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Discussion |
1 Department of Geological Sciences, University College London, London WC1E 6BT, UK (e-mail: j.milsom{at}ucl.ac.uk)
2 Veritas GeoServices, Suite 530, 3701 Kirby Drive, Houston TX 77098, USA (e-mail: rob.holt{at}veritasdgc.com)
3 10 Lorong 5/19A, 46000 Petaling Jaya, Selangor, Malaysia (e-mail: cshutchison{at}usa.net)
4 Dept. Geosciences, University of Texas at Dallas, TX 75083, USA (e-mail: bergman{at}utdallas.edu) and Dept. Geological Sciences, Southern Methodist Univ., Dallas, TX 75275-0395, USA (e-mail: scb@mail.smu.edu)
5 ARCO China, Shekou, Shaenzhen, Guandong Province, 518067, P.R. China (e-mail: dswauge{at}mail.arco.com)
6 Vastar Resources Inc., 15375 Memorial Drive, Houston, TX 77079, USA (e-mail: jgraves1{at}vastar.com)
Scientific editing by Alex Maltman.
| Introduction |
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The Hutchison et al. interpretations of the deep structure of Sabah were illustrated in a series of cross-sections in which some features (notably the topography) were amplified for the sake of clarity. There was, however, no suggestion that any features would be underemphasized, and the depth scales, although described as only rough guides, indicated normal 510 km thicknesses for oceanic crust. Therefore, and in the light of the comments quoted above, the thin crust shown throughout Sabah and the generally somewhat greater thickness of the extended continental crust of the Dangerous Grounds must be regarded as essential elements of the model. The Late Miocene cross-section (
Fig. 1), showing the end of orogeny in Sabah, is a guide to the Hutchison et al. view of the present-day situation. Crust is less than 30 km thick beneath the Western Cordillera and less than 20 km thick elsewhere. We contend that these values are incompatible with the gravity field, and that it is no more acceptable to present a geological interpretation that ignores geophysical data than a geophysical interpretation that ignores geology. Some way must be found of reconciling the two.
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| Principles of whole-crust gravity modelling |
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| The Crocker-Trusmadi root and ophiolitic basement |
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Despite the claim by Hutchison et al., the models of
Holt (1998) included no ophiolitic basement, thick or otherwise.The crust was characterized as continental on the cross-sections but, more cautiously, of continental density in the text. It is on the Hutchison et al. cross-sections that normal oceanic crust is labelled ophiolite. To object to this is not mere pedantry. It has long been recognized that many ophiolites are forearc rather than normal ocean crust (e.g.
Pearce et al. 1984). They are, moreover, characteristically emplaced by thrusting, and even the largest examples (e.g. eastern Papua, Oman and eastern Sulawesi) overlie sialic metamorphics or sediments on thrusts that are in places shallow dipping or horizontal. We feel that the term ophiolitic basement is inappropriate even on land, and is best avoided.
| Ophiolitic rocks of eastern Sabah |
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| Continental crust beneath Sabah |
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This summary presents obvious problems, not least in having an older tonalite intruding a younger ophiolite, but these were at least minimized by the subsequent claim that other similar intrusions were very low in potassium and therefore components of the ophiolite.
Leong (1998), however, has disputed this, arguing that only one of the potassium values obtained from acid/intermediate rocks in the Upper Segama could be considered low (let alone extremely low) and that the supposedly spurious Jurassic KAr dates have been confirmed by all later determinations.
It is not our intention to become involved in arguments between geologists based on purely geological evidence, particularly as Hutchison et al. will soon publish new KAr and geochemical data. It is, however, fair to point out that not all geologists agree with their interpretation of the outcrops.
| Gravity constraints on crustal thickness in eastern Sabah |
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The Hutchison et al. crustal thickness of about 15 km where Mesozoic ophiolitic basement is at sea level (
Fig. 1) could be compatible with the gravity field only if the underlying mantle were very light. Mantle here might have been hot during Miocene rifting, but even active spreading ridges seldom reach sea level. Todays cooler mantle is thus very unlikely to support subaerial oceanic crust. Moreover, the boundaries of any thermal anomaly would be gradational, but the low Bouguer gravity measured onshore changes, in only a few tens of kilometres, to gravity patterns characteristic of a normal ocean basin in the SE Sulu Sea.
Sedimentation on oceanic crust might, eventually, produce crust as thick as that of a normal continent, and correspondingly low Bouguer gravity. However, although there is a rough correlation between low Bouguer values and sediment outcrops, there are also low values in areas shown as ophiolite by Hutchison et al.. Even the high fields in Darvel Bay are much too low for in situ oceanic crust, but are comparable with fields over ophiolites which are demonstrably thrust-emplaced (e.g.
Milsom 1973).
In contrast to the problems posed by the oceanic solutions, there are few obstacles to interpretation in terms of originally thick continental or island-arc crust, rifted and thinned by southwards propagation of Sulu Sea spreading to provide space for melange and clastic sediments. Gravity alone cannot determine sediment or basement thickness in the basins, since similar fields could be produced by various combinations of these parameters with plausible crustal and sediment densities. What is important, in evaluating the geotectonic setting of Sabah, is the gravitational evidence for crust 3040 km thick along the rift flanks.
