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PESGB London Evening Meeting
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| The PESGB thank
ENI for sponsoring
this
London Evening wine reception |
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Global Neoproterozoic Petroleum
Systems:
Snowballs, Source Rocks and the search for "Old Oil"
Jonathan Craig, ENI
(jonathan.craig@agip.it)
Tuesday 12th
September 2006, doors open 5.45
pm for 6 pm
NB: Change of Venue:
Royal
Over-Seas League, Park Place, St James's Street, London
SW1A 1LR
To view Fig
1, Fig 2
The Neoproterozoic eon, stretching from
1000 Ma to the base of the Cambrian at 542 Ma, is relatively poorly known
from a petroleum perspective despite the existence of proven plays in many
parts of the world including Oman, Mauritania, Siberia, India, Pakistan,
Australia and the United States. In geological terms, the Neoproterozoic
was a period of massive atmospheric, climatic and tectonic change. It was
dominated by the “Freeze-Fry” cycles of the Cryogenian (850-650 Ma)
“Snowball Earth” glaciations (Fig. 1) when global mean surface temperature
oscillated between -50°C and +50°C over periods of ±5-10 Ma and
atmospheric CO2 levels may have periodically reached up to 350
times those of today. Perceived wisdom suggests that these extreme
climatic variations were ultimately responsible for the emergence of the
first recognisable animal life around 600 Ma during the Ediacaran (630 Ma
– 542 Ma) and, in turn, for the eventual explosion of life forms in the
latest Neoproterozoic and Early Cambrian.
Many of the proven
“Infracambrian” (Neoproterozoic to Early Cambrian) hydrocarbon plays
around the world depend on the presence of prolific “Infracambrian” source
rocks. There is increasing evidence that deposition of many of these
organic-rich units was triggered by strong post-glacial sea level rises on
a global scale following “Snowball Earth” type glaciations, coupled, in
some areas at least, with basin development and rifting on a more local
scale.
One region of the
Neoproterozoic world which is exciting interest in the search for
stratigraphically deeper “Infracambrian” plays and associated “Old Oil”
(or even, gas) is the so-called “North Gondwana Margin”, which extends
from northern South America, across North Africa and the Middle East and
into Pakistan and N.W. India (Fig. 2). The interest is rooted in the
greatly improved understanding of the prolific Neoproterozoic to Early
Cambrian (Huqf Supergroup), intra-salt Ara “Stringer” carbonate and Athel
silicilyte plays, and the increasingly important older “pre-salt” plays,
in the South Oman Salt Basin. Similar plays are already being actively
parsued within the age-equivalent Marwar and Machh supergroups to the
east, in the Sindh and Punjab regions of Pakistan and in Rajasthan in
Western India. However, attention is increasingly turning to the potential
for age-equivalent and possibly older Neoproterozoic plays across the rest
of the Middle East and North Africa.
The equivalent
“Infracambrian” succession in North Africa is now widely accessible for
research and is already emerging as a hydrocarbon exploration target with
considerable potential and with proven petroleum systems in several
different areas. Large basins with excellent surface outcrops and thick
sedimentary fills of Neoproterozoic and Early Palaeozoic age are
widespread throughout North Africa and the Middle East (Fig. 2).
New biostratigraphic
analysis has recently provided the first definitive Late Riphean (Tonian –
Cryogenian) age dates for reservoir sequences containing gas in the
Taoudenni Basin in Mauritania (to add to similar dates obtained for
subsurface sequences in the Cyrenaica Platform bordering the East Sirte
Basin of Libya in the 1970’s). New fieldwork in the Taoudenni Basin, in
the Anti-Atlas region of Morocco and in the Kufra Basin in Libya has also
added to our understanding of Infracambrian reservoir, source and seal
relationships and confirmed the widespread presence of stromatolitic
carbonate units of potential reservoir facies across many parts of North
Africa.
Neoproterozoic to Early
Cambrian organic-rich strata were deposited in both high latitudes (e.g.
Mauritania) and low latitudes (e.g. Oman) along the North Gondwana Margin.
Some of the black shales encountered on the West African Craton may be as
old as 1000 Ma and clearly predate the Pan-African orogenic event. These
are substantially older than the majority of the Infracambrian
organic-rich units that occur across much of North Africa and the Middle
East (including those in Oman) which predominantly range from c. 850 to c.
540 Ma in age. Infracambrian black shales and organic-rich dolomites,
which are broadly age equivalent to the prolific Infracambrian source
rocks in Oman, are known to generate light oil and heavy oil respectively,
further east in Pakistan and India.
Post-glacial black shale
deposition is also a well-documented phenomenon in northern Gondwana
during subsequent Palaeozoic times. A post-glacial sea level rise of some
50-100 m, following the Late Ordovician Saharan glaciation, flooded large
areas of northern Africa and Arabia during the earliest Silurian. The
associated transgression was global and pushed the coastline of northern
Gondwana southwards by many hundreds of kilometres. As appears to be the
case during the Infracambrian, Silurian black shale deposition was
restricted to the anoxic parts of the infrashelf basins. The Late
Ordovician-Early Silurian systems may form a good analogue for
post-glacial source rock depositional systems, both spatially and
temporally.
Further investigations of
the Infracambrian black shales globally are required in order for us to
better understand their relationship with the “Snowball Earth”
glaciations. In particular, high resolution biostratigraphic, isotope and
other palaeotemperature proxy records need to be documented for suitable
type sections of the organic-rich facies and constrained with absolute
radiometric dates, so that the onset and termination of black shale
deposition can be compiled with precision and placed within the
Neoproterozoic to Early Cambrian climatic context.
Our knowledge of the
Neoproterozoic and its petroleum systems is improving rapidly. There is
already a widespread and growing perception that the “Infracambrian”
succession will continue to form an important target for future
exploration, not only in North Africa, but elsewhere along the North
Gondwana Margin and globally.
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