Apple trains its own AI model for China market with Alibaba’s support – sources

Imagine living on a world where the start of the day and the end of the day aren’t just different times, but entirely different environments. On one horizon, morning arrives in a chilly mist where vaporized rocks might condense into glittering, mineral clouds. On the opposite horizon, evening sets in as a roaring, hyper-heated furnace hot enough to shred water molecules into raw hydrogen and oxygen. This isn’t sci-fi world-building, it is the reality of WASP-121 b, an extreme exoplanet located roughly 850 light-years from Earth. Astronomers analyzing data from NASA’s James Webb Space Telescope (JWST) have uncovered unprecedented details about this distant world, proving for the first time that its morning and evening twilight zones are fundamentally different from one another. A World Locked in Perpetual Extremes WASP-121 b belongs to a class of cosmic objects known as hot Jupiters: giant gas planets that orbit extraordinarily close to their parent stars. Because of this extreme proximity, the planet is tidally locked. Just as the Moon always presents the same face to Earth, WASP-121 b always presents the exact same hemisphere to its star. One side endures an unrelenting, eternal day with scorching temperatures topping 2,500 degrees Celsius (4,500 degrees Fahrenheit). The opposite side faces permanent night, staring into cold space. For years, astrophysicists hypothesized that the narrow transition zones between day and night. The planet’s terminators might harbor complex, asymmetrical weather patterns. However, confirming this required measuring subtle variations in starlight as the planet passed in front of its star. How Jet Streams Reshape Alien Skies Using JWST’s Near-Infrared Spectrograph (NIRSpec), researchers tracked how starlight filtered through different parts of WASP-121 b’s atmosphere. The findings revealed a dramatic contrast between the morning transition and the evening transition. The driver behind this strange weather is a planetary-scale jet stream. Superheated air on the dayside doesn’t stay still; it rushes toward the cooler nightside at extreme speeds. Because the planet rotates toward the east, these violent winds carry thermal energy around the globe and dump the bulk of that heat directly into the evening region. As a result, WASP-121 b’s evening atmosphere grows significantly hotter than its morning counterpart. Heat causes gases to expand, puffing up the evening sky like a inflated balloon. When starlight filters through this swollen atmospheric layer, it reveals an environment so fierce that water molecules cannot survive intact. Clouds of Metal and Torn Molecules In the searing furnace of the evening sky, chemical bonds break. Water vapor brought in from the dayside is torn apart by the heat, leaving behind a sky depleted of chemical stability. As those same winds continue their journey around the cold nightside, the atmosphere gradually cools down. By the time the air sweeps around to form the morning twilight, the story flips. Here, temperatures drop enough for chemical compounds to reassemble. Scientists suspect that in this cooler morning zone, minerals such as silicates condense out of the gas phase. Instead of water clouds like those on Earth, WASP-121 b’s morning sky likely features reflective clouds made of liquid rock or iron droplets. These metallic clouds block radiation from deeper layers, making the morning side appear even cooler to space observatories. A New Era of Exoplanet Meteorology Until recently, studying alien worlds meant treating entire planets as single, uniform points of light. This discovery demonstrates that modern space telescopes can resolve climate dynamics across distinct regions of a world hundreds of light-years away.   By capturing the contrast between a planet’s morning and evening, astronomers are moving from simply discovering exoplanets to mapping their active weather systems. WASP-121 b may be far too hostile for life as we know it, but understanding its violent atmospheric currents brings us one step closer to reading the skies of smaller, cooler, and potentially habitable worlds in the future.