14 August 2000
C. S. Hutchison, S. C. Bergman, D. A. Swauger & J. E. Graves reply: We thank Milsom & Holt for their comments and welcome the opportunity to expand upon aspects we were not able to adequately address. Our main purpose was to provide and interpret new thermochronological data relevant to the Cenozoic denudation history of the collisional mountain belt. We offered a geological context, a tectonic synthesis, and schematic cross-sections to illustrate our main ideas. Milsom & Holt are bothered by our lack of attention to gravity data and the nature of our cross-sections (figs 5 & 6). They were stated to be schematic cartoons in which . . . The scale is only a rough guide and certain features are amplified for the sake of clarity. Our proposed model is based on integrated geological and thermochronological data. The gravity data of Milsom & Holt lack the necessary independent seismic calibration and supporting crustal property data to adequately test our model. The Late Miocene section should not be used as the present-day situation, as Milsom & Holt have suggested. During the intense Late Miocene compressional tectonism, which led to the Crocker Ranges fold and thrust belt, crustal thickening of originally thinned continental crust of the southern South China Sea (c. 515 km thick) undoubtedly occurred, leading to a crust c. 1030 km thick. Milsom & Holt state that their model was based on . . . only crust, mantle, sea water and offshore sediments. Greater complexity is not justified since there are large probable errors in elevation and terrain corrections in the cordillera. This approach ignores the very thick sedimentary rock sequences which are well known in onshore Sabah and have significantly lower densities than standard crust (see
Table 1), and therefore allow for a thin dense basement. We now respond to each section of the Milsom & Holt criticisms.
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| Principles of whole crust gravity modelling |
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| The CrockerTrusmadi root and ophiolitic basement |
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The Kinabalu batholith and satellite stocks intrude Mesozoic ophiolitic rocks and overlying Trusmadi and Crocker Formation turbidites. This complex situation of low density sandstone (c. 2.5 g cc1) and biotitehornblende granitoid (c. 2.62.7 g cc1), juxtaposed against high density mafic and ultramafic rocks (c. 2.9 g cc1) with an unknown contact geometry, makes gravity modelling highly tenuous, especially in the absence of accurate and precise elevation and terrain corrections.
The regional low Bouguer gravity field of much of Sabah is an inescapable fact, yet its origin is open to discussion. We offer two alternatives: (1) the underlying upper mantle is heterogeneous and possesses anomalously low density; (2) crustal densities are heterogeneous and anomalously low. The labeling of portions of our cross-sections as ophiolite was ambiguous and simply reflected the dominant lithology shown on the cartoon sections. We should have labeled them as mafic/ultramafic crust to remove potential confusion with oceanic crust. We labeled the South China Sea crust as ophiolite, in a broad sense to include fore-arc and back-arc mafic/ultramafic lithosphere, or even arc material itself, accreted to the margin of Sundaland during the late Cretaceous and early Cenozoic.
| Ophiolitic rocks of Eastern Sabah |
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| Continental crust beneath Sabah |
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The provenance of the feldspar-bearing Crocker Formation and younger sandstones indicates a granitic source character, which conflicts with the abundance of mafic and ultramafic basement rocks exposed throughout much of Sabah. Zircon fission-track age data for these sandstones which we presented indicate a Cretaceous granitic provenance, which lies outside of Borneo or was eroded during the Paleogene denudation event that produced the Crocker turbidites. We believe the provenance for Crocker turbidites was mainland Asia (e.g., Southern China), which was much more proximal to Borneo during the Palaeogene prior to extrusion of Indochina and subsequent offset of >500700 km along the Ailao ShanRed River Shear Zone through China and Vietnam (
Leloup et al. 1995,
2000). The apparent contradiction of the exposed mafic crystalline basement and quartz-rich felsic Cenozoic sandstone provenance is but one of the many enigmas in Sabah geology. A useful analogue may be made with the thick quartz-rich Miocene turbidites, probably derived from erosion of the Crocker Ranges, which occur in the deep marginal basins of the southern Sulu and Celebes Seas (
Hutchison 1996, pp. 49).
| Gravity constraints on crustal thickness in eastern Sabah |
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Mount Kinabalu is an enigma in the regional tectonic history and should be emphasized. The Crocker Ranges and the Kinabalu massif may be in isostatic disequilibrium due to the youth of the orogenesis. Our new data tightly constrain the intrusion and cooling history between >700°C to <60°C to within the Late Miocene (13.77 Ma), whereas previous radiometric age data disparately ranged from 2 to 20 Ma (
Jacobsen 1970;
Vogt & Flower 1989). We interpret the available geochemical and petrologic data to indicate that the granitic melts originated by lithospheric melting, probably caused by collisional processes, perhaps involving slab-break off, rather than normal subduction-related processes. The intrusion and denudation of the Kinabalu massif coincided with the rapid cooling of the Crocker Ranges induced by compressional tectonics and denudation of over 34 km of overburden since 1015 Ma.
In conclusion, we agree with several of the points raised by Milsom & Holt, regret several minor errors in our paper, and emphasize that our cross-sections are simply schematic cartoons to illustrate aspects of our proposed tectonic model. The Milsom & Holt model, which considered only one alternative that conflicts with a variety of geological data, is unlikely. Alternative gravity models considering reasonable geological assemblages should be evaluated using independently calibrated crustal thickness. We look forward to seeing the fruits of future geological and geophysical studies to constrain better the tectonic evolution of this enigmatic collisional belt, and to reconcile many of the apparently conflicting facts of Sabah geology.
18 September 2000
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