Aretz et al_2011.pdf - ORBi - Université de Liège
Aretz et al_2011.pdf - ORBi - Université de Liège
Aretz et al_2011.pdf - ORBi - Université de Liège
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Kölner Forum Geol. P<strong>al</strong>äont., 19 (2011)<br />
M. ARETZ, S. DELCULÉE, J. DENAYER & E. POTY (Eds.)<br />
Abstracts, 11th Symposium on Fossil Cnidaria and Sponges, <strong>Liège</strong>, August 19-29, 2011<br />
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Upper Ordovician and Lower Silurian cor<strong>al</strong>s from the Pin Formation<br />
(Spiti V<strong>al</strong>ley, Northern India)<br />
Thomas SUTTNER & Erika KIDO<br />
Austrian Aca<strong>de</strong>my of Sciences (CPSA) c/o University of Graz, Institute for Earth Sciences (Geology &<br />
P<strong>al</strong>eontology), Heinrichstrasse 26, A-8010 Graz, Austria; thomas.suttner@uni-graz.at,<br />
erikakido07@yahoo.co.jp<br />
The late Katian is known as the time when reefs flourished and expan<strong>de</strong>d glob<strong>al</strong>ly (compare WEBBY<br />
2002) before the ons<strong>et</strong> of the Hirnantian ice age, which tremendously affected biota world-wi<strong>de</strong> (SHEEHAN<br />
2001). This interv<strong>al</strong> conforms to the Boda Event (FORTEY & COCKS 2005), which is consi<strong>de</strong>red as interglaci<strong>al</strong><br />
phase during the late Ordovician ice-house. Faun<strong>al</strong> and flor<strong>al</strong> climax conditions are documented especi<strong>al</strong>ly<br />
by increased abundance and a wi<strong>de</strong>ning of the latitudin<strong>al</strong> distribution-belt of carbonate factories (see<br />
WEBBY 2002) which produced limestone <strong>de</strong>posits at higher latitu<strong>de</strong>s on the peri-Gondwana shelf<br />
interrupting clastic sedimentation dominant at that time (e.g., LOI <strong>et</strong> <strong>al</strong>. 2010).<br />
During the early P<strong>al</strong>aeozoic the Indian subcontinent was part of northern Gondwana inheriting a<br />
p<strong>al</strong>aeo-position of approx. 25-30°S. Among sever<strong>al</strong> loc<strong>al</strong>ities, especi<strong>al</strong>ly the succession in the Spiti V<strong>al</strong>ley in<br />
northern India (recent geographic position) is known for sh<strong>al</strong>low marine carbonate <strong>de</strong>posits of Ordovician<br />
to Silurian age yielding plenty of sm<strong>al</strong>l patch reefs (Takche Member of the Pin Formation, compare Fig. 1).<br />
One of these cor<strong>al</strong> bearing units was referred to as “Silurian reef<strong>al</strong> buildups” of the Takche Formation (syn.<br />
Pin Fm) by BHARGAVA & BASSI (1986). The age constrain of these bioclastic limestones was based on data<br />
from macrofossils provi<strong>de</strong>d by REED (1912), who <strong>de</strong>scribed most of the materi<strong>al</strong> from the Him<strong>al</strong>ayan fossil<br />
collection of Hay<strong>de</strong>n and Krafft. Since then that unit remained assigned to Silurian age. In 2001 a first<br />
attempt was ma<strong>de</strong> to apply mo<strong>de</strong>rn microfossil biostratigraphy by dissolving sever<strong>al</strong> hundred kilos of<br />
carbonate rock samples from the type section, which fin<strong>al</strong>ly produced a quite diverse conodont fauna<br />
referring to Katian age (SUTTNER 2003).<br />
Actu<strong>al</strong>ly, the stratotype of the Pin Formation is exposed in the Pin V<strong>al</strong>ley (Spiti) near the sm<strong>al</strong>l village of<br />
Farka Muth (<strong>al</strong>titu<strong>de</strong>: 3750m), Northern India. The Spiti region is part of the Himach<strong>al</strong> Pra<strong>de</strong>sh district and<br />
lies in the high north-western Him<strong>al</strong>ayas. The Pin Formation comprises a 280 m thick sedimentary<br />
succession of late Ordovician and Silurian rocks. HAYDEN (1904) divi<strong>de</strong>d the formation into horizon 1 to 8<br />
(see Fig. 1). Some years later the Ordovician/Silurian boundary was fixed by REED (1912) b<strong>et</strong>ween horizons<br />
5 and 6 as he conclu<strong>de</strong>d that the assemblage of cor<strong>al</strong>s in Horizon 6 had affinities mainly with Silurian<br />
species (Horizon 6 equates with the above mentioned “Silurian reef<strong>al</strong> buildups” of the Takche Formation<br />
(syn. Pin Fm) by BHARGAVA & BASSI 1986). SUTTNER (2007) divi<strong>de</strong>d the Pin Formation into 17 lithologic<strong>al</strong><br />
units (P/1-17) in ascending or<strong>de</strong>r and assigned P/1-6, P/7-13 and P/14-17 to the Farka Muth, Takche, and<br />
Mikkim members, respectively (Fig. 1). During the work on the lithostratigraphy and facies of this<br />
formation <strong>al</strong>so the position of O/S boundary within the Pin Formation could be revised by the application<br />
of microfossil biostratigraphy and put b<strong>et</strong>ween HAYDEN’S (1904) horizons 6 and 7 (unit P/13 and P/14<br />
sensu Suttner 2007). It turned out that the entire Takche Member, which is correlated with HAYDEN’S<br />
horizons 2 to 6, yield conodonts referring to the Amorphognathus ordovicicus Zone (Katian, Upper<br />
Ordovician). However, age assignment for the other two members is still uncertain. Based on some few<br />
ozarkodinid conodont specimens an early Silurian (Llandovery?) age is suggested for the Mikkim Member.<br />
Hirnantian <strong>de</strong>posits are missing in this area, which is linked to the glob<strong>al</strong> lowstand. Solely a mixed<br />
conodont fauna (Ordovician and Silurian species) is observed in the uppermost part of unit P/13 (compare<br />
SUTTNER <strong>et</strong> <strong>al</strong>. 2007).<br />
Apart from conodonts, abundant fossils, such as foraminifera, stromatoporoids, cor<strong>al</strong>s, gastropods,<br />
orthocerids, trilobites, tentaculites, brachiopods, bryozoans and graptolites, have been known from the<br />
Takche Member (e.g. REED 1912; BHARGAVA & BASSI 1986, 1998; SUTTNER & ERNST 2007). Quite well<br />
preserved tabulate and rugose cor<strong>al</strong>s are documented from the units P/7, 8, 10, 11 and 13 (Takche Member)<br />
and P/16 (Mikkim Member). The range chart in Fig. 1 shows that most of them appeared within the late<br />
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