T293 Hello (Ancient) World!: Exploring the Neoproterozoic to Cambrian Interval by Quantitatively Probing the Rock Record

Wednesday, 25 September 2019
1:30 PM - 5:30 PM
Room 226ABC, North Building

ICE OR FIRE? CONSTRAINING THE ORIGIN OF ISOTOPICALLY ANOMALOUS CAP CARBONATE CEMENTS BY SIMS

Paper number: T293-4
Program: Technical Sessions
Time: 2:05 PM – 2:20 PM

Authors

Abstract

The Marinoan glaciation (a.k.a. the Snowball Earth) represents a profound paleoclimatic anomaly in deep time. However, the detailed mechanism of its termination remains largely unknown. It was hypothesized that massive releases of methane via clathrate destabilization at ~635 Ma may have played a role in terminating the glaciation. A key piece of supporting evidence is the finding of methane-derived authigenic calcite cements (MDACCs, δ13Ccarb values down to –48‰) within the Marinoan cap carbonates in South China. However, a more recent study based on clumped isotope (Δ47) measurements suggests that the MDACCs are hydrothermal (T as high as 476 °C) in origin. If correct, the MDACCs cannot be used to infer paleoenvironments right after the glaciation. To test these contrasting hypotheses (ice vs. fire), we conducted a detailed investigation via μXRF, CL, SEM, and SIMS. The SIMS data show a 60‰ range of δ13Ccarb values with positive values (as high as +6.3‰) exclusively in dolomites and negative values (as low as –53.8‰) in calcites. Both the positive δ13Ccarb values and the lowest δ13Ccarb values are revealed in this study for the first time. Our results show that the dolomite crystals are typically euhedral, anomalously large (up to 200 μm) in size, have positive δ13Ccarb values, and are Mn-poor with dull or red luminescence under CL, with dolomite cores partly or almost completely replaced by low-δ13Ccarb calcite. The calcites have low δ13Ccarb values, are Mn-rich with bright orange luminescence under CL, showing multiple stages of vug-filling cements surrounding the preexisting dolomite crystals. These results suggest that the dolomites have been significantly recrystallized during burial or hydrothermal diagenesis and the MDACCs formed even later, postdating the recrystallized dolomites. We conclude that the MDACCs are post-depositional and formed during late diagenesis. Our conclusion is consistent with the prior work based on clumped isotope analysis. The present study casts further doubt on using MDACCs as evidence for methane clathrate in deep time. The role of methane in terminating the Snowball Earth should be re-assessed.

Geological Society of America Abstracts with Programs. Vol. 51, No. 5

doi: 10.1130/abs/2019AM-332456

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