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meteor shower





Geminid meteors 2012
Geminid meteors, December 2012. Image credit: Tony Burt
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.


Principal night-time meteor showers
shower begins peaks ends max. rate radiant
R.A. /  Dec.
parent object
Quadrantids Jan 1 Jan 3 Jan 6 110 15.5h / +50°  
Alpha Centaurids Jan 28 Feb 8 Feb 21 6 14.0h / -59°  
Gamma Normids Feb 25 Mar 22 Mar 13 8 16.6h / -51°  
Lyrids Apr 16 Apr 22 Apr 25 15 18.1h / +32° Comet 1861 I (Thatcher)
Eta Aquarids Apr 19 May 5 May 28 60 22.8h / 00° Halley's Comet
June Lyrids Jun 10 Jun 15 Jun 21 8 18.5h / +35°  
Pisces Australids Jul 15 Jul 27 Aug 10 8 22.7h / -30°  
Delta Aquarids Jul 15 Jul 28 Aug 19 20 22.6h / -10°  
Alpha Capricornids Jul 3 Jul 29 Aug 15 8 20.3h / -12°  
Perseids Jul 25 Aug 12 Aug 18 100 3.1h / +58° Comet Swift-Tuttle
Alpha Aurigids Aug 25 Aug 31 Sep 5 10 05.6h / +42°  
Draconids Oct 6 Oct 9 Oct 10 var 18.0h / +54° Comet Giacobini-Zinner
Orionids Oct 16 Oct 21 Oct 26 30 06.4h / +15° Halley's Comet
Taurids Oct 20 Nov 4 Nov 25 12 03.7h / +22° Encke's Comet
Cepheids Nov 7 Nov 9 Nov 11 8 23.5h / +63°  
Leonids Nov 15 Nov 17 Nov 19 var 10.1h / +22° Comet Tempel-Tuttle
Puppid-Velids Dec 1 Dec 7 Dec 15 10 08.2h / -45°  
Geminids Dec 7 Dec 14 Dec 15 58 07.5h +32° 3200 Phaethon
Ursids Dec 17 Dec 22 Dec 24 12 14.5h +76° Comet Tuttle B


Meteor storm

A meteor storm is a rare, short-lived event that occurs when Earth encounters a clump of particles within a meteoroid stream – a trai of material that has been released from a comet or asteroid. Meteor storms involve meteor rates exceeding 1,000 per hour.


Related category

   • METEORS AND METEORITES