A uniformly valid asymptotic representation of satellite motion around the smaller primary in the restricted three-body problem.
Perturbation technique to study three-body problem of motion of close satellite
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Perturbation technique to study three-body problem of motion of close satellite
Orbit determination with Davidon method in obtaining maximum likelihood values
Planetary approach orbit determination target errors using Mariner IV Doppler tracking data
Timing data and real time orbit determination computer program
Influence of Doppler tracking system oscillator instability on orbit accuracy
Orbit determination of two spacecraft using earth based multiple link Doppler tracking data
Systems manual program description R 104 Master Orbit Tape Routine for computing inertial, geocentric, geodetic position, velocity, real field, and geomagnetic data for satellites
On-board tracking system of two-way coherent Doppler between entry capsule and orbiting bus for determining orbit of entry capsule and estimating atmospheric parameters.
Booster and upper stage system capabilities of placing payloads into Mars orbit
Effect of nodal regression of orbit on gravity gradient precession of gyroscopic satellite in testing general theory of relativity
Orbital prediction and differential correction using Vintis spheroidal theory for artificial satellites
Numerical and analytical methods for orbit computation in celestial mechanics during and beyond collision by introduction of regularized coordinates
Manned orbiting stopover round trips to Venus are studied for departure dates between 1975 and 1986 over a range of trip times and stay times. The use of highly elliptic parking orbits at Venus leads to low initial weights in Earth orbit compared with circular orbits. For the elliptic parking orbit, the effect of constraints on the low altitude observation time on the initial weight is shown. The mission can be accomplished with the Apollo level of chemical propulsion, but advanced chemical or nuclear propulsion can give large weight reductions. The Venus orbiting mission weights than the corresponding Mars mission.
Set of uniform variational orbit parameters for space trajectory analysis
Photograph evaluation for determining orbits of meteor bodies
Quasilinear set of formulas developed for finite transformations
Numerical lunar theory for satellite moving in orbital planes with higher inclinations than orbit plane of sun