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Bright ringlets and dark gaps at the inner edge of the C ring sweep across
this scene. The C ring contains numerous "plateaus" -- broad ring regions
that are bright and surrounded by fainter material.
The image was taken in visible light with the Cassini spacecraft
narrow-angle camera on July 23, 2006. The view was captured from 14
degrees below the ring plane and at a distance of approximately 272,000
kilometers (169,000 miles) from Saturn. Image scale is 1 kilometer (0.6
mile) 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 Cassini spacecraft looks to the night side of Saturn and its rings for
a view that includes Dione.
Dione (1,123 kilometers, or 698 miles across) is in the top right of the
image. Tiny Pandora (81 kilometers, or 50 miles across) can also be seen
outside the F ring near the center of the image. Dione was overexposed in
this image and has been dimmed by a factor of seven.
This view looks toward the sunlit, northern side of the rings from about
12 degrees above the ringplane.
The image was taken with the Cassini spacecraft wide-angle camera on Sept.
22, 2009 using a spectral filter sensitive to wavelengths of near-infrared
light centered at 742 nanometers. The view was obtained at a distance of
approximately 1.3 million kilometers (808,000 miles) from Saturn. Image
scale is 72 kilometers (45 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
Image Addition Date:
2009-11-09
Simple Planetary gears - www.thingiverse.com/thing:16897
Printed out perfectly, gears mesh so well! Very fun little toy to play with, but also a great demonstration of how you can actually print very usable gears with 3D printing!
The planets revolve in the same direction around the sun, this constant explosion of a billion H-bombs. A Mercury year lasts !è days, but for Pluto it takes 249 years.
(Chocolate Jacques educational chromos, picture album "Race to the Stars", 1960's)
These side-by-side views of a star seen through Saturn's densely populated
B ring show marked contrast between the region where spokes -- the ghostly
radial features periodically seen in the B ring -- are produced and
regions where no spokes are seen.
In the view at left, the ring displays an uneven grainy texture, with a
great deal of variability in brightness along the direction of ring
particle motion. In the view at right, the ring is far smoother and more
uniform along the same longitudinal direction.
Ring scientists on the Cassini Imaging Team are studying images such as
these to understand the processes by which spokes are created. This
difference in appearance from one location to another on the ring could
provide the researchers with helpful insights into the features'
formation.
The views were acquired about half an hour apart as the Cassini spacecraft
looked toward the unlit side of the rings from about 33 degrees above the
ringplane.
The images were taken in visible light with the Cassini spacecraft
narrow-angle camera on Sept. 26, 2006 at a distance of approximately
515,000 kilometers (320,000 miles) from Saturn and at a
Sun-Saturn-spacecraft, or phase, angle of 102 degrees. Image scale is
about 3 kilometers (2 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
Never like to admit and research this subject of ancient aliens.....leave it almost an year back... but still it reminds of that Vishnu....not sure what he cooks .....and why........what's the ending chapter of his created story...
Overexposed Mimas stands starkly against the disk of Saturn as the dim
shadow of Epimetheus is captured through the C ring in the planet's rings
(right of center at the bottom of the image). In reality, Mimas orbits in
the same plane as the rings; it is Cassini's viewing geometry that tricks
our eyes.
The image was taken in blue light with the Cassini spacecraft wide-angle
camera on Nov. 26, 2008 at a distance of approximately 915,000 kilometers
(569,000 miles) from Mimas and at a Sun-Mimas-spacecraft, or phase, angle
of 28 degrees. Image scale is 55 kilometers (34 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 highly reflective moon Enceladus appears as a bright dot beyond a crescent Saturn in this Cassini image.Enceladus (504 kilometers, or 313 miles across) is visible above the ringplane to the left of the center of the image, and the moon is farther away from Cassini than the planet is. This view looks toward the northern, sunlit side of the rings from just above the ringplane.The image was taken with the Cassini spacecraft wide-angle camera on Oct. 23, 2009 using a spectral filter sensitive to wavelengths of near-infrared light centered at 728 nanometers. The view was obtained at a distance of approximately 2.8 million kilometers (1.7 million miles) from Enceladus and 2.6 million kilometers (1.6 million miles) from Saturn. Image scale is 149 kilometers (93 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 Image Addition Date: 2010-04-16
Incredible swirling details in Saturn's northern clouds can be seen in
this dazzling view. Shadows cast by the rings embrace the northern
hemisphere.
