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Meteors

Leonids

General data

ShowerLeonids
IAU Shower Number13
IMO AcronymLEO
Activity intervalNov 8 - Nov 28
Date of maximum in 2010November 17 21:37 UT
Geocentric Velocity71 km/s
Population index2.5

Notes:

  • Population index gives the magnitude distribution of the shower meteors: indexes below 2.5 correspond to distributions where bright meteors are more frequent than average, while values over 3.0 mean that the fraction of faint meteors is larger than usual.

Description

This shower is best known for producing strong meteor storms about every 33 years, which is related to the orbital period of its parent body, comet 55P/Tempel-Tuttle. Last epoch of stormlike activity was between 1999 and 2002.

Meteoroids are fast, with very bright fireballs.

Radiant position and activity

Local circumstances have been computed for latitude ? and longitude ?. Click on any of the two coordinates to set them manually with a map.

DateR.A.Decl.ZHRRise% moon
Maximum154°22°1579
September 4 (0h UTC)Inactive

Meaning of columns is the following:

  • R.A. and Decl.: Right ascension and declination of radiant at maximum, referred to ICRS. ICRS is the reference system used by modern star catalogs.
  • ZHR: Zenith Hourly Rate. It is the maximum number of meteors that an observer could see under ideal conditions, with clear skies and the radiant at zenith.
  • Rise: Time of geometric rise of the radiant, expressed in local time. Symbol * means that the radiant is circumpolar for your latitude.
  • % Moon: Percentage of Moon's illumination at 0h UTC of the given date.

If you are in doubt about these concepts, please visit the meteor area.