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Shoemaker-Levy 9
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Unlike its famous cousins, comet Wild-2 (pronounced "Vilt-2") is a relatively dim, new arrival to the inner solar system. Until recently it circled the Sun in an orbit between Jupiter and Uranus, but everything changed in September 1974 when Wild-2 passed within 0.006 AU of Jupiter. That encounter with the giant planet, at only 10 times the distance which fragmented P/Shoemaker-Levy 9 in 1994, altered Wild-2's orbit so that its closest approach to the Sun now lies just inside the orbit of Mars.
During its first passage relatively near to Earth (1.21
AU) on January 6, 1978, the comet was discovered by Paul Wild.
Since then, the best apparition of Wild-2 was in March 1997 when
it passed within 0.85 AU of our planet, brightening to an unimpressive
10th magnitude. That's too faint to be seen with the naked eye,
but bright enough for modest amateur telescopes.
So, why was the Stardust spacecraft mission targeted to visit an obscure, hard-to-see object like Wild-2, when there are so many more notorious comets to choose from? There are two important reasons:
#1 It's fresh. Before its near miss with Jupiter in 1974 comet Wild-2 was well-preserved in the frigid outer solar system. With its new orbit, Wild-2 now comes much closer to the Sun. When a comet passes close enough to the Sun, some of its material is boiled off into interplanetary space. After about a thousand trips past the Sun, it loses most of its volatile materials and no longer generates a coma or tail. Since Wild-2 has passed the Sun only a few times, it still has most of its dust and gases - it is "pristine." By the time Stardust encounters the comet, Wild-2 will have made only five trips around the Sun. By contrast, Comet Halley has passed the Sun more than 100 times.
#2 It's in the right place at the right time. Wild-2 presents
a unique opportunity -- it is in the right place at the right
time. Scientists found a flight path that allowed the spacecraft
to fly by the comet at a relatively low speed, only 13,600 mph.
Because of this "low velocity" flyby, comet dust can
be captured by collectors on the spacecraft, rather than blowing
right through the collectors and out the back side! This comet
dust can then be brought back to the Earth to be analyzed.
When Stardust caught up with comet Wild-2 on 2 January 2004, both the comet and spacecraft were beyond the orbit of Mars. Although they are far from the Sun, solar heating is still sufficient to cause particles to bubble off the surface of the comet's nucleus. The spacecraft flew within 240 kilometers (149 miles) of Wild-2. Cometary debris hit the dust catcher at up to six times the speed of a bullet fired from a high-powered rifle. To protect Stardust against the blast of expected cometary particles and rocks, the spacecraft rotated so it was flying in the shadow of its "Whipple Shields." The shields are named for American astronomer Dr. Fred L. Whipple, who, in the 1950s, came up with the idea of shielding spacecraft from high-speed collisions with the bits and pieces ejected from comets.
A unique substance called aerogel is the medium that is used to catch and preserve the high speed dust samples. Aerogel is the lightest known solid, and is considered the best substance available for capturing fragile particles from a comet without damaging them. When a high-velocity dust particle hits the aerogel, it buries itself in the material, creating a carrot-shaped track up to 200 times its own length. Since aerogel is translucent scientists can use these tracks to find the tiny particles. The track is largest at the point of entry, and the particle can be collected intact at the point of the cone.
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