Secular dynamics of selected asteroid families
Sekularna dinamika izabranih familija asteroida
Докторанд
Tsirvoulis, GeorgiosМентор
Novaković, BojanЧланови комисије
Knežević, ZoranTsiganis, Kleomenis
Kovačević, Anđelka
Метаподаци
Приказ свих података о дисертацијиСажетак
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...