ON THE CRITICAL INCLINATION IN SATELLITE THEORY
Abstract
The long-range perturbations of an artificial satellite are investigated in the vicinity of the critical inclination, considering the effect of the second and fourth zonal harmonics in the earth's gravitational field. The traditional remedy to avoid the small divisor by developing into powers of square root of J sub 2 instead of J sub 2 fails even in this relatively simple case. A more involved converging development is given to represent the trajectories. The qualitative properties of the trajectories alter when the eccentricity at the critical inclination becomes smaller than a quantity of the order square root of J sub 2. For the case of small eccentricities the use of Poincare type variables is convenient. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Mar 14, 1962
- Accession Number
- AD0274347
Entities
People
- Imre G. Izsak
Organizations
- Smithsonian Astrophysical Observatory