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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🌎 Astronomers have recorded powerful radio signals from space known as pulsars. These are rapidly spinning neutron stars emitting beams of electromagnetic radiation, pulsing at regular intervals. The first pulsar was discovered in 1967, and some spin hundreds of times per second. ✨
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🪐 The ultra-dense pulsar PSR B1257+12, located in the constellation Virgo about 2,300 light-years from Earth, hosts the first confirmed exoplanets ever discovered. These three worlds—each orbiting this spinning neutron star—endure intense radiation, making them some of the most hostile planets in the known galaxy. ✨
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🪐 Deep in the heart of galaxy 4C +37.11, astronomers have found a pair of supermassive black holes separated by just 24 light-years, each powering its own quasar—an extremely bright object fueled by matter falling into a black hole. Quasars outshine entire galaxies, and the unique twin system in 4C +37.11 gives scientists a rare look at how two powerful quasars can exist side by side, lighting up their galaxy with intense energy streams. ✨
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🪐 In July 2023, the NANOGrav collaboration announced the detection of a subtle, continuous "hum" of gravitational waves rippling through the Milky Way, likely created by pairs of supermassive black holes orbiting each other in distant galaxies. Gravitational waves are tiny ripples in space itself, first predicted by Einstein, and their detection with pulsar timing arrays—using rapidly spinning stars that act as cosmic clocks—opens a new era for exploring invisible giants and the history of galaxy mergers across the universe. ✨
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🪐 In 2023, scientists using pulsars—ultra-dense, spinning stars that emit radio pulses like cosmic clocks—detected a faint background hum of gravitational waves rippling through our galaxy. These gravitational waves, created by supermassive black holes merging in distant galaxies, gently stretch and squeeze the fabric of space, opening an entirely new window into the universe’s most titanic collisions. ✨
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🪐 In the nearby galaxy Messier 82, astronomers have detected a pulsar that produces incredibly bright X-ray flashes, making it one of the brightest known X-ray pulsars in the universe. Unlike most pulsars, which are remnants of massive exploded stars spinning rapidly and emitting beams of energy, this X-ray pulsar (named M82 X-2) pulls in material from a companion star, causing it to outshine even many black holes in its intense brilliance. ✨
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🪐 The quasar TON 618, found more than 10 billion light-years away in the constellation Canes Venatici, hosts one of the largest known black holes with a mass over 60 billion times that of our Sun. Quasars are incredibly bright objects powered by material falling into supermassive black holes, while pulsars—like the famous Vela Pulsar in our galaxy—are ultra-dense, spinning neutron stars that send out regular beams of radio waves, acting like cosmic lighthouses for astronomers. ✨
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🪐 In 1967, astronomers discovered the first pulsar, now known as PSR B1919+21, a rapidly spinning neutron star that sends out regular radio pulses like a cosmic lighthouse. Unlike pulsars, quasars such as 3C 273 are the blazing hearts of distant galaxies, powered by supermassive black holes devouring matter and shining brighter than whole galaxies—making both objects among the most extreme and mysterious beacons in the universe. ✨
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🪐 Deep inside the galaxy 3C 273, astronomers have identified a quasar—a super-bright region powered by a supermassive black hole eating up material, causing it to shine with light brighter than entire galaxies. Meanwhile, the Crab Pulsar in the Crab Nebula is a rapidly spinning neutron star left over from a massive star’s explosion, sending out beams of radio waves and light as it spins—a cosmic lighthouse flashing 30 times a second. ✨
#quasars⚡#pulsars⚡#supernova⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The pulsar PSR J0537−6910, spinning an incredible 62 times per second, sits in the Tarantula Nebula of the Large Magellanic Cloud and holds the record for the fastest known "glitches." Glitches are sudden jumps in a pulsar’s rotation speed—caused by internal adjustments in these ultra-dense, spinning neutron stars—and PSR J0537−6910’s frequent glitches help scientists unlock secrets about the strange matter inside these cosmic lighthouses. ✨
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🪐 Deep in the constellation Virgo, the double pulsar system PSR J0737−3039A/B is made of two neutron stars—tiny, ultra-dense remnants of massive stars—that both emit regular radio pulses as they orbit each other every 2.4 hours. This unique cosmic pair lets scientists observe the effects of extreme gravity, as one pulsar passes through the other’s powerful wind and their orbit slowly shrinks—confirming predictions from Einstein's theory of general relativity in an environment unlike anywhere else in the universe. ✨
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🪐 Deep in the constellation Draco lies the pulsar PSR J2222−0137, a unique spinning neutron star about 900 light-years from Earth that forms a binary system with a faint white dwarf. PSR J2222−0137 spins once every 33 milliseconds, and its partner is one of the coolest known white dwarfs, so cold that its surface may be made of crystallized oxygen—offering a rare glimpse of two extreme stellar remnants circling each other in quiet cosmic partnership. ✨
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