JOHANNES GUTENBERG-UNIVERSITÄT MAINZ - International ...
JOHANNES GUTENBERG-UNIVERSITÄT MAINZ - International ...
JOHANNES GUTENBERG-UNIVERSITÄT MAINZ - International ...
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<strong>JOHANNES</strong> <strong>GUTENBERG</strong>-<strong>UNIVERSITÄT</strong> <strong>MAINZ</strong><br />
Institut für Geowissenschaften<br />
Prof. A. Kröner<br />
A. Kröner • Universität Mainz • Geowissenschaften • 55099 Mainz •<br />
Tel.: +49 6131/3922163<br />
Fax: +49 6131/3924769<br />
E-mail: kroener@mail.uni-mainz.de<br />
Prof. J. Negendank 28 December 2006<br />
Secretary-General, <strong>International</strong> Lithosphere Program<br />
GeoForschungsZentrum Potsdam<br />
Telegrafenberg<br />
14473 POTSDAM<br />
Germany<br />
Re: Report 2006 for ILP Task Force 1 (Project ERAS - Earth Accretionary Systems)<br />
Dear Jörg,<br />
This is a progress report on activities of the ERAS Initiative for the calendar year 2006.<br />
The ERAS proposal was originally formulated by P.A. Cawood (Perth, Australia), B.F. Windley<br />
(Leicester, UK), A. Kröner (Mainz, Germany), T. Kusky (St. Louis, USA) and W. Mooney (Menlo<br />
Park, USA) and submitted to ILP in 2003. It aims at multidisciplinary studies of accretionary<br />
orogens and accretion processes though Earth history since these are much less well understood<br />
than collisional orogens and are an important element of crustal growth and crustal recycling.<br />
The Project was officially accepted by the ILP Board at its meeting during the Annual Meeting<br />
of the European Geosciences Union (EGU) in Vienna in April 2005 and is now designated as ILP<br />
Task Force 1 and is chaired by Peter Cawoood and myself.<br />
In April 2006 Task Force 1 organized and sponsored two symposia at EGU in Vienna. The first<br />
entitled "Accretionary orogens and crustal growth: facts, fiction, fantasy" chaired by P.A. Cawood,<br />
P. Clift, A. Kröner, and the second "Composition, structure and evolution of the Caribbean<br />
lithosphere" organized by A. Perez-Estaun, A. Garcia-Casco and Y. Rojas-Agramonte. Both<br />
symposia were well attended and provided broad spatial and temporal coverage of the world’s<br />
accretionary orogens, their role on generation of continental crust and the detailed character of their<br />
assembly, deformation and metamorphism.<br />
Also in April, Task Force 1 co-sponsored the joint meeting of the Geological Society of<br />
America and Asociatíon Geológica Argentina, entitled “Backbone of the Americas - Patagonia to<br />
Alaska” held in Mendoza, Argentina.<br />
In June 2006 Task Force 1 co-sponsored a highly successful Penrose-Conference in Lander,<br />
Wyoming, USA, on when plate tectonics began. This was organized by Kent Condie, Alfred
Kröner and Robert Stern and attended by 60 scientists from around the world. The main<br />
issue was to discuss criteria and evidence concerning the beginning of plate tectonics in the<br />
Precambrian, and a summary report was published in NATURE by one of the attending journalists<br />
(Annexure 1). Accretionary orogens featured prominently at this meeting since Japanese geologists<br />
claim to have recognized Japan-style ocean plate stratigraphy in early Archaean rocks at Isua,<br />
Barberton and in the Pilbara greenstones of Western Australia. This issue will be the topic of a<br />
forthcoming ERAS field workshop in 2007 (see below).<br />
2<br />
ERAS organized a whole-day symposium at the Australian Earth Sciences Convention in<br />
Melbourne on July 6 entitled “Accretionary Orogens: their composition, structure and evolution”<br />
and chaired by P.A. Cawood, W. Collins and G. Skilbeck. The symposium honoured the<br />
contribution of Professor Evan Leitch who spent a life time unravelling the accretionary history of<br />
the Palaeozoic New England Orogen in eastern Australia. Gordon Lister gave the keynote address<br />
on “Contrasting styles in accretionary versus collisional orogens”. The symposium was attended by<br />
over 100 scientists, and topics ranged from Palaeoproterozoic accretionary tectonics in central<br />
Australia to Gondwana assembly and through to modern arc systems of the Western Pacific, but<br />
with a focus on the Palaeozoic accretionary architecture of eastern Australia.<br />
ERAS scientists Bor-ming Jahn and Alfred Kröner organized and sponsored a super-session on<br />
"Composition and Evolution of the Asian Lithosphere" at the third meeting of the Asia-Oceania<br />
Geoscience Society in Singapore in early July 2006. This super-session included 11 separate<br />
sessions list below (for complete descriptions see Annexure 2):<br />
1. Evolution of the Asian continental mantle lithosphere - constraints from xenolith studies<br />
(Bill Griffin, Sue O'Reilly, and Kuo-Lung Wang)<br />
2. Lithospheric and mantle dynamics (David Yuen and Huai Zhang)<br />
3. Growth and evolution of the Asian continent (M. Zhai, S. Wilde, G. Zhao, M. Cho)<br />
4. Orogenic processes in Asia: regimes of continental collision (S.L. Chung, Mike Searle)<br />
5. Orogenic processes in Asia: regimes of continental accretion (Alfred Kröner)<br />
6. Generation of granitoids in Asia and Australia (W. Collins, T. Nakajima, Fuyuan Wu)<br />
7. Deep Structure and Tectonics of the Asian Lithosphere: The Geophysical Perspective<br />
(Larry Brown, Dapeng Zhao, Bor-Shouh Huang, Wangping Chen)<br />
8. Evolution of the SW Pacific and South China Sea (S.K. Hsu, R. Shinjo, T.Y. Lee)<br />
9. Crustal deformation and neotectonics in Asia (Yue-Gau Chen, Jian-Cheng Lee, Kerry<br />
Sieh, Yuichi Sugiyama)<br />
10. Ore deposits and economic geology in Asia (Shunso ISHIHARA, Jingwen MAO)<br />
11. Gem materials - from diamond to pearls (W. Hofmeister, Vu Xuan Quang)<br />
A highlight of the year’s activities was an ERAS field workshop in Japan in September<br />
consisting of a 1.5 day symposium and a 4 day field trip, organized by Gaku Kimura, Yukio Isozaki<br />
and Shigenori Maruyama (see Annexure 3). The workshop enabled scientists from Precambrian and<br />
Phanerozoic accretionary terranes from around the world to see the classic arc accretionary<br />
sequences exposed in the subduction complex assemblages including the ocean floor stratigraphic<br />
sequences preserved therein. The symposium was divided into a half day open session as part of the<br />
Geological Ssociety of Japan Annual Meeting and a one day closed session limited to ERAS<br />
participants. Talks focused on the spectacular onland and offshore accretionary complexes in Japan.
3<br />
Task Force 1 also co-sponsored a 4-day Sino- German workshop in Beijing on the evolution<br />
of Palaeozoic to Mesozoic orogenic belts in Central Asia. This was funded by the Sino-German<br />
Centre for Research Promotion and organized by Wenjiao Xiao (Beijing) and Alfred Kröner<br />
(Mainz) and attended by 30 Chinese, 12 German, two Australian one British, one French and one<br />
Russia scientist. Emphasis of the discussion was on tectonics, petrology of UHP terranes,<br />
geochronology and palaeomagnetism (Annexure 4). Qincheng Wang, the Chinese Member of the<br />
ILP Bureau, attended this meeting, and suggested to establish a Regional Working Group for the<br />
Central Asian Orogenic Belt under Task Force 1 and supported by the Regional Committee for<br />
Asia in view of the increasing interest of scientists from China, Russia, Kazakhstan and Kyrgyzstan<br />
in this region.<br />
Alfred Kröner and Larry Brown initiated discussions on a major seismic-geologic traverse<br />
across the Central Asian Orogenic Belt from the Siberian craton to the Sino-Korean craton (see<br />
Annexure 4). This multi-disciplinary “Lithoprobe-style” project should be organized under the<br />
umbrella of Task Force 1 and will require major funding from both China and Russia. Discussions<br />
so far have been very encouraging, and a technical workshop will be held in Beijing in April 2007.<br />
Plans for 2007 include a field workshop in the Pilbara region of western Australia. This region is<br />
critical in evaluating the time of formation of the worlds earliest accretionary processes as well as<br />
the initiation of plate tectonics. Controversy surrounds the region with some geologists favouring<br />
an ocean floor setting involving generation of ocean lithosphere and its conveyor belt like motion to<br />
a subduction zone, whereas others dispute this claim. Our aim is to have both groups present their<br />
evidence at the critical outcrops along with a group of ERAS scientists to evaluate the evidence.<br />
This region was selected by the GSA Penrose conference on the initiation of plate tectonics in June<br />
2006 as a key issue to be resolved.<br />
Task Force 1 will co-sponsor the Third Field Workshop of IGCP-Project 480 in Beijing, to be<br />
held in August 2007 with a field trip to examine accretion tectonics and Palaeozoic ophiolites in<br />
Inner Mongolia. ERAS will also co-sponsor the <strong>International</strong> Symposium on Precambrian<br />
Chronology and Tectonic Evolution (ISPCTE), to be held in Beijing in August 2007, with four field<br />
trips to Proterozoic and Archaean areas in China.<br />
Also in 2007, a major book “Accretionary Orogens in Space and Time” edited by Peter A.<br />
Cawood and Alfred Kröner, will be published as a Geological Society of London Special<br />
Publication. The ILP logo will appear on the book. This will be a major output from Task Force 1.<br />
March is set as the date for submission of papers, and it is hoped to have the revised and accepted<br />
chapters submitted to the Geological Society for publishing by the second half of 2007. To date 29<br />
chapters are planned with 13 providing an overview and discussion of general processes in<br />
accretionary orogens and the remainder devoted to studies of specific orogens ranging in age from<br />
early Archaean to Recent (a complete discretion of the books contents in given in Annexure 5) .
