The libration of a lunar satellite
Energy and motion equations for libration of lunar satellite
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Energy and motion equations for libration of lunar satellite
Spacecraft mission to libration centers of Earth- Moon system for collecting meteoroids and photographic program carried out for establishing presence of material at centers
Lagrange-Laplace theory of lunar physical librations extended to include reduced estimate of mechanical ellipticity of lunar equator
Numerical solutions for librational motion of Mercury obtained by applying Runge-Kutta integration
Instability of periodic motions near collinear points of libration in plane restricted three- body problem examined with Liapunov theory
Mathematical analysis of lunar libration point for anchoring communications satellite to backside of moon
Lunar gravity field and physical librations of moon
Motion of spacecraft near triangular libration point of Earth-Moon system
Long period of nonperiodic librational motion about equilateral points of restricted three-body problem
Nonperiodic librational motions in restricted three-body problem for relatively elliptic motion of two finite masses
Structural and librational dynamics of satellite deploying flexible booms or antennas
Feedback control system to position satellite in vicinity of unstable collinear libration point with application to lunar communication problem
Stability analysis of long period Trojan librations treated as short period oscillations about long period reference solution
Periodic motion around triangular libration point in restricted four-body problem of earth-moon-sun system
Feedback control system to position satellite in vicinity of unstable collinear libration point applied to lunar communication problem
Due to the constant observation environment and low energy access of Sun-Earth libration point orbits, they have become extremely popular for many NASA science missions. The nonlinearity and instability of the orbits have made mission analysis more difficult as traditional approximations are no longer applicable. But the sensitivity of the orbits also provides greater flexibility in orbit design. Some typical mission trajectories are examined.
In order to fly an occulter in formation with a telescope at the Sun-Earth L2 (SEL2) Libration Point, one must have a detailed understanding of the dy-namics that govern the restricted three body system. For initial purposes, a linear approximation is satisfactory, but operations will require a high-fidelity modeling tool along with strategic targeting methods in order to be successful. This paper focuses on the challenging dynamics of the transfer trajectories to achieve the relative positioning of two spacecraft to fly in formation at SEL2, in our case, the Wide-Field Infrared Survey Telescope (WFIRST) and a proposed Starshade. By modeling the formation transfers using a high fidelity tool, an accurate V approximation can be made to as-sist with the development of the subsystem design required for a WFIRST and Starshade formation flight mission.
Mission analysis of libration orbit trajectories at Sun-Earth/Moon L2 typically includes predictions of lunar and Earth eclipses during the mission life-time. The NASA James Webb Space Telescope (JWST) trajectory, by design, avoids these eclipses by pruning its launch window. In an off-nominal scenario where an eclipse is predicted, a maneuver strategy is needed. In this paper, trade studies are examined for JWST that characterize the burn magnitude, location, and epochs of multiple maneuver plans to avoid an eclipse. The results enable analysts to explore the space of feasible maneuver strategies during routine operations.