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An illuminated quarter of the moon Tethys is imaged near a swath of Saturn rings. Though the moon appears to be hanging directly below the rings, Tethys is actually farther from NASA Cassini spacecraft, and the rings are in the foreground.
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Saturn rings lie in the distance as NASA Cassini spacecraft looks toward Titan and its dark region called Shangri-La, east of the landing site of the Huygens Probe.
Ver en NASA ↗Data from NASA Cassini spacecraft show that the sizes and patterns of dunes on Saturn moon Titan vary as a function of altitude and latitude left. Images of Earth dunes Oman and Kalahari are shown at right as seen by NASA Terra spacecraft.
Ver en NASA ↗Shadows are cast by Daphnis and the moon attendant edge waves in this image from NASA Cassini spacecraft taken about a month and a half before the Saturn August 2009 equinox.
Ver en NASA ↗Jupiter, Saturn, Uranus, and Neptune are known as the jovian Jupiter-like planets because they are all gigantic compared with Earth, and they have a gaseous nature. This diagram shows the approximate distance of the jovian planets from the Sun.
Ver en NASA ↗NASA Cassini spacecraft looks at an example of a ray crater on the leading hemisphere of Saturn moon Dione. The ray crater is in the upper-left of the image and ejecta rays show up as brighter material emanating from the crater.
Ver en NASA ↗This image shows an updated map of Saturn icy moon Enceladus, generated by NASA Cassini imaging team. The map incorporates new images taken in 2008, with better image processing techniques.
Ver en NASA ↗Saturn moon Tethys orbits in front of the wide shadows cast by the rings onto the planet for this view from NASA Cassini spacecraft. Tethys appears just below the rings near the center of the image.
Ver en NASA ↗Cassini briefly turned its gaze from Saturn and its rings and moons to marvel at the Carina Nebula, a brilliant region 8,000 light years from our solar system and more than 200 light years across
Ver en NASA ↗Saturn moon Epimetheus casts a shadow across colorful rings in this image taken by NASA Cassini spacecraft before the planet August 2009 equinox. Epimetheus is visible as a small dot at the center of the bottom of the image.
Ver en NASA ↗This image taken by NASA Cassini spacecraft shows that rather than being an unchanging disk of peaceful particles, the material that makes up Saturn rings is constantly pushed and pulled into spectacular shapes. At left is the moon Daphnis.
Ver en NASA ↗Saturn rings appear curved in this view from NASA Cassini spacecraft, which also shows the moon Janus in the distance. Janus is at the bottom of the image and is farther from the spacecraft than the rings are.
Ver en NASA ↗Saturn rings lie between a pair of moons in this view from NASA Cassini spacecraft that features Mimas and Prometheus. Mimas is the more noticeable of the two moons at top left, Prometheus is near the center of image and closest to Cassini.
Ver en NASA ↗This Cassini spacecraft view shows a group of more than a dozen spokes in Saturn outer B ring. The B ring displays the azimuthal asymmetry, or variation with longitude around the planet, that is characteristic of the spoke-forming region
Ver en NASA ↗A pair of Saturn small moons orbit near the planet rings, which appear well illuminated in this view captured by NASA Cassini spacecraft. Janus is near the center of the image and Pandora is on the left.
Ver en NASA ↗About a month after Saturn August 2009 equinox, shadows continue to grace the planet rings in this image taken by NASA Cassini Orbiter. Pan runs through the center of this image.
Ver en NASA ↗NASA Cassini spacecraft takes a close look at a row of craters on Saturn moon Tethys during the spacecraft April 14, 2012, flyby of the moon. Three large craters are visible along the terminator between day and night on Tethys.
Ver en NASA ↗Saturn rings occupy the space between two of the planet moons in this image, taken by NASA Cassini spacecraft, which shows the highly reflective moon Enceladus in the background and the smaller moon Janus in the fore.
Ver en NASA ↗This graphic, using data from NASA Cassini spacecraft, shows how the south polar terrain of Saturn moon Enceladus emits much more power than scientists had originally predicted.
Ver en NASA ↗While the moon Epimetheus passes by, beyond the edge of Saturn main rings, the tiny moon Daphnis carries on its orbit within the Keeler gap of the A ring in this image from NASA Cassini spacecraft.
Ver en NASA ↗Tiny, dust-sized particles in Saturn rings become much easier to see at high phase angle -- the angle formed by the Sun, the rings and the spacecraft. The brightest ring is the F ring; the next feature to the left is the outer edge of the A ring
Ver en NASA ↗Subtle color differences on Saturn moon Mimas are apparent in this false-color view of Herschel Crater captured during NASA Cassini spacecraft on its closest-ever flyby of that moon.
Ver en NASA ↗Dione beautiful wispy terrain is brightly lit alongside Saturn elegant rings in this image captured by NASA Cassini spacecraft. The wisps are relatively young fractures on the trailing hemisphere of Dione icy surface.
Ver en NASA ↗This view from NASA Cassini spacecraft look toward the south polar region of Saturn largest moon, Titan, and show a depression within the moon orange and blue haze layers near the south pole.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.