Saturn’s rings do more than just look pretty. New data from the Cassini-Huygens spacecraft orbiting the planet shows their shadow can actually change the planet’s atmosphere.
Illustration: NASA/JPL-Caltech
The new research from scientists in Sweden and the United States demonstrates a clear difference between the particles in the Northern and Southern parts of the planet’s ionosphere, its electrically charged upper layer. But the star of the paper is Cassini. The probe is continuing to deliver, even three months after plummeting into the planet.
[referenced url=”https://gizmodo.com.au/2017/09/cassini-is-gone-and-im-not-crying-youre-crying/” thumb=”https://i.kinja-img.com/gawker-media/image/upload/t_ku-large/copel51tsyniilk9qzqa.jpg” title=”Cassini Is Gone And I’m Not Crying You’re Crying” excerpt=”After a 20-year sojourn in the final frontier, at approximately 10.00PM AEST tonight, NASA’s Jet Propulsion laboratory lost contact with the Cassini spacecraft, which had plunged into Saturn’s atmosphere about an hour and a half prior, ending its 13-year exploration of the Saturn system.”]
“One can imagine this as the grand finale phase of the Cassini mission as an entirely new mission with the veteran spacecraft,” William Kurth, a scientist at the University of Iowa’s Department of Physics and Astronomy, told Gizmodo. “There was never any plan to go this close to Saturn… we’re just getting our feet wet with the fresh data that we have.”
Scientists define the “surface” of Saturn, a gas giant, as the place where its pressure equals one bar – a little less than the average pressure at sea level, 60,268km from its centre. The ionosphere begins around 300km up and goes way out to 5000km up. Earth’s ionosphere goes from 60km to 1000km up and its radius is around 6400km, for comparison. This region is populated by particles that have been ionised, or have become charged by losing electrons thanks to the Sun’s radiation.
Cassini entered Saturn’s ionosphere on April 27 of this year and began orbiting, during which scientists were able to collect data with its Radio and Plasma Wave Science (RPWS) instrument package. Aside from measuring the density of electrons and ionised particles, it found that the A and B rings were causing noticeable dips in the amount of ionisation in the Southern portion of the ionosphere. The scientists published the results today in the journal Science and discussed them today at the American Geophysical Union’s Fall meeting in New Orleans.
These results are important for the way they can help explain how particles move around the planet and its atmosphere – information we could perhaps extrapolate to other gas giants.
You can bet there’s a whole lot more data that the scientists need to analyse to fully understand the planet’s atmosphere. Kurth cautioned that these results relied on only one of the probe’s instruments and the first 11 of many orbits, nor do the results use data from the probe’s final plunge.
This data is the capstone of many years of important science from the mission, said Kurth.
“It’s just terrific,” he said. “It’s sad that the spacecraft is no longer with us, but it’s left such a legacy in terms of observation not just for the last six months but the entire 13 years.”
[Science]