Jun Liu

In 2019, astronomers unveiled the first-ever image of a black hole's shadow — a dark void encircled by a lopsided orange ring. This is the supermassive black hole at the heart of galaxy M87, 55 million light-years away. The ring isn't just glowing: one side is noticeably brighter than the other, like a campfire burning unevenly, with flames leaping higher on one side.

Radio telescopes scattered across the globe pick up waves from distant black holes. But two telescopes placed almost side by side see only a blurry blob — fine details are beyond them. Usually, such pairs are considered useless and discarded. But that's a mistake: even a blurry blob holds clues.

A flexible screen as thin as a human hair is glass you can bend. But this marvel has a quirk: touch it, and an invisible electric charge lingers on the surface. Like dust on polished furniture, it builds up and interferes with operation.

A factory smokestack releases carbon dioxide into the air, and nearby stands a unit that captures this gas and, under sunlight, assembles ethylene molecules from it — the feedstock for plastic bags and pipes. Materials scientists have brought this scenario closer by modifying a crystal of the semimetal PdSn4 with a small amount of platinum.

At the center of the Milky Way lies the supermassive black hole Sagittarius A*. It is four million times more massive than the Sun, but by cosmic standards it behaves quietly: it only occasionally flares up when it swallows a clump of gas.

Fall 1956. Kurt Gödel puts pen to paper, drafting a question for the dying John von Neumann: Can the satisfiability of a Boolean formula be checked faster than brute-force trial and error? The answer comes 69 years later, and it turns out to be the bite of the logical ouroboros, the mythical serpent that devours its own tail. The serpent is born from randomness.

In April 2021, the antennas of the Event Horizon Telescope (EHT)—a global network of millimeter-wave radio telescopes — zeroed in on a tiny spot in the constellation Virgo.