Lunar orbits for telecommunication and navigation services  

作　　者：Marco Cinelli Emiliano Ortore Giovanni Mengali Alessandro A.Quarta Christian Circi 

机构地区：[1]Istituto di Astrofisica e Planetologia Spaziali(IAPS),Istituto Nazionale di Astrofisica(INAF),Via del Fosso del Cavaliere 100,Roma,00133,Italy [2]School of Aerospace Engineering,Sapienza University of Rome,Via Salaria 881,Rome,00138,Italy [3]Department of Civil and Industrial Engineering,University of Pisa,Pisa,56122,Italy [4]Department of Astronautical,Electrical,and Energy Engineering,Sapienza University of Rome,Via Salaria 851,Rome,00138,Italy

出　　处：《Astrodynamics》2024年第1期209-220,共12页航天动力学（英文）

基　　金：M.Cinelli was supported by the G4S_2.0 project,developed under the auspices of the Italian Space Agency(ASI)within the framework of the Bando Premiale CICOT-2018-085;the co-participation of the Italian Institute for Astrophysics(INAF)and the Politecnico di Torino(POLITO).

摘　　要：Orbits that are frozen in an averaged model,including the effect of a disturbing body laying on the equatorial plane of the primary body and the influence of the oblateness of the primary body,have been applied to probes orbiting the Moon.In this scenario,the main disturbing body is represented by the Earth,which is characterized by a certain obliquity with respect to the equatorial plane of the Moon.As a consequence of this,and of the perturbing effects that are not included in the averaged model,such solutions are not perfectly frozen.However,the orbit eccentricity,inclination,and argument of pericenter present limited variations and can be set to guarantee the fulfillment of requirements useful for lunar telecommunication missions and navigation services.Taking advantage of this,a practical case of a Moon-based mission was investigated to propose useful solutions for potential near-future applications.

关 键 词：lunar orbits frozen orbits lunar telecommunications lunarnavigation services 

分 类 号：O17[理学—数学]