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The Relativity Effect in Planetary Motions

G. M. Clemence

G. M. Clemence

  • U. S. Naval Observatory, Washington, D. C.

Rev. Mod. Phys. 19, 361 – Published 1 October, 1947

DOI: https://doi.org/10.1103/RevModPhys.19.361

References (12)

  1. A. S. Eddington, The Mathematical Theory of Relativity (Cambridge University Press, Teddington, England, 1924), second edition, p. 89
  2. A. Einstein, "Die Grundlage der allgemeinen Relativitätstheorie," Ann. d. Physik 49, 769 (1916)
  3. G. M. Clemence, "The motion of Mercury 1765-1937," Astro. Pap. Am. Ephemeris 11, 1 (1943)
  4. H. R. Morgan, "The earth's perihelion motion," Astro. J. 50, 127 (1945)
  5. Eric Doolittle, "The secular variations of the elements of the orbits of the four inner planets computed for the epoch 1850.0 G.M.T.," Trans. Am. Phil. Soc. 22, 37 (1925)
  6. J. H. Oort, "The constants of precession and of galactic rotation," Bull. Astro. Inst. Netherlands 9, 424 (1943)
  7. N. E. Dorsey, "The velocity of light," Trans. Am. Phil. Soc. 34, 1 (1944)
  8. W. de Sitter, edited and completed by Dirk Brouwer, "On the system of astronomical constants," Bull. Astro. Inst. Netherlands 8, 213 (1938)
  9. Dirk Brouwer, "The motion of a particle with negligible mass under the gravitational attraction of a spheroid," Astro. J. 51, 223 (1945)
  10. F. Tisserand, Traité de Mécanique Céleste 4, 537 (1896)
  11. H. N. Russell, Note on ellipticity in eclipsing binaries, Astrophys. J. 90, 641 (1939)
  12. Lloyd Motz, "The apsidal motion in binary stars built on a point-source convective-core model with varying guillotine factor," Astrophys. J. 94, 253 (1941)

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