The Juno probe's recent discoveries are impressive, including cyclones on Jupiter and a moon with flowing magma
NASA's Juno mission unveils Jupiter's cyclones and Io's active volcanism.

NASA's Juno mission, which arrived at the Jupiter system in 2016, has been providing unprecedented insights into the largest planet in our solar system and its moons. A recent highlight from Juno's discoveries includes the observation of a cap of stratospheric haze at Jupiter's north pole, which is cooler by 52 degrees Fahrenheit than its surroundings. Moreover, the pole hosts a large cyclone approximately 1,864 miles in diameter, surrounded by eight smaller cyclones ranging between 1,490 and 1,790 miles each, creating a turbulent atmospheric dance.
These cyclones aren't stationary; they engage in what's known as 'beta drift,' a process related to the Coriolis effect that influences their movement and interaction. On Earth, cyclones typically lose strength as they approach the poles due to the lack of warm, moist air. However, Jupiter's unique atmospheric conditions allow these cyclones to persist and even 'bounce' off each other, as explained by Yohai Kaspi from the Weizmann Institute of Science, likening the motion to springs in a mechanical system, thus creating stability in their configuration.
Io, one of Jupiter's moons, known for its volcanic activity, has also been a part of Juno's remarkable findings. During a flyby on December 27, 2024, Juno recorded the most energetic volcanic eruption observed on Io. The spectacle continued until a subsequent observation on March 2, 2025, with the eruption expected to persist into Juno's next flyby on May 6, 2025, where the spacecraft will approach as close as 55,300 miles from Io’s surface.
Through the combination of Juno's Microwave Radiometer (MWR) and the Jovian Infrared Aurora Mapper (JIRAM), researchers have become particularly excited about the presence of molten magma flows beneath Io's surface. This discovery provides vital clues about the moon's geothermal dynamics, indicating that about 10% of Io's subsurface is composed of these cooling flows, effectively acting like a car radiator to dissipate heat into space, as explained by Shannon Brown of NASA’s Jet Propulsion Laboratory.
NASA's findings from the Juno mission were recently presented at the European Geosciences Union's General Assembly, offering the scientific community crucial data on Jupiter’s atmospheric phenomena and Io's volcanic activities. These observations help bridge knowledge gaps about the intricate processes on Jupiter and its moons, promising further exploration and understanding of our planetary neighbors.
Sources: Space.com, NASA, European Geosciences Union, Weizmann Institute of Science