* Astronomy

The Cassini spacecraft has confirmed earlier suspicions of an unseen moon hidden in a gap in Saturn's outer A ring. A new image and movie show the new moon and the waves it raises in the surrounding ring material.

The moon, provisionally named S/2005 S1, was first seen in a time- lapse sequence of images taken on May 1, 2005, as Cassini began its climb to higher inclinations in orbit around Saturn. A day later, an even closer view was obtained, which has allowed a measure of the moon's size and brightness.
The tiny object is located in the centre of the Keeler gap and the wavy patterns in the gap edges that are generated by the moon's gravitational influence. The Keeler gap is located about 250 kilometres inside the outer edge of the A ring, which is also the outer edge of the bright main rings.


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The new object is about 7 kilometres across and reflects about half the light falling on it -- a brightness that is typical of the particles in the nearby rings.
"It's too early to make out the shape of the orbit, but what we've seen so far of its motion suggests that it is very near the exact centre of the gap, just as we had surmised." - Dr. Joseph Spitale, imaging team associate and planetary scientist at the Space Science Institute in Boulder, Colo.

The new moonlet orbits approximately 136,505 kilometres from the centre of Saturn.
S/2005 S1 is the second known moon to exist within Saturn's rings. The other is Pan, 25 kilometres across, which orbits in the Encke gap. Atlas and other moons exist outside the main ring system, as do the two F ring shepherd moons, Prometheus and Pandora.
Imaging scientists had predicted the new moon's presence and its orbital distance from Saturn after last July's sighting of a set of peculiar spiky and wispy features in the Keeler gap's outer edge. The similarities of the Keeler gap features to those noted in Saturn's F ring and the Encke gap led imaging scientists to conclude that a small body, a few kilometres across, was lurking in the centre of the Keeler gap, awaiting discovery.
An estimate of the moon's mass, along with a measure of its size, yields information on its physical makeup. For instance, the new moonlet might be quite porous, like an orbiting icy rubble pile. Other moons near the outer edge of Saturn's rings - like Atlas, Prometheus and Pandora - are also porous. Whether a moon is porous or dense says something about how it was formed and its subsequent collision history.
The Keeler gap edges also bear similarities to the scalloped edges of the 322-kilometer-wide Encke gap, where the small moon Pan (25 kilometres across) resides. From the size of the waves seen in the Encke gap, imaging scientists were able to estimate the mass of Pan. They expect to do the same eventually with this new moon.

"Some of the most illuminating dynamical systems we might hope to study with Cassini are those involving moons embedded in gaps. By examining how such a body interacts with its companion ring material, we can learn something about how the planets in our solar system might have formed out of the nebula of material that surrounded the Sun long ago. We anticipate that many of the gaps in Saturn's rings have embedded moons, and we'll be in search of them from here on." - Dr. Carolyn Porco, imaging team leader at the Space Science Institute.



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