U.S.-U.K. Collaborative Research: Origin of the Solar System

美英合作研究：太阳系的起源

• 批准号: 9024676
• 负责人: Douglas N. Lin
• 金额: $ 1.83万
• 依托单位: University of California-Santa Cruz
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 1991
• 资助国家: 美国
• 起止时间: 1991-08-01 至 1992-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9024676&HistoricalAwards=false
• 关键词: U.S.; U.K.; Collaborative; Research; Origin

This award will support collaborative research in solar system astronomy between Dr. Douglas Lin, University of California at Santa Cruz, and three British scientists: Dr. Sverre Aarseth, Institute of Astronomy, Cambridge University, and Drs. John Papaloizou and Philip Palmer, School of Mathematical Sciences, Queen Mary and Westfield College, London. The objective of the project is to investigate the formation of prototerrestrial planets and protogiant planetary cores in the solar nebula environment. The specific tasks are: 1) to develop an analytical model for the dynamics of planetesimals, 2) to carry out N-body numerical simulations to examine the dynamical evolution and mass coagulation of planetesimals, 3) to investigate the effects of hydrodynamic drag and tidal interaction on the dynamics of planetesimals and protoplanets, and 4) to determine the dynamical impact of protoplanets on the structure and evolutions of the solar nebula. These theoretical investigations will be carried out with the aid of analytic formalisms and numerical schemes recently developed by the investigators. Data from solar system exploration and ground based observations of protostellar disks around young stellar objects will be used to constrain theoretical models. The project will benefit from the complementary expertise of the investigators and their successful history of past collaboration. Results of this research will contribute to the understanding of the origin of the solar system, one of the most outstanding problems in astrophysics and planetary science.

该奖项将支持加州大学圣克鲁斯分校的 Douglas Lin 博士和三名英国科学家：剑桥大学天文学研究所的 Sverre Aarseth 博士和John Papaloizou 和 Philip Palmer，伦敦玛丽皇后学院和韦斯特菲尔德学院数学科学学院。 该项目的目标是研究太阳星云环境中原地球行星和原巨行星核心的形成。 具体任务是：1）建立星子动力学分析模型，2）进行N体数值模拟以研究星子的动力学演化和​​质量凝结，3）研究水动力阻力和潮汐的影响星子和原行星动力学的相互作用，4) 确定原行星对太阳星云结构和演化的动力学影响。 这些理论研究将借助研究人员最近开发的分析形式主义和数值方案来进行。 来自太阳系探索和年轻恒星周围原恒星盘地面观测的数据将用于约束理论模型。该项目将受益于研究人员的互补专业知识及其过去合作的成功历史。 这项研究的结果将有助于理解太阳系的起源，这是天体物理学和行星科学中最突出的问题之一。