The family of Near Rectilinear Halo Orbits (NRHO) is a promising staging location for future missions to the Moon and to the solar system. Many recent researches proved the effectiveness of such orbits as staging locations, thanks to their low station-keeping cost and low access Δv; the family also provides cheap transfer possibilities to Low Lunar Orbits (LLO) and lunar surface. The paper investigates rendezvous and proximity operations in NRHOs, assuming a reference scenario of a chaser spacecraft that joins a target, controlled but uncooperative, orbiting in a lunar NRHO. The analysis is first conducted under the Circular Restricted Three-Body Problem (CR3BP) assumptions, in order to highlight some features of the orbits and to identify dynamical structures, to be exploited for rendezvous operations. A suitable region for rendezvous is identified, by analysing the spectrum of the State Transition Matrix (STM) of the orbit; the analysis underlines how operations should be performed in an arc, near the aposelene, where the eigenstructure of the STM is more regular, while the periselene region should be avoided, due to the more unstable dynamical behaviour. First, phasing trajectories are analysed, to obtain ballistic phases that allow the two object to be in proximity. Then, the STM is once again exploited, to identify the central eigenvector, i.e. the direction that guarantees a periodic, bounded motion in the neighbourhood of the target orbit. This central direction is used as a reference state, where the chaser spacecraft shall be injected, to obtain a safe hovering trajectory prior to the final approach. Such eigenvector denotes a direction in the six-dimensional position-velocity state, so one degree of freedom is left to the analyst to size the amplitude of the hovering motion. Eventually, the chaser spacecraft is injected into a stable approach trajectory, employing the stable eigenvector of the STM or a direct transfer, according to time-fuel mission constraints.

Relative dynamics analysis and rendezvous techniques for Lunar Near Rectilinear Halo Orbits

BUCCI, LORENZO;Lavagna, Michele;
2017-01-01

Abstract

The family of Near Rectilinear Halo Orbits (NRHO) is a promising staging location for future missions to the Moon and to the solar system. Many recent researches proved the effectiveness of such orbits as staging locations, thanks to their low station-keeping cost and low access Δv; the family also provides cheap transfer possibilities to Low Lunar Orbits (LLO) and lunar surface. The paper investigates rendezvous and proximity operations in NRHOs, assuming a reference scenario of a chaser spacecraft that joins a target, controlled but uncooperative, orbiting in a lunar NRHO. The analysis is first conducted under the Circular Restricted Three-Body Problem (CR3BP) assumptions, in order to highlight some features of the orbits and to identify dynamical structures, to be exploited for rendezvous operations. A suitable region for rendezvous is identified, by analysing the spectrum of the State Transition Matrix (STM) of the orbit; the analysis underlines how operations should be performed in an arc, near the aposelene, where the eigenstructure of the STM is more regular, while the periselene region should be avoided, due to the more unstable dynamical behaviour. First, phasing trajectories are analysed, to obtain ballistic phases that allow the two object to be in proximity. Then, the STM is once again exploited, to identify the central eigenvector, i.e. the direction that guarantees a periodic, bounded motion in the neighbourhood of the target orbit. This central direction is used as a reference state, where the chaser spacecraft shall be injected, to obtain a safe hovering trajectory prior to the final approach. Such eigenvector denotes a direction in the six-dimensional position-velocity state, so one degree of freedom is left to the analyst to size the amplitude of the hovering motion. Eventually, the chaser spacecraft is injected into a stable approach trajectory, employing the stable eigenvector of the STM or a direct transfer, according to time-fuel mission constraints.
2017
68th International Astronautical Congress (IAC 2017)
9781510855373
Aerospace Engineering; Astronomy and Astrophysics; Space and Planetary Science
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11311/1060479
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