The P/Halley Stream: Meteor Showers on Earth, Venus and Mars

  • Apostolos A. ChristouEmail author
  • Jeremie Vaubaillon
  • Paul Withers
Chapter 1: Meteor Shower Activity, Forecasting, Dust Orbits


We have simulated the formation and evolution of comet 1P/Halley’s meteoroid stream by ejecting particles from the nucleus 5000 years ago and propagating them forward to the present. Our aim is to determine the existence and characteristics of associated meteor showers at Mars and Venus and compare them with 1P/Halley’s two known showers at the Earth. We find that one shower should be present at Venus and two at Mars. The number of meteors in those atmospheres would, in general, be less than that at the Earth. The descending node branch of the Halley stream at Mars exhibits a clumpy structure. We identified at least one of these clumps as particles trapped in the 7:1 mean motion resonance with Jupiter, potentially capable of producing meteor ourbursts of ZHR~ 1000 roughly once per century.


1P/Halley Mars Venus Meteors Meteor outbursts Meteor showers 


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Copyright information

© Springer Science+Business Media B.V. 2007

Authors and Affiliations

  • Apostolos A. Christou
    • 1
    Email author
  • Jeremie Vaubaillon
    • 2
    • 3
  • Paul Withers
    • 4
  1. 1.Armagh ObservatoryArmaghNorthern Ireland, UK
  2. 2.IMCCEObservatoire de ParisParisFrance
  3. 3.CalTech/IPAC/SSCPasadenaUSA
  4. 4.Center for Space PhysicsBoston UniversityBostonUSA

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