4<br />
In 2008 Peter Cawood, Raimo Lahtinen and Yukio Isozaki will hold an ERAS symposium<br />
at the Oslo <strong>International</strong> Geological Congress entitled “Accretionary Orogens: Character and<br />
Processes”.<br />
Yours sincerely,<br />
Alfred Kröner, Co-Chairman<br />
Annexures:<br />
1. Report in NATURE on Penrose-Conference, June 2006<br />
2. Description of Super-Session at AOGS Singapore, July 2006<br />
3. ERAS field workshop in Japan, September 2006<br />
4. Report on Sino-German Workshop on Central Asian tectonics in Beijing, December 2006<br />
5. Proposal for a seismic-geologic transect across the Central Asian Orogenic Belt<br />
6. Proposed Geological Society of London Special Publication on Accretionary Orogens.<br />
Selected Publications<br />
Buchan, C., Cawood, P.A., 2006. Linking accretionary orogenesis with supercontinent assembly.<br />
Earth Sci. Rev., in press.<br />
Cawood, P.A., Johnson, M.R.W. and Nemchin, A.A., 2006. Early Palaeozoic orogenesis along the<br />
Indian margin of Gondwana: Tectonic response to Gondwana assembly. Earth Planet. Sci.<br />
Lett., in press.<br />
Cawood, P.A., Kröner, ,A, Pisarevsky, S., 2006. Precambrian plate tectonics – Criteria and<br />
evidence. GSA Today, 16, No. 7, 4-11.<br />
Isozaki, Y., 2006. "Overview: Evolution of the Japanese Islands" and "The Jurassic accretionary<br />
complex in Inuyama". In: Fieldtrip guidebook for Int. Workshop ERAS (Earth Accretionary<br />
Systems in space and time)-2006, 1-20, J1-J30.<br />
Kawai, T., Windley, B.F., Terabayashi, M., Yamamoto, H., Maruyama, S., and Isozaki, Y., 2006.<br />
Mineral isograd and zones of the Anglesey blueschist belt, UK: implications for the<br />
metamorphic development of a Neoproterozoic subduction-accretion complex. J. Metam.<br />
Geol., 24, 591-602.<br />
Kröner, A., Windley, B.F., Badarch, G., Tomurtogoo, O., Hegner, E., Jahn, B.M., Gruschka, S.,<br />
Khain, E.V., Demoux, A., Wingate, M.T.D., 2006. Accretionary growth and crust-formation<br />
in the Central Asian Orogenic Belt and comparison with the Arabian-Nubian Shield. In: R.D.<br />
Hatcher, Jr. (ed.), in: 4-D framework of the continental crust - Integrating crustal processes<br />
through time. Memoir, Geol. Soc. America, in press.<br />
Li, Songlin; Mooney, Walter, Fan, Jichang, 2006. Crustal structure of mainland China from deep<br />
seismic sounding data. Tectonophysics, 420,<br />
Liu, Mingjun; Mooney, Walter; Li, Songlin; Okaya, Nihal and Detweiler, Shane, 2006. Crustal<br />
Structure of the northeastern margin of the Tibetan Plateau from the Songpan-Ganzi terrane<br />
to the Ordos basin. Tectonophys, 420,
5<br />
Osozawa, S., Tsolmon, G., Majigsuren, U., Sereenen, J., Jahn, B.M., 2006. Structural<br />
evolution of the Bayanhongor region, west-central Mongolia. J. Asian Earth. Sci., in review.<br />
Ota, A. and Isozaki, Y., 2006. Fusuline biotic turnover across the Guadalupian-Lopimgian<br />
(Middle-Upper Permian) boundary in mid-oceanic carbonate buildups: Biostratigraphy of<br />
accreted limestone in Japan. J. Asian Earth Sci. 26, 353-368.<br />
Pisarevsky, S.A., Murphy, J.B., Cawood P.A.,, Collins, A.S., 2006. Late Neoproterozoic and early<br />
Cambrian palaeogeography: models and problems. In Pankhurst, R. et al (eds.), Geol. Soc.<br />
London, Spec. Publ., in press.<br />
Rojas-Agramonte, Y., Kröner, A., Sukar, K., Mattinson, J., Somin, M. & Wingate, M.T.D., 2006.<br />
Timing of Cretaceous island arc granitoid magmatism in Cuba as revealed by U-Pb SHRIMP<br />
zircon dating: Significance for arc magmatism in the Caribbean. J. Geol., submitted.<br />
Romanyuk, Tanya; Mooney, Walter; Detweiler, Shane, 2006. Two lithospheric profiles across<br />
Southern California derived from gravity and seismic data. J. Geodynamics, submitted.<br />
Trubitsyn, V., Kaban, M., Monney, W., Reigber, C., Schwintzer, P., 2006. Simulation of active<br />
tectonic processes for a convecting mantle with moving continents. Geophys. J. Internat., 164, 3,<br />
611-623.<br />
Vijaya Rao, V., Sain, K., Reddy, P.R., Mooney, W.D., 2006. Crustal structure and tectonics of the<br />
northern part of the Southern Granulite terrane, India, Earth Planet. Sci. Lett., 251, 90-103.<br />
Wang, Tao, Hong, Da-wei, Jahn, B.M., Tong Y., Wang Yan-bin, Han Bao-fu, Wang Xiaoxia,<br />
2006. Timing, petrogenesis and setting of Paleozoic synorogenic intrusions from the Altai<br />
Mountains, Northwest China: implications for the tectonic evolution of an accretionary orogen.<br />
J. Geol., 114, 735-751.<br />
Wang, Tao, Jahn. B.M., Kovach, V.P., Tong, Y., Wilde, S.A., Hong, D.W., Wang, X.X., 2006.<br />
Identification and petrogenesis of Mesozoic anorogenic granitic magmatism in the Altai<br />
Paleozoic accretionary orogen (NW China) and its geological significance: U-Pb zircon age,<br />
element and isotopic evidence (Lithos, in review.<br />
Windley, B.F., Alexeiev, D., Xiao, W.J., Kröner, A., Badarch G., 2007. Tectonic models for<br />
accretion of the Central Asian orogenic belt. J. Geol. Soc. London, 164, 31-47.<br />
Zhao, J.M., Mooney, W.D., Zhang, X.K., Li, Z.C. Jin, Z.J., and Okaya, N., 2006, Crustal structure<br />
across the Altyn Tagh Range at the northern margin of the Tibetan plateau and tectonic<br />
implications. Earth Planet. Sci. Lett., 241, 804-814.
NEWS FEATURE NATURE|Vol 442|13 July 2006<br />
On a sunny, breezy day in the Wind<br />
River Mountains of Wyoming, a<br />
group of geologists are peering<br />
intently at a dark ridge of rock. Some<br />
2.7 billion years ago, these rocks were alive with<br />
volcanic fire. Today, they jut out of a mountainside<br />
like the spiny tail of a sleeping dragon.<br />
This rock, says Kevin Chamberlain, a geologist<br />
from the University of Wyoming in<br />
Laramie, could be a special kind — a lava<br />
called a komatiite. Today, Earth’s interior is too<br />
cool to produce this particular rock; 2.7 billion<br />
years ago, the hot lava would have run like<br />
water over the barren landscapes.<br />
But as the other geologists chip off fresh layers<br />
and scrutinize them through hand lenses,<br />
murmurs of dissent start to grow. Most geologists<br />
have never seen a komatiite; they are<br />
found almost exclusively among rocks of the<br />
Archaean era, which are more than 2.5 billion<br />
years old and thus very rare. But these men<br />
and women are experts in the truly old. And<br />
on the Wyoming hillside few of them are convinced<br />
that they are seeing the rock textures<br />
typically found in komatiites.<br />
The scene brings home the difficulties of trying<br />
to study the early Earth — there aren’t many<br />
old rocks to look at, and those that are around<br />
are often so altered, chemically and physically,<br />
as to be nearly indecipherable. But as if to recompense<br />
those who study them, such ancient<br />
rocks, particularly of Archaean age, offer geologists<br />
great rewards. It is in the Archaean that the<br />
first earthly ecosystems are found, with their<br />
clues to life’s earliest days on the planet. And it is<br />
in the Archaean that scientists can look for the<br />
beginnings of plate tectonics.<br />
Plate tectonics is the grand unified theory of<br />
geology. Everything we see today, from the<br />
abyssal plains of the oceans to the heights of<br />
the Himalayas, is shaped by plate tectonics. As<br />
far back as there has been complex life — and<br />
perhaps even before — continents have come<br />
together and moved apart in a dance that has<br />
altered climates and geographies, opening up<br />
new possibilities for life and sometimes closing<br />
down old ones.<br />
But it may not always have been so. Plate tectonics<br />
is driven by Earth’s heat and constrained<br />
by the physical and chemical properties of the<br />
crust and mantle. The further back in time you<br />
go, the more different these things are likely to<br />
have been. It’s been argued that on the early<br />
Earth, crustal plates, floating on a heat-softened<br />
layer of material beneath, would have<br />
simply been too thick and buoyant to get<br />
dragged beneath each other as they are today.<br />
And the greater temperature of the early Earth’s<br />
innards would probably have made them move<br />
128<br />
The start of the world as we know it<br />
Plate tectonics has created oceans and pushed up mountain ranges. But when did the process<br />
that shapes the planet get going? Alexandra Witze joins the geologists debating the issue.<br />
Ancient rocks, such as those in the Wind River Mountains, could help determine when plate tectonics began.<br />
in very different patterns from those typical of<br />
today’s tectonics.<br />
On other Earth-like planets there’s no evidence<br />
for today’s plate tectonics. Planets do<br />
not have to work this way, and there was probably<br />
a time when this one didn’t. “You don’t<br />
just make a silicate planet and plate tectonics<br />
starts,” says Robert Stern, a geologist at the<br />
University of Texas, Dallas. “Something special<br />
has to happen.”<br />
Dynamic planet<br />
The nature of that special something cuts to<br />
the discipline’s philosophical heart. Since the<br />
early nineteenth century, geology has been<br />
ruled by the principle of uniformitarianism —<br />
that the planet operates on unchanging laws,<br />
and that the present can be used as a key to the<br />
past. But how can that approach hold up when<br />
a science from a world where plate tectonics<br />
©2006<br />
Nature Publishing Group<br />
explains more or less everything is applied to a<br />
world that may have lacked it? How can you<br />
understand ancient rocks when you do not<br />
know what processes put them there?<br />
The geologists clustered around the possible<br />
komatiites in the Wyoming hills had gathered<br />
to discuss these questions. Their visit to<br />
the mountain ridge had been organized as<br />
part of a June conference held in Lander,<br />
Wyoming. The specific aim of the meeting<br />
was to try to fix a date for the onset of plate<br />
tectonics: the earliest possibility is pretty<br />
much straight after the planet formed, about<br />
4.5 billion years ago; the latest is just<br />
1 billion years ago.<br />
To help them decide, the scientists brought<br />
to the table data from an array of disciplines.<br />
Geochemistry can help clarify the temperature<br />
and pressure at which Archaean rocks formed.<br />
Fragments of zircon crystals dated even earlier<br />
A. WITZE
NATURE|Vol 442|13 July 2006 NEWS FEATURE<br />
— to the Hadean eon, which stretches from<br />
about 3.8 billion years ago to the planet’s birth<br />
— can provide hints about what Earth’s surface<br />
environment was like back then. Palaeomagnetic<br />
studies can show how land masses<br />
moved across latitudes. And structural geology<br />
can identify features that, in today’s world<br />
at least, seem to be indicative of plate tectonics.<br />
But in all these approaches, as with the komatiites,<br />
age makes the picture hard to discern.<br />
Crashing continents<br />
Scant and difficult-to-interpret evidence presents<br />
one set of problems; slippery definitions<br />
present another. Plate tectonics has lots of constituent<br />
parts. It’s not just a theory of how<br />
things move, but of how they are made and<br />
from what. For example, explanations for different<br />
sorts of volcanism in different settings<br />
also explain why the mineral make-up of continental<br />
crust and the crust beneath the oceans<br />
is so different.<br />
Working out which attributes are essential<br />
