1982
DOI: 10.1130/0091-7613(1982)10<43:oecbaw>2.0.co;2
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“Oman Exotics”—Oceanic carbonate build-ups associated with the early stages of continental rifting

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Cited by 125 publications
(47 citation statements)
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“…The Bisotoun and Radiolarite zones resulted from thinning of the Arabian Plate during Neotethys opening in PermianTriassic time (Searle and Graham, 1982;Kazmin et al, 1986;Fontaine et al, 1989). The Bisotoun zone (or Bisotoun platform) is composed of thick carbonate deposits at the northeastern rim of the Arabian Plate.…”
Section: Tectonic Settingmentioning
confidence: 99%
“…The Bisotoun and Radiolarite zones resulted from thinning of the Arabian Plate during Neotethys opening in PermianTriassic time (Searle and Graham, 1982;Kazmin et al, 1986;Fontaine et al, 1989). The Bisotoun zone (or Bisotoun platform) is composed of thick carbonate deposits at the northeastern rim of the Arabian Plate.…”
Section: Tectonic Settingmentioning
confidence: 99%
“…If the ophiolite formed by this`r idge-centered thrust'' model, then amphibolites of the metamorphic sole and volcanics of the ophiolite should have the same geochemical characteristics and form in the same tectonic setting (at a mid-ocean ridge spreading center). In Oman this is clearly not the case; abundant data show that amphibolites of the metamorphic sole are oceanic tholeiites, similar to Jurassic tholeiitic basalts in the Haybi melange, and are unrelated to rocks of the ophiolite [e.g., Alabaster et al, 1982;Lippard et al, 1986;Searle and Cox, 1999;Searle and Graham, 1982;. [60] Ridge collision/subduction ended the formation of normal ophiolitic crust (layered gabbros, ultramafic intrusives, calc-alkaline stocks and sills) because the young oceanic lithosphere was too buoyant to subduct, and the ophiolite entered a phase of intraoceanic thrusting along a shallow decollement ( Figure 7f).…”
Section: Stage 4: Deathmentioning
confidence: 99%
“…It has been suggested that Tethyan ophiolites like Oman formed in small, intracontinental ocean basins only a few hundred kilometers wide (``Red Sea model [Lippard et al, 1986;Robertson, 1986]). In the case of Oman this claim is difficult to understand in light of the fact that the Haybi melange contains late Permian to Triassic oceanic basalts and that sedimentary records show that rifting to form the passive margin of Oman began in the middle Permian and was complete by the early Triassic at the latest [Gealey, 1977;Glennie et al, 1974;Searle and Graham, 1982;Searle and Malpas, 1980]. If we assume a modest spreading rate of only 40 mm/ yr (20 mm/yr half rate) and 150 million years of spreading (early Triassic at 245 Ma to late Cretaceous at 95 Ma), then at least 6000 km of ocean basin must have existed!…”
Section: Stage 5: Resurrectionmentioning
confidence: 99%
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“…Jebel Akdar is one of the regional tectonic windows opening through the oceanic allochthon of the Hawasina volcano-sedimentary nappe complex and the overlying Semail ophiolite (Poupeau et al 1998). The Hawasina Nappes are remnants of the distal part of the south Neotethyan continental margin, whereas the Arabian Platform corresponds to its shallow-water (neritic) proximal part (Searle and Graham 1982;Béchennec et al 1988). The lowgrade greenschist-facies Late Proterozoic rocks in the Jebel Akhdar dome are unconformably overlain by weakly metamorphosed middle Permian to Cenomanian carbonates.…”
Section: Geological Settingmentioning
confidence: 99%