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Applications of the Kustaanheimo-Stieffel transformation of the perturbed two-body problemThe Newtonian differential equations of motion for the two-body problem can be transformed into four linear harmonic-oscillator equations by simultaneously applying the regularization step dt/ds = r and the Kustaanheimo-Stieffel (KS) transformation. The regularization step changes the independent variable from time to a new variable s, and the KS transformation transforms the position and velocity vectors from Cartesian space into a four-dimensional space. A derivation of a uniform, regular solution for the perturbed two-body problem in the four-dimensional space is presented. The variation-of-parameters technique is used to develop expressions for the derivatives of ten elements (which are constants in the unperturbed motion) for the general case that includes both perturbations which can arise from a potential and perturbations which cannot be derived from a potential. This ten-element solution has mixed secular terms that degrade the long-term accuracy during numerical integration. Therefore, to eliminate these terms, the solution is modified by introducing two additional elements.
Document ID
19740034844
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Bond, V. R.
(NASA Johnson Space Center Houston, Tex., United States)
Date Acquired
August 7, 2013
Publication Date
July 1, 1973
Subject Category
Space Sciences
Report/Patent Number
AAS PAPER 73-219
Meeting Information
Meeting: Astrodynamics Conference
Location: Vail, CO
Country: US
Start Date: July 16, 1973
End Date: July 18, 1973
Sponsors: American Astronautical Society, American Institute of Aeronautics and Astronautics
Accession Number
74A17594
Distribution Limits
Public
Copyright
Other

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