to the theory, and which incidental, is not easy.<br />
The 65 attendees at the Wyoming conference<br />
came up with 18 different definitions of plate<br />
tectonics. Three components, most agreed,<br />
were key: there must be rigid plates at the surface<br />
of the Earth; those plates must move apart<br />
through ocean spreading, with new crust<br />
being made where the sea floor pulls apart;<br />
and the plates must on occasion dive beneath<br />
each other at subduction zones (see graphic).<br />
The problem is that Earth could display one<br />
or even two of these properties without necessarily<br />
having a system like that described by<br />
modern plate tectonics (see ‘A world without<br />
tectonics’). Take rigid plates. Palaeomagnetic<br />
and other studies show that sections of Earth’s<br />
crust moved relative to each other in the<br />
Archaean, just as modern crustal plates do.<br />
But ice floes on a polar sea move in the same<br />
way, points out geophysicist Don Anderson of<br />
the California Institute of Technology in<br />
Pasadena — and those ice floes aren’t experiencing<br />
plate tectonics.<br />
Of the three, it seems subduction is closest<br />
to being diagnostic of plate tectonics. Subduction<br />
is the process by which one crustal plate<br />
THE DRIVING FORCES OF PLATE TECTONICS<br />
Volcano<br />
Continental<br />
plate<br />
slips beneath another, to be recycled into the<br />
mantle. Subduction requires rigid plates, and<br />
as it involves the destruction of crust, new<br />
crust must be created elsewhere, presumably<br />
at oceanic spreading ridges (see graphic); otherwise,<br />
continental crust would eventually disappear.<br />
Some argue that this means plate<br />
tectonics should date further back than the<br />
earliest firm evidence for subduction.<br />
A dramatic use of this argument is that<br />
made by Stern. In a paper published last year,<br />
he took an extreme position, proposing that<br />
Earth has been free of plate tectonics for<br />
almost four-fifths of its life, with the system we<br />
“You don’t just make a silicate<br />
planet and plate tectonics starts.<br />
Something special has to happen.”<br />
— Robert Stern<br />
see today starting up only a billion years ago 1 .<br />
He had two lines of argument. One was that<br />
plate tectonics could not begin until Earth’s<br />
crust was cool enough, and that barrier was<br />
only passed about a billion years ago. The<br />
other was that the only reliable evidence for<br />
subduction on the early planet came from a<br />
period more recent than that.<br />
Stern points to the geological record of three<br />
types of rock. Ophiolites are distinctive sections<br />
of the ocean crust that gets mashed up,<br />
often through subduction, on the edges of<br />
continents. Stern argues that very few of these<br />
rocks are more than a billion years old. Metamorphic<br />
rocks called blueschists, produced by<br />
squeezing the basalt from which oceanic crust<br />
is made at high pressures but not very high<br />
temperatures, are being made in today’s subduction<br />
zones; none, Stern says, has been<br />
found that is more than 800 million years old.<br />
And rocks from ‘ultra-high-pressure terranes’<br />
of the sort produced where one plate rides over<br />
another are at most 630 million years old.<br />
He also makes a more general point. A dramatic<br />
shift, such as the introduction of plate<br />
tectonics, must have had huge planetary consequences.<br />
And between 780 million and 580<br />
Subducting oceanic plate<br />
Oceanic<br />
spreading ridge<br />
Mantle<br />
upwelling<br />
©2006<br />
Nature Publishing Group<br />
million years ago, Stern says, there was a series<br />
of glaciations, some very extreme — giving rise<br />
to the term ‘snowball Earth’. “It was a wild time<br />
of change,” says Stern. “The biosphere was out<br />
of control.” On the basis that dramatic effects<br />
require dramatic causes, he argues that the<br />
introduction of plate tectonics, and with it an<br />
increase in planet-cooling volcanic eruptions,<br />
might have precipitated the great glaciations.<br />
An age gone by<br />
After reading Stern’s arguments, Alfred<br />
Kröner of the University of Mainz in Germany<br />
fired off a rebuttal. He argues that there’s<br />
plenty of evidence for plate tectonics stretching<br />
back at least 3.1 billion years 2 — including<br />
geochemical work, seismic images of the<br />
‘sutures’ where colliding continents join and,<br />
indeed, a few ancient ophiolites. “I believe we<br />
can see these features all the way back” — possibly<br />
all through the Archaean, says Kröner.<br />
The exchange of papers led to the Wyoming<br />
conference. “It was overdue,” says Kröner.<br />
“Nobody ever talks to one another.” In<br />
Wyoming, they did: palaeomagnetists clustered<br />
around a white board with field geologists;<br />
geophysicists sat down for a beer<br />
with geochemists.<br />
Some of the newly shared data favour an<br />
early start for plate tectonics. Geoff Davies, a<br />
modeller at Australian National University in<br />
Canberra, presented work suggesting that one<br />
of the biggest stumbling blocks to an early start<br />
may have been removed. In the early 1990s,<br />
computer models created by Davies and others<br />
suggested that the crust on the early Earth<br />
would have been too thick and buoyant to get<br />
dragged down beneath another plate during<br />
subduction. But new simulations, using more<br />
sophisticated calculations, suggest that the<br />
crust may have been thinner than once<br />
thought 3 — as thin as 4 kilometres or less —<br />
which would be thinner than today’s crust.<br />
“Maybe plate tectonics on the early Earth was<br />
viable after all,” says Davies.<br />
In other cases, recent findings overturned<br />
evidence for early plate tectonics. In 2001, a<br />
team reported that an ophiolite from Dongwanzi,<br />
China, was 2.5 billion years old — mak-<br />
Passive continental<br />
margin (no subduction)<br />
129
NEWS FEATURE NATURE|Vol 442|13 July 2006<br />
Clues to the past: zircon crystals (inset) in the Jack Hills of Western Australia have been used to argue for an early start to plate tectonics.<br />
ing it by far the oldest such subduction remnant<br />
yet discovered 4 . Now Guochun Zhao, of<br />
the University of Hong Kong, has re-dated<br />
those rocks, giving them an age of just 300 million<br />
years.<br />
Timothy Kusky of St Louis University in<br />
Missouri, who led the original study, says that<br />
Zhao took samples from a part of the rock<br />
already known to be much younger than the<br />
main part of the ophiolite. But several attendees<br />
at the meeting said they found Zhao’s data<br />
convincing. If true, it would pull the earliest<br />
evidence for ophiolites at least half a billion<br />
years towards the present, leaving the<br />
Archaean an ophiolite-free zone.<br />
The Chinese ophiolite isn’t the only evi-<br />
130<br />
dence that is getting fresh scrutiny. For a while<br />
two independent groups have been quietly<br />
warring over the significance of a pile of<br />
ancient zircons from the Jack Hills region of<br />
Western Australia. The zircons are crystals<br />
that formed in the Hadean and later became<br />
incorporated into younger rocks.<br />
Last year in Science 5 , geochemist Mark Harrison<br />
of the University of California, Los Angeles,<br />
and colleagues used the Jack Hills zircons to<br />
argue that continental crust was present 4.4 billion<br />
to 4.5 billion years ago. The evidence<br />
comes in the form of hafnium isotope ratios in<br />
the zircon crystals, which preserve signals of<br />
the lighter minerals typical of continental crust.<br />
The data also suggest, Harrison argues, that<br />
Time to talk: Earth scientists gathered at a meeting in Wyoming to present diverse data on the early Earth.<br />
©2006<br />
Nature Publishing Group<br />
that crust was being recycled down into the<br />
mantle by 4.4 billion years ago — perhaps<br />
though a process similar to plate tectonics.<br />
Simon Wilde of the Curtin University of<br />
Technology in Perth, Australia, isn’t so sure.<br />
“You have to be very careful with these rocks,”<br />
he says. Measuring one spot on a crystal, as<br />
opposed to another, can yield very different<br />
hafnium values that lead to very different interpretations,<br />
he says. Wilde argues that the zircons<br />
should be interpreted more conservatively<br />
— that the evidence points to there being some<br />
continental crust, but not plate tectonics and its<br />
associated recycling, by 4.4 billion years ago 6 .<br />
Ground forces<br />
Such differences of interpretation make the<br />
problem of solving when plate tectonics began<br />
extremely difficult. In many cases, data can be<br />
interpreted in several completely different<br />
ways — all of which may seem valid.<br />
For instance, another Australian geologist<br />
presented seemingly convincing evidence that<br />
plate tectonics had begun by 3.3 billion years<br />
ago in Western Australia, based on the very<br />
different histories of two sections of an ancient<br />
rock formation called the Pilbara. Hugh<br />
Smithies of the Geological Survey of Western<br />
Australia says that the eastern part of the Pilbara,<br />
between 3.5 billion and 3.2 billion years<br />
old, “shows no clear evidence for modern-style<br />
plate tectonics”. It contains some geochemical<br />
markers that suggest subduction, but they<br />
could just as easily be explained by hot<br />
upwellings of rock known as mantle plumes or<br />
other non-tectonic phenomena.<br />
In contrast, looking at the western part of the<br />
Pilbara — which is 3.3 billion to 3.0 billion years<br />
old — Smithies sees plenty of evidence for plate<br />
tectonics. There are geochemical signatures that<br />
cannot be explained by other factors, and the<br />
M. HARRISON<br />
A. J. VAN DER VELDEN
NATURE|Vol 442|13 July 2006 NEWS FEATURE<br />
Slow work: geologists hunt for structural signatures in rocks that can only be explained by plate tectonics, to try to identify when the process started.<br />
rocks show features that hint that plates had<br />
interacted along their edges. Smithies thinks the<br />
western Pilbara contains the remains of an<br />
oceanic arc — the sort of line of islands, such as<br />
the Aleutians of Alaska, that are characteristic<br />
of some oceanic subduction zones 7 .<br />
But then along came Julian Pearce of Cardiff<br />
University in Wales, who argued that each of<br />
the geochemical markers in the western Pilbara<br />
can be explained by other phenomena,<br />
A WORLD WITHOUT<br />
TECTONICS<br />
With so much uncertainty over Earth’s early<br />
history, not many geologists are willing to<br />
imagine entirely different ways in which the<br />
world might have worked before plate<br />
tectonics. One of the brave few is Jean<br />
Bédard, a geologist at the Geological Survey<br />
of Canada.<br />
At a June conference held in Lander,<br />
Wyoming, Bédard presented one of the few<br />
fully worked out accounts of how a pre-platetectonic<br />
Earth might have worked. In his<br />
model, hot upwellings of rock known as<br />
mantle plumes partly melt the crust above<br />
them. This melting distills the crust, producing<br />
material from which light, continental-style<br />
crust is made.<br />
The material left behind as the melt is<br />
creamed off — denser than it was before the<br />
