Buch, Englisch, 123 Seiten, Format (B × H): 160 mm x 241 mm, Gewicht: 3435 g
Reihe: Springer Theses
Buch, Englisch, 123 Seiten, Format (B × H): 160 mm x 241 mm, Gewicht: 3435 g
Reihe: Springer Theses
ISBN: 978-3-662-52691-0
Verlag: Springer
This prizewinning PhD thesis presents a general discussion of the orbital motion close to solar system small bodies (SSSBs), which induce non-central asymmetric gravitational fields in their neighborhoods. It introduces the methods of qualitative theory in nonlinear dynamics to the study of local/global behaviors around SSSBs. Detailed mechanical models are employed throughout this dissertation, and specific numeric techniques are developed to compensate for the difficulties of directly analyzing. Applying this method, several target systems, like asteroid 216 Kleopatra, are explored in great detail, and the results prove to be both revealing and pervasive for a large group of SSSBs.
Zielgruppe
Research
Autoren/Hrsg.
Fachgebiete
- Naturwissenschaften Astronomie Astrophysik
- Technische Wissenschaften Maschinenbau | Werkstoffkunde Technische Mechanik | Werkstoffkunde Statik, Dynamik, Kinetik, Kinematik
- Technische Wissenschaften Verkehrstechnik | Transportgewerbe Luft- und Raumfahrttechnik, Luftverkehr
- Mathematik | Informatik Mathematik Numerik und Wissenschaftliches Rechnen Chaos-Theorie
- Naturwissenschaften Physik Angewandte Physik Astrophysik
- Mathematik | Informatik EDV | Informatik Professionelle Anwendung Computersimulation & Modelle, 3-D Graphik
- Mathematik | Informatik Mathematik Geometrie Dynamische Systeme
- Technische Wissenschaften Bauingenieurwesen Technische Dynamik (Modalanalyse), Erdbebensicherheit
- Mathematik | Informatik Mathematik Numerik und Wissenschaftliches Rechnen Nichtlineare Wissenschaft
Weitere Infos & Material
Introduction.- SSSB Model and equations of motion.- Stability of equilibrium points and the local behavior of orbits.- Topology and stability of large-scale periodic orbits.- Resonant orbit near the equatorial plane.- Free motion of a particle close to the surface of SSSBs.- Conclusions and future directions.