Voyager 1 Encounters SaturnUnited States. National Aeronautics and Space Administration
Science
Voyager 1 Encounters Saturn
United States. National Aeronautics and Space Administration
Saturn (Planet) -- Photographs from space; Saturn probes; Voyager Project
D-RING
C-RING
B-RING
“SPOKE”
CASSINI DIVISION
ENCKE DIVISION
A-RING
F-RING
[Illustration: 11/8/80 6 million km (3.7 million mi)
The Cassini Division is filled with numerous ringlets. Discovered by
Cassini in 1675, this area between the A- and B-Rings had long been
thought devoid of material. The Voyager observation of well-defined
rings within the Cassini Division was an unexpected discovery.]
[Illustration: 11/12/80 740,000 km (460,000 mi)
Saturn’s ring system, viewed from below, appears dramatically
different from its appearance on the sunlit side. This
computer-processed image shows the F-Ring circling outside the
A-Ring, the A-Ring with its Encke Division, the multiple ringlets in
the Cassini Division, and the optically thick B-Ring, seen here in
magenta hues (the coloration is an artifact of processing and is not
real). The B-Ring appears dark from below the ring plane because it
is dense enough to reflect most of the sunlight, causing it to
appear very bright when seen from the sunward side. The opaline
brightness of the Cassini Division here indicates a great deal of
sunlight being scattered through this region. The Encke Division may
really be empty, since it appears dark from both above and below.]
[Illustration: 11/12/80 720,000 km (450,000 mi)
Outbound and above the ring plane, Voyager 1 gave us this view of
Saturn’s rings eight hours after its closest approach to the planet.
The unique lighting accentuates the many hundreds of bright and dark
ringlets comprising the ring system. The C-Ring (dark gray area)
seems to blend into the brighter B-Ring as the concentric features
radiate out from the planet. The dark spoke-like features seen in
images taken during the approach to Saturn now appear as bright
streaks, indicating that they may be composed of small particles.]
[Illustration: 11/12/80 750,000 km (470,000 mi)
Two narrow, braided rings in the F-Ring are evident in this view, as
well as a broader, very diffuse component about 35 kilometers (20
miles) across. A totally unexpected discovery, the braided rings
trace distinctly separate orbits intertwining each other. The
“knots” may be local clumps of ring material or tiny moons. It is
difficult to explain this complicated structure using only the
gravitational forces known to be affecting the particles of this
ring. It is possible that additional, electrostatic forces may also
influence these particles.]
[Illustration: 11/8/80 7 million km (4.3 million mi)
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account