The South Range Breccia Belt of the Sudbury Impact Structure: A possible terrace collapse feature
The South Range Breccia Belt of the Sudbury Impact Structure: A possible terrace collapse feature
复制标题
萨德伯里冲击构造的南岭角砾岩带:可能的台地塌陷特征
DOI:
10.1111/j.1945-5100.2000.tb01432.x
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发表时间:
2000
影响因子:
2.2
通讯作者:
J. Spray
中科院分区:
文献类型:
--
作者:
R. G. Scott;J. Spray
Abstract— The South Range Breccia Belt (SRBB) is an arcuate, 45 km long zone of Sudbury Breccia in the South Range of the 1.85 Ga Sudbury Impact Structure. The belt varies in thickness between tens of meters to hundreds of meters and is composed of a polymict assemblage of Huronian Supergroup (2.49–2.20 Ga), Nipissing Diabase (2.2 Ga), and Proterozoic granitoid breccia fragments ranging in size from a few millimeters to tens of meters. The SRBB matrix is composed of a fine‐grained (∼100 μm) assemblage of biotite, quartz, and ilmenite, with trace amounts of plagioclase, zircon, titanite, epidote, pyrite, chalcopyrite, pyrrhotite, and occasionally chlorite. The SRBB hosts the Frood‐Stobie, Vermilion, and Kirkwood quartz diorite offset dykes, the former being associated with one of the largest Ni‐Cu‐PGE sulphide deposits in the world.