羅賓·克納

羅賓·M·克納（英語：Robin M. Canup，1968年11月20日—）是一名美國天體物理學家。她於杜克大學取得理學學士的學位，並在科羅拉多大學波德分校取得博士學位。她主要的研究領域涉及行星和衛星的起源^[1]。在2003年，她獲頒哈羅德·C·尤里獎^[2]。在2022年4月，羅賓·克納擔任調查指導委員會的聯合主席，與菲力浦·克里斯藤森（英語：Philip R. Christensen）一起介紹了行星科學十年調查（英語：Planetary Science Decadal Survey）的結果^[3]。

克納為眾所周知的研究是基於巨大撞擊假說，並涉及有關建模測試，模擬行星實際上是如何的碰撞^[4]^[5]^[6]^[7]。克納認為地球和月球形成於兩個行星結構體的大規模碰撞，每個個體都大於火星，並且是再碰撞才形成現在我們所謂的地球^[8]；而且再碰撞之後，包圍在地球附近的物質結合起來，形成了月球^[9]。她寫了一本關於地球和月球起源的書^[10]。克納還出版了描述冥王星和冥衛一起源於巨大撞擊的研究^[11]。

克納也是有才能（學識淵博）的芭蕾舞者，並且在完成她的論文一週後，擔任博爾德芭蕾舞團維妮（Coppélia）劇中的主角^[12]。

書目提要

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)

參考資料

^ University of Boulder Profile （頁面存檔備份，存於互聯網檔案館）, 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]. （原始內容存檔於2008-07-03）.
^ Smith, David; Chamberlain, Megan; Brown, Mia. Planetary Science and Astrobiology Decadal Survey 2023-2032. 華盛頓哥倫比亞特區: National Academies of Sciences, Engineering, and Medicine. [2024-10-01]. （原始內容存檔於2021-03-29）（英語）.
^ 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. （原始內容存檔於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. （原始內容存檔於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]. （原始內容存檔於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]. （原始內容存檔於2020-09-20）.

外部連結

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

[1] University of Boulder Profile （頁面存檔備份，存於互聯網檔案館）, 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]. （原始內容存檔於2008-07-03）.

[3] Smith, David; Chamberlain, Megan; Brown, Mia. Planetary Science and Astrobiology Decadal Survey 2023-2032. 華盛頓哥倫比亞特區: National Academies of Sciences, Engineering, and Medicine. [2024-10-01]. （原始內容存檔於2021-03-29）（英語）.

[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. （原始內容存檔於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. （原始內容存檔於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]. （原始內容存檔於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]. （原始內容存檔於2020-09-20）.

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