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Secular dynamics of selected asteroid families

Sekularna dinamika izabranih familija asteroida

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2019
Disertacija.pdf (72.97Mb)
IzvestajKomisije23298.pdf (77.57Kb)
Author
Tsirvoulis, Georgios
Mentor
Novaković, Bojan
Committee members
Knežević, Zoran
Tsiganis, Kleomenis
Kovačević, Anđelka
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Abstract
Asteroid families are populations of asteroids in the Main Belt that share a common origin, that is they are the fragments of energetic collisions between two asteroids. Their study over the years has produced a number of important results concerning the collisional and dynamical evolution of the Main Belt, the physical properties of the primordial bodies of the Solar System and the physics of energetic collisions, to name a few. The contribution of the present thesis can be summarized into two main topics: The first is the discovery of a new mechanism that leads to significant perturbations on the orbits of asteroids, and consequently on the evolution of asteroid families affected by it, and the second is the discovery of a couple of new families, each with its own peculiarities...
Asteroidne familije predstavljaju populacije asteroida u glavnom prstenu koji vode zajedničko poreklo, tj. predstavljaju fragmente nastale u sudaru dve asteroida...
Faculty:
University of Belgrade, Faculty of Mathematics
Date:
22-05-2019
Keywords:
asteroids / asteroidi / dynamics / families / resonances / dynamika / familije / rezonance
[ Google Scholar ]
Handle
https://hdl.handle.net/21.15107/rcub_nardus_17474
URI
http://eteze.bg.ac.rs/application/showtheses?thesesId=7629
https://fedorabg.bg.ac.rs/fedora/get/o:22637/bdef:Content/download
http://vbs.rs/scripts/cobiss?command=DISPLAY&base=70036&RID=51952143
https://nardus.mpn.gov.rs/handle/123456789/17474

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