Salīdzināt metodes

	N-ķermeņu simulācija	Lamberta problēma (orbītas noteikšana)
Nozare	Lietišķā fizika	Lietišķā fizika
Saime	Process / pipeline	Process / pipeline
Izcelsmes gads	1687	1761
Autors	Isaac Newton	Johann Heinrich Lambert
Tips	Computational simulation algorithm	Orbital computation algorithm
Pirmavots	Poincaré, H. (1892). Les méthodes nouvelles de la mécanique céleste. Gauthier-Villars.	Lambert, J. H. (1761). Acta Helvetica. Physico-Mathematico-Anatomico-Botanico-Medica.
Citi nosaukumi	gravitational N-body problem, many-body simulation	Lambert's problem, Lambert-Godstein trajectory problem
Saistītās	5	4
Kopsavilkums	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.	Lambert's problem is a classical astrodynamics boundary-value problem that determines an orbit connecting two points in space given a transfer time. Formulated by Johann Heinrich Lambert in the 18th century, it is fundamental to trajectory design for interplanetary missions and spacecraft maneuvers. The solution provides the orbital elements and velocities needed to transition between two positions.