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By Keith W.L., Rand R.H.

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1997, ``Planetary ring'', in Encyclopedia of Planetary Sciences, edited by Shirley and Fairbridge, pp. 602±608. , editor, 1997, ``Those magni®cent rings'', in Passage to a Ringed World, The Cassini-Huygens Mission to Saturn and Titan, NASA SP-533, pp. 41±52. Time-Life Books, 1991, ``Mysterious ring worlds', in Moons and Rings (part of a series entitled ``Voyage Through the Universe''), pp. 92±133. jpg [Ch. 1 FIRST OBSERVATIONS OF SATURN'S COMPANIONS The invention of the telescope ended the age of naked-eye astronomy.

Anyone observing this occultation would otherwise turn o€ their recorders a few minutes after the star emerged from behind the planet. There would be no reason to keep recording unless there was a need to con®rm the data dropouts found by the KAO team. Meanwhile, back on the ground, Robert Millis's team also saw the brightness variations in their occultation data. And they too wondered if the dropouts were caused by clouds, equipment problems, or rings. Unfortunately, their Perth Observatory was further east than the KAO ¯ight path and was only able to record the occultation ingress.

The more distant of the two rings (2003U1R) is almost twice the radial distance of the Epsilon ring, the most distant of the previously known rings. The inner of the two new rings (2003U2R) has a radius of 67,300 km and is bounded by the satellite Portia on the inside and Rosalind on the outside [18]. 8). On December 22, 2005, Imke De Pater, Heidi B. Hammel, and Seran Gibbard released an image of these two newly discovered rings. 9). The team had to combine 30 (2-min exposure) images, equivalent to a single one-hour exposure, to make the rings visible [20].

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11 and 21 phase entrainment in a system of two coupled limit cycle oscillators by Keith W.L., Rand R.H.


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