Saturn’s rings are so prominent that they can be seen through a small telescope from Earth, but the other gas giant planets, Jupiter, Uranus, and Neptune, have ring systems as well.
Jupiter’s rings were discovered by Voyager 1 in a single image that was targeted specifically to search for a possible ring system. Voyager 2 was reprogrammed en route to take a more complete set of pictures. The image above is from that series. We now known that the system has three major components. The Main ring is about 7,000 km wide and has an abrupt outer boundary roughly 129,000 km from the center of the planet. This ring encompasses the orbits of two small moons, Adrastea and Metis, which probably are the source for the material that makes up most of the ring. The main ring merges gradually into the Halo on the side toward Jupiter. The halo is a broad, faint, donut of material about 20,000 km thick and extending halfway from the main ring down to the planet’s cloudtops.
Around the main ring is the broad and exceedingly faint Gossamer ring. It extends out beyond the orbit of the moon Amalthea and is probably composed of dust particles less than 10 µm in diameter. That’s roughly the size of cigarette smoke particles. It extends to an outer edge of about 129,000 km from the center of the planet and inward to about 30,000 km. The origin of the ring is probably material knocked loose by micrometeorite bombardment of the tiny moons orbiting within the ring.
Jupiter’s rings and moons exist within an intense radiation belt of electrons and ions trapped in the planet’s magnetic field. These particles and fields make up the Jovian magnetosphere or magnetic environment which extends up to 7 million km toward the Sun and stretches outward 750 million km in a windsock shape to Saturn’s orbit.
Image Credit: NASA
I think so, Brain … but lots of toons have a giant red spot for a nose.
Here is NASA’s description of this video: This animation takes the viewer on a simulated flight into, and then out of, Jupiter’s upper atmosphere at the location of the Great Red Spot. It was created by combining an image from the JunoCam imager on NASA’s Juno spacecraft with a computer-generated animation. The perspective begins about 2,000 miles (3,000 kilometers) above the cloud tops of the planet’s southern hemisphere. The bar at far left indicates altitude during the quick descent; a second gauge next to that depicts the dramatic increase in temperature that occurs as the perspective dives deeper down. The clouds turn crimson as the perspective passes through the Great Red Spot. Finally, the view ascends out of the spot.
Video Credit: NASA
This swirling storm on Jupiter spanned about 30,000 km when it was photographed by the Juno spacecraft last July, making it just about as wide as planet Earth. The disturbance rotated counter-clockwise and showed a cloud pattern that includes light-colored updrafts thought to be composed predominantly of ammonia ice. These light clouds were top deck of the system casting discernable shadows toward the right of the picture.
Image Credits: NASA / JPL-Caltech / SwRI / MSSS
Processing: Gerald Eichstädt & Seán Doran
This view of Jupiter’s northern aurora was put together with data taken by Juno‘s Ultraviolet Imaging Spectrograph on 11 December, 2016, as the spacecraft approached Jupiter, passed over its poles, and plunged towards the planet’s equator.
Image Credits: NASA / JPL-Caltech / Bertrand Bonfond