| dbo:abstract |
Su-Shu Huang (黃授書, April 16, 1915 – September 15, 1977) was a Chinese-born American astrophysicist. A graduate of the University of Chicago, Huang began his career with the study of the continuous absorption coefficients of two-electron systems, but eventually his research focus turned to the study of stellar atmospheres, radiative transfer, and binary and multiple star systems. In subsequent years, Huang began to cover the topic of life on extrasolar planets and the prerequisites thereof, coining the term "habitable zone" to refer to the region around a star where planets could support liquid water at their surfaces at a 1959 conference of the Astronomical Society of the Pacific. (en) Su-Shu Huang (Changshu, 16 avril 1915 - Pékin, 15 septembre 1977) est un astrophysicien américain d'origine chinoise. (fr) 黄 授書（こう じゅしょ、1915年4月16日 - 1977年9月15日）は、中国出身のアメリカの天体物理学者。シカゴ大学を卒業した黄授書は、2つの電子の連続吸収係数の研究からキャリアをスタートさせたが、最終的に、恒星大気、放射層、および連星系と恒星系研究に焦点を当てた。その後、太陽系外惑星の生命の話題とその前提条件を取り上げ始め、1959年の会議で、惑星が表面で液体の水を支えることができる星の周りの領域を指す「ハビタブルゾーン」という用語を誕生させた。 (ja) 黃授書 （1915年4月26日－1977年9月15日），男，江苏常熟人，美籍华裔天體物理學家。黄畢業於芝加哥大學。職業生涯早期致力於双電子系統中連續吸收係數的研究，后轉向了恆星大氣層、輻射轉換、和聯星與多星系統。在隨後的幾年，開始研究太陽系外行星的生命及其存在條件，於1959年在太平洋天文學會的一次會議中創造了適居帶這個名詞，指稱在恆星周圍能夠讓行星表面的水維持液態的區域。 (zh) |
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dbr:United_States |
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dbr:Otto_Struve |
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dbr:University_of_Chicago dbr:Zheijiang_University Tsing Hua University (en) |
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Guggenheim Foundation Fellow (en) |
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(en) |
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Explorations of the circumstellar habitable zone and prerequisites of extraterrestrial life (en) |
| dbp:name |
Su-Shu Huang (en) |
| dbp:nativeName |
(en) |
| dbp:nativeNameLang |
Chinese (en) |
| dbp:p |
Huáng Shòu-shū (en) |
| dbp:s |
黄授书 (en) |
| dbp:t |
黃授書 (en) |
| dbp:thesisTitle |
Wave Mechanical Calculations in Astrophysical Interest (en) |
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1949 (xsd:integer) |
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dbr:Astrophysicist |
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| rdfs:comment |
Su-Shu Huang (黃授書, April 16, 1915 – September 15, 1977) was a Chinese-born American astrophysicist. A graduate of the University of Chicago, Huang began his career with the study of the continuous absorption coefficients of two-electron systems, but eventually his research focus turned to the study of stellar atmospheres, radiative transfer, and binary and multiple star systems. In subsequent years, Huang began to cover the topic of life on extrasolar planets and the prerequisites thereof, coining the term "habitable zone" to refer to the region around a star where planets could support liquid water at their surfaces at a 1959 conference of the Astronomical Society of the Pacific. (en) Su-Shu Huang (Changshu, 16 avril 1915 - Pékin, 15 septembre 1977) est un astrophysicien américain d'origine chinoise. (fr) 黄 授書（こう じゅしょ、1915年4月16日 - 1977年9月15日）は、中国出身のアメリカの天体物理学者。シカゴ大学を卒業した黄授書は、2つの電子の連続吸収係数の研究からキャリアをスタートさせたが、最終的に、恒星大気、放射層、および連星系と恒星系研究に焦点を当てた。その後、太陽系外惑星の生命の話題とその前提条件を取り上げ始め、1959年の会議で、惑星が表面で液体の水を支えることができる星の周りの領域を指す「ハビタブルゾーン」という用語を誕生させた。 (ja) 黃授書 （1915年4月26日－1977年9月15日），男，江苏常熟人，美籍华裔天體物理學家。黄畢業於芝加哥大學。職業生涯早期致力於双電子系統中連續吸收係數的研究，后轉向了恆星大氣層、輻射轉換、和聯星與多星系統。在隨後的幾年，開始研究太陽系外行星的生命及其存在條件，於1959年在太平洋天文學會的一次會議中創造了適居帶這個名詞，指稱在恆星周圍能夠讓行星表面的水維持液態的區域。 (zh) |
| rdfs:label |
Su-Shu Huang (fr) 黄授書 (ja) Su-Shu Huang (en) 黃授書 (zh) |
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wikipedia-en:Su-Shu_Huang?oldid=1007894933&ns=0 |
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Su-Shu Huang (en) |
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wikipedia-en:Su-Shu_Huang |
