Author
Listed:
- D. A. Evans
(California Institute of Technology)
- N. J. Beukes
(Rand Afrikaans University)
- J. L. Kirschvink
(California Institute of Technology)
Abstract
One of the most fundamental enigmas of the Earth's palaeoclimate concerns the temporal and spatial distributions of Precambrian glaciations. Through four billion years of Precambrian history, unequivocally glacial deposits have been found only in the Palaeoproterozoic and Neoproterozoic record1. Nonetheless, some of these deposits are closely associated with tropical— rather than just polar—palaeolatitudinal indicators such as carbonate rocks, red beds, and evaporites1,2. These observations are quantitatively supported by palaeomagnetic results indicating a ∼5° latitude for Neoproterozoic glaciogenic rocks in Australia3–5. Similarly reliable palaeolatitudes for the older, Palaeoproterozoic glaciogenic rocks have not yet been obtained, as such deposits commonly suffer from poor preservation and secondary magnetic overprinting. The Archaean–Palaeoproterozoic 'Transvaal Supergroup' on the Kaapvaal craton in South Africa is, however, exceptionally well preserved, and is thus amenable to the palaeomagnetic determination of depositional palaeolatitudes. Within this supergroup the ∼2.2 billion-year old Ongeluk lavas are a regionally extensive, largely undeformed and unmetamorphosed, extrusive volcanic succession6, which conformably overlies glaciogenic deposits (the Makganyene diamictite). Here we report a palaeomagnetic estimate of 11 ± 5° depositional latitude for the lavas, and hence for the underlying contemporaneous glacial rocks. The palaeoclimate enigma is thus deepened; a largely ice-free Precambrian world was apparently punctuated by two long ice ages, both yielding glacial deposits well within tropical latitudes.
Suggested Citation
D. A. Evans & N. J. Beukes & J. L. Kirschvink, 1997.
"Low-latitude glaciation in the Palaeoproterozoic era,"
Nature, Nature, vol. 386(6622), pages 262-266, March.
Handle:
RePEc:nat:nature:v:386:y:1997:i:6622:d:10.1038_386262a0
DOI: 10.1038/386262a0
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