[{"data":1,"prerenderedAt":-1},["ShallowReactive",2],{"article-detail":3},{"lang":4,"article":5,"alternate":19,"related":24,"latest":33},"en",{"id":6,"slug":7,"title":8,"content":9,"summary":10,"thumbnail":11,"metaDescription":12,"metaKeywords":13,"created":14,"modified":14,"author":15,"authorEn":15,"categoryId":16,"commentCount":17,"thumbnailToContent":18},12758,"icecube-neutrino-ghost-particle-pqmr","IceCube Neutrino Detector: Ghost Particle Hunter | stellarx","\u003Cp style=\"margin:0 0 18px;\">At 11:45 a.m. on October 6, 2026, Stockholm time, the Royal Swedish Academy of Sciences announced the 2026 Nobel Prize in Physics. The winner was Francis Halzen, honored for his decisive contributions to the IceCube Neutrino Observatory and to the discovery of high-energy neutrinos of astrophysical origin.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">\u003Cimg src=\"\u002Fattachment\u002F20261007\u002Fc96cc003cad5429d9929f2fefb35a583.webp\" alt=\"img_01.webp\">\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">The neutrino is a particle so small that it hides the deepest secrets of the entire universe inside itself. What exactly is the IceCube Neutrino Observatory? And why do high-energy neutrinos matter? This is the story of the man who dug ice, moved mountains, and found a Nobel Prize.\u003C\u002Fp>\n\u003Ch2 style=\"color:#111;font-size:21px;line-height:1.4;margin:28px 0 12px;\">\u003Cstrong>A \"Ghost Particle\" That Lived in Predictions\u003C\u002Fstrong>\u003C\u002Fh2>\n\u003Cp style=\"margin:0 0 18px;\">As early as 1930, the physicist Wolfgang Pauli predicted the neutrino's existence. At the time, experiments showed that during beta decay, energy inside atomic nuclei seemed not to be conserved — some beta particles came out with slightly more energy, some with slightly less.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">To explain this, Pauli made a bold assumption: in beta decay, besides electrons, some particles invisible to human observation were also produced, carrying away part of the energy. That was why energy looked non-conserved.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">That particle was the neutrino. We cannot observe it easily because its mass is tiny, it carries no charge, and it almost never interacts with matter — which is why ordinary methods struggle to detect it.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">\u003Cimg src=\"\u002Fattachment\u002F20261007\u002F633c6218175f4e0787bb1f1b1c291127.webp\" alt=\"img_02.webp\">\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">This is also why many people call neutrinos \"ghost particles.\" In fact, neutrinos from the Sun are bombarding Earth at a terrifying density — about 1,000 trillion neutrinos pass through your body every single second, and you never notice a thing.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">It was not until 1956 that the American physicist Frederick Reines and his collaborators first forced this \"ghost\" to reveal itself with an ingenious method. He received the 1995 Nobel Prize in Physics for it. (One aside: Reines's collaborator Clyde Cowan had already passed away before the prize was awarded — so if you want a Nobel, stay alive.)\u003C\u002Fp>\n\u003Ch2 style=\"color:#111;font-size:21px;line-height:1.4;margin:28px 0 12px;\">\u003Cstrong>The Universe's Messengers\u003C\u002Fstrong>\u003C\u002Fh2>\n\u003Cp style=\"margin:0 0 18px;\">So what do neutrinos have to do with the universe? To see the universe clearly, you have to learn to read the information streams arriving from space. Before neutrinos, humanity received cosmic messages through three main channels:\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">The first is visible light — what human ancestors could already see. Look up on any clear day and you see the Sun, the Moon, the stars. But visible light is blocked by interstellar dust; it cannot reach the depths of the universe.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">The second is electromagnetic waves such as gamma rays. These too are absorbed by interstellar matter, and they decay along the way.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">The third is cosmic rays, discovered in 1912. These are essentially streams of high-energy particles. Because they usually carry charge, they are deflected by the magnetic fields of interstellar space during their journey, making their origins impossible to trace.