Muutke küpsiste eelistusi

Complex Planetary Systems II (IAU S382): Latest Methods for an Interdisciplinary Approach (KavliIAU) [Kõva köide]

Edited by (University of Namur, Belgium), Edited by (University of Namur, Belgium)
Teised raamatud teemal:
Teised raamatud teemal:
IAU Symposium 382, Complex Planetary Systems II (CPS II), presented a real opportunity to show the power of interdisciplinary collaboration through gathering astronomers of many disciplines together. Complex systems are those composed of interacting parts whose local behavior, resulting from the interactions between them, cannot provide a complete understanding of the global, macroscopic behaviour. This requires complex systems to be studied by transdisciplinary teams, who together are able to understand the whole construction and critically analyze the connections among the different levels of description. The huge number of available observations, from ground and space, their improved precision, and the computational power available today, have spectacularly changed the nature of the dynamical models, especially for planetary evolution studies. CPS II, a Kavli–IAU Symposium, opened new doors, created collaborations, exchanges of ideas, and combinations of techniques – sometimes unexpected – to meet the challenges of the complex astronomical systems.

The huge number of available observations, from ground and space, their improved precision, and the computing power available today, have spectacularly changed the nature of dynamical models of planetary evolution. IAU S382 (CPS II) gathered astronomers of many disciplines together to critically analyse these complex astronomical systems.

Muu info

In IAU S382 (CPS II) astronomers from many disciplines critically analyse the complex systems involved in planetary evolution studies.
1. The obliquity of Mercury: Models and interpretation Rose-Marie
Baland;
2. Dynamics of circumstellar planets in binary star systems Man Hoi
Lee;
3. Long-term stability and dynamical spacing of compact planetary
systems Antoine Petit;
4. Long-term evolution of exoplanet systems Cristobal
Petrovich;
5. Derivation and properties of the angular momentum relative
amended potential Daniel Scheeres;
6. Progress report on the BEBOP search for
circumbinary planets with radial velocities Thomas Baycroft;
7. Transversal
Yarkovsky acceleration for Apophis through jet transport Luis Benet;
8. Tidal
effects in resonant chains of close-in planets: TTV analysis of Kepler-80
Carolina Charalambous;
9. Revisiting the Cassini states of synchronous
satellites with an angular momentum approach Alexis Coyette;
10. Lagrangian
descriptors and their applications to deterministic chaos Jérôme Daquin;
11.
Deconvolving the complex structure of the asteroid belt Stanley Dermott;
12.
Towards a complete picture of the evolution of planetary systems around
evolved stars Mats Esseldeurs;
13. Multi-planet systems explored: the case of
the HD34445 system revisited Nikolaos Georgakarakos;
14. Stability maps for
the 5/3 mean motion resonance between Ariel and Umbriel with inclination
Sérgio Gomes;
15. Migration of giant planets in low viscosity discs and
consequences on the Nice model Philippine Griveaud;
16. Secular resonances
and terrestrial planet formation in planetary systems with multiple stars
Nader Haghighipour;
17. Positive weathering feedback compensates carbonates
at shallow ocean depths Kaustubh Hakim;
18. Hazardous asteroids and space
situational awareness Do Look Up! Daniel Hestroffer;
19. Secular resonance
maps Zoran Kneevi;
20. On the retrograde planar co-orbital asteroid motion
with Jupiter Thomas Kotoulas;
21. Sun-planets tidal interactions: an extended
catalog Sergey Kudryavtsev;
22. New semi-analytical calculation of lunar,
solar and planetary perturbations in motion of Earth satellites Sergey
Kudryavtsev;
23. Can the stellar dynamical tide destabilize the resonant
chains of planets formed in the disk? Leon Ka-Wang Kwok;
24. Medium Earth
orbit secular resonances and navigation satellites Edoardo Legnaro;
25.
Investigation of the dynamical evolution of planetary systems with
isotropically varying masses Mukhtar Minglibayev;
26. On the long-term
orbital evolution of a satellite revolving around an oblate body Gabriela
Nadabaica;
27. Food for thought Yael Naze;
28. On the computation of resonant
tidal dissipation in the liquid layers of planets and stars Jeremy Rekier;
29. Secular dynamics of a coplanar, non-resonant planetary system, consisting
of a star and two planets Vladislav Sidorenko;
30. Chaotic diffusion in the
GJ 876 exoplanetary system Raphael Silva;
31. Jovian encounter manifolds
Nataa Todorovi;
32. On the predictability horizon in Impact Monitoring of
Near-Earth Objects Giacomo Tommei;
33. Excitation of the obliquity of
Earth-like planets via tidal forcing using the Andrade rheology Ema Valente;
34. Comparison of Mars rotation angle models Marie Yseboodt;
35. Collision
outcomes due to planetesimal and planetary embryo interactions in inclined
binary star systems Maximilian Zimmermann.