2017
DOI: 10.1016/j.actaastro.2017.02.025
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On the advantages of exploiting the hierarchical structure of astrodynamical models

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Cited by 17 publications
(13 citation statements)
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References 23 publications
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“…Comparatively, the SP is reached more often when departing from smaller halos. Also, there are less multiple SP passage for increasing out-of-plane amplitude; see plots of A z vs other parameters and histograms in position (6,6).…”
Section: Exploration In the Sun-earth-moon Rfbpmentioning
confidence: 99%
See 1 more Smart Citation
“…Comparatively, the SP is reached more often when departing from smaller halos. Also, there are less multiple SP passage for increasing out-of-plane amplitude; see plots of A z vs other parameters and histograms in position (6,6).…”
Section: Exploration In the Sun-earth-moon Rfbpmentioning
confidence: 99%
“…Orbits are sought in the Circular Restricted Three-Body Problem (CRTBP) with Sun and Earth as primaries, in the bicircular Restricted Four-Body Problem (RFBP) that includes the Moon, as well as in a full-ephemeris, three-dimensional restricted n-body model stated in a roto-pulsating frame incorporating non-gravitational forces [7], termed Roto-Pulsating Restricted n-Body Problem (RPRnBP). This design strategy follows the hierarchy of astrodynamical models presented in [6]. A large scale survey is completed encompassing more than 200, 000 initial conditions on several L 1,2 libration point orbits.…”
Section: Introductionmentioning
confidence: 99%
“…The target orbit is a Halo at the L2 point of the Earth-Moon system, with a period of about half a synodic period. The mission has an expected mission lifetime of 1 year [15,16], starting from the 21 March 2024 epoch to 21 March 2025. The trajectory is plotted in Fig.…”
Section: Lumio Trajectorymentioning
confidence: 99%
“…An exhaustive description of the orbit design for LUMIO can be found in [9]. A set of quasi-periodic halo orbits about Earth-Moon L 2 are found by employing the methodology described in [10]. Fourteen quasi-halo orbits are computed in the high-fidelity roto-pulsating restricted n-body problem and saved as SPICE kernels.…”
Section: Orbitmentioning
confidence: 99%