LOS ANGELES - Astronomers aided by the
Hubble Space Telescope have spied two more rings encircling Uranus, the first additions to the planet's ring system in nearly two decades.
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The faint, dusty rings orbit outside of Uranus' previously known rings, but within the orbits of its large moons, said Mark Showalter, an astronomer at the SETI Institute in Mountain View, Calif., who made the discovery.
Details will appear online Friday in the journal Science. The discovery, announced Thursday, means scientists now believe the seventh planet from the sun possesses 13 rings.
In 1986, Voyager 2 became the first spacecraft to zip past Uranus and beam back thousands of images of its dazzling rings and numerous moons. It found two new rings in addition to the nine previously discovered from Earth.
Scientists peering through the Hubble Space Telescope made the latest ring discoveries in 2004. Then they went back to process hundreds of images taken by Voyager and found the rings in the pictures. Scientists speculate that the rings may not have been discovered during the spacecraft flyby because of their faintness.
The newly discovered rings are made up of short-lived, faint bands of dust grains that are constantly being replenished by erosion of larger space bodies. Scientist think the dust in the outermost ring is being supplied by the moon Mab, discovered in 2003.
Scientists also measured changes in the orbits of Uranus' inner moons since 1994. The new measurements suggest the moons are in a "random and chaotic" fashion, said Jack Lissauer of the
NASA Ames Research Center.
Because of the moons' instability, scientists think the satellites will collide with one another in the next few million years.
Uranus, four times the size of Earth, is one of the solar system's giant, gaseous planets that also include Jupiter, Saturn and Neptune.
New rings for Uranus
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Topic authorPlutonianEmpire
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New rings for Uranus
http://news.yahoo.com/s/ap/20051222/ap_ ... anus_rings
Terraformed Pluto: Now with New Horizons maps! :D
Apparently, two more Uranian moons have been discovered as well. Check this out:
NASA's Hubble Discovers New Rings and Moons Around Uranus
12.22.05
(Source: NASA Headquarters/National Imagery and Mapping Agency)
Dec. 22, 2005
Dwayne Brown/George Deutsch
Headquarters, Washington
(202) 358-1726/1324
Ray Villard
Space Telescope Science Institute, Baltimore
(410) 338-4514
RELEASE: 05-590
NASA'S HUBBLE DISCOVERS NEW RINGS AND MOONS AROUND URANUS
NASA's Hubble Space Telescope photographed a new pair of rings around Uranus and two new, small moons orbiting the planet.
The largest ring is twice the diameter of the planet's previously known rings. The rings are so far from the planet, they are being called Uranus' "second ring system." One of the new moons shares its orbit with one of the rings. Analysis of the Hubble data also reveals the orbits of Uranus' family of inner moons have changed significantly over the past decade.
"The detection of these new interacting rings and moons will help us better understand how planetary systems are formed and sustained, which is of key importance to NASA's scientific exploration goals,"
said Dr. Jennifer Wiseman, program scientist for Hubble at NASA Headquarters.
Since dust orbiting Uranus is expected to be depleted by spiraling away, the planet's rings must be continually replenished with fresh material. "The new discoveries demonstrate that Uranus has a youthful and dynamic system of rings and moons," said Mark Showalter of the SETI Institute, Baltimore.
Showalter and Jack Lissauer of NASA's Ames Research Center, Moffet Field, Calif., propose that the outermost ring is replenished by a 12-mile-wide newly discovered moon, named Mab, which they first observed using Hubble in 2003.
Meteoroid impacts continually blast dust off the surface of Mab. The dust then spreads out into a ring around Uranus. Mab's ring receives a fresh infusion of dust from each impact. Nature keeps the ring supplied with new dust while older dust spirals away or bangs back into the moon.
Showalter and Lissauer have measured numerous changes to the orbits of Uranus' inner moons since 1994. The moon's motions were derived from earlier Hubble and Voyager observations. "This appears to be a random or chaotic process, where there is a continual exchange of energy and angular momentum between the moons," Lissauer said. His calculations predict moons would begin to collide as often as every few million years, which is extraordinarily short compared to the 4.5 billion year age of the Uranian system.
Showalter and Lissauer believe the discovery of the second ring, which orbits closer to the planet than the outer ring, provides further evidence that collisions affect the evolution of the system. This second ring has no visible body to re-supply it with dust. The ring may be a telltale sign of an unseen belt of bodies a few feet to a few miles in size. Showalter proposes that a previous impact to one of Uranus' moons could have produced the observed debris ring.
Hubble uncovered the rings in August 2004 during a series of 80, four-minute exposures of Uranus. The team later recognized the faint new rings in 24 similar images taken a year earlier. Images from September 2005 reveal the rings even more clearly.
Showalter also found the rings in archival images taken during Voyager 2's flyby of Uranus in 1986. Uranus's first nine rings were discovered in 1977 during observations of the planet's atmosphere.