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Once the neutrino's existence was confirmed, physicists immediately fixed their attention on the high-energy neutrino streams of the cosmos. As mentioned, neutrinos carry no charge and barely interact with other matter — their paths are almost completely undisturbed by anything in interstellar space.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">\u003Cimg src=\"\u002Fattachment\u002F20261007\u002F97e27f287def472da2d32d66d6ce1e4b.webp\" alt=\"img_03.webp\" s impression of a high-energy neutrino source_>\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">That means if we can catch a neutrino, we can trace its trajectory back to where it started and \"see through\" the celestial object that produced it. It is like receiving a letter from a distant part of the universe with perfect precision. Capturing high-energy cosmic neutrinos became the dream of every astrophysicist.\u003C\u002Fp>\n\u003Ch2 style=\"color:#111;font-size:21px;line-height:1.4;margin:28px 0 12px;\">\u003Cstrong>The Enticing Blue Light Underwater\u003C\u002Fstrong>\u003C\u002Fh2>\n\u003Cp style=\"margin:0 0 18px;\">Neutrinos are hard to catch, but not completely invisible. When one occasionally interacts with matter, it produces charged particles — for example, electrons, and muons (particles similar to electrons).\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Because cosmic neutrinos are extremely energetic, the charged particles they produce move at incredible speeds. The problem: these particles vanish in an instant. The key to experiment design was catching them before they disappeared.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Scientists hit on a method: Cherenkov radiation. This radiation is a bit like the Mach cone produced when a supersonic aircraft breaks the sound barrier.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">When a plane flies faster than the speed of sound in air, the sound waves get \"pushed along\" by the plane, forming a cone-shaped wavefront behind it.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Similarly, when a charged particle moves faster than the speed of light \u003Ci>in a medium\u003C\u002Fi>, it drags the medium's electromagnetic field along with it, forming a cone-shaped light wavefront behind the particle. That is Cherenkov radiation.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">When we detect this radiation, we can work backward to the direction of the charged particle — and since that particle was produced by a high-speed neutrino collision, its direction points back to where the neutrino came from. A perfect closed loop.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">But wait — physics teachers say the speed of light is the fastest speed in the world. How can anything exceed it?\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Here is the trick: the qualifier is \"the speed of light \u003Ci>in a medium\u003C\u002Fi>.\" Light in a vacuum cannot be beaten, but in water or ice, light slows down dramatically. So a charged particle \u003Ci>can\u003C\u002Fi> exceed the speed of light in that medium, producing Cherenkov radiation.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">\u003Cimg src=\"\u002Fattachment\u002F20261007\u002F941abf4b40d24ede884768658cc9e4c2.webp\" alt=\"img_04.webp\">\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">In other words: put your experiment in water or ice, and you can catch high-energy neutrinos through Cherenkov radiation.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Still, the neutrino is unimaginably small. The probability that one hits an atomic nucleus as it crosses water is extremely low. To give a rough sense: it is like randomly throwing one grain of rice somewhere in the solar system and having it land exactly on another grain of rice.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">To collect enough neutrino interactions and accumulate enough signals, physicists need an enormous volume of detection medium. So they naturally looked to the ocean: place detectors on the seafloor and use the huge mass of seawater itself. Today, experiments like KM3NeT sit deep in the Mediterranean.\u003C\u002Fp>\n\u003Ch2 style=\"color:#111;font-size:21px;line-height:1.4;margin:28px 0 12px;\">\u003Cstrong>A Secret Base Sealed in Polar Ice\u003C\u002Fstrong>\u003C\u002Fh2>\n\u003Cp style=\"margin:0 0 18px;\">Readers may be getting impatient — where is Halzen in all this? Don't worry; heroes appear at the most crucial moment.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Water works, and the ocean offers volume in abundance. But it has obvious drawbacks: ocean currents, radioactive backgrounds, and even fish that glow in the dark!