Title
Secular dynamics of selected asteroid families: doctoral dissertation
Creator
Tsirvoulis, Georgios, 1987-, 36776551
Copyright date
2019
Object Links
Select license
Autorstvo-Nekomercijalno-Bez prerade 3.0 Srbija (CC BY-NC-ND 3.0)
License description
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Language
English
Cobiss-ID
Theses Type
Doktorska disertacija
description
Datum odbrane: 22.05.2019.
Other responsibilities
mentor
Novaković, Bojan, 1976-, 36796263
član komisije
Knežević, Zoran, 1949-, 17794663
član komisije
Tsiganis, Kleomenis, 1974-, 58163209
član komisije
Kovačević, Anđelka, 1972-, 12839783
Academic Expertise
Prirodno-matematičke nauke
Academic Title
-
University
Univerzitet u Beogradu
Faculty
Matematički fakultet
Alternative title
Sekularna dinamika izabranih familija asteroida
Publisher
[G. Tsirvoulis]
Format
159 listova
description
Astronomy-Planetary astronomy/Astronomija-Planetarna astronomija
Abstract (en)
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...
Abstract (sr)
Asteroidne familije predstavljaju populacije asteroida u glavnom prstenu koji vode
zajedničko poreklo, tj. predstavljaju fragmente nastale u sudaru dve asteroida...
Authors Key words
asteroids, dynamics, families, resonances
Authors Key words
asteroidi, dynamika, familije, rezonance
Classification
523.44:519.654(043.3)
Type
Tekst
Abstract (en)
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...
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