
Strange vertical structures in
Saturn's B ring. Credit:
NASA/JPL/Space Science Institute
Where the Long Shadows Fall
Apr
27, 2011
Wall-like formations in Saturn's
rings could be due to
electromagnetic effects.
A recent press release argues that
Saturn's rings could behave like
spiral galaxies. The same forces
that create galactic "arms" might be
responsible for the unusual features
that have been seen
rising vertically from
the gas giant's ring plane, as well
as for the
oscillations in the B
ring.
According to
Carolyn Porco of NASA's
Cassini-Equinox mission team: "We
have found what we hoped we'd find
when we set out on this journey with
Cassini nearly 13 years ago:
visibility into the mechanisms that
have sculpted not only Saturn's
rings, but celestial disks of a far
grander scale, from solar systems,
like our own, all the way to the
giant spiral galaxies."
Cassini has been in orbit around
Saturn since July 1, 2004. On August
11, 2009 the spacecraft was in
position to observe the giant
planet's
equinox, when its rings
turned edge-on to the Sun, something
that happens every 15 years. During
that phase, several complex
configurations were seen within the
rings: so-called "propellors,"
ridges, and waves rising up as high
as four kilometers. Since the rings
had been long thought to be about
twenty meters thick, anomalous
meta-stable shapes of such dimension
were a complete surprise to mission
specialists.
How do
clumps, undulations, and
ridges form? Researchers suggest
collisions and shock waves initiate
the resonant vibrations.
Gravitational attraction from
so-called "shepherd moons" is said
to be an additional source of
influence. Small moons, such as
Daphnis, do move up and down through
the ring plane, affecting the motion
of ring particles.
However, a far stronger force
than gravity is neglected in their
speculations: Saturn's rings and
moons are electrically charged
objects
moving within its vast
plasmasphere. Instabilities inherent
in that system probably contribute
to the formation of the
perpendicular features.
The effect of shepherd moons is
not like a wind. Gravitational
torque is not seen acting on a cloud
of fine particles. Instead, sine
waves, perpendicular "braids," and
cylindrical arcs are seen. Some are
multiply woven, like those in the
remote F ring. In fact, NASA
scientists now think that the
observed oscillations in the B ring
are not caused by moons or any other
body. Instead, "unforced 'free'
waves grow on their own and then
reflect back again at the edge."
Those waveforms are also thought
to exist within spiral galaxies.
So-called "density wave theory" was
designed to explain how mass
variations within a galaxy, along
with tidal forces from other
galaxies, can induce ordered
structure like spiral arms. Although
those motions can never be observed
on the galactic scale, only in
computer simulations, it is assumed
that a small-scale version is
occurring in Saturn's rings.
Important factors are not
considered in this theory. Bodies
immersed in plasma are not isolated,
they are connected by circuits. Most
of the time they are not in
equilibrium because they are in
unstable conditions. The majority of
them are moving across the plasma
filaments that exist in the Solar
System, in the plasmaspheres around
planets, or in interstellar and
intergalactic space. Currents in
plasma contract into those filaments
and the force between filaments is
linear, so the electromagnetic
fields created by them are the most
powerful long-range attractors in
the Universe, as well as short-range
repulsors.
Those magnetic fields also trace
out the spiral arms in galaxies
because electric current flows
through them, both from the
intergalactic circuit feeding the
galaxy and from the homopolar action
of the galaxy itself. The magnetic
fields exist because the spiral arms
behave as large Birkeland current
filaments.
Since, like a galaxy, Saturn's
ring plane possesses a magnetic
field, diocotron instabilities might
occur in the same fashion as seen in
NGC 3646, for example. It
is in this way that Saturn and
galaxies relate.
Stephen Smith
|