The spacecraft will not revisit the battered, porous moon before its mission concludes in 2017
Color-composite image of Saturn’s moon Hyperion.
On Sunday, May 31, 2015, NASA's made its latest and final flyby of Hyperion, Saturn's spongy moon. At around 9:36 a.m. EDT Cassini came within 21,000 miles (34,000 km) of Hyperion's surface—not its closest approach ever but certainly close enough to grab some fantastic images of this porous and punched-in world.
The image above is a color composite made from images acquired in optical wavelengths (i.e., Cassini's red, green, and blue color filters) with some contrast enhancement and a bit of boosting as well. This is about what would look like to an astronaut's eyes, if she happened to have been riding along with Cassini last Sunday.
At 255 x 163 x 137 miles (410 x 262 x 220 kilometers), Hyperion is the largest of Saturn's irregularly-shaped moons and its eighth-largest overall. Scientists think it could be what's left over from a larger moon that was blown apart in the distant past. []
Because of its porosity and low , impacts on Hyperion tend to create punched-in craters with little to no ejecta, giving it its strange spongelike appearance.
In fact some of may come from Titan, as hydrocarbons from its atmosphere get blown into orbit by the solar wind and eventually fall on Hyperion, where they concentrate in low spots and impact craters.
article was provided by
SPACE.com
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