Porovnať metódy

	Simulácia N telies	Hohmannov prenos
Odbor	Aplikovaná fyzika	Aplikovaná fyzika
Rodina	Process / pipeline	Process / pipeline
Rok vzniku	1687	1925
Tvorca	Isaac Newton	Walter Hohmann
Typ	Computational simulation algorithm	Trajectory optimization algorithm
Pôvodný zdroj	Poincaré, H. (1892). Les méthodes nouvelles de la mécanique céleste. Gauthier-Villars.	Hohmann, W. (1925). Die Erreichbarkeit der Himmelskörper. R. Oldenbourg.
Ďalšie názvy	gravitational N-body problem, many-body simulation	Hohmann-Vallado transfer, two-impulse maneuver
Príbuzné	5	4
Zhrnutie	N-body simulation is a computational method for modeling the dynamics of a system of particles under mutual gravitational forces. Originating from Newton's laws of motion and gravitation, it solves the fundamental equations of celestial mechanics. This technique is essential for understanding planetary orbits, star cluster evolution, and cosmological structure formation.	The Hohmann transfer is a maneuver that transfers a spacecraft between two circular orbits using two impulsive burns (velocity changes). Introduced by German engineer Walter Hohmann in 1925, it is the most fuel-efficient method for coplanar orbital transfers when the transfer time is not severely constrained. The transfer orbit is an ellipse tangent to both the initial and final orbits.