In a recent radio experiment, the Cassini spacecraft mapped the structure of Saturn Ring with clarity never before available, the US space agency NASA said on Monday.

This is the first of many such observations Cassini will be conducting over the summer. During its lifetime, Cassini will obtain 20 radio occultations and 80 stellar occultations, providing far more detailed knowledge of the ring structures, according to the Jet Propulsion Laboratory of the National Aeronautics and Space Administration (NASA), which is operating the spacecraft.

An occultation means that if you watch Cassini from Earth, Cassini would appear hidden behind the rings. During a radio occultation, Cassini sends a radio signal from the spacecraft through the rings to Earth.

Scientists then watch how the strength of the radio signal is affected as the signal passes through ring material. The denser a ring is, the weaker the signal received. The experiment helps scientists map the distribution of the amount of ring material and determine the ring particle sizes.

During this occultation, Cassini has obtained a first ever look ever at Saturn's B ring, which has eluded previous robotic explorers. Its structure seems remarkably different from its two neighbors, rings A and C.

The origin of Saturn's rings is a mystery. The rings are an enormous, complex structure. From edge-to-edge, the ring system would not even fit in the distance between Earth and the Moon. The seven main rings are labeled in the order they were discovered. From the planet outward, they are D, C, B, A, F, G and E.

"The structure of those remarkable rings is a sight to behold. All ring features appear to be populated by a broad range of particle sizes that extend to many meters in diameter at the upper end," said Essam Marouf, Cassini radio science team member.

Marouf said that at the lower end, particles of about 5 centimeters in diameter or less seem to be scarce in ring B and inner ring A. In rings C and outer ring A, particles of less than about 5 centimeters in diameter seem to be abundant.

Cassini found that the inner and outer parts of ring B contain rings that are hundreds of kilometers wide and vary greatly in the amount of material they contain.

A thick, 5,000-km-wide core contains several bands with ring material that is nearly four times as dense as that of ring A and nearly 20 times as dense as that of ring C.

The dramatically varying structure of ring B is in sharp contrast to the relatively flat structure of ring A or the gentle, wavy structure of ring C, where many dense, narrow and sharp-edged ringlets permeate its outer part.

Cassini also detected more than 40 wavy features called " density waves" in ring A, many near its outer region, close to the moons orbiting just outside the ring. The density wave observations will tell more about the ring surface mass density, its vertical thickness and other physical properties.

"A marvelous array of waves, caused by gravitational interactions with nearby moons, has been uncovered throughout ring A," said Marouf in a statement.

"We also see a major density wave in the dense ring B. Some of these waves have been seen in Voyager and other Cassini observations, but not in this large number and not with this exceptional clarity."

Cassini conducted this first radio occultation observation of Saturn's rings, atmosphere and ionosphere on May 3, 2005. This occultation was the first ever to use three radio signals of different frequencies transmitted simultaneously from a spacecraft to Earth-receiving stations of NASA's Deep Space Network.

Source: Xinhua