Stability of Collinear Points in the Generalized Photogravitational Robes Restricted Three-Body Problem  

Stability of Collinear Points in the Generalized Photogravitational Robes Restricted Three-Body Problem

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作  者:AbdulRazaq AbdulRaheem 

机构地区:[1]不详

出  处:《International Journal of Astronomy and Astrophysics》2011年第1期6-9,共4页天文学与天体物理学国际期刊(英文)

摘  要:In studying the effects of radiation and oblateness of the primaries on the stability of collinear equilibrium points in the Robes restricted three-body problem we observed the variations of the density parameter k with the mass parameter μ for constant radiation and oblateness factors on the location and stability of the collin-ear points L1, L2and L3. It is also discovered that the collinear points are unstable for k > 0 and stable for k < 0.In studying the effects of radiation and oblateness of the primaries on the stability of collinear equilibrium points in the Robes restricted three-body problem we observed the variations of the density parameter k with the mass parameter μ for constant radiation and oblateness factors on the location and stability of the collin-ear points L1, L2and L3. It is also discovered that the collinear points are unstable for k > 0 and stable for k < 0.

关 键 词:STABILITY COLLINEAR POINTS Robes Problem DENSITY PARAMETERS 

分 类 号:O1[理学—数学]

 

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