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The annual Leonid meteor shower occurs when debris from Comet Tempel-Tuttle
intercepts the Earth at a very high velocity. This debris lies in a collection
of narrow streams produced by different passes of the comet. These streams
are pretty well understood, which has led to high accuracy in predicting
Leonid shower performance. Except for periods of high activity that occur for
several years around Tempel-Tuttle's near passage of Earth (every 33 years),
the Leonids are a fairly minor shower. We are currently in a long period of "normal" Leonid activity,
on the order of 20-40 visual meteors per hour at the maximum. There was no interference from the Moon this year. This is a composite image of
48 Leonid meteors collected on the morning of November 17. Because the
images were collected over several hours, the radiant of the shower is spread out. Not shown in the composite are meteors that were not part of the Leonid shower: 9 Southern Taurids, 7 Northern Taurids, 7 Alpha Monocerotids, and 12 sporadics.
Long necklace-like chains are the trails of stars and planets, rotating around Polaris at the north celestial pole. |