Trajectory Design for the ESA LISA Mission

被引:47
作者
Martens, Waldemar [1 ]
Joffre, Eric [2 ]
机构
[1] European Space Technol Ctr, Robert Bosch Str 5, D-64293 Darmstadt, Germany
[2] European Space Technol Ctr, Keplerlaan 1, NL-2200 AG Noordwijk, Netherlands
关键词
Formation flying; Laser Interferometer space antenna; Trajectory design; Trajectory optimisation; Deep space navigation;
D O I
10.1007/s40295-021-00263-2
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The three Laser Interferometer Space Antenna (LISA) spacecraft are going to be placed in a triangular formation in an Earth-trailing or Earth-leading orbit. They will be launched together on a single rocket and transferred to that science orbit using Solar Electric Propulsion. Since the transfer Delta v depends on the chosen science orbit, both transfer and science orbit have been optimised together. For a thrust level of 90 mN, an allocation of 1092 m/s per spacecraft is sufficient for an all-year launch in 2034. For every launch month a dedicated science orbit is designed with a corner angle variation of 60 degrees +/- 1.0 degrees and an arm length rate of maximum 10 m/s. Moreover, a detailed navigation analysis of the science orbit insertion and the impact on insertion errors on the constellation stability has been conducted. The analysis shows that Range/Doppler measurements together with a series of correction manoeuvres at the beginning of the science orbit phase can reduce insertion dispersions to a level where corner angle variations remain at about 60 degrees +/- 1.1 degrees at 99% C.L. However, the situation can become significantly worse if the self-gravity accelerations acting during the science orbit phase are not sufficiently characterised prior to science orbit insertion.
引用
收藏
页码:402 / 443
页数:42
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