distillation — then detaches itself from the<br />
crust and sinks back into the mantle. There, it<br />
would mix with more mantle material — and<br />
the whole process would start all over again 9 .<br />
Bédard himself admits that he has no idea if<br />
his proposal is right. But it is, he says, a<br />
detailed alternative theory to plate<br />
tectonics, and one that can be tested<br />
with further studies. A.W.<br />
such as magmas with an unusual amount of<br />
water in them, or crustal material from different<br />
places getting mixed up. The various<br />
researchers are hoping to settle the matter with<br />
a field trip. An excursion is already planned for<br />
next year, to re-examine the evidence for plate<br />
tectonics in the western Pilbara.<br />
Field trips don’t always resolve things. In the<br />
Wind River Mountains, the meeting attendees<br />
continued to argue about plate tectonics as<br />
they hiked from outcrop to outcrop. But a<br />
week of communing at the conference and<br />
under the high mountain sun brought them<br />
toward a consensus of sorts.<br />
Meeting organizers polled the attendees<br />
twice on when they thought plate tectonics<br />
began. At the beginning of the meeting, guesses<br />
were spread over more than 3 billion years of<br />
Earth history. At the end, a closing ballot<br />
showed that many had begun to push their<br />
thinking further back into the past; a majority<br />
of attendees voted for plate tectonics having<br />
started between 3 billion and 4 billion years ago.<br />
Kent Condie, one of the meeting organizers,<br />
calls that a success. “We’ve got a majority<br />
favouring a definition and approach,” says<br />
Condie, of the New Mexico Institute of Mining<br />
and Technology in Socorro, New Mexico.<br />
“Sure, there will be a minority point of view.”<br />
At the conference, that minority pretty<br />
much constituted Stern. By the end of the<br />
meeting, he remained the one person voting<br />
for a start to plate tectonics at 1 billion years<br />
ago. “It’s not a simple question,” he maintains.<br />
And on that, at least, others agree.<br />
Michael Brown, a geologist at the university<br />
of Maryland in College Park, doesn’t endorse<br />
Stern’s late start. But he does think that the<br />
nature of plate tectonics changed around that<br />
time. In a paper in press in Geology 8 , Brown<br />
suggests that there have been two styles of<br />
©2006<br />
Nature Publishing Group<br />
plate tectonics: the modern kind that we see<br />
today, and an earlier version that lasted from<br />
about 2.7 billion to 700 million years ago. Evidence<br />
for the earlier style, he says, comes from<br />
minerals that are typical of higher-temperature,<br />
lower-pressure environments; these suggest<br />
a hotter Earth where plates did not<br />
subduct beneath each other to great depths<br />
and pressures. Minerals characteristic of highpressure<br />
environments typify the later style.<br />
The properties of these minerals suggest to<br />
him that true plate tectonics, in which one<br />
plate subducts deeply beneath another, did not<br />
begin until about 700 million years ago.<br />
And there is a possible further complication.<br />
Geophysicist Paul Silver, of the Carnegie<br />
Institution of Washington, raised the notion<br />
that plate tectonics may have started and<br />
stopped several times during Earth’s history.<br />
This is also an idea that Stern is comfortable<br />
with — he uses it to explain the presence of a<br />
small number of ophiolites about 2 billion<br />
years ago.<br />
An ‘intermittent approach’ would be a wonderful<br />
way to reconcile things — but it takes<br />
geology even further from the comforting<br />
realm of uniformitarianism, into a world<br />
where the most basic principles come and go<br />
in fits and starts. ■<br />
Alexandra Witze is Nature’s chief of<br />
correspondents for America.<br />
1. Stern, R. J. Geology 33, 557–560 (2005).<br />
2. Cawood, P. A., Kröner A., Pisarevsky, S. GSA Today 16, 4–11<br />
(2006).<br />
3. Davies, G. F. Earth Planet. Sci. Lett. 243, 376–382 (2006).<br />
4. Kusky, T. M., Li, J-H. & Tucker, R. D. Science 292, 1142–1145<br />
(2001).<br />
5. Harrison, T. M. et al. Science 310, 1947–1950 (2005).<br />
6. Valley, J. W. et al Science 312, 1139a (2006).<br />
7. Smithies, R. H. et al. Gondwana Res. (in the press).<br />
8. Brown, M. Geology (in the press).<br />
9. Bédard, J. Geochim. Cosmochim. Acta 70, 1188–1214<br />
(2006).<br />
131<br />
A. POLAT
ERAS Report for 2006 - Annexure 2<br />
Solid Earth (SE) Super-session on<br />
AOGS-2006 (July 10-14, Singapore)<br />
"Composition and Evolution of the Asian Lithosphere"<br />
Bor-ming Jahn (Taipei) and Alfred Kröner (Mainz)<br />
Prof. Bor-ming Jahn,<br />
Institute of Earth Sciences, Academia Sinica<br />
P.O. Box 1-55, Nankang<br />
Taipei, 11529 Taiwan<br />
e-mail: jahn@earth.sinica.edu.tw<br />
Prof. Alfred Kröner<br />
Institut fuer Geowissenschaften, Universität Mainz<br />
55099 Mainz, Germany<br />
e-mail: kroener@mail.uni-mainz.de<br />
Component sessions and their descriptions:<br />
1. Evolution of the Asian continental mantle lithosphere - constraints from xenolith<br />
studies (Bill Griffin, Sue O'Reilly, and Kuo-Lung Wang)<br />
The continents are underlain by roots of sub-continental lithospheric mantle (SCLM), which<br />
vary in thickness, composition and thermal state depending on the age and tectonothermal<br />
history of the overlying crust and its tectonic setting. Understanding the evolution of the<br />
SCLM, and its causes, is essential to understanding the growth and stability of continents and<br />
long-term mantle processes. Recent studies document a change from thick, cool and depleted<br />
Archaean SCLM to thin, hot and fertile SCLM in eastern China. What mechanisms can cause<br />
thinning and replacement of ancient SCLM, which is gravitationally stable? How does new<br />
lithosphere form?<br />
Professor Suzanne Y. O'Reilly<br />
GEMOC Key Centre, Department of Earth and Planetary Sciences<br />
Macquarie University<br />
Sydney NSW 2109, Australia<br />
E-mail: soreilly@els.mq.edu.au<br />
Professor William L. Griffin<br />
GEMOC Key Centre, Department of Earth and Planetary Sciences<br />
Macquarie University<br />
Sydney NSW 2109. Australia<br />
E-mail: wgriffin@els.mq.edu.au<br />
Dr. Kuo-Lung Wang<br />
Institute of Earth Sciences, Academia Sinica<br />
128, Sec. 2 Academia Road<br />
Nankang, Taipei 115<br />
Taiwan, R.O.C.<br />
E-mail: kwang@earth.sinica.edu.tw
2. Lithospheric and mantle dynamics (David Yuen and Huai Zhang)<br />
This session will focus on fundamental issues of heat and mass transfer in the Earth's mantle<br />
and its nonlinear interaction with the crust and lithosphere. We welcome contributions from<br />
many vantage points, especially from multiscale points of view, towards this goal. Topics<br />
ranging from both laboratory experiments to numerical simulations are appropriate.<br />
Constraints from other geochemical and geophysical observations, in particular seismology<br />
and mineral physics, are particularly welcome. We encourage contributions from younger<br />
scientists.<br />
Prof. David A. Yuen<br />
Dept. of Geology and Geophysics and Minnesota Supercomputer Institute,<br />
University of Minnesota,<br />
Minneapolis, MN 55455-0219, USA<br />
e-mail: davey@krissy.geo.wmn.edu<br />
Prof. Huai Zhang,<br />
Laboratory of Computational Geodynamics,<br />
Chinese Academy of Sciences, Beijing, China<br />
e-mail: hzhang@gweas.ac.cn<br />
2<br />
3. Growth and evolution of the Asian continent (M. Zhai, S. Wilde, G. Zhao, M. Cho)<br />
Asia is evolving into the next supercontinent, composed of diverse terranes; each with its own<br />
unique story. Outstanding issues include the nature and distribution of the earliest crustal<br />
components; the relative roles of mantle plumes versus subduction-related processes in the<br />
Archean; the nature and timing of anorogenic magmatic and rifting events in the Proterozoic;<br />
the evidence for, and timing of, continental collisions; crustal growth during the Phanerozoic;<br />
evaluating geological correlations between various crustal components; and detailing the<br />
consequences of mantle processes as they impinge on the evolving crust. We welcome<br />
contributions on these and other related issues.<br />
Mingguo Zhai,<br />
Institute of Geology & Geophysics,<br />
Chinese Academy of Sciences, PO Box 9825,<br />
Beijing 100029, China<br />
e-mail: mgzhai@mail.igcas.ac.cn<br />
Simon Wilde,<br />
Department of Applied Geology,<br />
Curtin University of Technology, PO Box U1987,<br />
Perth, 6845, Western Australia<br />
e-mail: wildes@lithos.curtin.edu.au<br />
Guochun Zhao,<br />
Department of Earth Sciences,<br />
The University of Hong Kong,<br />
Pokfulam Road, Hong Kong<br />
e-mail: gzhao@hkucc.hku.hk<br />
Moonsup Cho,<br />
School of Earth & Environmental Sciences,<br />
Seoul National University,<br />
Seoul, 151-747, South Korea
e-mail: moonsup@snu.ac.kr<br />
3<br />
4. Orogenic processes in Asia: regimes of continental collision (S.L. Chung, Mike Searle)<br />
Collision between two continental plates would induce uplift of the crust and hence making<br />
mountains of high elevation. However, due to the diverse lithologies and heterogeneous stress<br />
fields, the resulting uplift cannot be identical in different parts of a collisional orogen. This<br />
has been well demonstrated for the Tibetan plateau. The Himalayan-Tibetan orogen is the<br />
most outstanding natural laboratory for studying the collisional orogeny and the influence of<br />
its uplifted topography on the ocean water chemistry and climatic changes on Earth.<br />
Continental collision also leads to subduction of apparently unsubductible continental crust.<br />
This has tremendous implications for crustal recycling and for our understanding of<br />
metamorphic processes in ultrahigh pressure conditions.<br />
Prof. Sun-Lin Chung<br />
Dept of Geological Sciences<br />
National Taiwan University,<br />
Taipei, Taiwan<br />
e-mail: sunlin@ntu.edu.tw<br />
Dr. M.P.Searle<br />
Dept. Earth Sciences, Oxford University,<br />
Parks Road., Oxford, OX1 3PR, UK<br />
e-mail: Mike.Searle@earth.ox.ac.uk<br />
5. Orogenic processes in Asia: regimes of continental accretion (Alfred Kröner)<br />
Orogenic collages of Asia consist mostly of subduction-accretion complexes. They provide<br />
an excellent possibility to reconstruct regimes of accretion in the Phanerozoic history of the<br />
Earth and their role in the formation of the continental crust. The Pacific side of Asia where<br />
modern rock and structural assemblages of almost all possible varieties reveal gradual<br />
transitions to the assemblages of the geological past is the best laboratory for deciphering of<br />
the regimes of accretion. Their examination and comparison with the assemblages of Inner<br />
Asia may stop a simplistic approach, in which a search for explanations of inconsistency in<br />
stratigraphic, magmatic, and structural history is substituted by recognition of mute terranes.<br />
Prof. Alfred Kröner<br />
Dept. of Geosciences, University of Mainz<br />
55099 Mainz, Germany<br />
e-mail: kroener@mail.uni-mainz.de<br />
6. Generation of granitoids in Asia and Australia (W. Collins, T. Nakajima, Fuyuan Wu)<br />
In contrast to the eastern pacific rim (North and South America), where granites generally<br />
formed in narrow ((
e-mail: bill.collins@townsville.edu.au<br />
Dr. Takashi Nakajima<br />
