![]() The one-revolution dust trail is dust that has completed one orbit: the stream of dust released in the return of the comet prior to the current 1862 return. This results in an April Lyrid meteor outburst. ![]() Occasionally, the shower intensifies when the planets steer the one-revolution dust trail of the comet into Earth's path, an event that happens about once every 60 years. However, some meteors can be brighter, known as "Lyrid fireballs", cast shadows for a split second and leave behind smokey debris trails that last minutes. April Lyrid meteors are usually around magnitude +2. Nights without the Moon in the sky will reveal the most meteors. As a result of light pollution, observers in rural areas will see more than observers in a city. Counts typically range from 5 to 20 meteors per hour, averaging around 10. The shower usually peaks around April 22 and the morning of April 23. The Lyrids have been observed and reported since 687 BC no other modern shower has been recorded as far back in time. The April Lyrids are the strongest annual shower of meteors from debris of a long-period comet, mainly because as far as other intermediate long-period comets go (200–10,000 years), this one has a relatively short orbital period of about 415 years. The source of the meteor shower are particles of dust shed by the long-period Comet C/1861 G1 Thatcher. The peak of the shower is typically around April 22 each year. The radiant of the meteor shower is located in the constellation Lyra, near its brightest star, Vega. The April Lyrids are a meteor shower lasting from April 16 to April 25 each year. Radiant point of the April Lyrid meteor shower, active each year around April 22
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