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
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.