We get to see four of Saturn;s moons in this Cassini image. NASA describes them below. They do not comment on one of more spectacular shots of the rings Cassini has taken; they show up better in the larger versions at the NASA website.
Two pairs of moons make a rare joint appearance. The F ring’s shepherd moons, Prometheus and Pandora, appear just inside and outside of the F ring (the thin faint ring furthest from Saturn). Meanwhile, farther from Saturn the co-orbital moons Janus (near the bottom) and Epimetheus (about a third of the way down from the top) also are captured.
Prometheus (53 miles, or 86 kilometers across) and Pandora (50 miles, or 81 kilometers across) sculpt the F ring through their gravitational influences. Janus (111 miles, or 179 kilometers across) and Epimetheus (70 miles, or 113 kilometers across) are famous for their orbital dance, swapping places about every four years. They are also responsible for gravitationally shaping the outer edge of the A ring into seven scallops.
This view looks toward the sunlit side of the rings from about 47 degrees above the ringplane. The image was taken in visible light with the Cassini spacecraft wide-angle camera on Oct. 11, 2013.
The view was acquired at a distance of approximately 810,000 miles (1.3 million kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 47 degrees. Image scale is 47 miles (76 kilometers) per pixel.
13 years of Cassini for a Day! This is a great opportunity for both teachers and students, espeically students. Looking for a project? You could enter this and (or) use the essay at school. Surely an entry would earn some extra credit.
Students must be in grades 5 to 12 and the entry deadline is 17 April 2014. Note: that is a US deadline, other counties may have different deadlines which are not yet listed, typically they indeed different. The International link on the site is not yet current but it will be shortly.
Cassini Scientist for a Day is an essay contest designed to give students a taste of life as a scientist.
Students study three possible targets that the Cassini spacecraft can image during a given time set aside for education. They are to choose the one image they think will yield the best science results and explain their reasons in an essay.
The three targets are:
Target 1 is Saturn’s F ring. Cassini will be taking 70 images of the F ring using the spacecraft’s Narrow Angle Camera to make a movie showing how the F ring changes as it orbits Saturn.
Target 2 is Saturn’s largest moon, Titan. Cassini will be taking nine images of Titan’s north polar region using its Narrow Angle Camera. These images will be stitched together to form a mosaic.
Target 3 is the planet Saturn. The Cassini spacecraft will use its Wide Angle Camera and its Narrow Angle Camera to image Saturn’s north pole, studying the hurricane at the north pole and the hexagon-shaped polar vortex.
A nearly full Rhea shines in the sunlight in this recent Cassini image.
Rhea (949 miles, or 1,527 kilometers across) is Saturn’s second largest moon.
Lit terrain seen here is on the Saturn-facing hemisphere of Rhea. North on Rhea is up and rotated 43 degrees to the left. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Sept. 10, 2013.
The view was obtained at a distance of approximately 990,000 miles (1.6 million kilometers) from Rhea. Image scale is 6 miles (9 kilometers) 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 in Washington. 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.
An interesting offering from the Cassini spacecraft. The JPL caption (below) says “the ring appears to separate from the core of the ring”. It looks more to me as if the ring isn’t so much separated as it is sort of folded, but then I’m no expert. Click the image and have a look to see what you think.
Saturn’s F ring often appears to do things other rings don’t. In this Cassini spacecraft image, a strand of ring appears to separate from the core of the ring as if pulled apart by mysterious forces.
Some ring scientists believe that this feature may be due to repeated collisions between the F ring and a single small object.
Eight stars are also visible in this image.
This view looks toward the unilluminated side of the rings from about 49 degrees below the ringplane. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Oct. 19, 2013.
The view was obtained at a distance of approximately 1.2 million miles (1.9 million kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 120 degrees. Image scale is 6.8 miles (11 kilometers) per pixel.
The bright spot you can see on the rings of Saturn is called an “opposition surge” was taken in August 2013 and just released.
The opposition surge happens when the Sun-Ring-Cassini angle gets to zero degrees. The image here was taken through a polarized filter on the camera. The filter acts to allow only light polarized in one direction pass this reduces the scattering of light. This is very similar to the polarized lenses we have on our sunglasses.
Using the polarized filter and the size and magnitude of the spot scientists can learn about the properties of the particles making up the rings.
The image above was taken from a distance of 1.1 million km / 712,000 miles. The actual Sun-rings-Cassini phase angle here was seven degrees, this could account for the spot maybe not as clearly defined as the 2006 image.
I hope everybody saw the new year come in and enjoyed yourselves. I am working again today so I didn’t make it very long into the night. If all goes well today will be my Friday and it is quite overdue after working for two weeks straight.
The image here is a very nicely detailed look at Saturn’s polar vortex and a fine way to bring in 2014.
The vortex at Saturn’s north pole — seen here in the infrared — takes on the menacing look of something from the imagination of Edgar Allan Poe. But really, of course, it’s just another example of the amazing, mesmerizing meteorology on Saturn.
The eye of the immense cyclone is about 2,000 kilometers (1,250 miles) wide, 20 times larger than most on Earth. For another view of the vortex, see PIA14946.
This view is centered on clouds at 89 degrees north latitude, 109 degrees west longitude. North is up and rotated 33 degrees to the left. The image was taken with the Cassini spacecraft narrow-angle camera on June 14, 2013 using a spectral filter sensitive to wavelengths of near-infrared light centered at 750 nanometers.The view was acquired at a distance of approximately 476,000 miles (766,000 kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 45 degrees. Image scale is 3 miles (5 kilometers) per pixel.
The globe of Saturn, seen here in natural color, is reminiscent of a holiday ornament in this wide-angle view from NASA’s Cassini spacecraft. The characteristic hexagonal shape of Saturn’s northern jet stream, somewhat yellow here, is visible. At the pole lies a Saturnian version of a high-speed hurricane, eye and all.
This view is centered on terrain at 75 degrees north latitude, 120 degrees west longitude. Images taken using red, green and blue spectral filters were combined to create this natural-color view. The images were taken with the Cassini spacecraft wide-angle camera on July 22, 2013.
This view was acquired at a distance of approximately 611,000 miles (984,000 kilometers) from Saturn. Image scale is 51 miles (82 kilometers) 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.