A veteran astronomer has found that Saturn’s huge ring system is warming the planet’s higher environment, a phenomenon by no means earlier than noticed in our photo voltaic system. By analyzing 40 years of ultraviolet information from a number of area missions, together with NASA’s Hubble Area Telescope, the Cassini spacecraft, Voyager 1 and a couple of, and the Worldwide Ultraviolet Explorer, the researcher discovered that particles from icy rings are raining down on the environment of Saturn, inflicting warming. This groundbreaking discovery not solely highlights an sudden interplay between the planet and its rings, but additionally opens up the opportunity of utilizing this data to foretell the existence of Saturn-like ring programs round exoplanets.
A bathe of icy particles is affecting the local weather of the large planets
The planet
” data-gt-translate-attributes=”[{” attribute=””>Saturn is easily recognizable for its opulent ring system that can easily be seen through a small telescope. Astronomers have now found that the rings are not as placid as they look. The icy rings particles are raining down onto Saturns atmosphere. This is heating the upper atmosphere. It took a collection of 40 years worth of Saturn observations, gleaned from four 
Hubbles look at Saturn on September 12, 2021, shows rapid and extreme color changes of the bands in the planets northern hemisphere, where it was early autumn. The bands have varied throughout Hubble observations in both 2019 and 2020. Notably, Saturns iconic hexagonal storm, first discovered in 1981 by the Voyager 2 spacecraft, was difficult to distinguish in 2020, but it is again clearly evident in 2021. Hubbles Saturn image catches the planet following the southern hemispheres winter, evident in the lingering blue-ish hue of the south pole.Credit: NASA, ESA, A. Simon (NASA-GSFC), and M. H. Wong (UC Berkeley); Image Processing: A. Pagan (STScI)
Hubble Space Telescope Finds Saturns Rings Heating Its Atmosphere
The secret has been hiding in plain view for 40 years. But it took the insight of a veteran astronomer to pull it all together within a year, using observations of Saturn from NASAs Hubble Space Telescope and retired Cassini probe, in addition to the Voyager 1 and 2 spacecraft and the retired International Ultraviolet Explorer mission.
The discovery: Saturns vast ring system is heating the giant planets upper atmosphere. The phenomenon has never before been seen in the solar system. Its an unexpected interaction between Saturn and its rings that potentially could provide a tool for predicting if planets around other stars have glorious Saturn-like ring systems, too.
The telltale evidence is an excess of ultraviolet radiation, seen as a spectral line of hot hydrogen in Saturns atmosphere. The bump in radiation means that something is contaminating and heating the upper atmosphere from the outside.
The most feasible explanation is that icy ring particles raining down onto Saturns atmosphere cause this heating. This could be due to the impact of micrometeorites, solar wind particle bombardment, solar ultraviolet radiation, or electromagnetic forces picking up electrically charged dust. All this happens under the influence of Saturns gravitational field pulling particles into the planet. When NASAs 
This is a composite image showing the Saturn Lyman-alpha bulge, an emission from hydrogen which is a persistent and unexpected excess detected by three distinct NASA missions, namely Voyager 1, Cassini, and the Hubble Space Telescope between 1980 and 2017. A Hubble near-ultraviolet image, obtained in 2017 during the Saturn summer in the northern hemisphere, is used as a reference to sketch the Lyman-alpha emission of the planet. The rings appear much darker than the planets body because they reflect much less ultraviolet sunlight. Above the rings and the dark equatorial region, the Lyman-alpha bulge appears as an extended (30 degree) latitudinal band that is 30 percent brighter than the surrounding regions. A small fraction of the southern hemisphere appears between the rings and the equatorial region, but it is dimmer than the northern hemisphere. North of the bulge region (upper-right portion of image), the disk brightness declines gradually versus latitude toward the bright aurora region that is here shown for reference (not at scale). A dark spot inside the aurora region represents the footprint of the spin axis of the planet.
Its believed that icy rings particles raining on the atmosphere at specific latitudes and seasonal effects cause an atmospheric heating that makes the upper atmosphere hydrogen reflect more Lyman-alpha sunlight in the bulge region. This unexpected interaction between the rings and the upper atmosphere is now investigated in depth to define new diagnostic tools for estimating if distant exoplanets have extended Saturn-like ring systems.
Credit: NASA, ESA, Lotfi Ben-Jaffel (IAP & LPL)
