![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]()
Pasadena CA (JPL) Dec 06, 2004 Zigzagging kinks and knots dance around Saturn in this movie of the F ring from Cassini. From a great distance, as during Cassini's initial approach to Saturn in mid-2004, the F ring appears as a faint, knotted strand of material at the outer fringe of Saturn's immense ring system. From this close vantage point, just after the spacecraft rounded the planet to begin its second orbit, the F ring resolves into several ringlets with a bright central core. The core of the F ring is about 50 kilometers (31 miles) wide and is located at a distance of approximately 80,100 kilometers (49,800 miles) from Saturn's cloud tops. Scientists have only a rough idea of the lifetime of features like knots and clumps in Saturn's rings, and studies of images, such as those comprising this movie, will help them piece together this story. The view here is from Cassini's southern vantage point, below the ringplane. During the course of the movie sequence, Cassini was headed on a trajectory that took the spacecraft away from the planet and farther south, so that the rings appear to tilt farther upward. To help visualize this, note that the top portion of the F ring is closer to the spacecraft, while the bottom portion is farther away and curves around the far side of Saturn. The movie consists of 44 frames taken three minutes apart, so that the span of time represented in the sequence is almost exactly two hours, or about one-eight of a Saturn rotation. The images that comprise this movie sequence were taken in visible light with the Cassini spacecraft narrow angle camera on Oct. 28, 2004, and at distances ranging from approximately 516,000 kilometers (321,000 miles) to 562,000 kilometers (349,000 miles). No enhancement was performed on the images.
To the left of the gap is the outer B ring with its sharp edge maintained by a strong gravitational resonance with the moon Mimas. To the right of the Huygens Gap are the plateau-like bands of the Cassini Division. The narrow ringlet within the gap is called the Huygens ringlet. The image was taken in visible light with the Cassini spacecraft narrow angle camera on Oct. 29, 2004, at a distance of about 819,000 (509,000 miles) from Saturn. The image scale is 4.5 kilometers (2.8 miles) per pixel.Image Credit: NASA/JPL/Space Science Institute. Community Email This Article Comment On This Article Related Links Cassini-Huygens mission at JPL Cassini imaging team SpaceDaily Search SpaceDaily Subscribe To SpaceDaily Express Explore The Ring World of Saturn and her moons Jupiter and its Moons The million outer planets of a star called Sol News Flash at Mercury
![]() ![]() With its thick, distended atmosphere, Titan's orange globe shines softly, encircled by a thin halo of purple light-scattering haze. |
![]() |
|
The content herein, unless otherwise known to be public domain, are Copyright 1995-2006 - SpaceDaily.AFP and UPI Wire Stories are copyright Agence France-Presse and United Press International. ESA PortalReports are copyright European Space Agency. All NASA sourced material is public domain. Additionalcopyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by SpaceDaily on any Web page published or hosted by SpaceDaily. Privacy Statement |