Geological Survey of Japan<br />
Institute of Geology and Geoinformation<br />
AIST Central-7, 1-1-1 Higashi, Tsukuba 305-8567, Japan<br />
e-mail. tngeoch.nakajima@aist.go.jp<br />
Dr. Fuyuan WU<br />
Institute of Geology and Geophysics<br />
Chinese Academy of Sciences<br />
P.O. Box 9825, Beijing 100029, China<br />
e-mail: wufuyuan@mail.igcas.ac.cn<br />
4<br />
7. Deep Structure and Tectonics of the Asian Lithosphere: The Geophysical Perspective<br />
(Larry Brown, Dapeng Zhao, Bor-Shouh Huang, Wangping Chen)<br />
A new generation of active and passive geophysical imaging experiments are revealing key<br />
details about the deep structure of the Asian lithosphere. These observations represent critical<br />
tests for tectonic speculations on the role of such fundamental issues as deep crustal flow,<br />
extensional exhumation, igneous underplating, mantle delamination, palaeoplate reconstruction<br />
and lithospheric plate recycling. This session will review recent geophysical surveys of the Asian<br />
lithosphere, with a focus on regional multi-disciplinary transects across key terranes.<br />
Prof. Larry D. Brown,<br />
Institute of the Study of Continents,<br />
Cornell University, Ithaca, NY, USA<br />
e-mail: brown@geology.cornell.edu<br />
Prof. Dapeng Zhao<br />
Geodynamics Research Center<br />
Ehime University<br />
Matsuyama 790-8577, Japan<br />
e-mail: zhao@sci.ehime-u.ac.jp<br />
Dr. Bor-Shouh Huang<br />
Institute of Earth Sciences<br />
Academia Sinica<br />
Taipei, Taiwan 11529<br />
e-mail: hwbs@earth.sinica.edu.tw<br />
Prof. Wangping Chen<br />
University of Illinois<br />
Department of Geology<br />
Urbana-Champagne, IL, USA<br />
e-mail: wpchen@uiuc.edu<br />
8. Evolution of the SW Pacific and South China Sea (S.K. Hsu, R. Shinjo, T.Y. Lee)<br />
The SW Pacific and South China Sea region is characterized by the presence of trench-arcback-arc<br />
systems. During recent years, new observations and insights about the SW Pacific<br />
and South China Sea have been accumulated. However, the formation and evolution of this<br />
region is still under debate. To understand the complex system and evolution of the SW<br />
Pacific and South China Sea, integration of works including onshore and offshore geological,
5<br />
geophysical and geochemical investigations is required. This session will serve as a venue for<br />
reexamining the evolutionary history of the SW Pacific and South China Sea and, hopefully,<br />
leads to new discussions for the plate interactions and marginal basins formation.<br />
Prof. Shu-Kun Hsu<br />
Institute of Geophysics, National Central University,<br />
Chung-Li 32001, Taiwan<br />
Email: hsu@oc.gep.ncu.edu.tw<br />
Prof. Ryuichi Shinjo<br />
Department of Physics and Earth Sciences, University of the Ryukyus<br />
Senbaru-1, Nishihara,<br />
Okinawa 903-0213, Japan<br />
E-mail: rshinjo@sci.u-ryukyu.ac.jp<br />
Prof. Tung-Yi Lee<br />
Department of Earth Sciences, National Taiwan Normal University,<br />
88, Sec. 4, Tingjou Rd., Wenshan Chiu,<br />
Taipei,Taiwan<br />
E-mail: t44001@cc.ntnu.edu.tw<br />
9. Crustal deformation and neotectonics in Asia (Yue-Gau Chen, Jian-Cheng Lee, Kerry<br />
Sieh, Yuichi Sugiyama)<br />
Asia is undergoing various styles of crustal deformation in response to diverse tectonic<br />
settings. Regardless of their distribution, inter- or intra-plate and coseismic or interseismic,<br />
scientists have long been studying the processes of deformation. Recently, the earthquake<br />
related neotectonics draw much attention due to the disasters occurred in the past decade. In<br />
order to explore the mechanism and behavior of the active crustal deformation, a great<br />
number of scientific projects have been launched for such purposes using either traditional<br />
investigation or novel remote sensing methods. Based on the published materials, it is<br />
obvious that some results are consistent and sensible, but others are still in debate. This<br />
session is aimed to discuss a variety of problems related to neotectonics, paleoseismology,<br />
tectonic geomorphology, seismology, and geodesy of Asia.<br />
Prof. Yue-Gao Chen<br />
Dept of Geological Sciences, National Taiwan University,<br />
Taipei, Taiwan<br />
e-mail: ygchen@ntu.edu.tw<br />
Dr. Jian-Cheng Lee<br />
Institute of Earth Sciences, Academia Sinica<br />
Taipei, Taiwan 11529<br />
e-mail: jclee@earth.sinica.edu.tw<br />
Prof. Kerry Sieh<br />
California Institute of Technology, Seismological Lab,<br />
MS 252-21, Pasadena, CA 91125, USA<br />
e-mail: sieh@gps.caltech.edu<br />
Dr. Yuichi Sugiyama<br />
e-mail: sugiyama-y@aist.go.jp
10. Ore deposits and economic geology in Asia (Shunso ISHIHARA, Jingwen MAO)<br />
Recent fast economic growth in the Asian countries have yielded a strong demand on mineral<br />
resources, particularly Cu, Mo, W, In, Fe, Mn, PGE, Au, potash salt, etc., which are indispensable<br />
for keeping modern technological societies active in those countries. The economic<br />
geologists in that region have been encouraged to study on metallogenic models and their<br />
corresponding geodynamic and historic processes as well as new prospecting methods, and<br />
apply the results to actual mineral exploration. AOGS-2006 will provide an opportunity for<br />
academic and industrial colleagues to exchange what you have done and what you will do.<br />
Please bring your up-to-date research results to this conference. You are cordially invited to<br />
this session.<br />
Dr. Shunso ISHIHARA<br />
Geological Survey of Japan,<br />
AIST Tsukuba Central 7, Tsukuba, 305-8567, Japan<br />
e-mail: s-ishihara@aist.go.jp<br />
Dr. Jingwen Mao<br />
Institute of Mineral Resources,<br />
CAGS, Beijing 100037, China<br />
e-mail: jingwenmao@263.net<br />
6<br />
11. Gem materials - from diamond to pearls (W. Hofmeister, Vu Xuan Quang)<br />
Prominent deposits of gem materials of highest economic values are situated in Asia and<br />
Australia. Diamonds from Australia, ruby from Thailand, Vietnam, and Myanmar, zircon and<br />
sapphire from Sri Lanka, tourmaline and topaz from the Himalayan neighborhood, are highend<br />
geo-materials. There is an increasing demand of them worldwide. Study of gem materials<br />
is also essential for understanding of archaeological artifacts. Besides, bio-mineralogy is an<br />
exciting new field of research. Pearl and ivory production is important in the Asian-<br />
Australian region. We invite interested scientists to discuss the geology, market and nondestructive<br />
analytical methods for gem materials, and advance of research on the connection<br />
of inorganic and organic worlds.<br />
Prof. Wolfgang Hofmeister<br />
Institute of Geosciences<br />
Johannes Gutenberg-University<br />
D-55099 Mainz, Germany<br />
e-mail: hofmeister@uni-mainz.de<br />
Prof. Vu Xuan Quang,<br />
Institute of Materials Science,<br />
Vietnam Academy of Science and Technology,<br />
Hanoi, Vietnam<br />
e-mail: Quangvx@hn.vnn.vn
ERAS Report for 2006 - Annexure 2<br />
ERAS<br />
<strong>International</strong> Workshop on<br />
Accretionary Orogens and Continental Growth<br />
from the perspective of global mass circulation<br />
(Circular – 3 July 2006)<br />
Time: Sept 19 to 22, 2006<br />
Place: Kochi Univ. Convention Center, Kochi (conference<br />
meeting) and central Shikoku and Inuyama (field excursion)<br />
Conveners :<br />
Kimura Gaku, Dept. Earth and Planet. Sci. The Univeristy of Tokyo<br />
Isozaki Yukio, Dept. Integrated Science, The University of Tokyo<br />
Santosh M. Dept. Environmental Science, Kochi University<br />
Sponsor: JSPS (Japan Society of Promoting Sciences)<br />
Initiation and Aims of the workshop:<br />
(A) Accretionary orogens are major sites of continental growth and important miner-<br />
alization. They have been active throughout Earth history, and the modern<br />
circum-Pacific orogenic belts are the most typical of them. This workshop is<br />
aimed to discuss the processes for the initiation and development of accretionary<br />
orogens, and to better understand the processes responsible for the global mass<br />
circulation, cratonization and incorporation of accretionary orogens into<br />
continental nuclei.<br />
(B) The Japanese islands represent an excellent example of Phanerozoic accretionary<br />
orogeny and continental growth. The proposed field excursion will allow the<br />
participants to examine the geological evolution of East Asia.<br />
(C) An international project “ERAS (EaRth Accretionary Systems in space and<br />
time)” has been submitted to the <strong>International</strong> Lithosphere Program (ILP) for<br />
approval. The ILP is an important program of the IUGS and IUGG (<strong>International</strong><br />
Unions of Geological Sciences and Geophysical Sciences of ISU). This workshop<br />
will have an important publicity campaign for the project itself as well as for the
2<br />
promotion of scientific activity of Japan.<br />
(D) All invited speakers are heavy-weights in this research domain. Their<br />
participation and the timing of the workshop (to be held in the same place and the<br />
same time as the annual meeting of the Geological Society of Japan )will<br />
certainly attract a large group of audience.<br />
(E) We anticipate about 100 attendants at this meeting (but not the field excursion,<br />
which is limited to about 30 participants). Besides the local participants, the<br />
invited attendants come from Australia, UK, France, Germany, Canada, Korea.<br />
We expect that our young researchers will greatly benefit from the highly<br />
animated discussions provided by the international leading experts during the<br />
meeting. We will also give ample opportunity for our young scientists to<br />
exchange their ideas about on-going or pertinent research with the experts.<br />
Status of the workshop preparation (as of 3 July 2006):<br />
(A) The workshop comprises two parts: a one-and-a-half-day conference in the<br />
University Conference Center at Kochi, followed by a 2-day field excursion in<br />
central Shikoku and Inuyama area, central main island.<br />
(B) A full-day conference (May 19) will be allocated to invited talks on the type<br />
localities of world’s accretionary orogens. Different approaches (field-based,<br />
structural, geochemical, isotopic, geophysical, etc.) will be presented to address<br />
the orogenic processes and crustal growth. Differences between accretionary and<br />
collisional orogens will be underlined.<br />
(C) A half-day conference (May 20 morning) will be used to present the current<br />
models and interpretations on the geological evolution of the Mesozoic East Asia,<br />
as well as a brief introduction on the geology of the Japanese islands. This<br />
should form a good preparatory overview for the following 2-day field<br />
excursion.<br />
Provisional schedule (Sept. 18 to 22, 2006)<br />
Sept. 18 Monday – arrival of participants. All participants will be transported and<br />
lodged in the Hotel. Registration of the participants, Ice breaker<br />
Sept. 19 Tuesday – first day of the workshop<br />
9h00 to 12h00 – morning talks on accretionary orogens<br />
12h00 to 1300 – lunch<br />
13h00 to 16h30 –afternoon talks on accretionary orogens<br />
16h30 to 17h00-brief introduction of field excursion
Reception party of Japanese style cuisine.<br />
Sept. 20 Wednesday – second day of the workshop.<br />
3<br />
Morning – Visit Yokonami peninsula to observe the Cretaceous Shimanto<br />
accretionary complex, then travel to the Oboke gorge<br />
Afternoon - Observe Cretaceous high-P/T Sanbagawa metamorphic rocks.<br />
