https://www.astro-init.top/index.php?action=history&feed=atom&title=2015IOAA%E7%90%86%E8%AE%BA%E7%9F%AD%E9%97%AE%E9%A2%98%E7%AC%AC4%E9%A2%98-%E8%A7%82%E6%B5%8B%E9%BB%91%E6%B4%9E2015IOAA理论短问题第4题-观测黑洞 - 版本历史2026-05-04T08:42:15Z本wiki的该页面的版本历史MediaWiki 1.32.2https://www.astro-init.top/index.php?title=2015IOAA%E7%90%86%E8%AE%BA%E7%9F%AD%E9%97%AE%E9%A2%98%E7%AC%AC4%E9%A2%98-%E8%A7%82%E6%B5%8B%E9%BB%91%E6%B4%9E&diff=2170&oldid=prev某九流辣鸡民科：创建页面，内容为“==英文题目== Let us assume that an observer using a hypothetical, far-infrared, Earth-sized telescope (wavelength range 20 to 640 $$\mu m$$) found a static and n…”2022-03-18T12:26:50Z<p>创建页面，内容为“==英文题目== Let us assume that an observer using a hypothetical, far-infrared, Earth-sized telescope (wavelength range 20 to 640 $$\mu m$$) found a static and n…”</p>
<p><b>新页面</b></p><div>==英文题目==<br />
Let us assume that an observer using a hypothetical, far-infrared, Earth-sized telescope (wavelength range 20 to 640 $$\mu m$$) found a static and neutral supermassive black hole with a mass of $$2.1 \times 10^{10} M_{\odot}$$. Determine the maximum distance at which this black hole can be resolved by the observer.</div>某九流辣鸡民科