26-31 Aug 2019 Paris (France)
Meteoroid streams
Jérémie Vaubaillon  1  , Francois Colas  2  
1 : Institut de Mécanique Céleste et de Calcul des Ephémérides
Institut national des sciences de l\'Univers, Observatoire de Paris, Université de Lille, Sorbonne Université, Centre National de la Recherche Scientifique : UMR8028, Institut national des sciences de l\'Univers, Institut national des sciences de l\'Univers, Institut national des sciences de l\'Univers, Institut national des sciences de l\'Univers
2 : Institut de Mécanique Céleste et de Calcul des Ephémérides  (IMCCE)  -  Website
Université Pierre et Marie Curie - Paris 6, Institut national des sciences de l\'Univers, Observatoire de Paris, Centre National de la Recherche Scientifique : UMR8028, Institut national des sciences de l\'Univers
77 av Denfert-Rochereau 75014 Paris -  France

Meteoroid streams produce meteor showers (a.k.a. shooting stars). They evolve in the Solar System as dense swarms revolving around the Sun. When the Earth encounters zone of the streams, the usual risk of collision is multiplied by 3 to 3 orders of magnitude. They represente a threat for artificial satellites because of their space density and very high velocity. We will see how such events are forecasted ans which mitigation solution were implemented so far. Two practical exercises are be proposed:
-determination of the length of a meteor
-example of meteor eyewitness report


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