The Lower Triassic sedimentary and carbon isotope records from Tulong
(South Tibet) and their significance for Tethyan palaeoceanography
Thomas Brühwiler
a,
⁎, Nicolas Goudemand
a
, Thomas Galfetti
b
, Hugo Bucher
a,c
, Aymon Baud
d
,
David Ware
a
, Elke Hermann
a
, Peter A. Hochuli
a,c
, Rossanna Martini
e
a
Paläontologisches Institut und Museum der Universität Zürich, Karl Schmid-Strasse 4, 8006 Zürich, Switzerland
b
Holcim Group Support Ltd, Materials Technology, 5113 Holderbank, Switzerland
c
Department of Earth Sciences, ETH, Universitätsstrasse 16, 8092 Zürich, Switzerland
d
BGC, Parc de la Rouvraie 28, 1018 Lausanne, Switzerland
e
Department of Geology and Paleontology, University of Geneva, Rue des Maraîchers 13, 1205 Geneva, Switzerland
abstract article info
Article history:
Received 18 June 2009
Received in revised form 23 September 2009
Accepted 11 October 2009
Keywords:
Early Triassic
South Tibet
Microfacies
Palaeoenvironments
Carbon isotopes
The Lower Triassic sedimentary and carbonate/organic carbon isotope records from the Tulong area (South
Tibet) are documented in their integrality for the first time. New age control is provided by ammonoid and
conodont biostratigraphy. The basal Triassic series consists of Griesbachian dolomitic limestones, similar to
the Kathwai Member in the Salt Range (Pakistan) and to the Otoceras Beds in Spiti (India). The overlying
thin-bedded limestones of Dienerian age strongly resemble the Lower Ceratite Limestone of the Salt Range.
They are followed by a thick series of dark green, silty shales of Dienerian–early Smithian age without fauna
that strikingly resemble the Ceratite Marls of the Salt Range. This interval is overlain by thin-bedded, light
grey fossil-rich limestones of middle to late Smithian age, resembling the Upper Ceratite Limestone of the
Salt Range. These are followed by a shale interval of early Spathian age that has no direct counterpart in other
Tethyan sections. Carbonate production resumes during the late early and middle Spathian with the
deposition of red, bioclastic nodular limestone (“Ammonitico Rosso” type facies). Apart from its colour this
facies is similar to the one of the Niti Limestone in Spiti and of the Spathian nodular limestone in Guangxi
(South China). As in other Tethyan localities such as Spiti, the early–middle Anisian part of the Tulong section
is strongly condensed and is characterized by grey, thin-bedded limestones with phosphatized ammonoids.
As for many other Tethyan localities the carbon isotope record from Tulong is characterized by a late
Griesbachian–Dienerian positive δ
13
C
carb
excursion (2‰), and a very prominent positive excursion (5‰) at
the Smithian–Spathian boundary, thus confirming the well-documented perturbations of the global carbon
cycle following the Permian–Triassic mass extinction event.
© 2009 Elsevier B.V. All rights reserved.
1. Introduction
The end-Permian mass extinction is the biggest known crisis in
life history and wiped out more than 90% of all marine species (e.g.
Raup and Sepkoski, 1982). The subsequent Early Triassic recovery of
marine and terrestrial ecosystems is considered to have been delayed
when compared with other mass extinctions and to have lasted until
the end of the Early Triassic (e.g. Erwin, 1998). Many marine clades
such as corals (Stanley, 2003), foraminifers (Tong and Shi, 2000) or
radiolarians (Racki, 1999) did not completely recover until the
Spathian or the Anisian, and poorly diversified and small-sized ben-
thonic shelly faunas predominated during the Early Triassic (e.g.
Fraiser and Bottjer, 2004; Fraiser et al., 2005). Metazoan reef com-
munities were completely absent in the Early Triassic (Pruss and
Bottjer, 2005). On the other hand, ammonoids and conodonts
recovered very fast in comparison with other marine clades (Brayard
et al., 2006, 2009; Orchard, 2007). Moreover, recent analysis of outer
platform paleoenvironments from South China reveals that increasing
rates of diversity and abundance of skeletal material occurred already
during well-oxygenated carbonate episodes of early Smithian and
Spathian age, respectively (Galfetti et al., 2008).
Stable carbon isotope studies have shown that the global carbon
cycle was profoundly perturbed at the Permian–Triassic boundary
and that several large and short-lived fluctuations occur in the Early
Triassic, before the carbon cycle stabilizes in the Middle Triassic (Baud
et al., 1996; Atudorei and Baud, 1997; Atudorei, 1999; Payne et al.,
2004; Richoz, 2004; Corsetti et al., 2005; Galfetti et al., 2007a,b,c;
Horacek et al., 2007a,b). The coincidence of carbon isotope cycle
instabilities with the Early Triassic delayed recovery suggests a
relationship between carbon cycling and biological rediversification
in the aftermath of the extinction (Payne et al., 2004). Indeed, for
instance, the major positive δ
13
C excursion at the Smithian–Spathian
Sedimentary Geology 222 (2009) 314–332
⁎ Corresponding author. Tel.: +41 44 634 26 98; fax: +41 44 634 49 23.
E-mail address: bruehwiler@pim.uzh.ch (T. Brühwiler).
0037-0738/$ – see front matter © 2009 Elsevier B.V. All rights reserved.
doi:10.1016/j.sedgeo.2009.10.003
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