Yes. Jupiter has a narrow set of almost unperceivable rings with characteristics that have long speculated astronomers. A new report unveils how shadow and light are at work there, figuring out numerous mysteries right away.
Nowhere close as ocular as the rings of Saturn, which are bright and icy and hold numerous clumps as huge as houses, Jupiter’s rings are largely of dark dust. They were found out in 1979 by Voyager 1. Not before the time the Galileo satellite, revolving around Jupiter from 1995 – 2003, did astronomers discover the rings were made of dust brought up the meteoroids banging into Jupiter’s inner moons.
Still curiosities stayed that didn’t cope with theoretical statements: The rings project outside the orbit of the moon Thebe, and part of the ring structure is leant when compared to the middle ring.
The main ring is around 7,000km wide and bears a precipitous fringe 129,130 km from the middle of the planet. The main ring embraces the orbits of two tiny moons, Metis and Adrastea, which might act as the origin of dust that constitutes most of the ring. The ring requires a stable source of dust since tiny particles can only subsist for 100 to 1000 years. The dust is believed to develop from moons inside the rings due to micrometeorite effects. The primary ring conflates gently into the Halo ring. The Halo is a wide, indistinct tore of particles around 20,000 km dense and reaching out midway from the middle ring down to the planet’s cloudtops.
On the outer boundary of the middle ring and opposite of the halo ring, is the wide and highly wispy Amalthea Gossamer ring. This ring reaches out faraway the orbit of the moon Amalthea. Astronomers suppose that it is made up of dust grains smaller than 10 microns (i.e. around the size of cigarette smoke materials). It reaches out to an outer boundary of around 129,000 km from the center of the planet and inwards to around 30,000 km. The source of the ring is likely from micrometeoroid collision of the small moons revolving inside the ring. At the last is the Thebe Gossamer ring. This is the weakest of the Jovian Rings and stretched out from the orbit of the moon Thebe at around 226,000 km near the planet, stopping at around 129,000 km. The precise inner boundaries of the two gossamer rings are difficult to specify as they intersect the brighter middle ring.
Thus, the answer to “does Jupiter have rings” is yes, it bears four recognized rings. Check out the video to know more: