Scientists: Saturn’s magnetic field is warped
Using six years of archival data from the Cassini Saturn orbiter, scientists now think Saturn’s magnetic field is lopsided, pulled sideways due to the planet’s very fast rotation as well as the material that surrounds the ringed planet.
The graphic to the right, Figure 4 from the research paper [pdf], compares the Earth’s symmetric magnetic field (top) with that of Saturn’s (bottom). From the press release:
The team found that the cusp was dragged to the right as viewed from the Sun, and was located most often between 1:00 and 3:00 (as it might appear on a clockface), compared to 12:00 as it would be on Earth.
The researchers said this was likely because of Saturn’s extremely fast rotation (a Saturn day is 10.7 hours) and the heavy “soup” of plasma (ionised gas) it pulls around it, a product of gases emitted by Saturn’s moons, especially Enceladus. Together, these are thought to drag the magnetic field lines to the right. But more simulations are needed to confirm this interpretation.
When the solar wind hits the Earth’s magnetic field lines at the cusp, that wind is funneled down along those lines to the poles, where it produces the aurora. This new analysis at Saturn will help scientists better understand the behavior of Saturn’s aurora, which is made even more complex by the planet’s many moons.
Using six years of archival data from the Cassini Saturn orbiter, scientists now think Saturn’s magnetic field is lopsided, pulled sideways due to the planet’s very fast rotation as well as the material that surrounds the ringed planet.
The graphic to the right, Figure 4 from the research paper [pdf], compares the Earth’s symmetric magnetic field (top) with that of Saturn’s (bottom). From the press release:
The team found that the cusp was dragged to the right as viewed from the Sun, and was located most often between 1:00 and 3:00 (as it might appear on a clockface), compared to 12:00 as it would be on Earth.
The researchers said this was likely because of Saturn’s extremely fast rotation (a Saturn day is 10.7 hours) and the heavy “soup” of plasma (ionised gas) it pulls around it, a product of gases emitted by Saturn’s moons, especially Enceladus. Together, these are thought to drag the magnetic field lines to the right. But more simulations are needed to confirm this interpretation.
When the solar wind hits the Earth’s magnetic field lines at the cusp, that wind is funneled down along those lines to the poles, where it produces the aurora. This new analysis at Saturn will help scientists better understand the behavior of Saturn’s aurora, which is made even more complex by the planet’s many moons.












