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Table of contents
1 Introduction
1.1 Meteor showers
1.1.1 Meteoroids
1.1.2 Meteors
1.1.3 Meteorites
1.2 Asteroids and Comets
1.2.1 Asteroids
1.2.2 Comets
1.3 Known asteroids parent bodies of meteor showers
1.4 Motivation of this thesis
2 Analysis procedure based on dynamical parameters
2.1 D-criteria associations
2.2 Databases used in the simulations
2.3 Thresholds selections
2.4 Orbital evolution and Lyapunov time
2.5 Objects association probability
3 Planning and telescopic observations
3.0.1 Visible magnitude limit of telescopes
3.0.2 Airmass
3.1 Observation planing for targets selection
3.1.1 Ephemeride computation
3.1.2 Apparent magnitude computation
3.1.3 Two bodies orbital method vs. full numerical integration
3.2 Data extraction from observation
3.2.1 Photometry with charge coupled devices (CCD)
3.3 Large telescopes
3.3.1 Colors and reflectance extraction
3.3.2 Lightcurve
4 Results
4.1 Dynamical view
4.1.1 Results of other similar studies
4.2 Physical view
4.2.1 Rotation period contribution
4.2.2 Meteor showers and my associations
4.3 Fallen meteors – Meteor Showers – Asteroids association
4.4 Associated asteroids observed
4.4.1 Asteroid (363599) 2004 FG11
4.4.2 Asteroid (259221) 2003 BA21
4.4.3 Asteroid (85953) 1999 FK21
4.5 Results from observations
4.5.1 Asteroid (363599) 2004 FG11 lightcurve
4.5.2 Asteroid (259221) 2003 BA21 lightcurve
4.5.3 Colors and reflectances of asteroids (363599) 2004 FG11 and 85953) 1999 FK21
5 Conclusions and perspectives
A Pseudocode
B Objects found in SMASS–MIT UH–IRTF and processed with M4AST
C Meteor showers data used
D D-parameter and Lyapunov time
