Search for trapped electrons and a magnetic moment at mars by mariner iv.
Search for trapped electrons and magnetic moment at Mars by Mariner IV
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Search for trapped electrons and magnetic moment at Mars by Mariner IV
Radio and radar studies of lunar and planetary ionospheres, atmospheres, and surfaces, sun echoes, and spacecraft instrumentation
Life on small extinct stars and large dark planets
Spacecraft sterilization, discussing hardware development, reduction of biological loading, protection and internal and surface decontamination of lander
Analytical techniques and calculations in planetary quarantine and spacecraft sterilization
High power continuous wave radar transmitter for use as planetary radar system and as proving ground for equipment NASA space program
Astrogeologic studies - lunar and planetary research
Sample acquisition from planetary surface by unmanned probes in life detection experiments
Russian and American practices and policies regarding planetary contamination in connection with COSPAR requirements
Planetary quarantine constraints, noting prevention of Martian atmosphere contamination
Structural synthesis for ablating thermostructural panels in planetary entry environment
Transient thermal analysis and structural analysis for synthesis of ablating thermostructural panels in planetary entry environment
RF voltage breakdown facility for studying spacecraft antenna characteristics in space and planetary atmosphere environments
Test facility for simulating thermodynamic environments of planetary atmospheric entry
The development of slip-cast fused silica is discussed as a heat shield designed to meet the needs of outer-planet entry probes. The distinguishing feature of silica is its ability to reflect the radiation imposed by planetary-entry environments. This reflectivity is particularly sensitive to degradation by the presence of trace amounts of contaminants introduced by the starting materials or by processing. The microstructure of a silica configuration also significantly influences the reflectivity and other thermomechanical properties. The processing techniques attendant on controlling microstructure while maintaining purity are discussed. The selection of a starting material of essential purity precludes the use of purified natural quartz and requires the use of synthetic fused silica. The silica is characterized in a limited combined heating test environment. The surface mass loss is controlled by liquid runoff from a relatively low-temperature melt layer; the reflectance is basically maintained and the material achieves a surprisingly high heat of ablation.
An investigation of electrochemical waste treatment methods suitable for closed, or partially closed, life support systems for manned space exploration is discussed. The technique being investigated involves the electrolysis of solid waste where the aim is to upgrade waste material (mainly fecal waste) to generate gases that can be recycled in a space station or planetary space environment.
The preserved cratering record of Mars indicates that impacts play an important role in deciphering Martian geologic history, whether as a mechanism to modify the lithosphere and atmosphere or as a tool to sample the planet. The various roles of impact cratering in adding a broader understanding of Mars through returned samples are examined. Five broad roles include impact craters as: (1) a process in response to a different planetary localizer environment; (2) a probe for excavating crustal/mantle materials; (3) a possible localizer of magmatic and hydrothermal processes; (4) a chronicle of changes in the volcanic, sedimentary, atmospheric, and cosmic flux history; and (5) a chronometer for extending the geologic time scale to unsampled regions. The evidence for Earth-like processes and very nonlunar styles of volcanism and tectonism may shift the emphasis of a sampling strategy away from equally fundamental issues including crustal composition, unit ages, and climate history. Impact cratering not only played an important active role in the early Martian geologic history, it also provides an important tool for addressing such issues.
Laboratory experiments provide essential first-order constraints on processes affecting ballistic ejecta and styles of ejecta emplacement under different atmospheric environments at planetary scales. The NASA-Ames Vertical Gun allows impacting different fine-grained particulate targets under varying atmospheric pressure and density, thereby helping to isolate controlling variables. Further analysis now permits characterizing distinct modes of emplacement that reflect the degree of ejecta entrainment within a turbidity flow created by ejecta curtain movement through the atmosphere.