静态网站悖论
个人网站的两种不同实现方式:一种是复杂的内容管理系统(CMS),另一种是简单的静态 HTML 文件。文章指出,尽管大多数普通用户倾向于使用复杂的解决方案(如 WordPress),但实际上,只有少数专业软件工程师能够选择更简单的静态网站。
via HackerNews 2024 10 09
前两天刚好听朋友说 square space 已经涨到了近乎搞笑的 $25 月费,做不用来盈利的个人博客实在难以 justify。这篇文章中吐槽得很在点子上:
normal users are stuck with a bunch of greedy clowns that make them pay for every little thing, all while wasting ungodly amounts of computational power to render what could have been a static website in 99% of cases.
普通用户被困在了一群屁大点功能都要收费的贪婪小丑手里,与此同时浪费着人神共愤额度的算力来渲染 99% 的情况下都可以作为静态的网站。
当然原文中说的“只有少数专业软件工程师才能选择更简单的静态网站”略微夸张并不认同,因为静态站至少是比 self-host 的动态 CMS 少太多维护了。我的 backlog 里也一直躺了篇安利新手用静态站并拉踩 WP 的文,不过网上这种文已经有无数了也还是拦不住前赴后继往各种 CMS 的坑里冲的新手,觉得写了又有什么意义呢就还搁着没写。(当然迟早会像以前反复造的无数轮子一样被废话欲战胜的 but not today)
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🌎 Lurking in deep space, “dark matter” makes up about 27% of the universe, yet it remains invisible. Scientists infer its existence by observing gravity’s effects—like stars swirling faster than visible matter alone predicts. Its true nature is still unknown, but it outweighs all regular matter combined. ✨
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🌎 Mysterious dark matter makes up about 27% of the universe, but it does not emit or absorb light, making it invisible. Scientists detect dark matter only through its gravitational effects on galaxies and galaxy clusters. The leading candidates for dark matter particles are called WIMPs—Weakly Interacting Massive Particles. ✨
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🌎 Gamma-ray bursts are the most energetic explosions in the universe, releasing in seconds as much energy as the Sun emits over its entire 10-billion-year lifespan. They are detected by satellites as brief flashes of gamma radiation, and are thought to result from collapsing massive stars or merging neutron stars. ✨
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🪐 In the spiral galaxy NGC 4993, scientists observed a gamma-ray burst, GRB 170817A, that arrived just 1.7 seconds after gravitational waves from the merger of two neutron stars—ultra-dense stellar remnants. This remarkable event marked the first time both gravitational waves and a gamma-ray burst were detected from the same source, giving astronomers an unprecedented, multi-messenger view of a cosmic collision. ✨
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🪐 In 2022, the Event Horizon Telescope captured the first radio image of the supermassive black hole at the center of our galaxy, Sagittarius A*, revealing a glowing ring of hot gas swirling around the event horizon—the point beyond which nothing can escape. This image confirmed decades of theory about black holes and showed that matter falling in forms a bright, lopsided halo just outside the black hole’s shadow, unlocking new clues about how these cosmic giants really behave. ✨
#blackholes⚡#SagittariusA⚡#astrophysics⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The star HE 0107-5240, found in the constellation Phoenix, is one of the most metal-poor stars ever discovered, meaning it contains almost no elements heavier than hydrogen and helium. This rare "primordial" star likely formed from the material left over after the very first stars died, making it an ancient relic that helps scientists study the universe's earliest generations of stars. ✨
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🪐 The spiral galaxy Messier 83 has hosted more recorded gamma-ray bursts than almost any spiral galaxy nearby, becoming a hotspot for these mysterious explosions. Gamma-ray bursts are split-second flashes of the universe’s most energetic light, and their frequent appearance in Messier 83 helps scientists study how massive stars can end their lives in extreme, spectacular fashion. ✨
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🪐 The pulsar PSR J0437−4715, located about 500 light-years away in the constellation Pictor, spins nearly 174 times per second and is famous for its near-perfect "cosmic clock" precision. This ultra-stable pulsar allows astronomers to test the fundamental laws of physics and even hunt for elusive gravitational waves by tracking the tiny variations in its radio pulses over many years. ✨
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What If The Universe DID NOT Start With The Big Bang?
@PBS Space Time
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