«But a dirty secret
of planetary rings should be exposed: following exhaustive searches since 2004 using the Cassini spacecraft, it is almost certain that none of the numerous gaps in Saturn's C ring and in its Cassini Division (low density band between Saturn's main A and B rings) harbour any shepherds of the requisite size.»
Chancia and Hedman are well - versed in the physics
of planetary rings: both study Saturn's rings using data from NASA's Cassini spacecraft, which is currently orbiting Saturn.
Robin Canup came to the moon problem from studies
of planetary rings such as those girding the gas giants.
Through theoretical modeling, Aurélien Crida of the University of Nice Sophia - Antipolis and Sébastien Charnoz of the University of Paris Diderot found that the moon - formation action begins at the edge
of a planetary ring, where a satellite can take shape without being shredded by the gravitational pull of the planet.
Not exact matches
said
planetary scientist Jeff Cuzzi
of NASA's Ames Research Center in Moffett Field, Calif. «To me, this answers the question
of what makes the
rings red: It's organics.»
Some
of them, such as Saturn, Jupiter, Uranus and Neptune, additionally possess
planetary rings — a collection
of still smaller bodies
of different sizes that also orbit a planet.
In a breakthrough study, an international team
of scientists, including Professor Nikolai Brilliantov from the University
of Leicester, has solved an age - old scientific riddle by discovering that
planetary rings, such as those orbiting Saturn, have a universally similar particle distribution.
It is the first time a
ring has been discovered around a trans - neptunian object, and it shows that the presence
of rings could be much more common than was previously thought, in our Solar System as well as in other
planetary systems.
To answer that last question in particular, «you have to fly between the planet and the
rings,» says
planetary scientist Matthew Hedman
of the University
of Idaho in Moscow, who uses Cassini data to study the
rings.
The scientists» findings could help to increase the understanding
of the basic properties
of granular gases such as soot agglomeration in flue gases on Earth or in astrophysical phenomena such as cosmic dust in
planetary rings in space.
But now, data gathered during five
of Cassini's final 22 passes before it plunged into the planet are bringing the mass
of the B
ring into focus, Luciano Iess, a
planetary scientist at the Sapienza University
of Rome, announced at the AGU meeting today.
One
ring in particular owes its manicured appearance to no fewer than seven moons working together, according to new results released this week at the American Astronomical Society's Division
of Planetary Sciences meeting in Provo, Utah.
AUSTIN, TEXAS — Like a
planetary jewelry case, our solar system glitters with a dazzling variety
of rings.
Those measurements reveal that the B
ring, which makes up 80 percent
of the total
ring mass, is about 15 billion billion kilograms, or 0.4 times that
of Saturn's moon Mimas,
planetary scientist Luciano Iess
of Sapienza University
of Rome said at the meeting on December 12.
That's lightweight enough to be young, says
planetary scientist Larry Esposito
of the University
of Colorado Boulder, a longtime old
rings proponent who wasn't involved in the new work.
The paper «is a wonderful and gratifying confirmation
of what we found several years back,» says
planetary scientist and Cassini team member Carolyn Porco
of the Space Science Institute in Boulder, Colorado, who worked on the earlier examination
of the F
ring.
The constituent fragments that lie near the inner,
planetary side
of the
ring should constantly exchange angular momentum with fragments further out.
This spring, Buck Sharpton
of the Lunar and
Planetary Laboratory in Houston reported evidence that the Chicxulub crater along the Yucatan coast has multiple
rings and that its outer
ring is nearly 300 kilometres across.
There's not enough pollution in the
rings for them to have been around for a long time, argues
planetary scientist Paul Estrada
of the SETI Institute in Mountain View,
A dark
ring of dust and gas circling the star (dark bands, center), material that may one day coalesce into a
planetary system, acts like a belt, cinching the nebula into an hourglass shape.
By drilling into a circular ridge inside the 180 - kilometer - wide crater rim, researchers also hope to nail down the processes that form «peak
rings»: hallmarks
of the largest impact craters, which
planetary scientists have seen elsewhere in the solar system but which erosion has erased from other big craters on Earth.
