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Planets and Stars under the Magnifving Glass

机译:放大镜下的行星和恒星

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摘要

Looking out to the vastness of the night sky, stargazers often ponder questions about the universe, many wondering if planets like ours can be found somewhere out there. But teasing out the details in astronomical data that point to a possible Earth-like planet is exceedingly difficult. To find an extrasolar planet—a planet that circles a star other than the Sun— astrophysicists have in the past searched for Doppler shifts, changes in the wavelength emitted by an object because of its motion. When an astronomical object moves toward an observer on Earth, the light it emits becomes higher in frequency and shifts to the blue end of the spectrum. When the object moves away from the observer, its light become's lower in frequency and shifts to the red end. By measuring these changes in wavelength, astrophysicists can precisely calculate how quickly objects are moving toward or away from Earth.
机译:望着广阔的夜空,观星者经常思考关于宇宙的问题,许多人想知道是否可以在外面找到像我们这样的行星。但是,要弄清楚天文数据中的细节,指出可能有类似地球的行星,这是极其困难的。为了找到太阳系外行星(一个绕太阳以外的恒星旋转的行星),天体物理学家过去一直在寻找多普勒频移,即多普勒频移,因为该物体的运动会改变该物体发出的波长。当一个天文物体移向地球上的观察者时,它发出的光的频率变得更高,并移到光谱的蓝色末端。当物体移离观察者时,其光的频率降低,并移向红色末端。通过测量这些波长的变化,天体物理学家可以精确地计算出物体朝着地球移动或离开地球的速度。

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