Stay in Hotel<br />
Sept. 21 Thursday – third day of the workshop<br />
Morning – visit ultramafic rocks in the high-P/T unit, and return to Kochi<br />
airport.<br />
Afternoon – take a flight from Kochi to Komaki (north of Nagoya, central main<br />
island) and stay in the Inuyama <strong>International</strong> Youth Hostel with a good hot spa.<br />
Sept. 22 Friday – fourth day of the workshop<br />
Morning + early afternoon - observe the Jurassic accretionary complex of the<br />
Mino-Tanba belt. End of the workshop<br />
To Nagoya, Osaka, or Tokyo airport.<br />
(To Tokyo ca. 3 hours; to Osaka 2 hours)<br />
Please check Visa matter for participants with your travel agencies.<br />
Y-class international travel into and out from Japan, domestic<br />
transportation and accommodation (from 18 to 21: four nights and<br />
foods) fees for the workshop invitees are covered by the workshop.<br />
Accommodations for earlier arrival and later departure beyond the<br />
workshops are not covered by the workshop.<br />
Please contact with gaku@eps.s.u-tokyo.ac.jp for paper works of<br />
payment documents of invitees and any questions.<br />
List of invited speakers from foreign countries (Tentative):<br />
Borming Jahn – Taiwan National University, Taiwan<br />
Kröner, Alfred – professor, University of Mainz, Germany<br />
Windley, Brian F. – professor, University of Leicester, United Kingdom<br />
Cawood, Peter – professor, The University of Western Australia, Australia<br />
Laurent Jolivert – professor, University Pierre et Marie Curie, France<br />
Peter Clift – professor, University of Aberdeen, UK<br />
Hugh Smithies – Geological Survey of W. Australia<br />
John A. Pericival – Geological Survey of Canada, Ottawa<br />
Moonsap Cho – Seoul National University
List of domestic speakers (Tentative):<br />
4<br />
Tatsumi, Yoshiyuki – professor, Japan Marine Science and Technology Center, Japan<br />
Maruyama, Shigenori – professor, Tokyo Institute of Technology, Japan<br />
Tsuyoshi Komiya – assistant professor, TIT, Japan<br />
Dapeng Zhao – professor, Ehime University, Matusyama, Japan<br />
Hikaru Iwamori – associate professor, University of Tokyo, Japan<br />
Isozaki, Yukio – professor, University of Tokyo, Japan<br />
Kimura, Gaku – professor, University of Tokyo, Japan<br />
Field excursion leaders: Masaru Terabayashi, Kagawa University<br />
Yoshitaka Hashimoto, Kochi University
ERAS Report for 2006 – Annexure 4<br />
Sino-German Workshop on “Geodynamic Evolution of Central Asia in the Palaeozoic<br />
and Mesozoic”, Beijing, China, December 4-8, 2006<br />
The Sino-German Centre for Research Promotion (Chinesisch-Deutsches Zentrum für<br />
Wissenschaftsförderung), in Beijing, China, funded a 5-day thematic workshop on<br />
“Geodynamic Evolution of Central Asia in the Palaeozoic and Mesozoic” which was attended<br />
by more than 50 participants representing eight countries (Germany, UK, France, Russia,<br />
Australia, Italy, Cuba, and China). The workshop was co-sponsored jointly by Task Force I<br />
(Earth Accretionary Systems) of the <strong>International</strong> Lithosphere Program (ILP), IGCP Project<br />
480, and the State Key Laboratory of Lithospheric Evolution, Institute of Geology and<br />
Geophysics, Chinese Academy of Sciences (CAS). It was superbly organized by a term from<br />
the State Key Laboratory of Lithospheric Evolution, and Prof. Wenjiao Xiao, Head of this<br />
Laboratory, and Prof. Alfred Kröner of Mainz University, Germany, were the executive chairs<br />
of the workshop.<br />
The meeting was conducted in the Conference Hall of the Sino-German Center for<br />
Research Promotion with 4 days of oral presentations, followed by visits of the international<br />
guests to laboratories of the CAS, the Chinese Academy of Geological Sciences (CAGS), and<br />
China University of Geosciences.<br />
During the conference, 44 presentations were given orally, listed in an abstract volume,<br />
each followed by a long and heated discussion. The oral presentations were subdivided into<br />
two major sessions: (1) Evolution of the Qinling-Kunlun, Dabie-Sulu and Pamir Ranges; and<br />
(2) Evolution of the Central Asian Orogenic Belt. There were 15 talks in the first session and<br />
29 in the second session. These sessions covered a variety of topics ranging from the formation<br />
of the Chinese continent to specific mountain belts in Eastern and Central Asia, and emphasis<br />
was on tectonics, metamorphic petrology, geochemistry and geochronology. In the final part of<br />
the meeting, scientists from CAS, CAGS, China and Germany gave presentations of new<br />
research initiatives arising from the workshop and discussion, e.g. a proposed<br />
seismic-geologic traverse across the CAOB. There were also round-table discussions in small<br />
working groups on future research projects.<br />
Overall the workshop was of highly successful, and social events included an icebreaker<br />
welcoming party and splendid and opulent dinner parties in a well-known Chinese restaurant.<br />
All participants appreciated the scientific merit of the workshop and the chance to meet new<br />
colleagues and research partners. The foreign participants were particularly impressed by the<br />
high quality of analytical data presented by the Chinese researchers, and everybody agreed that<br />
the geology of Central and Eastern Asia plays a unique role in understanding processes of crust<br />
formation and continental evolution, since the area contains the largest Neoproterozoic to<br />
Mesozoic accretionary terrains on our planet. The participation of Reinhard Rutz, Director of<br />
Sino-German Center for Research Promotion, Zhenyu Yang, editor-in-chief of Episodes,<br />
Mingguo Zhai, Deputy Director of the Institute of Geology and Geophysics (CAS), and
2<br />
Qingchen Wang, Steering Committee of the <strong>International</strong> Lithospheric Program (ILP)<br />
enlightened the discussions and stimulated further cooperation between individual scientists<br />
and groups from various countries. All participants are looking forward to future collaboration,<br />
and individual research projects are now in the process of being formulated.<br />
We thank the Sino-German Centre for generous funding and hope that this workshop will<br />
result in new research initiatives and new friendships.<br />
Wenjiao Xiao<br />
State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese<br />
Academy of Sciences, China.<br />
E-mail: wj-xiao@mail.igcas.ac.cn<br />
Alfred Kröner<br />
Institut für Geowissenschaften, Universität Mainz, Becherweg 21, 55099 Mainz, Germany<br />
E-mail: kroener@mail.uni-mainz.der
ERAS Report for 2006 – Annexure 4<br />
Proposal for a seismic/geological traverse across the Central Asian Orogenic<br />
Belt from the Siberian craton to the North China craton<br />
Compiled by L. Brown, W.L. Griffin, B.-M. Jahn, A. Kröner, B.F. Windley, and W. Xiao<br />
The Central Asian Orogenic Belt (CAOB, Fig. 1) is one of the largest and least understood<br />
orogenic systems on Earth. It constitutes an orogenic collage of island arcs, microcontinents,<br />
accretionary wedges and ophiolitic mélange zones that evolved over a period of more than 700<br />
million years (Ma) from about 1000 to ~250 Ma (Kröner et al., 2006; Windley et al., 2006). The<br />
belt is considered to represent a major site of continental growth in the Neoproterozoic and<br />
Palaeozoic (Sengör et al., 1993; Jahn, 2004) and contains important world-class metal deposits, two<br />
of which have recently been discovered in southern Mongolia (Perello et al., 2001). The evolution<br />
of this extremely large and long-lived accretionary orogen has been the subject of considerable<br />
controversy for more than a decade since Sengör et al. (1993) proposed an innovative but highly<br />
speculative model, deriving the entire orogen from one single, giant intra-oceanic island arc from<br />
the early Cambrian (~540 Ma) Ma to the Permian (~260 Ma). The alternative, and more widely<br />
accepted, interpretation explains the CAOB in terms of southwest Pacific-style accretion of arcs and<br />
microcontinents and final collision between the Siberian and North China cratons (e.g. Ruzhentsev<br />
and Mossakovskiy, 1996; Badarch et al., 2002; Dobretsov et al., 2003; Xiao et al., 2003, Kröner et<br />
al., 2006; Windley et al, 2006, and references cited in all of the above).
2<br />
Fig. 1. Central Asian Orogenic Belt (CAOB) sandwiched between Siberian craton on the north and<br />
Tarim and Sino-Korean cratons in the south. Proposed seismic line extends from Lake Baikal to Inner<br />
Mongolia. Also shown are two major sutures in the CAOB.<br />
Although much new information has become available since the Sengör et al. (1993) synthesis<br />
was published, particularly in the fields of geochronology, isotope and trace element geochemistry,<br />
and sedimentology, there is still a lack of detailed structural work, particularly concerning the<br />
mechanism of arc accretion, the nature and evolution of accretionary prisms and ophiolite mélange<br />
zones, and the relationships and tectonic position, size and origin of microcontinents sandwiched<br />
between the arc complexes. There is also controversy on subduction polarities, the nature, age and<br />
origin of ophiolite complexes, and the origin of unusually large volumes of felsic magmatic rocks.<br />
Seismic profiles extending from the Siberian craton into the CAOB (Zorin et al., 1993) and<br />
across the Chinese Altai and Junggar belts (Wang et al., 2003) do not provide the kind of detailed<br />
information on crustal structure that are exemplied by LITHOPROBE profiles in the Canadian<br />
shield (e.g., Cook and Erdmer, 2005; Clowes and Li, 2005). Although modern attempts to use<br />
passive techniques to delineate lithospheric structure are suggestive (e.g. Figure 2), they still lack<br />
the resolution and credibility of contemporary active/passive imaging. Recent wide angle controlled<br />
source surveys have improved our image of gross crustal structure in the vicinity of Lake Baikal<br />
(e.g. Thybo et al., 2006), but near vertical deep reflection profiling is still lacking. We suggest that a<br />
new seismic profile across the width of the CAOB, using modern techniques such as broadband,<br />
reflection and refraction methods, in combination with a well defined structural/geochronological<br />
/geochemical traverse, would provide much needed information to fully understand the evolution of<br />
this belt. Seismic data would also help to resolve some of the many ambiguities such as size and<br />
extent of microcontinental blocks, subduction polarities, generation of granitoids and the structure<br />
of the subcrustal mantle beneath the CAOB.<br />
Major problems to be solved: The proposed traverse would cross the following trans-CAOB<br />
sutures (see Fig. 1), and it would be useful to establish whether they penetrate the entire crust and<br />
extend into the upper mantle and, in view of current differences in interpretation, to determine their<br />
polarities:<br />
a. The Mongol-Okhotsk suture in central-eastern Mongolia that formed in the early Mesozoic.<br />
Was subduction only to the north (Zorin, 1999), or to both north and south (Tomurtogoo et al.,<br />
2005)?<br />
b. The Main Mongolian Lineament that probably formed a plate boundary in the late Ordovician<br />
between already-accreted terranes to the north and open ocean to the south (Badarch et al.,<br />
2002; Kröner et al., 2006). The ocean was consumed by subduction to the north.