The Little Ghost (right) is a more classic
planetary nebula: Its doughnut is the steadily expanding
ring of star gas that has been ionized and set aglow by ultraviolet light from the central white dwarf.
The icy fragments would have encircled the solar system's second largest planet as
rings and eventually spalled off small moons
of their own that are still there today, says Robin Canup, a
planetary scientist at the Southwest Research Institute in Boulder, Colo..
The Cassini mission to Saturn has been one
of the most successful
planetary missions ever, revealing the
ringed giant and its moons as never before.
«The three
rings around this young star are nested like Russian dolls and undergoing dramatic changes reminiscent
of planetary formation,» says Mawet.
The mass and orbit
of planetary candidate «b» is similar to 79 Ceti b, depicted at left with
rings and two moons, as imagined by Bacon (more from NASA and Astronomy Picture
of the Day).
Lecture 9
of Dr. Bruce Betts» 2015 online Introductory
Planetary Science and Astronomy course covers Saturn's moon Titan and the Uranian and Neptunian systems including atmospheres, interiors,
rings, and moons including Triton.
Lecture 8
of Dr. Bruce Betts» 2015 online Introductory
Planetary Science and Astronomy course covers the Galilean Satellites (Io, Europa, Ganymede, Callisto)
of Jupiter, and the Saturnian System including atmosphere, interior,
rings, and moons including Iapetus and Enceladus.
© Walter Myers — larger image (Artwork from Computergraphic Vistas, used with permission) View
of a
ringed,
planetary candidate «b» from a rocky moon, as imagined by Myers (more).
Composite picture
of the Cat's Eye Nebula (NGC 6543), combining three images taken by the Hubble Space Telescope.This
planetary nebula has an unusually complicated structure, with concentric shells (seen as bright
rings), jets (the projections at upper left and lower right), and a number
of details that suggest complex interactions
of shock waves.
The vibrations
of these
rings mirror the actual
planetary orbital evolution that unfolds over millions
of years, making the approximation quite accurate.
Over at The
Planetary Society, Emily Lakdawalla highlighted an image taken by the Cassini spacecraft
of Saturn separate from its
rings.
Researchers shed light on scientific phenomenon which helps to better understand evolution
of interstellar dust and
planetary rings in space
Once these
planetary bodies acquire enough mass, they dramatically reshape the structure
of their natal disk, fashioning
rings and gaps as the planets sweep their orbits clear
of debris and shepherd dust and gas into tighter and more confined zones.
Though scientists are fairly certain the
rings indicate that planets are beginning to form, the structure pictured defies the time line they would have predicted in the process
of planetary formation.
He is one
of the discovers
of the first
ring around an asteroid (Chariklo) and with collaborators was the one to first use measurements
of planetary transits from space to measure the size
of the sun.
A clutch locks the
ring gear
of the
planetary gearset for a 7.0:1 speed reduction and torque multiplication ratio.
Torque biasing - Depending on the tooth ratio's
of the
planetary,
ring and sun gear, the desired ratio can be designed.
The
planetary gearset is what's responsible for changing gear ratios, and it consists
of a sun gear surrounded by smaller planet gears carried by a planet carrier enclosed in a
ring gear.
The
planetary gears are comprised
of the sun gear, which attaches to the main shaft and the
planetary gears, all
of which sits inside a
ring gear.
It is a moonless night, dark and rare, and the heat is oppressive, the kind
of heat where a deep breath leaves you unsatisfied, suspicious that there was nothing life - giving at all in what you've inhaled, and you are left air - hungry, wet at the pits, forehead greasy with sweat, wishing for the night to be over, for your daughters to exhaust their energy, to cool their dense, hot centers enough to sleep for one more night in this summer that seems to stretch into your future like a
planetary ring full
of debris, circling forever around something it can't escape.
In a simultaneous show at the Andre Zarre Gallery, «Matter in Outer Space,» solid - seeming discs, like the
rings of Saturn, floated near black and turquoise
planetary forms.