Titlebook: Long-Term Dynamical Behaviour of Natural and Artificial N-Body Systems; Archie E. Roy Book 1988 Kluwer Academic Publishers 1988 Celestial

Haphazard

Some Models for the Motion of the Co-orbital Satellites of Saturnyager spacecraft took in 1980 and 1981 of Saturn’s co-orbiting satellites Janus (1980S1) and Epimetheus (1980S3) (see Stone and Miner, 1981, and Smith et al. 1981, 1982), although there is evidence of previous optical observations of these satellites (Dollfus, 1981, Smith, 1980, Larson, 1981, Seidel

endure

漸強(qiáng)

Bravado

fixed-joint

蠟燭

Astrodynamics in the Real-World Environment (The Whole Truth and Nothing but the Truth)y and the accuracy of that theory. To do this, one needs to know the true orbit so that the differences between the predicted orbit and the true orbit can be measured. But how does one go about determining this “true orbit”? A commonly accepted procedure is to generate a reference for comparison by

鳥(niǎo)籠

Further Numerical Investigations into the Significance of Bode’s Laws. The results are not favourable to Bode’s Law. This is partly explained by the fact that the “l(fā)aw” loses much of its unusualness when it is a priori assumed that all stable planetary distributions obey the stronger “l(fā)aw of increasing differencws”.

initiate

骨

潰爛

Astrodynamics in the Real-World Environment (The Whole Truth and Nothing but the Truth)al system, but also on computational roundoff and truncation errors. With proper implementation, however, these errors can be minimized and the numerically generated ephemerides may be treated as a reliable reference which simulates a “true” orbit over a limited time period. This hypothetical refere