INTERPRETATION OF THE 3- TO 4-MICRON INFRARED SPECTRUM OF MARS
Interpretation of the 3-to 4- micron spectrum of mars through the study of infrared reflection spectra of organic and inorganic materials
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Interpretation of the 3-to 4- micron spectrum of mars through the study of infrared reflection spectra of organic and inorganic materials
Dual-cavity ruby maser mounted on a paraboloidal antenna is used to achieve stability in mars radar echo experiments
Effect of diurnal freeze-thawing on survival and growth of selected bacteria, under simulated martian conditions
Orbital rendezvous considerations for mars mission requiring tangential approach to, and departure from, orbit to achieve maximum propulsive efficiency
Radar observations of mars, with total echo power measured by a radiometer and analyzed into its frequency spectrum by the autocorrelation approach
Design requirements for a fleet of electrically propelled vehicles for a manned mars expedition, in view of crew safety and mission success
This Handbook contains a series of maps, graphs, and tables which will be of use to the preliminary design analyst in scheduling round-trip interplanetary missions to Mars and Venus in the time period 1965-1999. It constitutes the third in a series of space flight manuals prepared for the George C. Marshall Space Flight Center, NASA. The present Handbook, denoted as Volume 3 of this series, is divided into three Parts. Part 3-1 presents maps for obtaining departure and arrival speeds for trips to these planets, a listing of useful constants, planetary ephemerides, tables of important occurrences, and a number of auxiliary graphs. Although most of the basic calculations were performed for the period 1965 -1980, much of the information is also applicable to the years 1980- 1999, as is explained in the text.
Parts 2 and 3 present tabulations of trajectory data for scheduling flights to and from Venus and Mars during the period 1960-2000. Part 2 contains information for outbound flights to these planets; Part 3 contains information for trajectories returning from the planets to Earth. Each Part contains data for single-plane transfers, as well as for broken-plane transfers which employ a midcourse plane-change to eliminate the high speed "ridges." The mathematical analyses employed for all calculations are described in Part 1 of this handbook. To facilitate the construction of round-trip trajectories, the date at the target planet is held fixed while the trip duration is varied in 10-day increments from zero days to the length of that planet's synodic period with Earth. Dates of arrival at the target planet are presented in the extreme right-hand column of Part 2, and dates of departure from the target planet are presented in the extreme left-hand column of Part 3. Thus, by holding Part 2 directly to the left of Part 3, the analyst may easily and rapidly scan all trip possibilities which involve any desired stopover time at the target planet. Within approximately 200 days of each conjunction or opposition, data are presented in 10-day increments at the target planet. Only those trips are listed for which the hyperbolic excess speeds at either or both ends of the trajectory do not exceed 0.6 EMOS (Earth Mean Orbital Speed). For the remaining mission regions, the requirements are so smoothly varying that a 50-day interval in dates at the target planet may be employed; the 10-day interval in trip times is, however, preserved here. In these regions, only those trips are listed for which either or both speeds do not exceed 0.3 EMOS.
Average surface temperature of planet mars computed from radiation equilibrium
Mars nonstop round-trip trajectories using gravity supplemented by propulsion or aerodynamic forces
Survival of terrestrial microorganism under simulated martian conditions
Three-color photography of mars
Vehicle requirements and mission planning for manned space flight and exploration of mars during 1975-1985 time period
Radio emission theory of venus and mars
Mission for mariner space probe in late 1964 to mars vicinity and return
Feasibility of mars landing and return missions