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Leonid meteor shower

Leonids (LEO)
Leonid Meteor.jpg
A Leonid meteor during the peak of Leonids in 2009
Pronunciation /ˈlənɪdz/
Discovery date 902 AD (first record)
Parent body 55P/Tempel–Tuttle
Radiant
Constellation Leo
Right ascension 10h 08m
Declination +22°
Properties
Occurs during November 15 – November 20
Date of peak November 18
Velocity 71 km/s
Zenithal hourly rate Varies
See also: List of meteor showers

The Leonids (/ˈlənɪdz/ LEE-ə-nidz) are a prolific meteor shower associated with the comet Tempel–Tuttle. The Leonids get their name from the location of their radiant in the constellation Leo: the meteors appear to radiate from that point in the sky. Their proper Greek name should be Leontids (Λεοντίδαι, Leontídai), but the word was initially constructed as a Greek/Latin hybrid and it has been used since. They peak in the month of November.

Earth moves through the meteoroid stream of particles left from the passages of a comet. The stream comprises solid particles, known as meteoroids, ejected by the comet as its frozen gases evaporate under the heat of the Sun when it is close enough – typically closer than Jupiter's orbit. The Leonids are a fast moving stream which encounter the path of Earth and impact at 72 km/s. Larger Leonids which are about 10 mm across have a mass of half a gram and are known for generating bright (apparent magnitude -1.5) meteors. An annual Leonid shower may deposit 12 or 13 tons of particles across the entire planet.


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