W. G. Sears
Abstract Samples of the Dhajala H3.8 chondrite have been annealed for 10 hours at 600, 700, 800, 900 and 1000°C and at 1000°C for 1, 2, 20 and 100 h and their thermoluminescence (TL) properties measured. The TL sensitivity decreased by a factor of 2 after annealing at , but at higher temperatures fell by an order of magnitude. An abrupt increase in the temperature of the TL peak from 172 ± 9°Cto231 ± 8°C and a steady increase in the width of the peak from 169 ± 7°Cto212 ± 5°C were caused by the annealing treatment. The TL phosphor in Dhajala is thought to be feldspar predominantly in the high-temperature (disordered) form, but the present data indicate that a contribution from the low-temperature form is also present and that this low-temperature component is converted to the high form by the annealing treatment. The low-temperature feldspar is located in a few of the chondrules ( ∼ 20% of those separated from the meteorite) which are also noteworthy for having high TL sensitivities. These chondrules must have suffered greater crystallization of their mesostasis than the other chondrules, and equilibrated to lower temperatures. It is argued that, for compositional reasons, their mesostasis constituted less of a barrier to diffusion and therefore equilibration. Presumably the post-metamorphic cooling rate of the meteorite through the stability field of the low form was slow enough to permit some crystallization, and the width and temperature of the TL peaks for petrologic types 3.5–3.9 are somehow related to cooling rate. Based on TL, there is no indication of a correlation between petrologic type and cooling rate for types 3.5–3.9; this is not consistent with a simple, single internally heated meteorite parent body.
Meteoritics | 1995
R. Kyle Guimon; Steven J. K. Symes; Derek W. G. Sears; Paul H. Benoit
Meteoritics | 1995
Derek W. G. Sears; A. D. Morse; Robert Hutchison; R. Kyle Guimon; Lu Jie; C. M. O'd. Alexander; Paul H. Benoit; I. P. Wright; C. T. Pillinger; Tian Xie; Michael E. Lipschutz
Geophysical Research Letters | 1986
R. Kyle Guimon; Derek W. G. Sears; Gary E. Lofgren
Archive | 1993
Steven J. K. Symes; R. Kyle Guimon; Paul H. Benoit; Derek W. G. Sears
Archive | 1986
R. Kyle Guimon; Derek W. G. Sears
Archive | 1986
R. Kyle Guimon; Gary E. Lofgren; Derek W. G. Sears
Archive | 1986
R. Kyle Guimon; Derek W. G. Sears; Gary E. Lofgren