Inverse Problem of Astrodynamics  

作　　者：Yuri Menshikov 

机构地区：[1]Department of Mechanics and Mathematics, Dnepropetrovsk University, Dnepropetrovsk, Ukraine

出　　处：《World Journal of Mechanics》2015年第12期249-256,共8页力学国际期刊（英文）

摘　　要：We consider the problem of determining the center of mass of an unknown gravitational body, using the disturbances in the motion of observed celestial bodies. In this paper an universal approach to obtain the approximate and stable estimate of problem solution is suggested. This approach can be used in other fields of Science. For example, it can be applied for investigation of interactions between fields of forces and elementary particles using known trajectories of elementary particles motions.We consider the problem of determining the center of mass of an unknown gravitational body, using the disturbances in the motion of observed celestial bodies. In this paper an universal approach to obtain the approximate and stable estimate of problem solution is suggested. This approach can be used in other fields of Science. For example, it can be applied for investigation of interactions between fields of forces and elementary particles using known trajectories of elementary particles motions.

关 键 词：ASTRODYNAMICS LE Verrier Problem REGULARIZATION MAIN HYPOTHESIS 

分 类 号：O1[理学—数学]