2:15 PM - 2:30 PM
[SMP25-03] Average cooling rate of a Neoproterozoic-Cambrian UHT terrane (Rundvågshetta, Lützow-Holm Complex, East Antarctica)
Keywords:ultrahigh temperature metamorphism, zircon, cooling rate
Garnet in the studied sample has P-poor core, P-rich mantle and P-poor rim. Based on the detailed petrography of inclusions in garnet, [8] interpreted that the garnet core, mantle and rim were respectively formed in the prograde, peak and retrograde stages along a clockwise pressure-temperature evolution. Because the garnet rim is not replaced by orthopyroxene + cordierite symplectite, [8] interpreted that the garnet rim was formed after the post-peak isothermal decompression.
Zircon in the rock matrix and included in the garnet rim commonly has metamorphic rim with variable Th/U ratio of 0.08-1.13 [9]. The zircon rim includes sillimanite, K-feldspar and rutile and shows weighted mean age of 530.5 ± 4.9 Ma (2σ error, n = 13, MSWD = 1.5; [10]). Applying the Ti-in-zircon geothermometer [11] to the zircon rim gave 777-820 oC. Array plot analysis [12] of REE partitioning between the garnet and the zircon revealed that the zircon rim was formed in equilibrium with the garnet rim. Therefore, the U-Pb age of zircon rim (ca. 530 Ma) represents the timing of retrograde stage after the post-peak isothermal decompression, and thus the average cooling rate needs to be re-examined. By combining our zircon data with the biotite K/Ar age of [2], the average cooling rate after the post-peak isothermal decompression is calculated as ~ 13-20 oC/Myr. Therefore, if we assume the constant cooling rate from ~ 800 oC to ~ 300 oC, the 1 to 2 orders of magnitude rapid cooling suggested by [4] is not likely. Further studies using geochronometers with closure temperatures between ~ 800 oC to ~ 300 oC (e.g., rutile U-Pb dating; [13]) is required to test the rapid cooling model.
References
[1] Harley (2016) JMPS. [2] Fraser et al. (2000) JMG. [3] Harley et al. (2007) Elements. [4] Hiroi et al. (2019) JMPS. [5] Hiroi et al. (2020) Island Arc. [6] Ferrero & Angel (2018) J. Petrol. [7] Cesare et al. (2011) J. Virtual Explorer. [8] Suzuki & Kawakami (2020) Abstract of Annual Meeting of JAMS. [9] Suzuki et al. (2021) Abstract of the 12th Symposium on Polar Science. [10] Suzuki et al. (2022) Abstract of EGU General Assembly 2022. [11] Ferry & Watson (2007) CMP. [12] Taylor et al. (2017) JMG. [13] Johnson & Harley (2012) CUP.