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NASA's Cassini spacecraft will make an unprecedented "in your face" flyby of Saturn's moon Enceladus on Wed., March 12.
The spacecraft, orchestrating its closest approach to date, will skirt along the edges of huge Old-Faithful-like geysers erupting from giant fractures on the south pole of Enceladus.
The source of the geysers is of great interest to scientists who think liquid water, perhaps even an ocean, may exist in the area.
Saturn's second-largest moon Rhea may have a small ring around it - the first time a moon has been found to have a ring, an international team of researchers reported.
Rhea lies within a magnetized bubble that surrounds Saturn and contains trapped ions and electrons....
In terms of a spacecraft passing by a space body, this is like dipping its antenna into the pool. And, in this case, astronomers want to learn what materials compose that pool.
There is little danger to the spacecraft at this close distance. Trajectory experts will make sure that Cassini doesn’t impact the moon. And, the particles in the geyser plume are so small they little chance of damaging the spacecraft.
The ice-water particles contained in the plumes are thought to be about one ten-thousandth of an inch in diameter, or roughly the width of a human hair. In fact, Cassini crosses the path of much larger particles on a regular basis on its exploratory journey around Saturn and its moons
The Viking mission may have gone to within 20km of the Martian moon Phobos, but there is nothing in deep Solar System exploration history to compare with the pass being attempted by Cassini.
Since the speed of the radio signals is known (they travel at the speed of light), the round-trip distance can then be computed.
There are other factors to consider, too. How long did it take for the ranging tones to "turn around" inside the spacecraft's electronics? That miniscule delay is calculated from pre-launch testing.
How long did it take the ranging tones to travel through the cable from the computer in the Deep Space Network (DSN) signal-processing center out to the radio telescope antenna before leaving Earth? The DSN finds that value while calibrating the system prior to each tracking period.
And how far did the Earth move while the ranging pulses were traveling to the spacecraft? The navigators draw upon data gathered over years and years of observations by the astronomical community....
All three of these types of data that Cassini-Huygens uses for navigation, are subject to the round-trip-light time of around three hours across the distance between Earth and Saturn.
The first type of terrain has more craters than occur near Enceladus' South Pole. The other type of terrain has few craters but many ridges and grooves that may have been created by surface-shifting tectonic activity.
Exogeologists are currently poring over this and other Cassini images from last Wednesday's flyby to better understand the moon's patch-work surface, its unusual ice-geysers, and its potential to support life.
Cassini is scheduled to fly by Enceladus at least nine more times, including an even closer pass of just 25 kilometers this coming October.