Ladypolitik (ladypolitik) wrote in ontd_political,
Ladypolitik
ladypolitik
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ONTD_Political's PotD: May 27, 2010.


While we humans carry on with our daily lives down here on Earth, perhaps stuck in traffic or reading blogs, or just enjoying a Springtime stroll, a school-bus-sized spacecraft called Cassini continues to gather data and images for us - 1.4 billion kilometers (870 million miles) away. Over the past months, NASA's Cassini spacecraft has made several close flybys of Saturn's moons, caught the Sun's reflection glinting off a lake on Titan, and has brought us even more tantalizing images of ongoing cryovolcanism on Enceladus. Collected here are a handful of recent images from the Saturnian system.



In orbit around Saturn, NASA's Cassini spacecraft captured this image of Saturn's moon Tethys with its prominent Odysseus Crater slipping behind Saturn's largest moon Titan. Tethys (1,062 km, or 660 mi across) is more than twice as far from Cassini than Titan (5,150 km, or 3,200 mi across). Tethys is 2.2 million km (1.4 million mi) from Cassini, where Titan is only about 1 million km (621,000 mi) away. This image was obtained with the a narrow-angle camera on November 26, 2009. Image scale is 6 km (4 mi) per pixel on Titan and 13 km (8 mi) per pixel on Tethys. (NASA/JPL/SSI)



Saturn's tiny moon Mimas - only 396 km (246 mi) across - seen before part of the upper atmosphere of Saturn on November 26, 2008. Cassini was approximately 915,000 km away from Mimas. (NASA/JPL)



On February 13, 2010 Cassini approached closer to Mimas at approximately 70,000 km away, Saturn's limb and upper atmosphere visible in the background. (NASA/JPL)



In this view captured by Cassini on its closest-ever flyby of Saturn's moon Mimas, large Herschel Crater - 130 km (80 mi) wide - dominates the scene. Cassini came within about 9,500 km (5,900 mi) of Mimas on Feb. 13, 2010. (NASA/JPL/SSI)



The Cassini spacecraft captured this natural color view of Saturn almost a month after the planet's August 2009 equinox. The shadow cast on the planet by the rings remains narrow. Mimas can be seen as a speck at lower left. Image obtained with the Cassini spacecraft wide-angle camera on September 4th, 2009 from approximately 2.7 million km (1.7 million mi) away from Saturn. (NASA/JPL/SSI)



Seen on July 26, 2009, Saturn's moon Enceladus - 500km (310 mi) across - lies approximately 200,000 km away from Cassini. (NASA/JPL)



Icy jets of Enceladus are viewed by Cassini on May 18th, 2010 at a distance of approximately 17,000 km (11,000 mi). Cassini is on the night side of the moon, viewing brightly-lit plumes of ice being ejected from fissures at Enceladus' south pole. Image scale is 100 meters (329 feet) per pixel. (NASA/JPL/SSI)



A close view of Baghdad Sulcus on Enceladus, seen by Cassini on November 21, 2009. With a scale of approximately 12m (40ft) per pixel, relatively small surface features such as icy boulders appear visible. This image covers approximately 12 km (7.5 mi) from side to side. (NASA/JPL)



Enceladus continues to spew ice into space, seen by Cassini on October 14, 2009. (NASA/JPL)



Saturn's tiny moon Helene, seen here by Cassini on March 03, 2010. Discovered in 1980, Helene is only 35 km (28 mi) wide. (NASA/JPL)



An October 14th, 2009 view of Saturn's brightly lit moon Tethys. Tethys is one of the four Saturnian moons discovered by astronomer Giovanni Domenico Cassini, first seen in 1684. It is an icy body slightly larger than 1,000 km (620 mi) across. (NASA/JPL/SSI)



Saturn's moon Rhea looms near its sibling moon Epimetheus in this Cassini image with the planet and its rings in the background. The two moons aren't actually close to each other. The view was obtained at a distance of approximately 1.2 million km (746,000 mi) from Rhea and 1.6 million km (994,000 mi) from Epimetheus. The image was taken on March 24, 2010. Image scale is 7 km (5 mi) per pixel on Rhea and 10 km (6 mi) per pixel on Epimetheus. (NASA/JPL/SSI)



Cassini looks down on the clouds in the upper atmosphere of Saturn, just over the shoulder of the moon Helene, on March 03, 2010. (NASA/JPL)



This image shows the first flash of sunlight reflected off a lake on Saturn's moon Titan, detected on on July 8, 2009. The glint off a mirror-like surface is known as a specular reflection, and it confirmed the presence of liquid in the moon's northern hemisphere, where lakes are more numerous and larger than those in the southern hemisphere. Cassini scientists were able to correlate the reflection to the southern shoreline of a Titan lake called Kraken Mare. The sprawling Kraken Mare covers about 400,000 sq km (150,000 sq mi). (NASA/JPL/University of Arizona/DLR)



The shadow of Saturn's largest moon darkens a huge portion of the gas giant planet. Titan (5,150 km, or 3,200 mi across) is not pictured here, but its shadow is elongated across Saturn's upper atmosphere. The image was taken with the Cassini spacecraft wide-angle camera on November 7th, 2009 using a spectral filter sensitive to wavelengths of near-infrared light centered at 752 nanometers. The view was obtained at a distance of approximately 2.1 million km (1.3 million mi) from Saturn. (NASA/JPL/SSI)



Saturn's rings, made dark in part as the planet casts its shadow across them, cut a striking figure before Saturn's largest moon, Titan. The night side of the planet is to the left, out of the frame of the image. Illuminated Titan can be seen above, below and through gaps in the rings. The moon Mimas (396 km, 246 mi across) is near the bottom of the image. Atlas (30 km, 19 mi across) can barely be detected near the thin F ring just above the center right of the image. (NASA/JPL/SSI)



Saturn's moon Dione passes in front of the larger moon Titan, as seen from Cassini. The image was taken with the Cassini spacecraft narrow-angle camera on March 12, 2010. The view was obtained at a distance of approximately 2.2 million km (1.4 million mi) from Dione and 3.6 million km (2.2 million mi) from Titan. (NASA/JPL/SSI)



The moon Prometheus creates an intricate pattern of perturbation in Saturn's F ring while the moon Daphnis disturbs the A ring in this image taken after the planet's August 2009 equinox. Prometheus (86 km, or 53 mi across) can be seen between the thin F ring and the A ring in the middle left of the image. The gravity of potato-shaped Prometheus periodically creates streamer-channels in the F ring. Near the bottom of the image, Daphnis (8 km, or 5 mi across) can be seen creating edge waves in the Keeler Gap of the A ring. The moon has an inclined orbit and its gravitational pull perturbs the orbits of the particles of the A ring, forming the Keeler Gap's edge, and sculpts the edge into waves having both horizontal (radial) and out-of-plane components. Image acquired on Aug. 22, 2009 with a scale of 12 km (7 mi) per pixel. (NASA/JPL/SSI)



Titan's golden, smog-like atmosphere and complex layered hazes appear to Cassini as a luminous ring around the planet-sized moon. Images taken using red, blue and green spectral filters were combined to create this color view. Six images - two sets of three colors - were combined to create the mosaic. The images were acquired with the Cassini wide-angle camera on Oct. 12, 2009 at a distance of 145,000 km (90,000 mi) from Titan. (NASA/JPL)



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