Magnetosphere of Saturn

The magnetosphere of <a href="/facts/Saturn/D54LcGJ9">Saturn</a> is the cavity created in the flow of the <a href="/facts/Solar_wind/BvuB3dT8">solar wind</a> by the planet's internally generated <a href="/facts/Magnetic_field/Ta8Ev588">magnetic field</a>. Discovered in 1979 by the <a href="/facts/Pioneer_11/9QgrnSWp">Pioneer 11</a> spacecraft, Saturn's <a href="/facts/Magnetosphere/BXzgPoPy">magnetosphere</a> is the second largest of any planet in the Solar System after <a href="/facts/Jupiter/95m7XjMT">Jupiter</a>. The <a href="/facts/Magnetopause/HbXxbHqb">magnetopause</a>, the boundary between Saturn's magnetosphere and the solar wind, is located at a distance of about 20 Saturn radii from the planet's center, while its <a href="/facts/Magnetotail/BXzgPoPy">magnetotail</a> stretches hundreds of Saturn radii behind it.
Saturn's magnetosphere is filled with <a href="/facts/Plasma_(physics)/1d3btMVU">plasmas</a> originating from both the planet and its moons. The main source is the small moon <a href="/facts/Enceladus_(moon)/DyWXz9jl">Enceladus</a>, which ejects as much as 1,000 kg/s of water vapor from the <a href="/facts/Geyser/cjXV4fCP">geysers</a> on its south pole, a portion of which is ionized and forced to co-rotate with the Saturn's magnetic field. This loads the field with as much as 100 kg of water group <a href="/facts/Ion/3bePpDna">ions</a> per second. This plasma gradually moves out from the inner magnetosphere via the <a href="/facts/Interchange_instability/sjVVgbSL">interchange instability</a> mechanism and then escapes through the magnetotail.
The interaction between Saturn's magnetosphere and the solar wind generates bright oval <a href="/facts/Aurora_(astronomy)/6agpj9Qs">aurorae</a> around the planet's poles observed in visible, <a href="/facts/Infrared/44XdJNcc">infrared</a> and <a href="/facts/Ultraviolet/kncBUqn5">ultraviolet</a> light. The aurorae are related to the powerful saturnian kilometric radiation (SKR), which spans the frequency interval between 100 kHz to 1300 <a href="/facts/KHz/6Wshj5qm">kHz</a> and was once thought to modulate with a period equal to the planet's rotation. However, later measurements showed that the periodicity of the SKR's modulation varies by as much as 1%, and so probably does not exactly coincide with Saturn's true rotational period, which as of 2010 remains unknown. Inside the magnetosphere there are radiation belts, which house particles with energy as high as tens of <a href="/facts/Megaelectronvolt/YMT1fqX9">megaelectronvolts</a>. The energetic particles have significant influence on the surfaces of inner icy <a href="/facts/Moons_of_Saturn/HA64rVRw">moons of Saturn</a>.
In 1980–1981 the magnetosphere of Saturn was studied by the <a href="/facts/Voyager_program/cPm6qnNx">Voyager spacecraft</a>. Up until September 2017 it was a subject of ongoing investigation by <a href="/facts/Cassini%25E2%2580%2593Huygens/PWknrDeY">Cassini mission</a>, which arrived in 2004 and spent over 13 years observing the planet.

Magnetosphere of Saturn open-in-new

Magnetosphere of Saturn