
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/">
  <dc:language>eng</dc:language>
  <dc:identifier>https://phaidrabg.bg.ac.rs/o:22637</dc:identifier>
  <dc:identifier>cobiss:51952143</dc:identifier>
  <dc:identifier>thesis:7629</dc:identifier>
  <dc:contributor>Novaković, Bojan, 1976-, 36796263</dc:contributor>
  <dc:contributor>Knežević, Zoran, 1949-, 17794663</dc:contributor>
  <dc:contributor>Tsiganis, Kleomenis, 1974-, 58163209</dc:contributor>
  <dc:contributor>Kovačević, Anđelka, 1972-, 12839783</dc:contributor>
  <dc:rights>http://creativecommons.org/licenses/by-nc-nd/2.0/at/legalcode</dc:rights>
  <dc:type>info:eu-repo/semantics/bachelorThesis</dc:type>
  <dc:subject xml:lang="srp">OSNO - Opšta sistematizacija naučnih oblasti, Numerička matematika</dc:subject>
  <dc:subject xml:lang="eng">OSNO - Opšta sistematizacija naučnih oblasti, Numerička matematika</dc:subject>
  <dc:subject xml:lang="srp">OSNO - Opšta sistematizacija naučnih oblasti, Astronomski podaci i konstante</dc:subject>
  <dc:subject xml:lang="eng">OSNO - Opšta sistematizacija naučnih oblasti, Astronomski podaci i konstante</dc:subject>
  <dc:subject xml:lang="srp">asteroidi, dynamika, familije, rezonance</dc:subject>
  <dc:subject xml:lang="eng">asteroids, dynamics, families, resonances</dc:subject>
  <dc:date>2019</dc:date>
  <dc:title xml:lang="eng">Secular dynamics of selected asteroid families: doctoral dissertation : doctoral dissertation</dc:title>
  <dc:creator>Tsirvoulis, Georgios, 1987-, 36776551</dc:creator>
  <dc:format>159 listova</dc:format>
  <dc:format>76519001 bytes</dc:format>
  <dc:description xml:lang="eng">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...</dc:description>
  <dc:description xml:lang="srp">Asteroidne familije predstavljaju populacije asteroida u glavnom prstenu koji vode
zajedničko poreklo, tj. predstavljaju fragmente nastale u sudaru dve asteroida...</dc:description>
  <dc:description xml:lang="eng">Astronomy-Planetary astronomy/Astronomija-Planetarna astronomija  
Datum odbrane: 22.05.2019.</dc:description>
</oai_dc:dc>
