Proceedings of the Celestial Mechanics Conference: A modified Hansen lunar theory for artificial satellites

1958 ◽  
Vol 63 ◽  
pp. 430 ◽  
Author(s):  
Paul Herget ◽  
Peter Musen
2015 ◽  
Vol 2015 ◽  
pp. 1-3
Author(s):  
Antonio F. Bertachini A. Prado ◽  
Josep J. Masdemont ◽  
Maria Cecilia Zanardi ◽  
Silvia Maria Giuliatti Winter ◽  
Tadashi Yokoyama ◽  
...  

2012 ◽  
Vol 2012 ◽  
pp. 1-7
Author(s):  
Antonio F. Bertachini A. Prado ◽  
Maria Cecilia Zanardi ◽  
Tadashi Yokoyama ◽  
Silvia Maria Giuliatti Winter ◽  
Josep J. Masdemont

2013 ◽  
Vol 2013 ◽  
pp. 1-5 ◽  
Author(s):  
Antonio F. Bertachini A. Prado ◽  
Josep J. Masdemont ◽  
Maria Cecilia Zanardi ◽  
Silvia Maria Giuliatti Winter ◽  
Tadashi Yokoyama ◽  
...  

1966 ◽  
Vol 25 ◽  
pp. 363-371
Author(s):  
P. Sconzo

In this paper an orbit computation program for artificial satellites is presented. This program is operational and it has already been used to compute the orbits of several satellites.After an introductory discussion on the subject of artificial satellite orbit computations, the features of this program are thoroughly explained. In order to achieve the representation of the orbital elements over short intervals of time a drag-free perturbation theory coupled with a differential correction procedure is used, while the long range behavior is obtained empirically. The empirical treatment of the non-gravitational effects upon the satellite motion seems to be very satisfactory. Numerical analysis procedures supporting this treatment and experience gained in using our program are also objects of discussion.


2012 ◽  
Vol 3 (1) ◽  
pp. 1-19
Author(s):  
Giacaglia Giorgio Eugenio Oscare ◽  

2018 ◽  
Vol 3 (2) ◽  
pp. 207-216 ◽  
Author(s):  
David Fisher ◽  
Lionel Sims

Claims first made over half a century ago that certain prehistoric monuments utilised high-precision alignments on the horizon risings and settings of the Sun and the Moon have recently resurfaced. While archaeoastronomy early on retreated from these claims, as a way to preserve the discipline in an academic boundary dispute, it did so without a rigorous examination of Thom’s concept of a “lunar standstill”. Gough’s uncritical resurrection of Thom’s usage of the term provides a long-overdue opportunity for the discipline to correct this slippage. Gough (2013), in keeping with Thom (1971), claims that certain standing stones and short stone rows point to distant horizon features which allow high-precision alignments on the risings and settings of the Sun and the Moon dating from about 1700 BC. To assist archaeoastronomy in breaking out of its interpretive rut and from “going round in circles” (Ruggles 2011), this paper evaluates the validity of this claim. Through computer modelling, the celestial mechanics of horizon alignments are here explored in their landscape context with a view to testing the very possibility of high-precision alignments to the lunar extremes. It is found that, due to the motion of the Moon on the horizon, only low-precision alignments are feasible, which would seem to indicate that the properties of lunar standstills could not have included high-precision markers for prehistoric megalith builders.


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