Symmetrization of the two-body problem
Two-body problem symmetrization - application to atmospheric drag perturbations
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Two-body problem symmetrization - application to atmospheric drag perturbations
Recursive generation of expansion coefficients of time-dependent f and g series in two-body problem, using algebraic recurrence formulas
Transcendental functions and Kepler equation modifications in two body problem
Two-body problem completely generalized closed- form solution for coordinates and partial derivatives
Lagrange-Hamilton-Jacobi mechanics and application to two-body problem
Recursive computation of coefficients for time dependent f and g series solution to two-body problem of Keplerian motion
Coefficients calculated for Taylor series expansion about two points - application of Taylor expansion to two-body problem
Universal variable parameters and formulas used for two-body problem, differential correction and various orbits and perturbations
Perturbation theory for two-body problem, using regularized Levi-Civita variables
Modifications to minimum variance program for processing real data, including two-body problem solution, and modified Kalman filter with bias errors
Derivation of set of two body parameters and their associated perturbation equations - polar oblateness problem
Approximation of lunar trajectory by two fixed-center problem
Perturbation theory of two-fixed-center problem leading to approximation of three-body problem
Perturbation theory of two-fixed-center problem leading to restricted three-body approximation
Generalized problem of two fixed centers - motion of material point in conservative field with force function
Analytical expressions for two-body linear guidance matrices in velocity dependent coordinate system for variant motion equation solutions
An exploratory analysis of vehicle guidance during the approach to a target planet is presented. The objective of the guidance maneuver is to guide the vehicle to a specific perigee distance with a high degree of accuracy and minimum corrective velocity expenditure. The guidance maneuver is simulated by considering the random sampling of real measurements with significant error and reducing this information to prescribe appropriate corrective action. The instrumentation system assumed includes optical and/or infrared devices to indicate range and a reference angle in the trajectory plane. Statistical results are obtained by Monte-Carlo techniques and are shown as the expectation of guidance accuracy and velocity-increment requirements. Results are nondimensional and applicable to any planet within limits of two-body assumptions. The problem of determining how many corrections to make and when to make them is a consequence of the conflicting requirement of accurate trajectory determination and propulsion. Optimum values were found for a vehicle approaching a planet along a parabolic trajectory with an initial perigee distance of 5 radii and a target perigee of 1.02 radii. In this example measurement errors were less than i minute of arc. Results indicate that four corrections applied in the vicinity of 50, 16, 15, and 1.5 radii, respectively, yield minimum velocity-increment requirements. Thrust devices capable of producing a large variation of velocity-increment size are required. For a vehicle approaching the earth, miss distances within 32 miles are obtained with 90-percent probability. Total velocity increments used in guidance are less than 3300 feet per second with 90-percent probability. It is noted that the above representative results are valid only for the particular guidance scheme hypothesized in this analysis. A parametric study is presented which indicates the effects of measurement error size, initial perigee, and initial energy on the guidance requirements. Measurement error size significantly affects both guidance accuracy and velocity-increment expenditure. The initial trajectory, as given by its perigee and energy, affects the velocity-increment expenditure but not final guidance accuracy.
A trajectory-optimization process is described in which the optimum thrust equations are derived using the calculus of variations. The magnitude of the thrust is constrained within an upper and a lower bound, but the thrust direction is arbitrary. This formulation allows both the constant-thrust program and the variable-thrust program to be considered. For the constant-thrust program, certain propulsion-system parameters are optimized for maximum final vehicle mass. This theory has been used to study interplanetary missions to Venus and Mars using a power-limited propulsion system. Both one-way and round trip rendezvous trajectories are considered. The analysis employs a two-body inverse-square force-field model of three dimensions. An iterative routine used to solve the two-point boundary-value problem is described in the Appendix.