\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Halzen thought of another medium: Antarctic ice.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">To be fair, scientists had considered ice. Ice has several enticing advantages: it is quiet, transparent, free of biological interference, and once formed it barely flows. Antarctica's deep ice lies buried far below the surface, shielding it from surface interference and letting scientists \"listen to the sky\" undisturbed.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">The problem was that lab measurements of ice transparency showed bubbles and impurities scatter light severely, attenuating the Cherenkov signal badly.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Moreover, ice at this scale exists only in Antarctica, and building such a massive project there — even if it could be finished — would be a maintenance nightmare. Scientists once believed that using ice for a neutrino detector was pure paper talk.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">\u003Cimg src=\"\u002Fattachment\u002F20261007\u002F275b2dfa95d44efd9cc8ed17c71a0638.webp\" alt=\"img_05.webp\">\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">You can see this for yourself with an ice machine: water freezes and traps air, so ice cubes are never perfectly transparent.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">But Halzen insisted ice would work. To be fair to the skeptics, even Halzen later admitted: \"If I hadn't been completely ignorant of the optical properties of natural ice, I would have opposed this plan too.\"\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Halzen's most extraordinary quality was not a natural intuition for truth. It was his willingness to stick with his plan — to invest time and energy in testing an apparently absurd idea even when everyone else had written it off.\u003C\u002Fp>\n\u003Cfigure class=\"table\">\n \u003Ctable style=\"border-collapse:collapse;color:#333;font-size:14px;margin:18px 0;max-width:640px;width:100%;\">\n  \u003Ctbody>\n   \u003Ctr>\n    \u003Cth style=\"background-color:#f7f7f7;border:1px solid #ddd;padding:9px 10px;text-align:left;\">IceCube neutrino observatory\u003C\u002Fth>\n    \u003Cth style=\"background-color:#f7f7f7;border:1px solid #ddd;padding:9px 10px;text-align:left;\">Spec\u003C\u002Fth>\n   \u003C\u002Ftr>\n   \u003Ctr>\n    \u003Cth style=\"border:1px solid #ddd;padding:9px 10px;\">Location\u003C\u002Fth>\n    \u003Cth style=\"border:1px solid #ddd;padding:9px 10px;\">South Pole, Antarctica\u003C\u002Fth>\n   \u003C\u002Ftr>\n   \u003Ctr>\n    \u003Cth style=\"border:1px solid #ddd;padding:9px 10px;\">Detector depth\u003C\u002Fth>\n    \u003Cth style=\"border:1px solid #ddd;padding:9px 10px;\">1,450 m down to 2,820 m (bedrock), inside clear ice\u003C\u002Fth>\n   \u003C\u002Ftr>\n   \u003Ctr>\n    \u003Cth style=\"border:1px solid #ddd;padding:9px 10px;\">Optical module\u003C\u002Fth>\n    \u003Cth style=\"border:1px solid #ddd;padding:9px 10px;\">Diameter 35 cm; glass sphere housing sensor and cable\u003C\u002Fth>\n   \u003C\u002Ftr>\n   \u003Ctr>\n    \u003Cth style=\"border:1px solid #ddd;padding:9px 10px;\">Signal chain\u003C\u002Fth>\n    \u003Cth style=\"border:1px solid #ddd;padding:9px 10px;\">Muon neutrino in ice → muon; electron neutrino → electron; both emit Cherenkov light\u003C\u002Fth>\n   \u003C\u002Ftr>\n  \u003C\u002Ftbody>\n \u003C\u002Ftable>\n\u003C\u002Ffigure>\n\u003Cp style=\"margin:0 0 18px;\">Around 1988, Halzen and his collaborators began studying the feasibility of detecting neutrinos in Antarctic ice from a theoretical standpoint. Their calculations settled on a reasonable observatory plan.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">In 1990, the team ran a verification experiment on the Greenland ice sheet. In 1993, they formally began building the Antarctic Muon And Neutrino Detector Array (AMANDA) — the predecessor of IceCube — at the South Pole.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">At first, the team drilled a few hundred meters into the ice and found bubbles everywhere, with scattering so severe that Cherenkov detection was impossible.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">But Halzen did not give up. He pushed the team deeper. Below about 1,500 meters, the air bubbles — crushed by enormous pressure — transformed into clathrate hydrates. Scattering dropped dramatically, and the ice turned clear, almost matching the ideal detection medium in the lab.