The view looks toward the unilluminated side of the rings from about 16
degrees above the ringplane.
The image was taken with the Cassini spacecraft wide-angle camera on June
10, 2007 using a spectral filter sensitive to wavelengths of infrared
light centered at 939 nanometers. The view was acquired at a distance of
approximately 1.3 million kilometers (800,000 miles) from Saturn. Image
scale is 72 kilometers (45 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
Milo raps some Beastie Boys:
If you try to knock me you'll get mocked.
I'll stir fry you in my wok.
Your knees with quake and your fingers pop.
Like a pinch on the neck from Mr. Spock.
The Cassini spacecraft spies Enceladus and Epimetheus near the limb of Saturn.
Geologically active Enceladus is 505 kilometers (314 miles) across; smaller, more
irregularly shaped Epimetheus is 116 kilometers (72 miles) across.
This view looks toward the unilluminated side of the rings from less than a degree above
the ringplane.
The image was taken in polarized green light with the Cassini spacecraft narrow-angle
camera on Oct. 27, 2007. The view was acquired at a distance of approximately 1.4
million kilometers (857,000 miles) from Enceladus. Epimetheus is 91,000 kilometers
(57,000 miles) farther away from Cassini here. Image scale is about 8 kilometers (5 miles)
per pixel on both moons.
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
The Cassini imaging team homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute
Saturn's southern hemisphere is glimpsed through the gossamer veil of its
rings. Ring shadows adorn the low northern latitudes.
This view looks toward the unilluminated side of the rings from about 22
degrees above the ringplane. Images taken using red, green and blue
spectral filters were combined to create this natural color view. The
images were acquired with the Cassini spacecraft wide-angle camera on Dec.
16, 2007 at a distance of approximately 1.5 million kilometers (908,000
miles) from Saturn. Image scale is 84 kilometers (52 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
The Cassini imaging team homepage is at ciclops.org.
credit: NASA/JPL/Space Science Institute
This was very cool. Choose the planet on the monitor and the projection changes to fit the profile of the planet. Star Trek: Starfleet Academy Experience @Telus Spark, Calgary
December 1, 2008 around 6:00 pm in NJ, USA
For more info, please visit:
news.nationalgeographic.com/news/2008/12/081201-jupiter-v...
Lighting that looks for all the world (no pun intended!) like planets. Little adjustment just some slight cropping and curves adjustment to get the blacks to pure black.
The multitude of grooves for which Saturn's rings are famed, clumps in
the F ring, and three Saturnian moons are visible in this image. Moons
visible in the image are: Mimas (398 kilometers or 247 miles across)
above the rings at left; Epimetheus (116 kilometers or 72 miles across)
just above the A ring; Enceladus (499 kilometers or 310 miles across)
near upper right. The image was taken with the Cassini narrow angle
camera on May 10, 2004, at a distance of 27.1 million kilometers (16.8
million miles) from Saturn. Image scale is 162 kilometers (101 miles) per
pixel. Contrast in the image was enhanced to aid 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 Cassini-Huygens mission for NASA's Office of Space
Science, Washington, D.C. The Cassini orbiter and its two onboard cameras,
were designed, developed and assembled at JPL. The imaging team is based
at the Space Science Institute, Boulder, Colo.
For more information, about the Cassini-Huygens mission visit,
saturn.jpl.nasa.gov/ and the Cassini imaging team home page,
credit: NASA/JPL/Space Science Institute
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Although Saturn's moon Pan is absent from this image of the A ring's Encke
Gap, the moon's handiwork is still displayed.
The two ringlets seen in the gap are maintained by the gravitational
action of Pan (28 kilometers, or 17 miles across). To learn more about
this process, see PIA07528.
The point of light near the bottom of the image is a star.
This view looks toward the unilluminated side of the rings from about 41
degrees above the ringplane. The image was taken in visible light with the
Cassini spacecraft narrow-angle camera on April 17, 2009. The view was
obtained at a distance of approximately 1.3 million kilometers (808,000
miles) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 115
degrees. Image scale is 8 kilometers (5 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