Collaborative Research: Provenance and Thermal Evolution of the Chugach-Prince William Terrane Flysch, Southern Alaska

合作研究：阿拉斯加南部楚加奇王子 William Terrane Flysch 的起源和热演化

• 批准号: 1116536
• 负责人: Cameron Davidson
• 金额: $ 21.26万
• 依托单位: Carleton College
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2011
• 资助国家: 美国
• 起止时间: 2011-06-15 至 2017-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1116536&HistoricalAwards=false
• 关键词: Collaborative; Research; Provenance; Thermal; Evolution

The Chugach-Prince William terrane is an extensive accretionary complex that formed along the western margin of North America during subduction (under-thrusting) of oceanic lithosphere in the Cretaceous to Eocene. It was intruded by near-trench igneous rocks inferred to be related to the subduction of an oceanic ridge (where new ocean crust is formed), but the location of this terrane at the time of ridge interaction is under considerable debate. There are two prevailing hypotheses for its position at the time of formation: 1) The Chugach-Prince William terrane formed more or less in place and ridge interaction was related to the now-subducted Resurrection plate; or 2) the Chugach-Prince William terrane formed far to the south, was intruded by near-trench igneous rocks near a latitude of 48-49°N, and was subsequently translated along the continental margin to Alaska by strike slip faults similar to the San Andreas fault in California. The possible formation of the Chugach-Prince William terrane far to the south and subsequent translation along the continental margin is a defining event in western North American tectonics and makes testable predictions for the origin and thermal evolution of these rocks. We use geochronology, stratigraphy, petrology, structural geology, and geophysics to unravel the source region of this accretionary complex and subsequent thermal history. Together, these data are yielding important constraints on the accretion and translation history of the Chugach-Prince William terrane and has implications for the history of flanking basins such as the hydrocarbon-rich Cook Inlet basin.This research directly addresses several key problems in North American tectonics related to terrane formation, translation, accretion, and basin formation, and is helping advance geochronologic methods used for tracking the origin and thermal evolution of sedimentary rocks. The results from this work are providing a better tectonic framework for understanding the timing and nature of basin formation (including hydrocarbon-rich strata), and the timing and extent of precious metals deposits (gold) associated with intrusive rocks. This project also has a strong educational component aimed at increasing the number of students in the geoscience pipeline and ultimately the workforce, and our effort is partly focused on recruiting students under-represented in the Geosciences. We are involved in the direct training, mentoring, and assessment of undergraduate students through the Keck Geology Consortium. Students are recruited, and assessed through the existing framework of the Consortium and this effort includes involvement of 30% of the students from non-Keck schools. There is a strong commitment to increasing the number of under-represented students in the Geoscience pipeline (this group includes African American, Hispanic, and Native American) and the new diversity initiative at the Keck Geology Consortium guarantees greater participation by this cohort. The Keck Consortium is dramatically increasing the number of under-represented student participation by several strategies including internal recruitment and external partners. The Keck Geology Consortium plays a leading role in the research training of promising students, and the majority of these students pursue a MSc and/or PhD in the geosciences. Thus the Consortium supplies the geoscience pipeline with bright, talented, well-trained students and many become leaders in the field. It is well known that research active faculty provide a successful and productive learning environment, and that student research at the undergraduate level provides students with the motivation, capability, and preparation for graduate school that typically leads to a productive career in the geosciences.

楚加奇-威廉王子杂岩是一个广泛的增生杂岩，形成于沿着北美西缘，在俯冲（下逆冲）的大洋岩石圈在白垩纪至始新世。 它是由近海沟的火成岩侵入的，推测这与洋脊的俯冲（新的洋壳形成的地方）有关，但在洋脊相互作用时，这一火成岩的位置存在相当大的争议。 关于其形成时的位置有两种流行的假说：1）楚加奇-威廉王子板块在原地或多或少形成，洋脊相互作用与现今俯冲的复活板块有关;楚加奇-威廉王子岩系形成于楚加奇-威廉王子岩系的南部，在北纬48-49°附近被近海沟火成岩侵入，随后被类似于加州圣安德烈亚斯断层的走滑断层沿沿着大陆边缘平移到阿拉斯加。 楚加奇-威廉王子岩可能在遥远的南方形成，随后沿着大陆边缘平移，这是北美西部构造的一个决定性事件，并对这些岩石的起源和热演化做出了可检验的预测。我们使用地质年代学，地层学，岩石学，构造地质学和地球物理学来解开这个增生杂岩的源区和随后的热历史。这些数据共同对楚加奇-威廉王子地体的增生和平移历史产生了重要的约束，并对富含碳氢化合物的库克湾盆地等侧翼盆地的历史产生了影响。这项研究直接解决了北美构造中与地体形成、平移、增生和盆地形成相关的几个关键问题，并帮助推进用于追踪沉积岩起源和热演化的地质年代学方法。 这项工作的结果为理解盆地形成的时间和性质（包括富烃地层）以及与侵入岩有关的贵金属矿床（金）的时间和范围提供了更好的构造框架。 该项目也有一个强大的教育组成部分，旨在增加地球科学管道中的学生人数，并最终增加劳动力，我们的努力部分集中在招收地球科学中代表性不足的学生。我们通过凯克地质学联盟参与本科生的直接培训，指导和评估。通过联盟的现有框架招募和评估学生，这项工作包括来自非凯克学校的30%的学生参与。有一个强有力的承诺，以增加在地球科学管道代表性不足的学生的数量（这组包括非洲裔美国人，西班牙裔和美洲原住民）和凯克地质联盟的新的多样性举措保证了这一群体的更多参与。凯克财团正在通过内部招聘和外部合作伙伴等多种策略，大幅增加代表性不足的学生参与人数。凯克地质联盟在有前途的学生的研究培训中发挥着主导作用，这些学生中的大多数都在攻读地球科学硕士和/或博士学位。因此，该联盟为地球科学管道提供了聪明，有才华，训练有素的学生，许多人成为该领域的领导者。众所周知，研究活跃的教师提供了一个成功和富有成效的学习环境，在本科阶段的学生研究为学生提供了动力，能力和准备研究生院，通常导致在地球科学的生产性职业生涯。