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">\u003Cimg src=\"\u002Fattachment\u002F20261007\u002Fc16b8bf17af24eaaaa9a4315b138c083.webp\" alt=\"img_06.webp\">\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">After AMANDA succeeded, Halzen began pushing for a much larger observatory: IceCube. This time he was not fighting alone — physicists and engineers from many countries joined, and in 2011, IceCube was completed. Everyone waited in confidence for the messages of these visitors from beyond.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">\u003Cimg src=\"\u002Fattachment\u002F20261007\u002F381cb68f51fc48b8b38226e9ffd5abd5.webp\" alt=\"img_07.webp\">\u003C\u002Fp>\n\u003Ch2 style=\"color:#111;font-size:21px;line-height:1.4;margin:28px 0 12px;\">\u003Cstrong>Achievements and a Closing Word\u003C\u002Fstrong>\u003C\u002Fh2>\n\u003Cp style=\"margin:0 0 18px;\">From its completion onward, IceCube turned neutrinos from a by-product of cosmic-ray theory into a practical probe: locating active galactic nuclei, identifying heavily obscured sources, mapping galactic cosmic rays, and testing the Standard Model.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">For example, on September 22, 2017, IceCube detected a muon neutrino with an energy of about 290 TeV, traced to a flaring blazar. Less than a minute after detection, alerts went out around the globe, triggering follow-up observations by multi-wavelength telescopes.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">\u003Cimg src=\"\u002Fattachment\u002F20261007\u002F3458265195d849ba816d375216afe3ca.webp\" alt=\"img_08.webp\">\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Another example: in 2022, IceCube found multiple high-energy neutrinos from the direction of the galaxy NGC 1068. That galaxy was already known to harbor an active galactic nucleus shrouded in thick gas and dust. Neutrinos are almost unstoppable by such material, so they delivered information that traditional electromagnetic observations could not obtain.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Similar results are too many to count, and some already challenge our understanding of the universe. That is why IceCube is a milestone for cosmology.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">If you have ever frozen ice in a refrigerator, you know the drill: water wraps air bubbles inside, leaving the ice opaque.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Many people before Halzen had tried ice instead of water, but none persisted — they believed the bubbles were insurmountable.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Looking back, that is exactly what Halzen meant by being \"ignorant of the optical properties of natural ice.\" Yet this stubborn man, who walked his own road to the end, found large tracts of pure, transparent ice in the deeper layers. Perhaps that is nature's gift to persistent doers.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Science, sometimes, does not favor the clever. It favors those stubborn enough to take one more step where no one else walks.\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">There is a whole microscopic world around you that is just as invisible as a ghost particle — organisms that live inside bodies and pass by you every day without ever being seen. With WWAI, you can observe them the moment curiosity strikes, including a \u003Cstrong>tapeworm specimen\u003C\u002Fstrong> where flat ribbon-shaped proglottids are clearly visible. Search \"WWAI\" in your app store and download it today.\u003C\u002Fp>\n\u003Cdiv class=\"dp-template-card\" style=\"border-radius:8px;box-shadow:0 2px 8px rgba(0,0,0,0.1);margin:10px 0;max-width:100%;overflow:hidden;width:100%;\">\n \u003Ca style=\"display:block;text-decoration:none;\" href=\"https:\u002F\u002Fyun-hub.chat\u002Flink\u002F?app=wwai&clickid=stellarx&dplink=specimenid%3D1097\" target=\"_blank\">\u003Cimg class=\"image_resized\" style=\"display:block;height:auto;max-width:100%;width:100%;\" src=\"\u002Fattachment\u002F20260824\u002F5ba5dd3c38404fe785f43c44423830de.png\" alt=\"5ba5dd3c38404fe785f43c44423830de\">\n  \u003Cbutton style=\"align-items:center;background-color:#1f983e;border-radius:0 0 25px 25px;border-style:none;color:#ffffff;cursor:pointer;display:flex;font-family:Times New Roman;font-size:19px;height:40px;justify-content:center;padding:0;width:100%;\">EXPLORE NOW\u003C\u002Fbutton>\u003C\u002Fa>\n\u003C\u002Fdiv>\n\u003Ch2 style=\"color:#111;font-size:21px;line-height:1.4;margin:28px 0 12px;\">\u003Cstrong>References\u003C\u002Fstrong>\u003C\u002Fh2>\n\u003Cp style=\"margin:0 0 18px;\">Announcement: The Royal Swedish Academy of Sciences, Nobel Prize in Physics 2026 (6 October 2026, Stockholm).