PIA 12788
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While NASA's Cassini spacecraft was pointed to study Saturn's F ring, it happened to catch a globular star cluster passing through the camera's field of view.
This movie is a concatenation of 13 images each taken about three minutes apart that show NGC 5139, or Omega Centauri. Some of the cluster's stars can even be seen through the ring's narrow Keeler Gap near the end of the movie. The cluster was in Ptolemy's star catalogue but was officially discovered by Edmond Halley in 1677 and was recognized as a globular cluster by John Herschel.
This view looks toward the northern, unilluminated side of the rings from about 53 degrees above the ring plane. The stars on average were brightened by a factor of 10 relative to Saturn's rings. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on March 29, 2009. The view was acquired at a distance of approximately 1.2 million kilometers (746,000 miles) from Saturn and at a sun-Saturn-spacecraft, or phase, angle of 57 degrees. Image scale is 7 kilometers (4 miles) per pixel.
The Cassini Equinox Mission is a joint United States and European endeavor. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.
For more information about the Cassini Equinox Mission visit http://ciclops.org, http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.
Credit: NASA/JPL/Space Science Institute
Released: July 20, 2010 (PIA 12788)
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