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NASA’s Juno mission has discovered a world of cyclones at Jupiter’s north Jovian pole, a region of cooler stratospheric haze. The cyclones drift to the pole through a process the researchers refer to as “beta drift” via JunoCam and Jovian Infrared Aurora Mapper. The cyclones oscillate around their centres and can drift clockwise around the pole. Juno has also been making recurring flybys of the innermost Jovian moon, Io, revealing evidence of subterranean magma flows below its surface. These cooling flows could explain how Io’s volcanoes erupt, as about 10% of the moon’s subsurface has these flows.

Juno Spots Colliding Jupiter Cyclones and Magma Beneath Io’s Surface

As per the data presented by NASA at the European Geosciences Union General Assembly on April 29, Juno has observed a large central cyclone over 1,800 miles wide, encircled by eight slightly smaller cyclones. These weather systems, blowing at speeds over 100 miles per hour, interact through a phenomenon called beta drifts — similar to Earth’s cyclones but progressing to Jupiter’s pole.

Once enabled, researchers could visualise both visible and thermal activity in Jupiter’s atmosphere. The cyclones stabilise one another and slowly push in the same direction around the pole—in a clockwise direction, as the researchers noted. Jupiter’s cyclones differ from those on Earth since they do not weaken over time at the poles, when the planet has a different atmospheric makeup.

At the same time, exploring Io with Juno has made another discovery: that beneath the surface of the moon lie hidden flows of magma. By pairing infrared and microwave data, scientists picked up warm lava from a large eruption on Dec. 27, 2024. The volcano remained active through Juno’s next flyby in March and is expected to erupt again in May. These discoveries mark the most energetic volcanic eruption ever observed on Io.

The detection of subsurface magma confirms Io’s surface is constantly being renewed. Scientists calculate that 10% of the moon’s interior contains slowly cooling lava. These lava flows help transport heat from Io’s interior to the surface.

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New Analysis of 1977 Wow! Signal Reveals Stronger Cosmic Mystery

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The famous 1977 “Wow!” signal — a mysterious radio burst detected by Ohio’s Big Ear telescope — has been reanalyzed using modern computing techniques. Researchers digitized old telescope records, finding the signal was about four times stronger than first thought, peaking at 250 Janskys. The recalculations also refined its frequency and sky location, ruling …

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Astronomers Capture Sharpest-Ever Solar Flare Images with NSF’s DKIST Telescope

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Astronomers have achieved a major breakthrough by capturing the sharpest images of a solar flare ever recorded, using the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST). Observed at the hydrogen-alpha wavelength during the decay of an X1.3-class solar flare, the images unveiled hundreds of ultra-fine coronal loops averaging just 48 kilometers…

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James Webb Detects Carbon Dioxide–Dominated Coma in Interstellar Object 3I/ATLAS

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The James Webb Space Telescope observed 3I/ATLAS, the third interstellar object detected in our solar system. Its coma is unusually rich in carbon dioxide with little water or carbon monoxide, suggesting a CO₂-rich core or an insulating crust. Findings raise new questions about its cosmic origin.

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