\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 18px;\">Image credits: Nobel Prize official announcement illustration (Niklas Elmehed); IceCube Collaboration; DESY; National Science Foundation (NSF); KM3NeT Collaboration; Wikipedia (educational diagram). All images reproduced from the original source article's figures for educational science communication; locally adapted for this site's science-communication positioning.\u003C\u002Fp>\n\u003Cp style=\"color:#111;margin:28px 0 8px;\">\u003Cstrong>Related reading\u003C\u002Fstrong>\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 20px;\">\u003Ca style=\"color:#111;text-decoration:none;\" href=\"https:\u002F\u002Fstellarx.tech\u002Farticle\u002Ftetanus-bamboo-cut-lockjaw-tqrf\">\u003Cimg class=\"image_resized\" style=\"border-radius:8px;display:block;height:auto;margin-bottom:6px;max-width:520px;width:100%;\" src=\"https:\u002F\u002Fcdn.banyunjuhe.com\u002Fattachment\u002F20261003\u002F0fdf705e766448cb9cb929323ae7e776.webp\" alt=\"Tetanus From a Tiny Wound: No Rust Needed\">\u003C\u002Fa>\u003Cbr>\u003Ca style=\"color:#0b6cb0;text-decoration:none;\" href=\"https:\u002F\u002Fstellarx.tech\u002Farticle\u002Ftetanus-bamboo-cut-lockjaw-tqrf\">\u003Cstrong>Tetanus From a Tiny Wound: No Rust Needed\u003C\u002Fstrong>\u003C\u002Fa>\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 20px;\">\u003Ca style=\"color:#111;text-decoration:none;\" href=\"https:\u002F\u002Fstellarx.tech\u002Farticle\u002Fheartburn-gerd-esophageal-sphincter-vhqw\">\u003Cimg class=\"image_resized\" style=\"border-radius:8px;display:block;height:auto;margin-bottom:6px;max-width:520px;width:100%;\" src=\"https:\u002F\u002Fcdn.banyunjuhe.com\u002Fattachment\u002F20261003\u002F71726b5c88ea4367b428c61ab9fc79c6.webp\" alt=\"Heartburn or GERD: The Valve That Gives Up\">\u003C\u002Fa>\u003Cbr>\u003Ca style=\"color:#0b6cb0;text-decoration:none;\" href=\"https:\u002F\u002Fstellarx.tech\u002Farticle\u002Fheartburn-gerd-esophageal-sphincter-vhqw\">\u003Cstrong>Heartburn or GERD: The Valve That Gives Up\u003C\u002Fstrong>\u003C\u002Fa>\u003C\u002Fp>\n\u003Cp style=\"margin:0 0 20px;\">\u003Ca style=\"color:#111;text-decoration:none;\" href=\"https:\u002F\u002Fstellarx.tech\u002Farticle\u002Ffirefly-bioluminescence-luciferase-hwkc\">\u003Cimg class=\"image_resized\" style=\"border-radius:8px;display:block;height:auto;margin-bottom:6px;max-width:520px;width:100%;\" src=\"https:\u002F\u002Fcdn.banyunjuhe.com\u002Fattachment\u002F20261003\u002F7f75b43809b440dba3202fbb941ff04f.webp\" alt=\"Firefly Glow: A Cold Light Humans Learned to Copy\">\u003C\u002Fa>\u003Cbr>\u003Ca style=\"color:#0b6cb0;text-decoration:none;\" href=\"https:\u002F\u002Fstellarx.tech\u002Farticle\u002Ffirefly-bioluminescence-luciferase-hwkc\">\u003Cstrong>Firefly Glow: A Cold Light Humans Learned to Copy\u003C\u002Fstrong>\u003C\u002Fa>\u003C\u002Fp>","","\u002Fattachment\u002F20261007\u002F301e70c28a3745449f6e0f3b404e02bc.webp","Ghost particles pass through you every second. IceCube, buried in Antarctic ice, catches them by Cherenkov glow and traces them to their cosmic origins.","stellarx, wwai, neutrino, icecube, neutrino detector, cherenkov radiation, ghost particle","2026-10-07 19:53:02","Science Guide Wwai",77,0,false,{"id":20,"slug":21,"title":22,"lang":23},12765,"homochirality-life-mirror-hmls","同手性是什麼？2026 諾貝爾化學獎得主解開生命之謎","zh",{"prev":25,"next":29},{"id":26,"slug":27,"title":28,"categoryId":16},12759,"female-thigh-fat-curves-zwqd","Female Thigh Fat: A Second Sex Characteristic",{"id":30,"slug":31,"title":32,"categoryId":16},12757,"lobster-mushroom-parasitic-fungus-bkmt","Lobster Mushroom: The Fungus That Parasitizes Mushrooms",[34,39,44,49],{"id":35,"slug":36,"title":37,"thumbnail":38,"categoryId":16},12764,"homochirality-nobel-chemistry-hcmr","Homochirality Explained: Nobel Chemistry 2026 | stellarx","\u002Fattachment\u002F20261007\u002Fa7618c12a0c9425fa203d289db1adb65.webp",{"id":40,"slug":41,"title":42,"thumbnail":43,"categoryId":16},12763,"phone-in-bed-eye-strain-pbey","Is Using Your Phone in Bed Bad for Your Eyes?","\u002Fattachment\u002F20261007\u002F5aa7877553a74eddb313da52658c37a3.webp",{"id":45,"slug":46,"title":47,"thumbnail":48,"categoryId":16},12761,"bee-communication-waggle-dance-ptqs","How Do Bees Communicate? Dance and Pheromones","\u002Fattachment\u002F20261007\u002F74400cb78a5f43aaa6b22d1aaab0150c.webp",{"id":50,"slug":51,"title":52,"thumbnail":53,"categoryId":16},12760,"kidney-filtration-reabsorption-ghvf","How Kidneys Work: Filter, Reabsorb, Keep What Matters","\u002Fattachment\u002F20261007\u002F5add4cb5e77d4a06a8a6596d5df7b113.webp"]