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Article: Ultra-high pressure minerals in the Luobusa Ophiolite, Tibet, and their tectonic implications
Title | Ultra-high pressure minerals in the Luobusa Ophiolite, Tibet, and their tectonic implications |
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Authors | |
Issue Date | 2004 |
Publisher | Geological Society Publishing House. The Journal's web site is located at http://www.geolsoc.org.uk/sp |
Citation | Geological Society Special Publication, 2004, v. 226, p. 247-271 How to Cite? |
Abstract | Numerous ultra-high-pressure minerals have been recovered from podiform chromitites in the Luobusa ophiolite, Tibet. Recovered minerals include diamond, moissanite, Fe-silicides, wüstite, Ni-Fe-Cr-C alloys, PGE alloys and octahedral Mg-Fe silicates. These are accompanied by a variety of native elements, including Si, Fe, Ni, Cr and graphite. All of the minerals were hand-picked from heavy-mineral separates of the chromitites and care was taken to prevent natural or anthropogenic contamination of the samples. Many of the minerals and alloys are either enclosed in, or attached to, chromite grains, leaving no doubt as to their provenance. The ophiolite formed originally at a mid-ocean ridge (MOR) spreading centre at 177±33 Ma, and was later modified by suprasubduction zone magmatism at about 126 Ma. The chromitites were formed in the suprasubduction zone environment from boninitic melts reacting with the host peridotites. The UHP minerals are believed to have been transported from the lower mantle by a plume and incorporated in the ophiolite during seafloor spreading at 176 Ma. Blocks of the mantle containing the UHP minerals were presumably picked up by the later boninitic melts, transported to shallow depth and incorporated in the chromitites during crystallization. © The Geological Society of London 2004. |
Persistent Identifier | http://hdl.handle.net/10722/151268 |
ISSN | 2023 SCImago Journal Rankings: 0.687 |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Robinson, PT | en_HK |
dc.contributor.author | Bai, WJ | en_HK |
dc.contributor.author | Malpas, J | en_HK |
dc.contributor.author | Yang, JS | en_HK |
dc.contributor.author | Zhou, MF | en_HK |
dc.contributor.author | Fang, QS | en_HK |
dc.contributor.author | Hu, XF | en_HK |
dc.contributor.author | Cameron, S | en_HK |
dc.contributor.author | Staudigel, H | en_HK |
dc.date.accessioned | 2012-06-26T06:19:43Z | - |
dc.date.available | 2012-06-26T06:19:43Z | - |
dc.date.issued | 2004 | en_HK |
dc.identifier.citation | Geological Society Special Publication, 2004, v. 226, p. 247-271 | en_HK |
dc.identifier.issn | 0305-8719 | en_HK |
dc.identifier.uri | http://hdl.handle.net/10722/151268 | - |
dc.description.abstract | Numerous ultra-high-pressure minerals have been recovered from podiform chromitites in the Luobusa ophiolite, Tibet. Recovered minerals include diamond, moissanite, Fe-silicides, wüstite, Ni-Fe-Cr-C alloys, PGE alloys and octahedral Mg-Fe silicates. These are accompanied by a variety of native elements, including Si, Fe, Ni, Cr and graphite. All of the minerals were hand-picked from heavy-mineral separates of the chromitites and care was taken to prevent natural or anthropogenic contamination of the samples. Many of the minerals and alloys are either enclosed in, or attached to, chromite grains, leaving no doubt as to their provenance. The ophiolite formed originally at a mid-ocean ridge (MOR) spreading centre at 177±33 Ma, and was later modified by suprasubduction zone magmatism at about 126 Ma. The chromitites were formed in the suprasubduction zone environment from boninitic melts reacting with the host peridotites. The UHP minerals are believed to have been transported from the lower mantle by a plume and incorporated in the ophiolite during seafloor spreading at 176 Ma. Blocks of the mantle containing the UHP minerals were presumably picked up by the later boninitic melts, transported to shallow depth and incorporated in the chromitites during crystallization. © The Geological Society of London 2004. | en_HK |
dc.language | eng | en_US |
dc.publisher | Geological Society Publishing House. The Journal's web site is located at http://www.geolsoc.org.uk/sp | en_HK |
dc.relation.ispartof | Geological Society Special Publication | en_HK |
dc.title | Ultra-high pressure minerals in the Luobusa Ophiolite, Tibet, and their tectonic implications | en_HK |
dc.type | Article | en_HK |
dc.identifier.email | Malpas, J: jgmalpas@hku.hk | en_HK |
dc.identifier.email | Zhou, MF: mfzhou@hkucc.hku.hk | en_HK |
dc.identifier.authority | Malpas, J=rp00059 | en_HK |
dc.identifier.authority | Zhou, MF=rp00844 | en_HK |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.doi | 10.1144/GSL.SP.2004.226.01.14 | en_HK |
dc.identifier.scopus | eid_2-s2.0-5544306579 | en_HK |
dc.identifier.hkuros | 93744 | - |
dc.identifier.hkuros | 108959 | - |
dc.identifier.hkuros | 111506 | - |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-5544306579&selection=ref&src=s&origin=recordpage | en_HK |
dc.identifier.volume | 226 | en_HK |
dc.identifier.spage | 247 | en_HK |
dc.identifier.epage | 271 | en_HK |
dc.publisher.place | United Kingdom | en_HK |
dc.identifier.scopusauthorid | Robinson, PT=7403720506 | en_HK |
dc.identifier.scopusauthorid | Bai, WJ=9271474700 | en_HK |
dc.identifier.scopusauthorid | Malpas, J=7006136845 | en_HK |
dc.identifier.scopusauthorid | Yang, JS=49061676200 | en_HK |
dc.identifier.scopusauthorid | Zhou, MF=7403506005 | en_HK |
dc.identifier.scopusauthorid | Fang, QS=7202644200 | en_HK |
dc.identifier.scopusauthorid | Hu, XF=7404710867 | en_HK |
dc.identifier.scopusauthorid | Cameron, S=52163097800 | en_HK |
dc.identifier.scopusauthorid | Staudigel, H=7003773594 | en_HK |
dc.identifier.issnl | 0305-8719 | - |