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Creation 31(3):54–55, June 2009

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Enceladus: Saturn’s sprightly moon looks young

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NASA / JPL / Space Science Institute Geologically active ‘tiger stripes’ at the south pole of Enceladus
Geologically active ‘tiger stripes’ at the south pole of Enceladus

NASA’s flybys of Saturn’s moon Enceladus by their Cassini spacecraft reveal more evidence of an active world that continues to confound scientists.

William Herschel (1738–1822) discovered this moon in 1789 on his first night of viewing with the large new telescope he had built. Little was known about Enceladus until the 1980s, when the Voyager 1, Voyager 2 and Pioneer 11 spacecraft flew by Saturn.1

The images they returned to Earth were astounding. They showed the moon was only about 500 km (300 miles) in diameter and that it reflects almost 100% of the light it receives from the sun.

Most scientists expected Saturn’s moons to be cold and dead, and their surfaces to be covered with impact craters from exposure to meteors for billions of years. That’s because they believed that the sun and all the planets of our solar system formed when a hypothetical solar nebula condensed some 4.5 billion years ago.

Instead, the images from Voyager 2 revealed that Enceladus’ surface was mostly smooth. Scientists still asserted that the moon was billions of years old, but said it must have acquired a new surface in the recent past. NASA scheduled more space visits to investigate.2

The Cassini spacecraft was launched in 1997 but did not arrive at Saturn until 2004. It was 2005 before the cameras turned toward Enceladus. Since then there have been numerous flybys with spectacular images and more surprises.

The first was that powerful geysers were blasting water vapour and tiny ice particles hundreds of kilometres into space from vents near the South Pole. Enceladus should have been dead but it is still geologically active.

Scooting over the southern polar region, the Cassini spacecraft captured close-up images of distinctive fractures described as “tiger stripes”, V-shaped cracks up to 300 m (1,000 ft) deep.

This is the area with the powerful geysers. Such is the immense pressure behind them that the jets of water vapour and icy particles are spewed into space as fast as a supersonic jet. Infrared measurements estimated the energy produced by the geysers at 5.8 gigawatts—enough to power a city with 6 million people.

Subsequent flybys in 2008 captured even more detail, and a few daring manoeuvres took Cassini close enough to pass through the plume, collect samples and analyze them.

This tiny moon seems to have an enormous influence on the whole ring system of Saturn.

NASA / JPL / Space Science Institute Enhanced colour image of geysers spraying water vapour far into space
Enhanced colour image of geysers spraying water vapour far into space

First, the jets produce the material for the outermost E ring—a 300,000-km-wide (200,000 miles) donut-shaped mist of micron-sized particles. The gas from the jets is also ionized and tends to drag the magnetosphere so strongly that it distorts our measurements of Saturn’s rotation. And even more surprisingly, the plasma cloud around Saturn is being drawn into the brighter A ring, much closer to the planet.

But how can such a small moon have enough heat to power the geysers?

One suggestion was that radioactive substances inside the moon are heating it. But even though Enceladus is the rockiest of Saturn’s major moons, it could not contain enough radioactive material to produce the observed heat.3

Another idea is tidal heating. Just as our moon distorts the shape of the earth and creates ocean tides, the gravitational pull of Saturn changes the shape of Enceladus as it orbits every 1.37 days. It heats the moon like a metal wire heats when you bend it backwards and forwards.

But why is Enceladus still flexible? After 4.5 billion years the moon should be frozen solid and tidal friction should not work. When James Roberts and Francis Nimmo of the University of California modelled the moon’s interior, they found it would have frozen after only 30 million years—less than 1% of its supposed age.4

What about the effects of Enceladus’ out-of-round orbit imposed on it by Dione (a larger nearby moon of Saturn)? Again, no. Still not enough heat.5

Is it possible that Enceladus contained the heat when Saturn and its moons formed, and it has not cooled down yet? That is a simple idea and would explain the observations without any complicated mental gymnastics. But that would mean that Saturn and its moons are not billions of years old.

Such ideas are off limits. Most space scientists won’t entertain these options because they have a “sacred” secular belief that the solar system is billions of years old.

But the enigmatic moon of Saturn, with its deep, icy chasms and spectacular, shimmering fountains, fits beautifully with a solar system created just 6,000 years ago as biblical history records.

References

  1. Vittorio, S., Cassini visits Enceladus—new light on a bright world, <csa.com/discovery guides/enceladus/review.pdf>, July 2006. Return to text.
  2. Porco, C., The restless world of Enceladus, Scientific American 299(6):26–35, p. 26, December 2008. Return to text.
  3. Ref. 2, p. 31. Return to text.
  4. Schirber, M., Frigid future for ocean in Saturn’s moon, Astrobiology Magazine, <space.com/scienceastronomy/080619-am-enceladus-ocean.html> 19 June 2008. Return to text.
  5. Ref. 2, p. 32. Return to text.

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