mollwollfumble said:
CrazyNeutrino said:
“The textbooks all say that rings are small, located close to their planet.”
Looking up a good textbook now, De Pater & Lissauer (2001). It says that even back in 1995, Saturn’s E ring was known to be quite large, extending out to 8 Saturn radii. ie. extending further out from Saturn than the orbits of the moons Mimas, Enceladus, Tethys and Dione. The inner (A to F) rings have radial extent from 1.09 to 2.32 Saturn radii. The other outer ring, the G ring, has radial location 2.75 to 2.85 Saturn radii.
The E ring was observed by the Keck Telescope in August 1995, but its full extent wasn’t seen until a few months later in November when the Hubble Telescope took a good look. 1995 was a good year because in that year Saturn’s rings were seen edge on, making the more diffuse and distant rings easier to spot.
But that’s a long way short of 300 Saturn radii for the Phoebe ring. It’s not at all unusual for Moons to interact with rings, such as supplying particles, but this is really extreme.
> Iapetus is a moon that’s unlike anything else in the solar system, it’s black on one side and white on the other due to this Phoebe ring
That makes perfect sense. Iapetus is a lot further out than Dione, and the two-tone colour is definitely consistent with interaction with dust in a ring.
> Wise satellite
This small satellite has led to a whole heap of new discoveries. It was tuned to detect the radiation from asteroids and hotter objects. The rings of Saturn are considerably cooler than that, but would still be within the detection temperature range. Note that dithering was used by the WISE satellite to deliberately and artificially enlarge the size of small objects, so it wasn’t initially obvious that the dithering of Saturn wouldn’t swamp the picture taken of the rings.