米卢廷·米兰科维奇 Milutin Milanković

（重定向自Milankovitch）

米卢廷·米兰科维奇（塞尔维亚语：Милутин Миланковић，拉丁化：Milutin Milanković，发音：[milǔtin milǎːnkɔʋitɕ]，1879年5月28日－1958年12月12日）是一位塞尔维亚土木工程师、地球物理学家和天文学家。因为冰河时期的研究而闻名；他提出了地球长期气候变化和地球轨道的周期性变化关系，也就是今日的米兰科维奇循环。米兰科维奇提出了地球科学的两大贡献。第一个是关于地球日照的学说（Canon of the Earth's Insolation），该学说特别指出了太阳系各行星气候特征；第二个贡献是解释地球气候变迁是因为地球和太阳相对位置的变化，这解释了过去地球冰河时期的发生时间，并可预测地球未来气候变化。

Milutin Milanković 米卢廷·米兰科维奇

（重定向自Milankovitch）

Orbital eccentricity, obliquity and precession.

Milutin Milanković (Serbian Cyrillic:Милутин Миланковић, pronounced [milǔtin milǎːnkɔʋitɕ]; 28 May 1879 – 12 December 1958) was a Serbian mathematician, astronomer, climatologist, geophysicist, civil engineer, doctor of technology, university professor and popularizer of science. Milanković gave two fundamental contributions to global science. The first contribution is the "Canon of the Earth’s Insolation", which characterizes the climates of all the planets of the Solar system. The second contribution is the explanation of Earth's long-term climate changes caused by changes in the position of the Earth in comparison to the Sun, now known as Milankovitch cycles. This explained the ice ages occurring in the geological past of the Earth, as well as the climate changes on the Earth which can be expected in the future. He founded planetary climatology by calculating temperatures of the upper layers of the Earth's atmosphere as well as the temperature conditions on planets of the inner Solar system, Mercury, Venus, Mars, and the Moon, as well as the depth of the atmosphere of the outer planets. He demonstrated the interrelatedness of celestial mechanics and the Earth sciences, and enabled consistent transition from celestial mechanics to the Earth sciences and transformation of descriptive sciences into exact ones.

单词	Milankovitch
释义	Milankovitch 原声例句万物简史 Milankovitch wondered if there might be a relationship between these complex cycles and the comings and goings of ice ages. 米兰柯维契觉得，这些周期性的复杂变化与冰川期的产生和消退也许存在某种关系。万物简史 Milankovitch realized that the problem with Croll's theory was not that it was incorrect but that it was too simple. 他发现，克罗尔的理论的问题并不是它不正确，而是它太简单。 iBT新托福突破口 And one of the best-known is called the Milankovitch Hypothesis. Now what the Milankovitch Hypothesis is about? 最著名的假设之一是米兰科维奇假说。现在米兰科维奇假说是关于什么的？ iBT新托福突破口 Now, when Milankovitch first proposed this theory in the 1920s, many of his colleagues were skeptical. 现在，当 Milankovitch 在 1920 年代首次提出这一理论时，他的许多同事都持怀疑态度。万物简史 The calculations all had to be made in his spare time, but in 1914 Milankovitch suddenly got a great deal of that 计算都得在业余时间里进行，可是到了1914年，米兰柯维契突然有了许多空余的时间。 iBT新托福突破口 And from these samples they were able to put together a history of ocean temperatures going back hundreds of thousands of years, and this showed that earth’s climate had changed pretty much the way Milankovitch’s hypothesis suggested it would. 从这些样本中，他们能够将几十万年前的海洋温度历史放在一起，这表明地球的气候已经发生了很大的变化，就像米兰科维奇的假设所暗示的那样。中文百科米卢廷·米兰科维奇 Milutin Milanković （重定向自Milankovitch）米卢廷·米兰科维奇（塞尔维亚语：Милутин Миланковић，拉丁化：Milutin Milanković，发音：[milǔtin milǎːnkɔʋitɕ]，1879年5月28日－1958年12月12日）是一位塞尔维亚土木工程师、地球物理学家和天文学家。因为冰河时期的研究而闻名；他提出了地球长期气候变化和地球轨道的周期性变化关系，也就是今日的米兰科维奇循环。米兰科维奇提出了地球科学的两大贡献。第一个是关于地球日照的学说（Canon of the Earth's Insolation），该学说特别指出了太阳系各行星气候特征；第二个贡献是解释地球气候变迁是因为地球和太阳相对位置的变化，这解释了过去地球冰河时期的发生时间，并可预测地球未来气候变化。英语百科 Milutin Milanković 米卢廷·米兰科维奇（重定向自Milankovitch） Milutin Milanković (Serbian Cyrillic:Милутин Миланковић, pronounced [milǔtin milǎːnkɔʋitɕ]; 28 May 1879 – 12 December 1958) was a Serbian mathematician, astronomer, climatologist, geophysicist, civil engineer, doctor of technology, university professor and popularizer of science. Milanković gave two fundamental contributions to global science. The first contribution is the "Canon of the Earth’s Insolation", which characterizes the climates of all the planets of the Solar system. The second contribution is the explanation of Earth's long-term climate changes caused by changes in the position of the Earth in comparison to the Sun, now known as Milankovitch cycles. This explained the ice ages occurring in the geological past of the Earth, as well as the climate changes on the Earth which can be expected in the future. He founded planetary climatology by calculating temperatures of the upper layers of the Earth's atmosphere as well as the temperature conditions on planets of the inner Solar system, Mercury, Venus, Mars, and the Moon, as well as the depth of the atmosphere of the outer planets. He demonstrated the interrelatedness of celestial mechanics and the Earth sciences, and enabled consistent transition from celestial mechanics to the Earth sciences and transformation of descriptive sciences into exact ones.
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