Abstract
Newton’s final version (published in 1726) of Philosophiae Naturalis Principia Mathematica was a great scientific achievement of the time and contained sufficient information to allow calculation of the dynamics of terrestrial and celestial bodies; it also expounded on the absolute nature of time and space. As examples, Newton’s statements (Newton in Principia: the mathematical principles of natural philosophy, New York, 1726) that “Absolute, true, and mathematical time, of itself, and from its own nature flows equably without regard to anything external” and “Absolute space, in its own nature, without regard to anything external, remains always similar and immovable” were fundamental to Newtonian calculations. These Newtonian concepts of space and time were challenged and proven to be only approximate by Einstein through his 1905 paper on special relativity, as well as his discovery of general relativity in 1915. The implications for and applications of general relativity within the fields of space geodesy is discussed in this chapter.
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Acknowledgements
A script to generate Fig. 2.1 was kindly provided by Urs Hugentobler, Institute of Astronomical and Physical Geodesy, Technische Universität München. The comments and suggestions by Roberto Peron of Istituto di Fisica dello Spazio Interplanetario (IFSI-INAF) were very valuable and contributed to the readability of this chapter. This work is based on research supported by the National Research Foundation of South Africa under grant IFR2011041500034.
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Combrinck, L. (2013). General Relativity and Space Geodesy. In: Xu, G. (eds) Sciences of Geodesy - II. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-28000-9_2
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