Skip to product information
1 of 1
Regular price £83.99 GBP
Regular price £98.00 GBP Sale price £83.99 GBP
Sale Sold out
Free UK Shipping

Freshly Printed - allow 8 days lead

Multi-scale (Time and Mass) Dynamics of Space Objects (IAU S364)

IAU S364 covers advances in the multi-scale dynamics of natural and artificial space objects for graduate students and researchers.

Alessandra Celletti (Edited by), Cristian Beaugé (Edited by), C?t?lin Gale? (Edited by), Anne Lemaître (Edited by)

9781108490764, Cambridge University Press

Hardback, published 28 July 2022

284 pages
25.2 x 18 x 1.5 cm, 0.62 kg

The range of phenomena that manifest at all different time and length scales and the wide range of sizes of space objects, from minor bodies in the Solar System to exoplanets, and from dust particles to Jupiter-size bodies, require the development of dynamical modeling and analysis tools that can handle these different scales. This volume collects contributions given by distinguished scientists at the hybrid IAU Symposium 364. The methods in dynamics modeling of space objects have already reached a state of maturity, and their implementation provided a large number of important results pertaining to both the theory and their applications. The contributions cover the recent advances in the multi-scale dynamics of natural and artificial space objects from various perspectives, which will benefit graduate students and researchers working in the fields of celestial mechanics, astrodynamics, planetary sciences, applied mathematics and dynamical systems.

1. Dynamical constraints on the evolution of the inner asteroid belt and the sources of meteorites
2. On tides and exoplanets
3. Evolution of INPOP planetary ephemerides and Bepi-Colombo simulations
4. The Lidov-Kozai resonance at different scales
5. A numerical criterion evaluating the robustness of planetary architectures
6. New results on orbital resonances
7. Latitudinal variations of charged dust in co-orbital resonance with Jupiter
8. Chaos identification through the auto-correlation function indicator (ACFI)
9. Closed-form perturbation theory in the Sun-Jupiter restricted three body problem without relegation
10. The current orbit of Atlas (S XV)
11. Evolution and stability of Laplace-like resonances under tidal dissipation
12. Back-tracing space debris using proper elements
13. Four- and five-body periodic Caledonian orbits
14. Satellites' orbital stability through normal forms
15. Noise, friction and the radial-orbit instability in anisotropic stellar systems: stochastic N-body simulations
16. A cartographic study of spin-orbit coupling in binary asteroids
17. Probabilistic evolution of pairs of trans-Neptunian objects in close orbits
18. Multiple bifurcations around 433 Eros with Harmonic Balance Method
19. The effect of the passage of Gliese 710 on Oort cloud comets
20. Weak stability transition region near the orbit of the Moon
21. Secular dynamics in extrasolar systems with two planets in mutually inclined orbits
22. Dynamics around the binary system (65803) Didymos
23. Orbit propagation around small bodies using spherical harmonic coefficients obtained from polyhedron shape models
24. The semi-analytical motion theory of the third order in planetary masses for the Sun-Jupiter-Saturn-Uranus-Neptune's system
25. On the scattering and dynamical evolution of Oort cloud comets caused by a stellar fly-by
26. Planetary and lunar ephemeris EPM2021 and its significance for solar system research
27. Some of the most interesting cases of close asteroid pairs perturbed by resonance
28. Characterization of the stability for trajectories exterior to Jupiter in the restricted three-body problem via closed-form perturbation theory
29. Astrometry and photometry of asteroids from the UkrVO database of astroplates
30. Families of periodic orbits around asteroids: from shape symmetry to asymmetry
31. Oscillations around tidal pseudo-synchronous solutions for circumbinary planets
32. Apsidal alignment in migrating dust: crescent features caused by eccentric planets
33. Cascade disruption in Rampo family
34. An algorithm for automatic identification of asymmetric transits in the TESS database.

Subject Areas: Astrophysics [PHVB], Solar system: the Sun & planets [PGS], Astronomy, space & time [PG]

View full details