T159 Assembling Laurentia: Mesoproterozoic to Early Neoproterozoic Tectonic Evolution of Laurentia and Its Role within the Supercontinent Rodinia II
Wednesday, 28 October 2020
5:30 PM - 8:00 PM
Meeting Rooms
A DEEPER LOOK AT THE MESOPROTEROZOIC CA. 1.4 GA PICURIS OROGENY IN ARIZONA, USA: OBSERVATIONS FROM GRANULITE FACIES METAMORPHIC ROCKS IN THE SIERRA ESTRELLA MOUNTAINS
Paper number: T159-4
Program: Technical Sessions
Time: 5:55 PM – 6:05 PM
Authors
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Benjamin HallettUniversity of Wisconsin Oshkosh, Oshkosh, WI
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Christopher G. DanielBucknell University, Lewisburg, PA
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Arend MeijerUniversity of Arizona, Tucson, AZ
Abstract
Preliminary thermodynamic modeling of these two samples was performed with Theriak–Domino and the H&P ’98 data set. The Sil inclusions within Grt suggest Sil growth possibly during subsolidus St-breakdown or Ms-melting in both samples. The presence of Ky bearing melt textures in both samples may reflect prograde growth of Ky from Ms- or Bt-melting suggesting minimum P–T conditions > 7.5 kbar and > 700 °C. The replacement of Grt by Ky-Bt-Pl indicates melt crystallization at P > 7.5 kbar for sample R. A significant amount of retrograde Ms in sample R implies in-situ melt crystallization during retrograde cooling.
In sample W, the preservation of Kfs in the matrix and the lack of retrograde Ms, suggests cooling followed melt extraction at P above Crd stability (5-6 kbar). The preserved peak T assemblage yields modeled P–T constraints of 780–870 °C at 7.5–9 kbar with retrogression into the Sil+melt field.
Previously reported zircon ages for the area suggest partial melting near 1.4 Ga (Meijer, 2019). The timing and P-T conditions of metamorphism in the Sierra Estrella mountains are similar to high-grade metamorphic rocks in northern New Mexico and southern Colorado; these rocks likely represent the southwestern extension of the Picuris orogenic belt.
Geological Society of America Abstracts with Programs. Vol. 52, No. 6
doi: 10.1130/abs/2020AM-359971
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