Analysis of Rosetta Interplanetary Navigation

2003 ◽  
Author(s):  
Jose Manuel Sanchez Perez
2014 ◽  
Vol 51 (4) ◽  
pp. 1014-1028 ◽  
Author(s):  
T. J. Martin-Mur ◽  
G. L. Kruizinga ◽  
P. D. Burkhart ◽  
F. Abilleira ◽  
M. C. Wong ◽  
...  

1955 ◽  
Vol 8 (1) ◽  
pp. 35-40
Author(s):  
J. G. Porter

Most people know something about space ships nowadays, and probably think that navigation in space is quite a simple matter; at any rate, it is a subject that is glossed over very briefly in most books on the subject. In my view, space navigation is not a simple matter, and it has certainly not received the attention it deserves. Navigation on the Earth is easy, because of the one important fact that you are on the surface of the Earth. A couple of sights, measuring the angles from two stars down to the horizon, together with the azimuths of the stars and the distance from the centre of the Earth, will give an exact statement of position. But out in space there is no Earth, no horizon—in fact nothing whatever to use as a basis of measurement. Clearly then, two angles are not enough; a third one is needed, to give a sort of tripod of sights—two of the legs being anchored to two planets (or the Sun and a planet) because their positions in space at any time are known, and the distance between them can be used as a base-line. The solution of all the triangles involved is indeed a difficult problem, but there is also the impossibility of making three simultaneous observations. It might be thought that one could do as at sea and take one sight followed later by others, making allowance for the motion of the ship in the intervals. However, this involves the idea of dead reckoning, which, although a useful concept at sea, is quite impossible to apply in space, as the following example shows.


1950 ◽  
Vol 3 (4) ◽  
pp. 365-377
Author(s):  
R. d'E. Atkinson

It is clearly not possible, in the space of one paper, even to touch on all aspects of interplanetary navigation, and some whole fields must be ruled out from the start. This paper will not be concerned with any discussion of the space-flight as such; there is no point in considering navigational problems at all unless one can assume (at least for the sake of argument) that there is to be some practicable way of lifting a ship out of the Earth's gravitational field, and then of accelerating it out of the Earth's orbit; but even granting this major premise a considerable amount of selection is still essential.


1988 ◽  
Vol 11 (2) ◽  
pp. 103-109 ◽  
Author(s):  
J. Rodney Jee ◽  
Ahmad R. Khatib ◽  
Ronald J. Muellerschoen ◽  
Bobby G. Williams ◽  
Mark A. Vincent

1980 ◽  
Vol 56 ◽  
pp. 351-357
Author(s):  
J. L. Fanselow ◽  
O. J. Sovers ◽  
J. B. Thomas ◽  
F. R. Bletzacker ◽  
T. J. Kearns ◽  
...  

AbstractThe Jet Propulsion Laboratory of the California Institute of Technology has been developing a radio-astrometric catalogue for use in the application of radio interferometry to interplanetary navigation and geodesy. The catalogue consists of approximately 100 compact extragalactic radio sources whose relative positions have formal uncertainties of the order of 0”.01. The sources cover nearly all of the celestial sphere above -40° declination. By using the optical counterparts of many of these radio sources, we have tied this radio reference frame to the FK4 optical system with a global accuracy of approximately 0”.01. This paper describes the status of this work.


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