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The rings of Uranus are thought to be relatively young, at not more than 600 million years old.
All except two rings of Uranus are extremely narrow - they are usually a few kilometres wide.
Puck's orbit is located between the rings of Uranus and Miranda.
All rings of Uranus show azimuthal brightness variations.
These symmetric dips bear some similarity to the way by which the Rings of Uranus were found in 1977.
Cordelia acts as the inner shepherd satellite for Uranus' rings of Uranus.
James L. Elliot, 67, American astronomer, discovered rings of Uranus.
In addition, dust bands observed between the main rings of Uranus may be similar to the rings of Jupiter.
Since the rings of Uranus appear to be young, they must be continuously renewed by the collisional fragmentation of larger bodies.
From a vantage point in the Uranus system, the spacecraft examined a bright star winking on and off as the rings of Uranus passed by.
Narrow ringlets existing in the broad Saturnian rings also resemble the narrow rings of Uranus.
There is some debate on whether Elliot, et al. discovered the rings of Uranus, or whether William Herschel made an observation in 1797.
All inner moons are intimately connected to the rings of Uranus, which probably resulted from the fragmentation of one or several small inner moons.
The link between gelignite (invented by Alfred Nobel), saccharin, and the rings of Uranus is that they were all serendipitous discoveries.
The rings of Uranus are planetary rings (circles of rock and dust) that go around the planet Uranus.
March 10 - Rings of Uranus discovered by Kuiper Airborne Observatory measurements of star occultation.
The rings of Neptune are made of extremely dark material, likely organic compounds processed by radiation, similar to that found in the rings of Uranus.
In this respect the rings of Neptune are similar to faint dusty bands observed by Voyager 2 between the main rings of Uranus.
The newly discovered outer rings of Uranus are similar to the outer G and E rings of Saturn.
The first reliable detection of a ring was made in 1968 by stellar occultation, although that result would go unnoticed until 1977 when the rings of Uranus were discovered.
(Sofia's airborne predecessor, the Kuiper Airborne Observatory, discovered the rings of Uranus in a similar way 35 years ago.)
Tremaine, along with Peter Goldreich, correctly predicted that shepherd moons created Saturn's thin F ring, as well as the thin rings of Uranus in 1979.
The KAO made several major discoveries, including the first sightings of the rings of Uranus in 1977 and a definitive identification of an atmosphere on Pluto in 1988.
If they exist in the simulated form, the researchers believe that the crystal organisms could be found in the rings of Uranus and Saturn, which are made up of small grains of ice.
The outer rings of Uranus may be similar to the G and E rings of Saturn as E ring is extremely broad and receives dust from Enceladus.