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Orbit Motion Foundations

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Geostationary Satellites Collocation
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Abstract

An attempt is made in this chapter to figure out the main ideas concerning the motion of the Earth, time systems, space reference systems, as well as the non-perturbation Kepler orbit. The problems dealt with in this chapter make use of definitions used in a wide variety of scientific fields, such as astronomy, geodesy, celestial mechanics, timekeeping, and satellite tracking and control. Some certain considerations are taken into account to measure the geostationary orbit.

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References

  1. International Earth Rotation and Reference System Service (IERS). www.iers.org/IERS/EN/IERSHome/home.html?__nnn=true. Accessed 20 Feb 2013

  2. Lieske JH, Lederle T, Fricke W et al (1977) Expressions for the precession quantities based upon the IAU system of astronomical constants. Astron Astrophys 58:1–16

    Google Scholar 

  3. Lieske JH (1979) Precession matrix based on IAU system of astronomical constants. Astron Astrophys 73:282–284

    Google Scholar 

  4. Newcomb S (1898) Tables of the motion of the Earth on its axis and around the Sun. Astron Pap Am Ephemeris XI:1–170

    Google Scholar 

  5. Kinoshita H (1977) Theory of the rotation of the rigid earth. Celest Mech 15:277–326

    Article  MathSciNet  Google Scholar 

  6. Wahr JM (1981) The forced nutations of an elliptical, rotating, elastic, and oceanless earth. Geophys J R Astron Soc 64:705–728

    Article  MATH  Google Scholar 

  7. Seidelmann PK (1982) 1980 IAU theory of nutation: the final report of the IAU Working Group on Nutation. Celest Mech 27:79–106

    Article  MathSciNet  Google Scholar 

  8. Aoki S et al (1982) The new definition of universal time. Astron Astrophys 105:359–361

    Google Scholar 

  9. Montenbruck O, Gill E (2000) Satellite orbits – models, methods, and application. Springer, Berlin/Heidelberg

    Book  Google Scholar 

  10. Ziqing W (2008) China geodetic coordinate system 2000 and its comparison with WGS84. J Geodesy Geodyn 28(5):1–5 (in Chinese)

    Google Scholar 

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© 2014 National Defense Industry Press, Beijing and Springer-Verlag Berlin Heidelberg

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Li, H. (2014). Orbit Motion Foundations. In: Geostationary Satellites Collocation. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-40799-4_2

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  • DOI: https://doi.org/10.1007/978-3-642-40799-4_2

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-40798-7

  • Online ISBN: 978-3-642-40799-4

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