Leonids (LEO) | |
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A Leonid meteor during the peak of Leonids in 2009
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Pronunciation | /ˈliːənɪdz/ |
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 |
The Leonids (/ˈliːənɪdz/ 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.