During the Voyager encounters, two other inner rings and 10 moons were discovered. However, no one noticed the outer rings, because they are extremely faint and much farther from the planet than expected. Showalter was able to find them by a careful analysis of nearly 100 Voyager images.
Because the new rings are nearly transparent, they will be easier to see when they tilt edge-on. The new rings will increase in brightness every year as Uranus approaches its equinox, when the sun shines directly over the planet's equator. When it happens in 2007, all of the rings will be tilted edge-on toward Earth and easier to study.
These research data will appear in an upcoming issue of the journal Science.
The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. The Space Telescope Science Institute in Baltimore conducts Hubble science operations.
The Institute is operated for NASA by the Association of Universities for Research in Astronomy, Inc., Washington. The Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory.
For images and information about Hubble and this research on the Web,
visit:
http://www.nasa.gov/hubble
or
http://hubblesite.org/news/2005/33
Later!
J P
NASA's Hubble Discovers New Rings and Moons Around Uranus
12.22.05
(Source: NASA Headquarters/National Imagery and Mapping Agency)
Dec. 22, 2005
Dwayne Brown/George Deutsch
Headquarters, Washington
(202) 358-1726/1324
Ray Villard
Space Telescope Science Institute, Baltimore
(410) 338-4514
RELEASE: 05-590
NASA'S HUBBLE DISCOVERS NEW RINGS AND MOONS AROUND URANUS
NASA's Hubble Space Telescope photographed a new pair of rings around Uranus and two new, small moons orbiting the planet.
The largest ring is twice the diameter of the planet's previously known rings. The rings are so far from the planet, they are being called Uranus' "second ring system." One of the new moons shares its orbit with one of the rings. Analysis of the Hubble data also reveals the orbits of Uranus' family of inner moons have changed significantly over the past decade.
"The detection of these new interacting rings and moons will help us better understand how planetary systems are formed and sustained, which is of key importance to NASA's scientific exploration goals,"
said Dr. Jennifer Wiseman, program scientist for Hubble at NASA Headquarters.
Since dust orbiting Uranus is expected to be depleted by spiraling away, the planet's rings must be continually replenished with fresh material. "The new discoveries demonstrate that Uranus has a youthful and dynamic system of rings and moons," said Mark Showalter of the SETI Institute, Baltimore.
Showalter and Jack Lissauer of NASA's Ames Research Center, Moffet Field, Calif., propose that the outermost ring is replenished by a 12-mile-wide newly discovered moon, named Mab, which they first observed using Hubble in 2003.
Meteoroid impacts continually blast dust off the surface of Mab. The dust then spreads out into a ring around Uranus. Mab's ring receives a fresh infusion of dust from each impact. Nature keeps the ring supplied with new dust while older dust spirals away or bangs back into the moon.
Showalter and Lissauer have measured numerous changes to the orbits of Uranus' inner moons since 1994. The moon's motions were derived from earlier Hubble and Voyager observations. "This appears to be a random or chaotic process, where there is a continual exchange of energy and angular momentum between the moons," Lissauer said. His calculations predict moons would begin to collide as often as every few million years, which is extraordinarily short compared to the 4.5 billion year age of the Uranian system.
Showalter and Lissauer believe the discovery of the second ring, which orbits closer to the planet than the outer ring, provides further evidence that collisions affect the evolution of the system. This second ring has no visible body to re-supply it with dust. The ring may be a telltale sign of an unseen belt of bodies a few feet to a few miles in size. Showalter proposes that a previous impact to one of Uranus' moons could have produced the observed debris ring.
Hubble uncovered the rings in August 2004 during a series of 80, four-minute exposures of Uranus. The team later recognized the faint new rings in 24 similar images taken a year earlier. Images from September 2005 reveal the rings even more clearly.
Showalter also found the rings in archival images taken during Voyager 2's flyby of Uranus in 1986. Uranus's first nine rings were discovered in 1977 during observations of the planet's atmosphere.
During the Voyager encounters, two other inner rings and 10 moons were discovered. However, no one noticed the outer rings, because they are extremely faint and much farther from the planet than expected. Showalter was able to find them by a careful analysis of nearly 100 Voyager images.
Because the new rings are nearly transparent, they will be easier to see when they tilt edge-on. The new rings will increase in brightness every year as Uranus approaches its equinox, when the sun shines directly over the planet's equator. When it happens in 2007, all of the rings will be tilted edge-on toward Earth and easier to study.
These research data will appear in an upcoming issue of the journal Science.
The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. The Space Telescope Science Institute in Baltimore conducts Hubble science operations.
The Institute is operated for NASA by the Association of Universities for Research in Astronomy, Inc., Washington. The Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory.
For images and information about Hubble and this research on the Web,
visit:
http://www.nasa.gov/hubble
or
http://hubblesite.org/news/2005/33
Later!
J P
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I found information in the table here that could be used to add the two new rings.
http://pds-rings.seti.org/uranus/uranus_tables.html
http://pds-rings.seti.org/uranus/uranus_tables.html
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