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Periodic, Quasi-Periodic and Chaotic Motions in Celestial Mechanics: Theory and Applications

Overview of attention for book
Periodic, Quasi-Periodic and Chaotic Motions in Celestial Mechanics: Theory and Applications
Springer Netherlands

Table of Contents

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    Book Overview
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    Chapter 1 On the variational approach to the periodic n -body problem
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    Chapter 2 On families of periodic solutions of the restricted three-body problem
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    Chapter 3 Hip-hop solutions of the 2N-body problem
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    Chapter 4 Double choreographical solutions for n -body type problems
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    Chapter 5 From the circular to the spatial elliptic restricted three-body problem
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    Chapter 6 Stability of axial orbits in galactic potentials
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    Chapter 7 KAM tori for N -body problems: a brief history
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    Chapter 8 Analysis of the chaotic behaviour of orbits diffusing along the Arnold web
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    Chapter 9 The scattering map in the planar restricted three body problem
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    Chapter 10 On final evolutions in the restricted planar parabolic three-body problem
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    Chapter 11 Quaternions and the perturbed Kepler problem
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    Chapter 12 The 3:2 spin-orbit resonant motion of Mercury
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    Chapter 13 Symmetric and asymmetric librations in extrasolar planetary systems: a global view
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    Chapter 14 The influence of mutual perturbations on the eccentricity excitation by jet acceleration in extrasolar planetary systems
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    Chapter 15 Symmetric and asymmetric 3:1 resonant periodic orbits with an application to the 55Cnc extra-solar system
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    Chapter 16 Estimations of orbital parameters of exoplanets from transit photometry by using dynamical constraints
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    Chapter 17 Critical inclination in the main problem of a massive satellite
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    Chapter 18 Long-term effects of the Galactic tide on cometary dynamics
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    Chapter 19 Dependence on the observational time intervals and domain of convergence of orbital determination methods
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    Chapter 20 Collision risk against space debris in Earth orbits
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    Chapter 21 On target for Venus — set oriented computation of energy efficient low thrust trajectories
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    Chapter 22 Weak stability boundary trajectories for the deployment of lunar spacecraft constellations
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    Chapter 23 Aero-gravity assist maneuvers: controlled dynamics modeling and optimization
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    Chapter 24 Analytical theory of a lunar artificial satellite with third body perturbations
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    Chapter 25 Precise measurement of the solar gravitational red shift
Attention for Chapter 3: Hip-hop solutions of the 2N-body problem
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Chapter title
Hip-hop solutions of the 2N-body problem
Chapter number 3
Book title
Periodic, Quasi-Periodic and Chaotic Motions in Celestial Mechanics: Theory and Applications
Published in
Celestial Mechanics and Dynamical Astronomy, January 2006
DOI 10.1007/978-1-4020-5325-2_3
Book ISBNs
978-1-4020-5324-5, 978-1-4020-5325-2
Authors

Barrabes, Esther, Esther Barrabés, Josep Maria Cors, Conxita Pinyol, Jaume Soler, Cors Iglesias, Josep Maria, Pinyol, Conxita, Soler Villanueva, Jaume, Barrabés, Esther, Cors, Josep Maria, Soler, Jaume

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Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 1. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 07 January 2014.
All research outputs
#21,358,731
of 23,854,458 outputs
Outputs from Celestial Mechanics and Dynamical Astronomy
#458
of 504 outputs
Outputs of similar age
#154,819
of 158,740 outputs
Outputs of similar age from Celestial Mechanics and Dynamical Astronomy
#1
of 1 outputs
Altmetric has tracked 23,854,458 research outputs across all sources so far. This one is in the 1st percentile – i.e., 1% of other outputs scored the same or lower than it.
So far Altmetric has tracked 504 research outputs from this source. They typically receive a little more attention than average, with a mean Attention Score of 5.8. This one is in the 1st percentile – i.e., 1% of its peers scored the same or lower than it.
Older research outputs will score higher simply because they've had more time to accumulate mentions. To account for age we can compare this Altmetric Attention Score to the 158,740 tracked outputs that were published within six weeks on either side of this one in any source. This one is in the 1st percentile – i.e., 1% of its contemporaries scored the same or lower than it.
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