<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="zh-Hans-CN">
	<id>https://www.astro-init.top/index.php?action=history&amp;feed=atom&amp;title=2024%E5%B9%B4IOAA%E7%90%86%E8%AE%BA%E7%AC%AC3%E9%A2%98-%E5%B0%8F%E8%A1%8C%E6%98%9F</id>
	<title>2024年IOAA理论第3题-小行星 - 版本历史</title>
	<link rel="self" type="application/atom+xml" href="https://www.astro-init.top/index.php?action=history&amp;feed=atom&amp;title=2024%E5%B9%B4IOAA%E7%90%86%E8%AE%BA%E7%AC%AC3%E9%A2%98-%E5%B0%8F%E8%A1%8C%E6%98%9F"/>
	<link rel="alternate" type="text/html" href="https://www.astro-init.top/index.php?title=2024%E5%B9%B4IOAA%E7%90%86%E8%AE%BA%E7%AC%AC3%E9%A2%98-%E5%B0%8F%E8%A1%8C%E6%98%9F&amp;action=history"/>
	<updated>2026-05-05T10:03:08Z</updated>
	<subtitle>本wiki的该页面的版本历史</subtitle>
	<generator>MediaWiki 1.32.2</generator>
	<entry>
		<id>https://www.astro-init.top/index.php?title=2024%E5%B9%B4IOAA%E7%90%86%E8%AE%BA%E7%AC%AC3%E9%A2%98-%E5%B0%8F%E8%A1%8C%E6%98%9F&amp;diff=2732&amp;oldid=prev</id>
		<title>Quan787：创建页面，内容为“{{由ai生成}} ==英文题目==  '''T3. Asteroid (10 points)'''  A peculiar asteroid of mass, \(m\), was spotted at a distance, \(d\), from a star with mass, \(M\).…”</title>
		<link rel="alternate" type="text/html" href="https://www.astro-init.top/index.php?title=2024%E5%B9%B4IOAA%E7%90%86%E8%AE%BA%E7%AC%AC3%E9%A2%98-%E5%B0%8F%E8%A1%8C%E6%98%9F&amp;diff=2732&amp;oldid=prev"/>
		<updated>2025-03-06T14:54:57Z</updated>

		<summary type="html">&lt;p&gt;创建页面，内容为“{{由ai生成}} ==英文题目==  &amp;#039;&amp;#039;&amp;#039;T3. Asteroid (10 points)&amp;#039;&amp;#039;&amp;#039;  A peculiar asteroid of mass, \(m\), was spotted at a distance, \(d\), from a star with mass, \(M\).…”&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{由ai生成}}&lt;br /&gt;
==英文题目==&lt;br /&gt;
&lt;br /&gt;
'''T3. Asteroid (10 points)'''&lt;br /&gt;
&lt;br /&gt;
A peculiar asteroid of mass, \(m\), was spotted at a distance, \(d\), from a star with mass, \(M\). The magnitude of the asteroid’s velocity at the time of the observation was \(v = \sqrt{\frac{GM}{d}}\), where \(G\) is the universal gravitational constant. The distance \(d\) is much larger than the radius of the star.&lt;br /&gt;
&lt;br /&gt;
For both of the following items, express your answers in terms of \(M\), \(d\), and physical or mathematical constants.&lt;br /&gt;
&lt;br /&gt;
(a) (8 points) If the asteroid is initially moving exactly towards the star, how long will it take for it to collide with the star?&lt;br /&gt;
&lt;br /&gt;
(b) (2 points) If the asteroid is instead initially moving exactly away from the star, how long will it now take for it to collide with the star?&lt;br /&gt;
&lt;br /&gt;
==中文翻译==&lt;br /&gt;
&lt;br /&gt;
'''T3. 小行星（10分）'''&lt;br /&gt;
&lt;br /&gt;
一颗质量为\(m\)的特殊小行星在距离质量为\(M\)的恒星\(d\)处被发现。观测时小行星的速度大小为\(v = \sqrt{\frac{GM}{d}}\)，其中\(G\)为万有引力常数。距离\(d\)远大于恒星半径。&lt;br /&gt;
&lt;br /&gt;
对以下两问，答案需用\(M\)、\(d\)和物理/数学常数表示。&lt;br /&gt;
&lt;br /&gt;
(a) (8分) 若小行星初始直接朝向恒星运动，它需要多长时间会与恒星碰撞？&lt;br /&gt;
&lt;br /&gt;
(b) (2分) 若小行星初始直接背离恒星运动，它需要多长时间会与恒星碰撞？&lt;br /&gt;
&lt;br /&gt;
== 官方解答 ==&lt;br /&gt;
&lt;br /&gt;
(a) 该情况下小行星将沿退化椭圆轨道运动。根据开普勒第三定律：&lt;br /&gt;
&lt;br /&gt;
$$T = 2\pi d \sqrt{\frac{d}{GM}}$$&lt;br /&gt;
&lt;br /&gt;
利用开普勒第二定律计算碰撞时间：&lt;br /&gt;
&lt;br /&gt;
$$\Delta t = \left( \frac{\pi}{2} - 1 \right) d \sqrt{\frac{d}{GM}}$$&lt;br /&gt;
&lt;br /&gt;
(b) 当小行星初始背离恒星运动时，需遍历轨道面积II和III后返回：&lt;br /&gt;
&lt;br /&gt;
$$\Delta t = \frac{\pi}{2} d \sqrt{\frac{d}{GM}}$$&lt;br /&gt;
&lt;br /&gt;
[[分类:天体力学]]&lt;br /&gt;
[[分类:由ai生成]]&lt;/div&gt;</summary>
		<author><name>Quan787</name></author>
		
	</entry>
</feed>