Problems in Giant Planet Formation

巨行星形成的问题

• 批准号: 0507424
• 负责人: Peter Bodenheimer
• 金额: $ 27.94万
• 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: 2005
• 资助国家: 美国
• 起止时间: 2005-07-01 至 2009-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0507424&HistoricalAwards=false
• 关键词: Problems; Giant; Planet; Formation

AST-0507424INSTITUTION: University of California, Santa CruzPI: Peter BodenheimerTITLE: Problems in Giant Planet Formation ABSTRACTDr. Peter Bodenheimer and Dr. Douglas Lin, at the University of California, Santa Cruz, will undertake theoretical investigations of several areas relating to the formation of giant planets. Among the issues are: 1) What mechanisms may have slowed down migration of planets inward toward their host star; 2) What possible mechanisms exist for increasing the rate of gas accretion so that significant accretion can commence at small core masses; and 3) Did Jupiter form with a larger core, which was subsequently eroded and mixed with the gaseous envelope? These remain unsolved problems in understanding the origin of giant planets. The broader impact of the proposed work focuses on the integration of research and scientific education, by means of graduate and undergraduate involvement in the project. The research will also serve to broaden participation in the sciences, by including women in the research. Additionally, the project investigators will encourage broad dissemination of the scientific results, by means of public lectures on planetary science, as well as contributions to science journals for the general public.

AST-0507424机构：加州大学圣克鲁斯分校PI：Peter Bodenheimer标题：巨行星形成中的问题 摘要Dr.位于圣克鲁斯的加州大学的彼得·博登海默和道格拉斯·林博士将对与巨行星形成有关的几个领域进行理论研究。 这些问题包括：1）是什么机制减缓了行星向内向其主星星迁移的速度？2）存在什么可能的机制来增加气体吸积的速率，从而使显著的吸积可以在小的核心质量开始？3）木星是否形成了一个较大的核心，随后被侵蚀并与气体包层混合？ 这些仍然是理解巨行星起源的未解决问题。 拟议工作的更广泛的影响集中在研究和科学教育的整合，通过研究生和本科生参与该项目。 这项研究还将通过让妇女参与研究来扩大对科学的参与。此外，项目调查人员将鼓励通过行星科学公开讲座以及向科学期刊投稿等方式广泛传播科学成果。