This book describes a revolutionary new approach to determining
low energy routes for spacecraft and comets by exploiting regions
in space where motion is very sensitive (or chaotic). It also
represents an ideal introductory text to celestial mechanics,
dynamical systems, and dynamical astronomy. Bringing together
wide-ranging research by others with his own original work, much of
it new or previously unpublished, Edward Belbruno argues that
regions supporting chaotic motions, termed weak stability
boundaries, can be estimated. Although controversial until quite
recently, this method was in fact first applied in 1991, when
Belbruno used a new route developed from this theory to get a stray
Japanese satellite back on course to the moon. This application
provided a major verification of his theory, representing the first
application of chaos to space travel.
Since that time, the theory has been used in other space
missions, and NASA is implementing new applications under
Belbruno's direction. The use of invariant manifolds to find low
energy orbits is another method here addressed. Recent work on
estimating weak stability boundaries and related regions has also
given mathematical insight into chaotic motion in the three-body
problem. Belbruno further considers different capture and escape
mechanisms, and resonance transitions.
Providing a rigorous theoretical framework that incorporates
both recent developments such as Aubrey-Mather theory and
established fundamentals like Kolmogorov-Arnold-Moser theory, this
book represents an indispensable resource for graduate students and
researchers in the disciplines concerned as well as practitioners
in fields such as aerospace engineering.
General
Is the information for this product incomplete, wrong or inappropriate?
Let us know about it.
Does this product have an incorrect or missing image?
Send us a new image.
Is this product missing categories?
Add more categories.
Review This Product
No reviews yet - be the first to create one!