Introduction to orbital perturbations

Author(s):  
Howard D. Curtis
2021 ◽  
Vol 133 (3) ◽  
Author(s):  
Marilena Di Carlo ◽  
Simão da Graça Marto ◽  
Massimiliano Vasile

AbstractThis paper presents a collection of analytical formulae that can be used in the long-term propagation of the motion of a spacecraft subject to low-thrust acceleration and orbital perturbations. The paper considers accelerations due to: a low-thrust profile following an inverse square law, gravity perturbations due to the central body gravity field and the third-body gravitational perturbation. The analytical formulae are expressed in terms of non-singular equinoctial elements. The formulae for the third-body gravitational perturbation have been obtained starting from equations for the third-body potential already available in the literature. However, the final analytical formulae for the variation of the equinoctial orbital elements are a novel derivation. The results are validated, for different orbital regimes, using high-precision numerical orbit propagators.


Tellus ◽  
1980 ◽  
Vol 32 (4) ◽  
pp. 301-319 ◽  
Author(s):  
David Pollard ◽  
Andrew P. Ingersoll ◽  
John G. Lockwood

Tidal perturbations in the orbits of close Earth satellites permit the Love number K 2 and the phase lag ε 2 of the tidal effective Earth to be estimated. These parameters differ significantly from the nominal values of K 2 = 0.30 and ε 2 < 0.5° that would be expected if only the solid tide was important. This difference is due to the contribution of the oceans to the total tidal potential. This contribution is less well known than the solid tide potential and the study of the orbital perturbations permits an estimation of some of the long wavelength variations in the ocean tide. In this paper we discuss the method and the results obtained from two satellites for the S 2 and M 2 ocean tide. These tidal parameters are compared with and combined with numerical models of these tides to give improved parameters to be used in any orbital theory.


1983 ◽  
Vol 29 (1) ◽  
pp. 27-43 ◽  
Author(s):  
L. Anselmo ◽  
B. Bertotti ◽  
P. Farinella ◽  
A. Milani ◽  
A. M. Nobili

The satellite 1971–54A entered a near-circular orbit with period 95.9 min and inclination 90.2°. Between 1972 and 1978 the orbit passed slowly through 15th-order resonance, when the track over the Earth repeats after 15 revolutions, and the 15th- and 30th-order harmonics in the geopotential may produce substantial orbital perturbations. The values of orbital inclination and eccentricity from 269 weekly U. S. Navy orbits between November 1972 and January 1978 have been ana­lysed to determine 12 lumped harmonic coefficients of order 15 and 30. The analysis of inclination yields 15th-order coefficients accurate to 1.5 and 2.8%, and 30th-order coefficients accurate to 7 %. The analysis of eccentricity gives two 15th-order coefficients accurate to 3 and 4 %. These lumped harmonic coefficients are used to test the accuracy of the Goddard Earth Model 10B, which is complete to order and degree 36. The agreement with GEM 10B is excellent, for both 15th and 30th order, and shows that GEM 10B is more accurate than was expected. The 12 values of lumped harmonics obtained give 12 linear equations between individual coefficients of order 15 and 30, which will be used in a future solution for the individual coefficients.


2016 ◽  
Vol 47 (1) ◽  
pp. 112 ◽  
Author(s):  
H. Drinia ◽  
A. Antonarakou ◽  
S. Mihalakopoulos ◽  
E. Tsiolakis

The main objective of this work is to investigate the climatic influence on the sedimentation during mid to late Pliocene in Cyprus island. For this reason, a section located in Pissouri sub-basin, southern Cyprus, was chosen to be studied. The section comprises a nearly uninterrupted succession of marine sediments, dominated by grey marls, which are cyclically alternating with yellowish silty marls. The identification of age diagnostic planktonic foraminifera suggests a mid to upper Pliocene age. The calculated faunal parameters document cyclic fluctuations consistent with shifts in such climate belts. A good age resolution of the cycles and an indication of sedimentation rate would be required in order to connect cyclicity to orbital perturbations.


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