Photo Credit: Pixabay/TBIT 2r55l
The findings suggest these dark ovals are formed by swirling magnetic tornadoes
Magnetic vortices descending from NASA's Cassini spacecraft in 2000.
The study, published in the Nature journal, was led by Troy Tsubota, an undergraduate researcher at the University of California, Berkeley, in collaboration with Michael Wong from UC Berkeley, Amy Simon of NASA's Goddard Space Flight Center, and others.
The findings suggest these dark ovals are formed by swirling magnetic tornadoes generated due to friction between Jupiter's immense magnetic field lines and those in its ionosphere. These tornadoes are thought to stir aerosols, creating dense patches of UV-absorbing haze in the stratosphere.
The study highlights that Jupiter's magnetic field, among the strongest in the solar system, interacts with the Io Plasma Torus — a ring of charged particles released by volcanic activity on Jupiter's moon Io. This interaction generates friction, potentially initiating magnetic vortices that descend into the planet's atmosphere.
The exact mechanism remains unclear, with researchers debating whether these tornadoes dredge up material from deeper atmospheric layers or create the hazes independently.
The Outer Planet Atmospheres Legacy (OPAL) project, which captures annual images of Jupiter using the Hubble Space Telescope, played a pivotal role in the discovery. Between 2015 and 2022, dark ovals were observed at the south pole in 75% of images but were significantly rarer at the north pole. These formations typically appear over a month and dissipate within two weeks, resembling a magnetic “tornado alley.”
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