3<br />
c. The end-Permian Solonker suture in Inner Mongolia that represents the closure of the Palaeo-<br />
Asian Ocean and termination of the CAOB. Was subduction only to the south (Zhang et al.,<br />
2003) or to both north and south (Xiao et al., 2003)?<br />
Both the Mongol-Okhotsk and Solonker orogens have been described as of Himalayan-scale,<br />
with potential massive crustal thickening caused by thrusting and/or magma additions, followed by<br />
extensional collapse and formation of metamorphic core complexes (Zorin, 1999; Tomurtogoo et<br />
al., 2005 ; Xiao et al., 2003). Seismic profiles could define the thrust structure (thin- or thickskinned)<br />
and extensional detachments.<br />
One of the major problems in understanding the tectonic development of Mongolia is: what lies<br />
below the huge Hangay-Hentei basin – a Precambrian gneissic microcontinent or mafic arc-type<br />
rocks? This concerns the highly controversial existence of a major Mongolian orocline that<br />
dominates the structure of the northeastern CAOB (Sengör et al., 1993; Yakubchuk, 2002).<br />
The most appropriate route for the geophysical traverse would follow the main asphalt road from<br />
the Russian-Mongolian border at Sukhbaatar to Ulaanbaatar and then follow the road that parallels<br />
the railway line to the Chinese border at Erenhot, and south from there to Inner Mongolia. This<br />
straight-line road traverse would cross all the main sutures and orogens mentioned above.<br />
Why use seismology? Most international seismic profiling projects such as COCORP and BIRPS<br />
have studied collisional orogenic belts such as the Appalachians, Caledonides and Himalayas-Tibet.<br />
This proposed geophysical profile from Lake Baikal to Inner Mongolia will be the first to cross a<br />
major, wide accretionary orogenic belt that formed by processes similar to those that have created<br />
the Japanese Islands and are presently active in the SW Pacific. Accordingly, it will provide<br />
important new information on the fundamental structure of the continental crust.<br />
Although all geophysical methodologies have important contributions to make in detailing<br />
lithospheric structure, only seismology can provide the resolution of structure needed to correlate<br />
surface geological features to depth with any confidence. Modern lithospheric seismic surveys<br />
stress the combined acquisition and processing of near-vertical reflection recording of controlled<br />
sources for structural detail, wide-angle recording of similar sources for delineation of bulk velocity<br />
variations as a proxy for lithology, and passive seismic recording of teleseismic events to obtain<br />
gross structure variations of major geologic interfaces such as the Moho and the base of the<br />
lithosphere. Thus, seismic profiling is most often the core for any lithospheric survey
4<br />
Fig. 2. Crustal structure (bottom) deduced from velocity variations (top) computed from across<br />
from receiver function analysis of passive seismic data. From Zorin et al. (2002). Although this<br />
interpretation is highly speculative, it is indicative of the kinds of lithospheric complexity that need<br />
to be resolved by more detailed geophysical work in the future.<br />
Geophysical techniques to be used: In addition to the primary seismic surveys described above,<br />
magnetotelluric profiling coupled with gravity and magnetic data can provide key constraints on<br />
structural geometry and lithology at depth. All of these geophysical techniques, to be effective,<br />
require careful correlation to surface exposures. Thus they must be matched to petrologic,<br />
geochemical and geochronologic studies of surface geology along the proposed profile route. In<br />
addition, xenoliths from both crustal and mantle sources can provide unique information to help<br />
constrain interpretation of the geophysical results for the lithosphere at depth.
5<br />
Combination of geophysics with geological traverse: We suggest that the geophysical traverse is<br />
combined with field-based geological, petrological, geochemical asnd geochronological studies in a<br />
broad corridor along the proposed seismic line. This work should concentrate on structural studies<br />
to link seismic reflectors at depth to surface structures, with particular emphasis on defining terrane<br />
boundaries and understanding arc accretion and ophiolite emplacement. Petrological/geochemicalisotopic<br />
studies will help to reconstruct geodynamic environments, and geochronology will<br />
determine the ages of major magmatic, metamorphic and deformational events.<br />
Xenolith studies: The dynamic evolution of the CAOB during and after its assembly will be<br />
reflected in the relationships between the upper crust, the lower crust and the underlying<br />
lithospheric mantle. For example, delamination of oceanic/arc lithosphere may have allowed<br />
upwelling of the asthenospheric mantle, providing the heat necessary for the widespread felsic<br />
magatism that followed the accretion of the CAOB (Jahn, 2004; Kröner et al., 2006; Zheng et al.,<br />
2006). The traverse crosses a region with abundant Cenozoic basaltic rocks that carry xenoliths of<br />
the deep crust and upper mantle; key areas include the Baikal rift zone (Litasov and Taniguchi,<br />
2002) northern and central Mongolia ((Ionov et al. 1998), and the Dariganga lava plateau in<br />
southern Mongolia/northern China ((Ionov et al., 1999). Lower-crust and upper-mantle xenolith<br />
suites from localities near the traverse can be used to calibrate the seismic data in terms of rock<br />
types and temperatures at depth. Isotopic data on lower-crustal xenoliths can define the timing and<br />
nature of underplating events that contributed to crustal growth. Whole-rock and in-situ Re-Os<br />
analysis (eg Griffin et al., 2004, and references therein) of ultramafic xenoliths can provide<br />
constraints on the timing of mantle events, and to identify tectonic units (eg, microcontinents) that<br />
may have carried ancient lithospheric mantle with them into the tectonic collage.<br />
Isotopic studies: Radiogenic (Nd-Sr) and stable isotope (O) studies have significantly contributed<br />
to identification of mantle-derived juvenile crust and to estimation of the proportion of juvenile to<br />
recycled ancient crust (e.g., Jahn, 2004; Wickham et al., 1996). The CAOB is probably the most<br />
exemplary of accretionary orogens and is considered to represent the most important site of<br />
continental growth in the Phanerozoic (Sengör et al., 1993; Jahn, 2004), but the tectonic evolution<br />
of this belt has been the subject of considerable debate in the last decade. Like in Japan, the CAOB<br />
comprises magmatic arcs, ophiolites, accretionary complexes, and microcontinental blocks.<br />
Accretionary complexes are not necessarily composed largely of juvenile material, as shown in the<br />
case of the Japanese Islands. The characterization of any crustal segments in the CAOB must be<br />
approached by field work and isotope/geochemical study. Since batholithic granitoids (e.g., in
6<br />
Transbaikalia) represent melts derived by large-scale melting of the middle to lower crust, their<br />
isotopic compositions are the best to represent the bulk of individual crustal segments. In any case,<br />
zircon geochronology with Hf isotope measurements and Nd-Sr isotope studies will be carried out<br />
in concert with geophysical and field investigations.<br />
Schedule of Activities: We propose the following timescale to pursue the objectives outlined<br />
above:<br />
(1) An initial workshop for interested scientists to be held in conjunction with the IGCP-480<br />
meeting in Beijing in August 2007. Possibly also a technical workshop on processing of seismic<br />
data in Novosibirsk sometime in 2007.<br />
(2) Development of a core proposal to be used by participants in fund raising in late 2007,<br />
early 2008.<br />
(3) Initial geophysical surveys in the Fall of 2008.<br />
For more information, contact Alfred Kröner at kroener@mail.uni-mainz.de or Larry Brown at<br />
ldb7@cornell.edu.<br />
References cited<br />
Badarch, G., Cunningham, W.D. and Windley, B.F., 2002. A new terrane subdivision for Mongolia:<br />
implications for the Phanerozoic crustal growth of Central Asia. J. Asian Earth Sci., 21, 87-110.<br />
Clowes, R.M. and Li, C (comp.), 2005. Lithoprobe celebratory conference, oral and poster<br />
presentations. Lithoprobe Secretariat, Univ. British Columbia, Vancouver, Canada, Epublication<br />
#5, 2 CDs.<br />
Clowes, R.M., Calvert, A.J., Eaton, D.W., Hajnal, Z., Hall, J. & Ross, G.M. 1996. LITHOPROBE<br />
reflection studies of Archean and Proterozoic crust in Canada. Tectonophysics, 264, 65-88.<br />
Cook, F.A. and Erdmer, P. (eds.), 2005. The Lithoprobe Slave-Northern Cordillera lithospheric<br />
evolution (SNORCLE) transect. Can J. Earth Sci., 42, 869-1311.<br />
Dobretsov, N.L., Buslov, M.M. & Vernikovsky, V.A. 2003. Neoproterozoic to Early Ordovician<br />
evolution of the Paleo-Asian ocean: implications to the break-up of Rodinia. Gondwana Res., 6,<br />
143-159.<br />
Griffin, W.L., Graham, S., O’Reilly, S.Y. and Pearson, N.J. 2004. Lithosphere evolution beneath<br />
the Kaapvaal Craton. Re-Os systematics of sulfides in mantle-derived peridotites. Chem.<br />
Geol., 208, 89-118.
