The stability of Lagrangian points in the Earth-Moon system is studied. The problem is carried out when the non-zero eccentricity of the orbits of the two main attracting bodies is taken into consideration. A new criterion to establish stability regions is introduced to aim to be both closer to the Ljapunov definition and suitable for space engineering applications. Some relevant examples are presented.
Stability of the motion near L4 Equilateral lagrangian Point / Valente, Chiara; Marino, Luca; G., Orecchini. - In: ACTA ASTRONAUTICA. - ISSN 0094-5765. - STAMPA. - 46:(2000), pp. 501-506. [10.1016/S0094-5765(00)00010-2]
Stability of the motion near L4 Equilateral lagrangian Point
VALENTE, Chiara;MARINO, Luca;
2000
Abstract
The stability of Lagrangian points in the Earth-Moon system is studied. The problem is carried out when the non-zero eccentricity of the orbits of the two main attracting bodies is taken into consideration. A new criterion to establish stability regions is introduced to aim to be both closer to the Ljapunov definition and suitable for space engineering applications. Some relevant examples are presented.File allegati a questo prodotto
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