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	<title>2018年USAAAO短问题第1道 - 版本历史</title>
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	<updated>2026-04-29T17:42:45Z</updated>
	<subtitle>本wiki的该页面的版本历史</subtitle>
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		<id>https://www.astro-init.top/index.php?title=2018%E5%B9%B4USAAAO%E7%9F%AD%E9%97%AE%E9%A2%98%E7%AC%AC1%E9%81%93&amp;diff=1777&amp;oldid=prev</id>
		<title>Jingsong Guo：创建页面，内容为“==英文题目==  1. [5 pt] In order to detect an Earth-twin, we need significant advances in the precision of spectrographs to detect the periodic Doppler shift of…”</title>
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		<updated>2020-03-09T10:10:35Z</updated>

		<summary type="html">&lt;p&gt;创建页面，内容为“==英文题目==  1. [5 pt] In order to detect an Earth-twin, we need significant advances in the precision of spectrographs to detect the periodic Doppler shift of…”&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;==英文题目==&lt;br /&gt;
&lt;br /&gt;
1. [5 pt] In order to detect an Earth-twin, we need significant advances in the precision of spectrographs&lt;br /&gt;
to detect the periodic Doppler shift of nearby stars. Estimate the radial velocity semi-amplitude, in m/s,&lt;br /&gt;
that a planet with the mass, radius, and semi-major axis of Earth would cause in the motion of a star with&lt;br /&gt;
the mass of the Sun. Assume that the Earth-twin has zero eccentricity. Note that the mass of Earth is&lt;br /&gt;
$$5.97 × 10^{24}$$ kg, and the distance from the Earth to the Sun is $$1.5 × 10^8$$ m.&lt;/div&gt;</summary>
		<author><name>Jingsong Guo</name></author>
		
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