A Collision in Saturn’s Rings
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Saturday, Sept. 21, 2013, at 8:00 AM
A plume of derbis stretches out after a peice of cosmic debris collided with Saturn's rings. Click to encronusenate.
Photo by NASA/JPL-Caltech/Space Science Institute
Photo by NASA/JPL-Caltech/Space Science Institute
Our solar system is a big place. Big enough that it’s overwhelmingly
empty of stuff. You can travel for billions of kilometers and your
chances of smacking into something bigger than a dust particle are very
close to zero.
But given enough time, and enough stuff, eventually collisions do
happen. It helps if you have a big target, too. A really, really big
target. Like, say, Saturn’s rings.
Saturn’s rings aren’t solid: They’re composed of countless tiny
particles of ice. If a piece of interplanetary debris slams into them,
it creates a plume that can stretch for thousands of kilometers. We’ve
actually seen this happen, but only a few times;
the Cassini spacecraft has returned fewer than a dozen instances of
these collisions in the nine years it’s been circling the ringed planet.
But it just saw another. On June 20, 2013, the probe snapped the photo above of a collision in Saturn’s thin outermost discrete ring, called the F-ring.
A closer view of the F-ring event.
Photo by NASA/JPL-Caltech/Space Science Institute
Photo by NASA/JPL-Caltech/Space Science Institute
The ring is only a few hundred kilometers wide, making it a narrow
target. Still, something whacked it pretty well, creating that trail
(also nicknamed a “minijet”). These trails are formed by low-speed
collisions (and by "low-speed", I mean around the velocity of a rifle
bullet or faster; "slow" takes on a different meaning when you're
talking orbital mechanics), probably from a chunk of rock or ice already
orbiting Saturn, following a path slightly more elliptical and/or
slightly tilted with respect to the rings. Like two cars going around a
racetrack, they’re both traveling quite rapidly, but relative to each
other one passes the other somewhat slowly.
Amazingly, this isn’t the first time the F ring has been hit. In August 2009 there was an even more dramatic impact,
one of the first seen (more were discovered later in older pictures).
It’s odd that such a narrow target would get hit so often compared to
the broader rings, but it may be an issue of contrast: A hit in the thin
ring is far easier to spot against the black of space than one in the
wider rings, where you see it against the background of the rings
themselves.
The collision in 2009 was even more dramatic; you can see the shadow of the plume falling across the ethereally thin ring.
Photo by NASA/JPL-Caltech/Space Science Institute
Photo by NASA/JPL-Caltech/Space Science Institute
The impact events are interesting scientifically, since they can tell
us about the frequency of collisions in the outer solar system, the
average size of the objects involved (assuming we see enough collisions
to get some decent statistics), and how the rings react to such an event
(the debris cloud gets stretched out and sheared by orbital effects).
But there is also just something compelling about them, too. And it’s
more than just the idea of cosmic impacts occurring with wild abandon
in space because explosions are cool. It’s the very idea that such
forces continue to work in space all the time, that things change, that a
system as magnificent and vast as Saturn’s rings actually experience
sudden and dramatic effects like this.
When I was a kid, I would read novels about colonies in the outer
planets, excursions by intrepid astronauts to the exotic rings of
Saturn. Now I can see pictures like this and realize that what used to
be fiction is not necessarily always so. What I would give to see an
event like this unfold in real time in front of my eyes, as I hang in
front of a viewport orbiting Saturn itself…
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