Magnetic vortices descending from Jupiter’s ionosphere into its deep environment are believed to set off the formation of ultraviolet-absorbing anticyclonic storms, in keeping with a examine printed on November 26 in Nature Astronomy. These storms, showing as darkish ovals, span the dimensions of Earth and have been noticed primarily in Jupiter’s polar areas. The phenomenon was first detected in ultraviolet (UV) gentle by the Hubble House Telescope within the Nineteen Nineties and later confirmed by NASA’s Cassini spacecraft in 2000.
Analysis Unveils Twister Dynamics
The examine, printed within the Nature journal, was led by Troy Tsubota, an undergraduate researcher on the College of California, Berkeley, in collaboration with Michael Wong from UC Berkeley, Amy Simon of NASA’s Goddard House Flight Middle, and others.
The findings counsel these darkish ovals are fashioned by swirling magnetic tornadoes generated as a consequence of friction between Jupiter’s immense magnetic subject strains and people in its ionosphere. These tornadoes are thought to stir aerosols, creating dense patches of UV-absorbing haze within the stratosphere.
The Position of the Io Plasma Torus
The examine highlights that Jupiter’s magnetic subject, among the many strongest within the photo voltaic system, interacts with the Io Plasma Torus — a hoop of charged particles launched by volcanic exercise on Jupiter’s moon Io. This interplay generates friction, probably initiating magnetic vortices that descend into the planet’s environment.
The precise mechanism stays unclear, with researchers debating whether or not these tornadoes dredge up materials from deeper atmospheric layers or create the hazes independently.
Common Observations Affirm Patterns
The Outer Planet Atmospheres Legacy (OPAL) mission, which captures annual photographs of Jupiter utilizing the Hubble House Telescope, performed a pivotal function within the discovery. Between 2015 and 2022, darkish ovals have been noticed on the south pole in 75% of photographs however have been considerably rarer on the north pole. These formations sometimes seem over a month and dissipate inside two weeks, resembling a magnetic “twister alley.”
