9 Mining in the Rocky Mountain Region and Beyond: Risks and Opportunities
Monday, 4 May 2020
1:25 PM - 4:30 PM
Cascades E
USING TITANITE COMPOSITIONS TO IDENTIFY INTRUSIVE PHASES AND MO-W MINERALIZATION PATTERNS IN THE OLIGOCENE LITTLE COTTONWOOD STOCK, UTAH
Paper number: 9-3
Program: Theme Sessions
Time: 1:50 PM – 2:10 PM
Authors
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Rodney ChadburnBrigham Young University, Provo, UT
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Jeffrey D. KeithBrigham Young University, Provo, UT
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Eric H. ChristiansenBrigham Young University, Provo, UT
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Bart J. KowallisBrigham Young University, Provo, UT
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Collin JensenBrigham Young University, Provo, UT
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Porter HenzeBrigham Young University, Provo, UT
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Alan KetringBrigham Young University, Provo, UT
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Levi De CrescenzoProvo, UT
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Haley Mosher527 N 675 E, Lindon, UT
Abstract
Magmatic titanite crystallized in each of the intrusive phases and, due to slow diffusion rates and high closure temperature, appears to have retained element patterns characteristic of the parental magma in primary or unaltered grains. Thus, electron microprobe and LA-ICP-MS analysis of titanite has been used to “fingerprint” their parent magma. Phaneritic RP titanite have lower Ti, Ca, Nb, Mo, and W than WP titanite, while porphyritic RP titanite have still lower concentrations (though higher Mn).
Applied to several samples with ambiguous affinities, these titanite fingerprints have expanded our spatial and temporal understanding of the magmatic system and accompanying mineralization by increasing the known extent of the WP and RP intrusions relative to the LCS, and in showcasing the reduced nature of the hydrothermal fluids via the breakdown of titanite in the WP and RP to minerals such as ilmenite and rutile. In contrast to some Mo-W systems, where titanite Mo values are high (120+ ppm) in the mineralizing granite, Mo values in titanite in the LCS-WP-RP system gradually decrease (averaging 45 to 29 to 18 ppm, respectively) towards the mineralizing RP intrusion. This gives an example of the potential misuse for titanite as an indicator mineral for Mo-W mineralization.
Geological Society of America Abstracts with Programs. Vol. 52, No. 3
doi: 10.1130/abs/2020RM-346800
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