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perturbing body

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  • Discovery of Neptune — New Berlin Observatory at Linden Street, where Neptune was discovered observationally. Neptune was mathematically predicted before it was directly observed. With a prediction by Urbain Le Verrier, telescopic observations confirming the existence… …   Wikipedia

  • Tisserand's parameter — In Celestial Mechanics, Tisserand’s parameter (or Tisserand s invariant) is a combination of orbital elements used in a restricted three body problem.DefinitionFor a small body with semimajor axis a,!, eccentricity e,!, and inclination i,!,… …   Wikipedia

  • John Couch Adams — Infobox Scientist name = John Couch Adams box width = 300px image width = 240px caption = birth date = birth date|1819|06|15 birth place = Laneast, Cornwall, Great Britain death date = death date and age|1892|01|21|1819|06|15 death place =… …   Wikipedia

  • Pluto — This article is about the dwarf planet. For other uses, see Pluto (disambiguation). Pluto   …   Wikipedia

  • Gravitation — is a natural phenomenon by which objects with mass attract one another [http://math.ucr.edu/home/baez/physics/Relativity/GR/grav speed.html Does Gravity Travel at the Speed of Light?] , UCR Mathematics . 1998. Retrieved 3 July 2008] . In everyday …   Wikipedia

  • Secular resonance — A secular resonance is a type of orbital resonance. Secular resonances occur when the precession of two orbits is synchronised (a precession of the perihelion, of the ascending node, or both). A small body in secular resonance with a much larger… …   Wikipedia

  • History of gravitational theory — In physics, theories of gravitation postulate mechanisms of interaction governing the movements of bodies with mass. There have been numerous theories of gravitation since ancient times.AntiquityIn the 4th century BC, the Greek philosopher… …   Wikipedia

  • HAT-P-1b — Planetbox begin name=HAT P 1 bPlanetbox star star=ADS 16402 B constell=Lacerta RA=22h 57m 47s DEC=+38° 40 prime; 30 Prime; dist ly=453 ± 65 dist pc=139 ± 20 class=G0V Planetbox orbit semimajor=0.0553 ± 0.0014 period=4.4652934 ± 0.000093… …   Wikipedia

  • celestial mechanics — the branch of astronomy that deals with the application of the laws of dynamics and Newton s law of gravitation to the motions of heavenly bodies. [1815 25] * * * Branch of astronomy that deals with the mathematical theory of the motions of… …   Universalium

  • Newton's theorem of revolving orbits — Figure 1: An attractive force F(r) causes the blue planet to move on the cyan circle. The green planet moves three times faster and thus requires a stronger centripetal force, which is supplied by adding an attractive inverse cube force. The …   Wikipedia

  • Orbital perturbation analysis (spacecraft) — Isaac Newton in his Philosophiæ Naturalis Principia Mathematica demonstrated that the gravitational force between two mass points is inversely proportional to the square of the distance between the points and fully solved corresponding two body… …   Wikipedia

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