Saturn

Explanation of image.


Plot of the illumination in the rings as a function of the distance from Saturn (horizontal axis) and as a function of time (vertical axis). Data were taken in the near infrared with the University of Hawaii adaptive optics system mounted on the Canada-France-Hawaii telescope (f/35 focus). This 42-minute long time-sequence was taken on August 10, 1995 at a mid-time of 12:34 p.m.(Universal time), that is about 8 hours before the crossing. One sees sun light transmitted through the rings and scattered by particles in the C ring, the Cassini division, the Encke gap, and beyond the dark A ring all the way to the F ring. Objects in orbit produce inclined streaks. The brightest of them have been identified as indicated. S5 is one of the three objects discovered by the Hubble Space Telescope (IAU circular No. 6243). Unlabelled marks indicate new objects. Note the temporary disappearance of Epimetheus, in the shadow of the A ring. Adaptive optics observations (August 1995).