Enceladus on display in newest images from Cassini

May 3, 2012 By Jason Major
Enceladus' southern ice geysers are brilliant in backlit sunlight. Credit: NASA/JPL/SSI/J. Major

The latest images are in from Saturn’s very own personal paparazzi, NASA’s Cassini spacecraft, fresh from its early morning flyby of the ice-spewing moon Enceladus. And, being its last closeup for the next three years, the little moon didn’t disappoint!

The image above is a composite I made from two raw images assembled to show Enceladus in its crescent-lit entirety with jets in full force. The images were rotated to orient the moon’s southern pole — where the jets originate — toward the bottom.

was between 72,090 miles (116,000 km) and 90,000 miles (140,000 km) from Enceladus when these images were acquired.

This morning’s E-19 flyby completed a trio of recent close passes by Cassini of the 318-mile (511-km) -wide moon, bringing the spacecraft as low as 46 miles (74 km) above its frozen surface. The goal of the maneuver was to gather data about Enceladus’ internal mass — particularly in the region around its southern pole, where a reservoir of liquid water is thought to reside — and also to look for “hot spots” on its surface that would give more information about its overall energy distribution.

Enceladus' geysers in action on May 2, 2012. Credit: NASA/JPL/SSI

Cassini had previously discovered that Enceladus radiates a surprising amount of heat from its surface, mostly along the “tiger stripe” features — long, deep furrows (sulcae) that gouge its southern hemisphere, they are the source of the water-ice geysers.

Cassini also used the flyby opportunity to study Enceladus’ gravitational field.

Enceladus sprays ice into the hazy E ring, which orbits Saturn. Credit: NASA/JPL/SSI

By imaging the moon with backlit lighting from the Sun the highly-reflective ice particles in the jets become visible. More direct lighting reduces the jets’ visibility in images, which must be exposed for the natural light of the scene or risk “blowing out” due to Enceladus’ natural high reflectivity.

The images below are raw spacecraft downloads right from the Cassini’s imaging headquarters in Boulder, CO.

Cassini also swung closely by Dione during this morning’s flyby but the images from that encounter aren’t available yet. Stay tuned to Universe Today for more postcards from !

Explore further: Cassini returns images of bright jets at Enceladus

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kevinrtrs
1.2 / 5 (5) May 09, 2012
Cassini had previously discovered that Enceladus radiates a surprising amount of heat from its surface

What is surprising about this amount of energy is that they calculated/estimated that tidal friction and small internal radioactivity would supply about 1.1 GW. But what they've actually measured shows a power output of about 15.3 plus minus 3.1GW which is ten times more than what they expected, based on the nebular theory of planet formation.
This means that once again, actual observations simply do not play ball with the nebulous theory, instead they make mincemeat of it. Such a huge energy output should have disipated long ago if Enceladus was billions of years old - and the researchers know it. This is why the now standard wording is used: "a surprising...." was found.
As with most current observations, the actual physical evidence points to a much younger age for the moon. It's just philosophical blindness that wants to deny the evidence.

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