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Prometheus shows up bright in this image of the dark side of the rings.
The bright band that appears above Prometheus in this image is the Cassini
division separating the (very dark) B ring and the A ring. The C ring,
interior to the B ring, is clearly visible.
10532The image was taken in visible light with the Cassini spacecraft
narrow-angle camera on Oct. 20, 2008 at a distance of approximately 1.076
million kilometers (668,000 miles) from Prometheus and at a
Sun-Prometheus-spacecraft, or phase, angle of 26 degrees. Image scale is 6
kilometers (4 miles) per pixel.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
saturn.jpl.nasa.gov. The Cassini imaging team
homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute
The dramatic plane of Saturn's rings is indeed a huge expanse. Gazing
straight across the vertical center of this view, the Cassini spacecraft
takes in more than 200,000 kilometers (124,000 miles) from one side of the
rings to the other.
Atlas (32 kilometers, or 20 miles across) is gliding past below center.
This view looks toward the unilluminated side of the rings from about 2
degrees above the ringplane.
The image was taken in visible light with the Cassini spacecraft
narrow-angle camera on June 24, 2007 at a distance of approximately 1.7
million kilometers (1.1 million miles) from Atlas. Image scale is 10
kilometers (6 miles) per pixel.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
saturn.jpl.nasa.gov. The Cassini imaging team
homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute
Squinting at this view of Saturn's rings reveals not one but two of the
four narrow ringlets in the Encke Gap (325 kilometers, or 200 miles,
wide). The innermost of the two ringlets is much brighter and full of
clumps.
The complicated and dynamic features in the Encke Gap are extensively
influenced by the presence of Pan (26 kilometers, or 16 miles, across),
which orbits in the center of the gap. The Encke Gap may contain other
small moonlets, which imaging team members hope to discover in the future.
The image was taken in visible light with the Cassini spacecraft
wide-angle camera on Aug. 20, 2005, at a distance of approximately
273,000 kilometers (170,000 miles) from Saturn. The image scale is 13
kilometers (8 miles) per pixel.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit saturn.jpl.nasa.gov.
For additional images visit the Cassini imaging team homepage ciclops.org.
credit: NASA/JPL/Space Science Institute
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Just something I was messing around with today. This is one of my firsts attempts at doing something like this in photoshop, and I dont think it is half bad.
Ragazze Quartet, Kapok, Slagwerk Den Haag en Blauwe Uur spelen Planetary Sunrise: een nachtelijk, visueel en hallucinair concert-ritueel op Oerol, geïnspireerd door de ‘all night concerts’ van componist Terry Riley in de jaren ’70. Bij zonsondergang transformeert het duinlandschap van Terschelling zich tot een buitengewone wereld van patronen, kleuren en klanken.
These figures show four propeller-shaped structures discovered by the
Cassini spacecraft in close-up images of Saturn's A ring.
The propellers are about 5 kilometers (3 miles) long from tip to tip, and
the radial offset (the "leading" dash is slightly closer to Saturn) is
about 300 meters (1,000 feet). See PIA07791 and PIA07792 for
additional images and information about these features.
The figures were cropped from two original Cassini spacecraft narrow-angle
camera images and magnified for visibility. The images were then
re-projected so that orbital motion is to the left and Saturn is up. The
unseen moonlets lie in the center of each structure. The figures were
cropped from two original Cassini spacecraft narrow-angle camera images,
taken during Saturn orbit insertion on July 1, 2004, and magnified for
visibility.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
saturn.jpl.nasa.gov. The Cassini imaging team
homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute
Saturn's density is so low, and its rotation is so fast, that the planet
bulges around its waistline as is spins.
Saturn is nearly 12,000 kilometers (7,500 miles) wider at its equator than
at its poles, and its oblateness is clearly visible in this view.
The view looks toward the sunlit side of the rings from about 2 degrees
below the ringplane.
The image was taken in visible light with the Cassini spacecraft
wide-angle camera on Sept. 2, 2007. The view was obtained at a distance of
approximately 1.9 million kilometers (1.2 million miles) from Saturn.
Image scale is 109 kilometers (68 miles) per pixel.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
saturn.jpl.nasa.gov. The Cassini imaging team
homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute
In the Maxwell gap within Saturn's C ring resides a narrow, eccentric
ringlet of the same name. Astronomers are studying this ringlet to
understand how it is maintained.
One possibility is that a small moon or two lurk in the gap. Cassini plans
to search for any such moons.
The image was taken in visible light with the Cassini spacecraft
narrow-angle camera on Oct. 25, 2008 at a distance of approximately
876,000 kilometers (545,000 miles) from Saturn and at a
Sun-Saturn-spacecraft, or phase, angle of 36 degrees. Image scale is 5
kilometers (3 miles) per pixel.
The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, manages
the mission for NASA's Science Mission Directorate, Washington, D.C. The
Cassini orbiter and its two onboard cameras were designed, developed and
assembled at JPL. The imaging operations center is based at the Space
Science Institute in Boulder, Colo.
For more information about the Cassini-Huygens mission visit
saturn.jpl.nasa.gov. The Cassini imaging team
homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute