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Inside Jupiter's Chaotic Storm Maze! 🚀🪐
Nature's ultimate canvas, painted with supersonic winds and toxic ammonia storms. 🚀🌀 This mind-blowing close-up view captures the chaotic northern hemisphere of Jupiter, sent back by NASA’s Juno spacecraft during its 61st close flyby on May 12, 2024.
The Physics of Jovian Hydrodynamics:
The breathtaking patterns twisting across this image are a masterclass in fluid dynamics on a planetary scale. Because Jupiter is entirely composed of gas without a solid surface to slow things down, winds can rage undisturbed at speeds exceeding 400 km/h (250 mph). The bright, high-altitude white clouds are made of frozen ammonia crystals that have been pushed high into the upper atmosphere by deep thermal convection currents. The darker regions represent deeper, warmer layers of ammonium hydrosulfide gas. When these different chemical layers shear past each other at different velocities, they form turbulent Kelvin-Helmholtz wave patterns, turning the planet's northern atmosphere into a hyper-complex fluid maze that never stays the same from one orbit to the next.
We are staring directly into a beautiful cosmic blender, where raw physics transforms chaotic storms into stunning works of natural art.
✨ Looking at these swirling cosmic currents, does Jupiter's atmosphere remind you more of a stormy ocean on Earth or a living abstract painting?
Let's discuss below! 👇
#universia #Space #Astronomy #NASA #JunoSpacecraft #Jupiter #PlanetaryScience #JunoCam #FluidDynamics #Astrophysics #Cosmos #Universe #Reels
Видео Inside Jupiter's Chaotic Storm Maze! 🚀🪐 канала UNIVERSIA
The Physics of Jovian Hydrodynamics:
The breathtaking patterns twisting across this image are a masterclass in fluid dynamics on a planetary scale. Because Jupiter is entirely composed of gas without a solid surface to slow things down, winds can rage undisturbed at speeds exceeding 400 km/h (250 mph). The bright, high-altitude white clouds are made of frozen ammonia crystals that have been pushed high into the upper atmosphere by deep thermal convection currents. The darker regions represent deeper, warmer layers of ammonium hydrosulfide gas. When these different chemical layers shear past each other at different velocities, they form turbulent Kelvin-Helmholtz wave patterns, turning the planet's northern atmosphere into a hyper-complex fluid maze that never stays the same from one orbit to the next.
We are staring directly into a beautiful cosmic blender, where raw physics transforms chaotic storms into stunning works of natural art.
✨ Looking at these swirling cosmic currents, does Jupiter's atmosphere remind you more of a stormy ocean on Earth or a living abstract painting?
Let's discuss below! 👇
#universia #Space #Astronomy #NASA #JunoSpacecraft #Jupiter #PlanetaryScience #JunoCam #FluidDynamics #Astrophysics #Cosmos #Universe #Reels
Видео Inside Jupiter's Chaotic Storm Maze! 🚀🪐 канала UNIVERSIA
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5 июня 2026 г. 17:00:34
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