罗宾·克纳

罗宾·M·克纳（英语：Robin M. Canup，1968年11月20日—）是一名美国天体物理学家。她于杜克大学取得理学学士的学位，并在科罗拉多大学波德分校取得博士学位。她主要的研究领域涉及行星和卫星的起源^[1]。在2003年，她获颁哈罗德·C·尤里奖^[2]。在2022年4月，罗宾·克纳担任调查指导委员会的联合主席，与菲力浦·克里斯藤森（英语：Philip R. Christensen）一起介绍了行星科学十年调查（英语：Planetary Science Decadal Survey）的结果^[3]。

克纳为众所周知的研究是基于巨大撞击假说，并涉及有关建模测试，模拟行星实际上是如何的碰撞^[4]^[5]^[6]^[7]。克纳认为地球和月球形成于两个行星结构体的大规模碰撞，每个个体都大于火星，并且是再碰撞才形成现在我们所谓的地球^[8]；而且再碰撞之后，包围在地球附近的物质结合起来，形成了月球^[9]。她写了一本关于地球和月球起源的书^[10]。克纳还出版了描述冥王星和冥卫一起源于巨大撞击的研究^[11]。

克纳也是有才能（学识渊博）的芭蕾舞者，并且在完成她的论文一周后，担任博尔德芭蕾舞团维妮（Coppélia）剧中的主角^[12]。

书目提要[编辑]

Origin of the Earth and Moon. Robin M. Canup, Kevin Righter (eds.) 2nd. Tucson : Houston: University of Arizona Press. 2000-11-01. ISBN 978-0-8165-2073-2.
National Research Council (various). Defending Planet Earth:: Near-Earth Object Surveys and Hazard Mitigation Strategies. National Academies Press. 2010. ISBN 9780309149686. (member of Space Studies board)

参考资料[编辑]

^ University of Boulder Profile （页面存档备份，存于互联网档案馆）, boulder.swri.edu; accessed March 9, 2015.
^ Harold C. Urey Prize in Planetary Science. Division of Planetary Sciences of the American Astronomical Association. [2015-01-12]. （原始内容存档于2008-07-03）.
^ https://www.nationalacademies.org/our-work/planetary-science-and-astrobiology-decadal-survey-2023-2032 （页面存档备份，存于互联网档案馆） ^{[裸露网址]}
^ Canup, Robin M.; Asphaug, Erik. Origin of the Moon in a giant impact near the end of the Earth's formation. Nature. 2001-08-16, 412 (6848): 708–712 [2015-10-13]. ISSN 0028-0836. PMID 11507633. doi:10.1038/35089010. （原始内容存档于2017-02-17）.
^ Agnor, Craig B.; Canup, Robin M.; Levison, Harold F. On the Character and Consequences of Large Impacts in the Late Stage of Terrestrial Planet Formation. Icarus. 1999, 142 (1): 219–237 [2015-10-13]. Bibcode:1999Icar..142..219A. ISSN 0019-1035. doi:10.1006/icar.1999.6201.
^ Canup, Robin M. Simulations of a late lunar-forming impact. Icarus. 2004, 168 (2): 433–456 [2015-10-13]. Bibcode:2004Icar..168..433C. ISSN 0019-1035. doi:10.1016/j.icarus.2003.09.028. （原始内容存档于2016-12-28）.
^ Canup, Robin M. Dynamics of Lunar Formation. Annual Review of Astronomy and Astrophysics. 2004, 42 (1): 441–475 [2015-10-13]. Bibcode:2004ARA&A..42..441C. doi:10.1146/annurev.astro.41.082201.113457.
^ Canup, Robin M. Forming a Moon with an Earth-like Composition via a Giant Impact. Science. 2012-11-23, 338 (6110): 1052–1055. Bibcode:2012Sci...338.1052C. PMC 6476314 . PMID 23076098. doi:10.1126/science.1226073.
^ NASA Lunar Scientists Develop New Theory on Earth and Moon Formation. NASA Press Release (NASA). 2012-10-30 [2012-12-05]. （原始内容存档于2019-02-23）.
^ Origin of the Earth and Moon. Robin M. Canup, Kevin Righter (eds.) 2nd. Tucson : Houston: University of Arizona Press. 2000-11-01. ISBN 978-0-8165-2073-2.
^ Canup, Robin M. A Giant Impact Origin of Pluto-Charon. Science. 2005-01-28, 307 (5709): 546–550 [2015-10-13]. ISSN 1095-9203. PMID 15681378. doi:10.1126/science.1106818.
^ Finn, Ed. Robin Canup. Popular Science. 2004-10-29 [2015-10-13]. （原始内容存档于2020-09-20）.

外部链接[编辑]

Vimeo上的NAS Research Briefings: Robin M. Canup - Formation of Planetary Moons from National Academy of Sciences

[1] University of Boulder Profile （页面存档备份，存于互联网档案馆）, boulder.swri.edu; accessed March 9, 2015.

[2] Harold C. Urey Prize in Planetary Science. Division of Planetary Sciences of the American Astronomical Association. [2015-01-12]. （原始内容存档于2008-07-03）.

[3] ttps://www.nationalacademies.org/our-work/planetary-science-and-astrobiology-decadal-survey-2023-2032 （页面存档备份，存于互联网档案馆） ^{[裸露网址]}

[4] Canup, Robin M.; Asphaug, Erik. Origin of the Moon in a giant impact near the end of the Earth's formation. Nature. 2001-08-16, 412 (6848): 708–712 [2015-10-13]. ISSN 0028-0836. PMID 11507633. doi:10.1038/35089010. （原始内容存档于2017-02-17）.

[5] Agnor, Craig B.; Canup, Robin M.; Levison, Harold F. On the Character and Consequences of Large Impacts in the Late Stage of Terrestrial Planet Formation. Icarus. 1999, 142 (1): 219–237 [2015-10-13]. Bibcode:1999Icar..142..219A. ISSN 0019-1035. doi:10.1006/icar.1999.6201.

[6] Canup, Robin M. Simulations of a late lunar-forming impact. Icarus. 2004, 168 (2): 433–456 [2015-10-13]. Bibcode:2004Icar..168..433C. ISSN 0019-1035. doi:10.1016/j.icarus.2003.09.028. （原始内容存档于2016-12-28）.

[7] Canup, Robin M. Dynamics of Lunar Formation. Annual Review of Astronomy and Astrophysics. 2004, 42 (1): 441–475 [2015-10-13]. Bibcode:2004ARA&A..42..441C. doi:10.1146/annurev.astro.41.082201.113457.

[8] Canup, Robin M. Forming a Moon with an Earth-like Composition via a Giant Impact. Science. 2012-11-23, 338 (6110): 1052–1055. Bibcode:2012Sci...338.1052C. PMC 6476314 . PMID 23076098. doi:10.1126/science.1226073.

[SimultaneousFormation-9] NASA Lunar Scientists Develop New Theory on Earth and Moon Formation. NASA Press Release (NASA). 2012-10-30 [2012-12-05]. （原始内容存档于2019-02-23）.

[10] Origin of the Earth and Moon. Robin M. Canup, Kevin Righter (eds.) 2nd. Tucson : Houston: University of Arizona Press. 2000-11-01. ISBN 978-0-8165-2073-2.

[11] Canup, Robin M. A Giant Impact Origin of Pluto-Charon. Science. 2005-01-28, 307 (5709): 546–550 [2015-10-13]. ISSN 1095-9203. PMID 15681378. doi:10.1126/science.1106818.

[12] Finn, Ed. Robin Canup. Popular Science. 2004-10-29 [2015-10-13]. （原始内容存档于2020-09-20）.

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