苏格兰西北部 Stac Fada 成员撞击岩的蚀变撞击玻璃中的软玉撞击器地球化学证据

A. Goodwin, R. J. Garwood, R. Tartèse
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摘要

Stac Fada 成员(Stoer 组)是一个 ∼1.2 Ga 的富含熔体的撞击角砾岩,其源火山口及其邻近性仍存在争议。我们为来自斯托尔湾和第二海岸的斯塔克法达样本中的蚀变冲击熔体碎屑提供了详细的原位地球化学数据集。这些蚀变的撞击熔块目前主要由闪长岩组成。这种倩彩石的测地温度表明,喷出岩毯中的形成温度为 188-231°C ,与之前的估计一致。铂族元素Ir、Pt和Rh之间的正相关性--显然与Ni无关--表明铂族元素富集有两个地球化学来源。我们认为这两个来源分别是富含镁镍的软玉撞击体和目标岩性中的岩浆/超岩浆层状体。镍含量的空间变化表明,地球化学数据与实地观测相结合,可能有助于评估撞击坑的可能位置。
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Geochemical evidence for a chondritic impactor in altered impact glass from the Stac Fada Member impactite, NW Scotland
The Stac Fada Member (Stoer Group) is a ∼1.2 Ga melt-rich impact breccia whose source crater and, therefore, proximity remains debated. We present a detailed in situ geochemical dataset for altered impact melt clasts within Stac Fada samples from Bay of Stoer and Second Coast. These altered impact melt clasts are now predominantly composed of clinochlore. Geothermometry of this clinochlore indicates formation temperatures within the ejecta blanket at 188-231°C, in agreement with previous estimates. A positive correlation between platinum group elements Ir, Pt, and Rh — apparently independent of Ni — indicates two geochemical sources for platinum group elements enrichment. We propose that these represent an Mg-Ni rich chondritic impactor and a mafic/ultramafic layered body within the target lithology. Spatial variation in Ni content suggests that geochemical data, in combination with field observations, may be instrumental in assessing the likely location of the impact crater.
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