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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.


7<br />

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 />

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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

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