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Ionov, D.A., O’Reilly, S.Y. & Griffin, W.L. 1998. A geotherm and lithosphere section for Central<br />
Mongolia (Tarat region). In: Flowers, M.F.J. et al. Mantle Dynamics and Plate Interactions in<br />
East Asia. Amer. Geophys. Union, Geodynamics 27, 127-153.<br />
Ionov, D.A., Griffin, W.L. O’Reilly, S.Y. 1999. Off-cratonic garnet and spinel peridotite xenoliths<br />
from Dsun-Bussular, SE Mongolia. Proc. 7 th Int. Kimberlite Conf., Red Rook Design, Cape<br />
Town, v. 1, 383-389.<br />
Jahn, B.M.. 2004. The Central Asian orogenic belt and growth of the continental crust in the<br />
Phanerozoic. In: Malpas, J., Fletcher, C.J.N., Ali, J.R. and Aitchinson, J.C. (eds.) Aspects of the<br />
Tectonic Evolution of China. Geol. Soc. London, Special Publications, 226, 73-100.<br />
Kröner, A., Windley, B.F., Badarch, G., Tomurtogoo, O., Hegner, E., Jahn, B.M., Gruschka, S.,<br />
Khain, E.V., Demoux, A. & Wingate, M.T.D., 2006. Accretionary growth and crust-formation<br />
in the central Asian Orogenic Belt and comparison with the Arabian-Nubian shield. In: R.<br />
Hatcher (ed.) 4-D Framework of the Continental Crust - Integrating Crustal Processes through<br />
Time, Memoir, Geol. Soc. America, in press.<br />
Litasov, K. and Taniguchi, H. 2002. Mantle evolution beneath the Baikal Rift. CNEAS<br />
Monograph Series No. 5, Tohoku University. 221 pp.<br />
Perello, J., Cox, D., Garamjav, D., Sanjdori, S., Diakov, S., Schissel, D. Munkhbat, T. & Oyun, G.<br />
2001. Oyu Tolgoi, Mongolia: Late Siluro-Early Devonian porphyry Cu-Au-(Mo) and highsulphidation<br />
Cu mineralization with a Cretaceous chalcocite blanket. Econ. Geol., 96, 1407-<br />
1428.<br />
Ruzhentsev, S.V., and Mossakovskiy, A.A. 1996. Geodynamics and tectonic evolution of the<br />
Central Asian Paleozoic structures as the result of the interaction between the Pacific and Indo-<br />
Atlantic segments of the Earth: Geotectonics, 29, 294-311.<br />
Sengör, A.C., Natal’in, B.A, and Burtman, V.S., 1993. Evolution of the Altaid tectonic collage and<br />
Palaeozoic crustal growth in Eurasia. Nature, 364, 299-306.<br />
Thybo, H, Nielson, C., Jensen, M.-B., Suvorov, V.D., and Perchuc, E., 2006, Baikial explosion<br />
seismic transects, (abs), 12th <strong>International</strong> Symposium on Deep Seismic Profiling of the<br />
Continents and Margins, Hayama, Japan.<br />
Tomurtogoo, O., Windley, B.F., Kröner, A., Badarch, G. & Liu, D.Y. 2005. Zircon age and<br />
occurrence of the Adaatsag ophiolite and Muron shear zone, central Mongolia: constraints on the<br />
evolution of the Mongol-Okhotsk ocean, suture and orogen. J. Geol. Soc. London, 162, 125-134.<br />
Wang, Y., Mooney, W.D., Yuan, X. & Coleman, R.G. 2003. The crustal structure from the Altai<br />
mountains to the Altyn Tagh fault, northwest China. J. Geophys., Res., 108, B6, 2322,<br />
doi:10,1029/2001JB000552, 7/1-16.
8<br />
Wickham, S.M., Albertz, A.D., Zanvilevich, A.N., Litvinovsky, B.A., Bindeman, I.N., Schauble,<br />
A., 1996. A stable isotope study of anorogenic magmatism in East Central Asia. J. Petrol. 37,<br />
1063-1095.<br />
Windley, B.F., Alexeiev, D., Xiao, W., Kröner, A., and Badarch, G., 2006. Tectonic models for<br />
accretion of the Central Asian orogenic belt. J. Geol. Soc. London, in press.<br />
Xiao, W., Windley, B.F. Hao, J. and Zhai, M., 2003. Accretion leading to collision and the Permian<br />
Solonker suture, Inner, Mongolia, China: termination of the central Asian orogenic belt.<br />
Tectonics, 22, 1069, 8:1-20.<br />
Yakubchuk, A. 2002. The Baikalide-Altaid, Transbaikal-Mongolian and North Pacific orogenic<br />
collages: similarity and diversity of structural patterns and metallogenic zoning. In: Blundell,<br />
D.J., Neubauer, F. & von Quadt, A. (eds.) The Timing and Location of Major Ore Deposits in an<br />
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ERAS Report for 2006 – Annexure 6<br />
Geological Society, Special Publication – supported by the<br />
<strong>International</strong> Lithosphere Program (ILP)<br />
Title: Accretionary Orogens in Space and Time<br />
Editors: Peter A. Cawood 1 and Alfred Kröner 2<br />
1 Tectonics Special Research Centre, University of Western Australia, 35 Stirling<br />
Highway, Crawley, WA 6009, Australia<br />
e-mail pcawood@tsrc.uwa.edu.au<br />
2 Institut für Geowissenschaften, Universität Mainz, 55099 Mainz, Germany<br />
e-mail kroener@mail.uni-mainz.de<br />
Meeting:<br />
The proposed articles for this special publication are based on invited contributions by<br />
recognized experts but the initial idea for such a volume grew out of discussions at<br />
symposia held at the Supercontinents and Earth Evolution meeting in Perth,<br />
September 2005, GSA Salt Lake City, October 2005, and EGU, April 2006.<br />
Background and aims:<br />
Classic models of orogens involve a Wilson cycle of ocean opening and closing with<br />
orogenesis related to continent-continent collision. Such models fail to explain the<br />
geological history of a significant number of orogenic belts throughout the world in<br />
which deformation, metamorphism and crustal growth took place in an environment<br />
of ongoing plate convergence. These belts are termed accretionary orogens but have<br />
also been refereed to as non-collisional or exterior orogens, Cordilleran-, Pacific-,<br />
Miyashiro-, and Turkic-type orogens.<br />
This book aims to bring together key researchers on Accretionary Orogens in<br />
providing an up to date understanding of the both the processes operating in<br />
accretionary orogens and the distribution and character of these orogens in space and<br />
time.<br />
What are accretionary orogens:<br />
Accretionary orogens form at sites of subduction of oceanic lithosphere and consist of<br />
magmatic arcs systems along with material accreted from the downgoing plate and<br />
eroded from the upper plate. Accretionary orogens have been active throughout Earth<br />
history. They have been responsible for major growth of the continental lithosphere<br />
through the addition of juvenile magmatic products and include Archean greenstone<br />
belts, the Paleoproterozoic Birimian orogen (W. Africa), the Arabian-Nubian shield<br />
(Pan African) and Paleozoic orogens in Asia. They are also major sites of<br />
consumption and reworking of continental crust through time (e.g. Andean margin)<br />
and understanding the balance between crustal generation and consumption in<br />
accretionary orogens is fundamental to resolving models of continental growth<br />
throughout Earth history. Orogenesis takes place through coupling across the plate
oundary with strain concentrated in zones of mechanical and thermal weakening<br />
such as the magmatic arc and back arc region. Potential driving mechanisms for<br />
coupling include accretion of buoyant lithosphere (terrane accretion), flat slab<br />
subduction, and rapid absolute upper plate motion over-riding the downgoing plate.<br />
The Circum-Pacific region provides outstanding examples of accretionary orogens.<br />
2<br />
The book will appeal to a wide variety of researchers reflecting the diverse interests of<br />
those working on accretionary orogens. It will be particular relevant to those in the<br />
field of tectonics.<br />
We have broken the proposed articles into two broad headings: those concerned with<br />
processes operating in accreting orogens and those concerned with understanding<br />
specific orogens through space and time.<br />
Proposed Papers<br />
Overview and Processes<br />
1. Accretionary Orogens in Space and Time – P.A. Cawood and A. Kröner<br />
2. Metamorphic Patterns in Accretionary Orogens – Mike Brown<br />
3. Seismic Images of Accretionary Orogens – implications for lithosphere<br />
structure and development – Larry Brown & Bruce Goleby<br />
4. Magmatic Patterns and Geochemical Signature of Accretionary Orogens –<br />
Rob Kerrich and A. Polat,<br />
5. The rock and sediment fabric of modern subduction zones predict that<br />
truncated, thinned, and missing convergent-margin crust may be typical of the<br />
suture zones of ancient accretionary orogens. David Scholl and Roland von<br />
Huene.<br />
6. Sedimentary Evidence for Large-Scale Crustal Recycling at Active Plate<br />
Margins – Peter Clift<br />
7. Thermo-mechanical modeling of crustal reworking and the balance between<br />
crustal accretion and subtraction at subduction-related orogens – S. Sobolev<br />
8. Geodynamic modelling of accretionary orogens – Klaus Regenauer-Lieb<br />
9. Preservation and destruction of subcontinental lithosphere beneath<br />
accretionary orogens – W.L. Griffin, S.Y. O'Reilly, O. Alard and J. Zheng<br />
10. Driving mechanisms of deformation in accretionary orogens – Gordon Lister<br />
11. Ocean plate stratigraphy past and present – Brian Windley and Sigenri<br />
Maruyama<br />
12. Unraveling the nature and causes of arc-backarc migration patterns in<br />
accretionary orogens using geochemistry: the Lachlan Fold Belt example –<br />
Bill Collins<br />
13. Metallogeny of accretionary orogens - the connection between lithospheric<br />
processes and endowment. Frank Bierlein, David Groves and Peter Cawood
Regional Studies<br />
14. Earth’s earliest Accretionary Orogens – Friend and Nutman<br />
3<br />
15. Archean accretionary orogens in Australia: comparisons with modern<br />
orogens" authored by K. Cassidy, M. van Kranendonk, H. Smithies and D.<br />
Champion<br />
16. Accretionary history of the Superior Province - M. Sanborn-Barrie, G. M.<br />
Stott, T. Skulski and D. White<br />
17. Correlation of Archean to Mesoproterozoic units between Canada and<br />
Greenland: Constraining the accretionary history of Trans-Hudson Orogen<br />
within an upper plate/lower plate Asian (Himalayan) context for the<br />
Proterozoic. Marc R. St-Onge, Jeroen van Gool, Adam A. Garde, and David J.<br />
Scott.<br />
18. Palaeoproterozoic accretionary processes in Finland – Raimo Lahtinen<br />
19. Reworking of Palaeoproterozoic accretionary orogens in Laurentia – David<br />
Corrigan, Karl Karlstrom and Fred Cook<br />
20. The Timanian accretionary margin of Baltica –Johannes Glodny and Vicky<br />
Pease<br />
21. Evolution of the Central Asian Orogenic Belt: constraints from<br />
geochronology, palaeomagnetism and field relationships. A. Kröner, B.F.<br />
Widley, W.J. Xiao, P. Jian , D. Alexeiev and A. Didenko.<br />
22. Structural evolution of Arctic Eurasia and Altaid orogeny. Vicky Pease and<br />
Scott<br />
23. Lachlan Fold Belt accretionary orogen – David Gray, Dave Foster, Bob<br />
Gregory<br />
24. Accretionary processes in the Canadian Cordillera – Stephen Johnson<br />
25. Proto-Andean accretionary processes in the South American Cordillera –<br />
Ricardo Astini<br />
26. Accretionary processes in the Caribbean - Manuel Itturalde et al.<br />
27. Canadian Cordillera – Geophysical perspective. David Snyder et al.<br />
28. Accretionary processes in SE Asia – Robert Hall<br />
29. Phanerozoic accretionary orogen in Japan: a template for Precambrian<br />
analogues - Yukio Isozaki