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鲁伯特·维尔德1905—1976

Rupert Wildt

German-American astronomer (1905–1976)

英国皇家天文学会金质奖章

鲁珀特·维尔特,德国-美国天文学家。

摘自维基百科「鲁珀特·维尔特」,CC BY-SA 4.0

出生
1905 年 6 月 25 日,慕尼黑
逝世
1976 年 1 月 9 日,奥良(麻州)
国籍
德国、美国
学科
天文学、博物与综合
职业
天文学家
母语 / 工作语言
德语
母校
柏林洪堡大学
工作单位
威尔逊山天文台、耶鲁大学

研究领域

天文学

所获奖项(2)

  1. 1966爱丁顿奖章
  2. —英国皇家天文学会金质奖章

百科正文

维尔特出生于德国慕尼黑。1927年,他获得了柏林大学博士学位。他之后加入了哥廷根大学,专门研究大气层的性质。

奖项和荣誉

  • 爱丁顿奖章(1966年)
  • 小行星 1953 鲁珀特·维尔特以他的名字命名
  • 月球环形山维尔特以他的名字命名

以上内容摘自维基百科「鲁珀特·维尔特」,按 CC BY-SA 4.0 使用,去掉了参考文献、外部链接等尾部小节,公式改写成了纯文本。全文、配图和出处见原文。

英文维基百科补充中文条目比较短,下面是英文条目「Rupert Wildt」的原文

Rupert Wildt (; June 25, 1905 – January 9, 1976) was an American astronomer.

He was born in Munich, Germany, and grew up in that country during World War I and its aftermath. In 1927 he was awarded a Ph.D. from the University of Berlin. He joined the University of Göttingen, specializing in the properties of atmospheres.

In 1932 he studied the spectra of Jupiter, and other outer planets, and identified certain absorption bands as belonging to the hydrogen-rich compounds of methane and ammonia. The composition appeared consistent with a composition similar to the sun and other stars.

Assuming that the atmosphere was composed of these gases, during the 1940s and 1950s he constructed a model of the structure of these planets. He believed the core of the planets is solid and composed of a mixture of rock and metal, covered by a thick outer shell of ice, overlaid by a dense atmosphere. His model is still widely accepted.

In 1934 he emigrated to the United States, and became a research assistant at Princeton University from 1937 until 1942. He then became an assistant professor at the University of Virginia until 1947, before joining the faculty of the Yale University.

In 1937 he proposed that the atmosphere of Venus was composed of a mist of formaldehyde. His observations of the atmosphere did not find any water at the time, but later balloon-based measurements did show water in the atmosphere and so his proposal was abandoned. In 1940, however, he also hypothesized that the carbon dioxide in the Venusian atmosphere trapped heat, a phenomenon later called the greenhouse effect.

In 1939 he demonstrated that the major source of optical opacity in the Sun's atmosphere is the H− ion, and thus the main source of visible light for the Sun and stars.

From 1965 until 1968 he was president of the Association of Universities for Research in Astronomy. In the period 1966-1968 he also held the post of the chairman of the department of astronomy at Yale, and from 1973 until his death he was professor emeritus. He died in Orleans, Massachusetts.

Awards and honors

  • Awarded the Eddington Medal in 1966
  • Asteroid 1953 Rupertwildt is named after him
  • The crater Wildt on the Moon is named after him

以上内容摘自英文维基百科「Rupert Wildt」,按 CC BY-SA 4.0 使用,去掉了参考文献、外部链接等尾部小节,公式改写成了纯文本。全文、配图和出处见原文。

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