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Extra resources for A-10 Warthog in detail & scale - D&S Vol. 19
207–219, April–June 2005.  Carter, T. , ‘Fuel-Optimal Rendezvous Near a Point in General Keplerian Orbit’, Journal of Guidance, Control and Dynamics, Vol. 10, Issue no. 6, pp. 567–573, November–December 1987.  Vadali, S. , Vaddi, S. S. and Alfriend, K. , ‘A New Concept for Controlling Formation Flying Satellite Constellations’, in AAS/AIAA Space Flight Mechanics Meeting, Santa Barbara, California, February 11–14, 2001, AAS 01–218. indb 6 18/02/12 1:15 PM 2 Two body orbital motion Abstract: Orbital mechanics is the study of the motion of planets and satellites in Space.
The Celestial Sphere is an imaginary sphere of infinite radius upon which the celestial bodies are assumed to be fixed. This is the analogy with planetariums where the Earth’s center is at the center of the celestial bodies that are projected upon the inner walls of the planetarium. The Earth’s radius is not significant in comparison, and the calculations are based upon the assumption that the terrestrial observations are made from the center of the Earth rather than at the surface. The Celestial Equator is the great circle of the Celestial Sphere formed by extending the plane of the Earth’s equator until it cuts the celestial sphere (equinoctial equator).
Pedro A. S. in Electrical Engineering from the University of Puerto Rico at Mayaguez, Puerto Rico. He concentrated in analog and digital electronics and is certified in the analysis of satellite photos using remote sensing and pattern recognition. , he joined Dr. Peter M. Bainum as his graduate student at Howard University in Washington, DC. E. D. in Mechanical Engineering. In his graduate studies, he mainly researched space flight dynamics and control, and formation flying. In 2008, Dr. Capó-Lugo was employed by NASA George C.