KEPLER'S CHILDREN

TONY REICHHARDT

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KEPLER'S CHILDREN

机译：开普勒的孩子

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Dave latham had to be talked into making the discovery for which he's probably best known. One Friday afternoon in September 1984, Israeli astronomer Tsevi Mazeh, whom he'd never met, paid a visit to his office at the Harvard-Smithsonian Center for Astrophysics. Mazeh had an idea: Use the Center's "digital speedometer"-an instrument that measured the motions of distant stars by recording Doppler shifts in their spectra-to look for slight wobbles caused by the tug of Jupiter-size planets. Latham objected that his instrument wasn't nearly sensitive enough. It could measure these radial velocities down to a few hundred meters per second, but Jupiter's tugging effect on our sun, for example, is just 12 meters per second. What if the planet were much closer to its star, Mazeh wondered. Big planets don't orbit that close, answered Latham, citing then-current theory about how planets formed. Don't always be bound by what the theorists say, countered Mazeh.

机译：必须与戴夫·拉特罕（Dave latham）进行对话，以使他可能最出名的发现。 1984年9月的一个星期五下午，他从未见过的以色列天文学家Tsevi Mazeh造访了哈佛-史密森尼天体物理学中心的办公室。 Mazeh有个主意：使用中心的“数字测速仪”（一种通过记录光谱中的多普勒频移来测量遥远恒星运动的仪器）来寻找由木星大小的行星的拖轮引起的轻微摆动。莱瑟姆（Latham）反对他的乐器不够灵敏。它可以测量到每秒几百米的径向速度，但是木星对我们太阳的拉力作用仅为每秒12米。玛泽纳想知道，如果行星离它的恒星更近，该怎么办？莱瑟姆回答说，大行星并不会绕着如此接近的轨道运动，当时的理论是关于行星是如何形成的。反驳Mazeh的话，不要总是被理论家的话所束缚。

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《Air and Space》 |2016年第3期|52-59|共8页
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TONY REICHHARDT;
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1. Simulations of the Dynamics of the Debris Disks in the Systems Kepler-16, Kepler-34, and Kepler-35 [J] . Demidova T. V., Shevchenko I. I. Astronomy letters . 2018,第2期

机译：Systems Kepler-16，Kepler-34和Kepler-35中的碎片磁盘动态的模拟
2. Light curve analysis for eclipsing systems with exoplanets. The systems Kepler-5b, Kepler-6b, and Kepler-7b [J] . Gostev N.Y. Astronomy reports . 2011,第7期

机译：具有系外行星的日蚀系统的光曲线分析。系统Kepler-5b，Kepler-6b和Kepler-7b
3. The atmospheres of the hot-Jupiters Kepler-5b and Kepler-6b observed during occultations with Warm-Spitzer and Kepler [J] . Désert J.-M., Charbonneau D., Fortney J.J., The Astrophysical Journal. Supplement Series . 2011,第1期

机译：热杂志的孔孔-5B和孔6b的气氛在掩星期间观察到暖壶和开普勒
4. Re-examining the light curves of Kepler-6b, Kepler-8b and Kepler-40b [C] . O. Ozturk, A. Erdem Turkish Physical Society International Physics Congress . 2018

机译：重新检查Kepler-6B，Kepler-8B和Kepler-40B的光曲线
5. Understanding ancient math through Kepler: A presentation of a few geometric ideas from "The Harmony of the World" (Johannes Kepler). [D] . Arthur, Christopher Alan. 2002

机译：通过开普勒理解古代数学：“世界的和谐”（约翰内斯·开普勒）中的一些几何思想的介绍。
6. A SEARCH FOR LOST PLANETS IN THE KEPLER MULTI-PLANET SYSTEMS AND THE DISCOVERY OF A LONG PERIOD NEPTUNE-SIZED EXOPLANET KEPLER-150 F [O] . Joseph R. Schmitt, Jon M. Jenkins, Debra A. Fischer -1

机译：开普勒多行星系统中失物行星的搜索以及长周期海王星大小的EXOPLANET KEPLER-150 F的发现
7. Translations of Kepler’s Astrological Writings Part I. Kepler as Practising Astrologer Section 2. Kepler’s Clients Subsection 1. Kepler’s Methods of Astrological Interpretation for Rudolf II, 1602 [O] . 2010

机译：开普勒占星作品的翻译第I.普通师作为练习占星师第2节。开普勒的客户分期部分。雷普勒占Rudolf II的占星术解释方法，1602

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