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December 4, 1998:
1998 was a great year for meteor watching. In November the much-anticipated
Leonids produced an outburst of nearly 600 meteors per hour,
punctuated by a spectacular display of fireballs seen worldwide.
The October Giacobinids were also a pleasant surprise for many,
thanks to an outburst over Japan and east Asia. As 1998 winds
down, there is one more opportunity to view a dazzling sky show:
the annual Geminids meteor shower. Right: Artist Duane Hilton's concept of a Geminid fireball streaking above an eerie 12-ft salt tower (or "tufa") in Mono Lake, California. The shower officially begins on December 6th, but it doesn't peak until the night of the 13th. Unlike the Giacobinids and Leonids, the Geminid's broad maximum lasts nearly a full day, so observers around the globe have a good chance to see the show. At its peak the Geminids are expected to produce about one shooting star every 30 seconds. Most well known meteor showers, like the Perseids and Leonids, are old. They've been observed for hundreds or even thousands of years. The earliest record of a modern-day meteor shower is probably a notation in Chinese annals dated 36 AD, regarding the Perseids, where it is said that "more than 100 meteors flew thither in the morning." (ref.) |
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The Geminids are a different story. The first Geminid meteors suddenly appeared in the mid-1800's. Those early showers were unimpressive, boasting a mere 10-20 shooting stars per hour. Since then, however, the Geminids have grown in intensity until today it is one of the most spectacular annual showers. In 1996, the last time the Geminids appeared in a dark moon-less sky, observers saw as many as 110 per hour. Sky-watchers with clear skies should see at least that many this year if the Geminids continue to intensify. |
After the discovery of the Geminids in 1862 astronomers began searching for the parent comet. Most meteor showers result from debris that that boils off a comet's nucleus when it passes close to the sun. This debris orbits the sun along with the comet, forming a thin, elongated stream of meteoroids that become shooting stars when they hit Earth's atmosphere. |
Years of searching proved to no avail until finally, in 1983,
NASA's Infrared Astronomical Satellite discovered a curious object
moving in the same orbit as the Geminid meteoroid stream. The
orbital match was so good that it had to be the source of the
debris, but to the surprise of many it wasn't a comet. The source
of the Geminids was apparently a rocky asteroid. 3200 Phaethon, as the asteroid is now known, is in a highly elliptical 1.4 year orbit that brings it within 0.15 AU (astronomical units) of the Sun. It made its closest recent approach to Earth in December 1997 when it passed within 0.31 AU of our planet. |
Take a virtual tour of the solar system, complete with the curious asteroid 3200 Phaethon, the source of the Geminid meteors. |
So, is Phaethon a comet or an asteroid? There are arguments in favor of both. Phaethon's spectra look like those of a rocky asteroid, but its orbit is similar to that of a comet. When Phaethon passes by the sun it doesn't develop a cometary tail, but bits and pieces do break off to form the Geminid meteoroids. By studying photographic records of fireballs, scientists have estimated the density of the Geminid meteoroids to be between 1 and 2 gm/cc. That's less dense than typical asteroid material (3 gm/cc), but several times denser than cometary dust flakes (0.3 gm/cc). Many astronomers now believe that Phaethon is an extinct or dormant comet that has accumulated a thick crust of interplanetary dust grains. Phaethon's thick mantle gives it the outward appearance of an asteroid, but underneath lies the nucleus of a comet. The origin of the Geminids may not be fully understood until future space travelers pay a visit to the asteroid-comet 3200 Phaethon. Until then we can still enjoy the sky show and savor the mystery of the enigmatic Geminids. |
The image indicates the general region of the sky from which the Geminid meteors appear to emanate (red dot). This point, called the radiant, is really an optical illusion - the meteors are moving along parallel paths, but appear to come from a single point, just as a stretch of parallel railroad tracks will appear to meet at a point on the horizon. |
Web Links | |
Meteors for kids - from the NASA Liftoff Space Academy NASA Liftoff meteor shower pages - learn the basics about meteor showers. Includes tutorials, Java animations, and educational activities. Eyewitness accounts of the historic 1966 Leonid storm -- an Ames Research Center Archive Satellite Tracking - monitor satellites as they weather the storm NASA's Office of Space Science - press releases and other news related to NASA and astrophysics External Links: The Geminids -- from Gary Kronk Meteors and Comets web site December's generous Geminids -- Sky &Telescope article |
Related Stories: 27 Nov. 1998: A bust or a blast? -- New images of 1998 Leonid fireballs and their smokey remnants.23 Nov. 1998: Leonids Sample Return payload recovered! -- Scientists are scanning the "comet catcher" for signs of Leonid meteoroids. 19 Nov. 1998: Early birds catch the Leonids -- The peak of the Leonid meteor shower happened more than 14 hours earlier than experts had predicted. 18 Nov. 1998: A high-altitude look at the Leonids -- NASA science balloon catches video of 8 fireballs. 16 Nov. 1998: The Leonid Sample Return Mission -- NASA scientists hope to capture a Leonid meteoroid and return it to Earth. 16 Nov. 1998: NASA Spacecraft take cover from the Leonids -- but the Hubble Space Telescope won't stop observing. 10 Nov. 1998: Great Expectations: the 1998 Leonid meteor shower -- the basics of what the Leonids are and what might happen on November 17. |
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Tony Phillips |