meteor shower Meteors seen to fan out from a single point in the sky, known as the radiant, in a burst of activity lasting for several hours or days. A meteor shower consists of dusty debris, spread out along part of the orbit of a parent body, usually a comet, which Earth intersects at the time each year. In addition to the main meteor showers listed below, there are dozens of others that are more feeble or are detectable only with radar equipment during daylight hours. The Arietids, for example, reaches a maximum hourly rate of 60 on Jun. 7 but takes place unseen against the daytime sky. Some showers vary enormously from year to year. The Leonids are famous for this, normally putting on a modest annual show of up to 15 meteors per hour but, every 33 years or so, when the parent comet, Tempel-Tuttle, is at perihelion and in Earth's neighborhood, capable of staging a meteor storm. In years such as 1799, 1833, and 1966, when the Earth passed particularly close to the stream of debris following in the comet's wake, rates of up to 150,000 meteors per hour were reported. In other cases, the variability is more erratic and linked to changes or a complete breakup of the parent body. For example, the Draconids, also known as the Giacobinids, is usually so weak as to be unrecognizable to the untrained eye, but has been known to produce storms, as happened in 1933 and 1946 when several thousand meteors per hour were seen. The Andromedids, also known as the Bielids is best known for two sensational displays, on Nov. 27, 1872 and 1885, following the destruction of the parent, Biela’s Comet, in the mid-19th century, when the hourly rate reached 6,000 and 75,000, respectively. Since then, gravitational perturbations have gradually pulled the meteor stream out of Earth’s path until today the Andromedids are very weak.
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