Rings of Saturn
Page 4
The ring system of Saturn is divided into
5 major components: the
G, F, A, B, and C rings, listed from outside
to inside (but in reality,
these major divisions are subdivided into
thousands of individual
ringlets). The F and G rings are thin and
difficult to see, while the
A, B, and C rings are broad and easily visible.
The large gap
between the A ring and and the B ring is
called the Cassini division.
The adjacent image is a rare view of Saturn's
rings seen just after
the Sun has set below the ring plane, taken
with the Hubble Space
Telescope on Nov. 21, 1995. This perspective
is unusual because
the Earth is slightly above and the Sun
slightly below the rings.
Normally we see the rings fully illuminated
by the Sun.
Three bright ring features are seen: the
F Ring, the Cassini
Division, and the C Ring (moving from the
outer rings
to the inner). The low concentration of
material in these rings allows
light from the Sun to shine through them.
The
A and B rings are much denser, which limits
the amount of light that
penetrates through them. Instead, they are
faintly visible because they reflect light
from Saturn's disk (Ref).
Ring Structure and Composition
High resolution photographs from the Voyager
missions indicate
that the rings of Saturn are composed of
hundreds of thousands of
"ringlets", and that regions like the largest
"gap" called the
Cassini division, also contain fainter rings
(adjacent image). The
rings cannot be solid, because they lie
inside the Roche limit. They
presumably represent either a satellite
torn apart by tidal forces,
or (more likely) material that was never
allowed to condense into
moons because of the tidal forces. The evidence
indicates that the
rings are composed of particles that are
mostly ice crystals, with
sizes as large as centimeters or meters.
The total mass in the rings
is about the size of a medium mass moon,
and the rings are only
about 10 km thick.
Rings information
Saturn's Rings
Name
Radius inner
----
------
D-Ring
67,000
C-Ring
74,500
Maxwell Division 87,500
B-Ring
92,000
Cassini Division 115,800
Huygens Gap
117,680
A-Ring
122,200
Encke Minima
126,430
Encke Division 133,580
F-Ring
140,210
G-Ring
165,800
E-Ring
180,000
Saturn's Rings
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