Life in Extraterrestrial Environments Quarterly Status Report, Aug. 15 - Nov. 15, 1966
Extraterrestrial life in simulated Martian environment, and effects of barometric pressure and carbon dioxide
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Extraterrestrial life in simulated Martian environment, and effects of barometric pressure and carbon dioxide
Planetary reflection spectroscopy for studying extraterrestrial life
Simulated lunar materials research leading to utilization of extraterrestrial resources
Correlation between thermal and mechanical properties of extraterrestrial materials
Ecological experiments on bacteria growth response and survival in different soils simulating extraterrestrial environments
Extraterrestrial dust in stratospheric sampling collected by balloon-borne probe
Noctilucent cloud formation and extraterrestrial dust concentrations in upper atmosphere
Extraterrestrial particles in Greenland polar ice
Life studies of simulated extraterrestrial environments
Gulliver radioisotopic biochemical probe to detect extraterrestrial life
Extraterrestrial life detection method based on catalysis of isotopic oxygen exchange between water and oxygen-containing anions
Extraterrestrial life detection based on catalysis of oxygen exchange between labeled oxyanions and water, noting equipment
In the several years since the Alvarez report of anomalously high iridium concentrations at the Cretaceous-Tertiary boundary, evidence for the involvement of meteorite impacts in biological extinction has increased dramatically. Much more research will be needed, however, before meteorite impact is established as a general causal factor in extinction. Of ever greater long-term interest is the possibility that other extraterrestrial forces have had important influences on the evolution of life. To recognize the effects of such forces, it will be necessary to coordinate the research of astronomy and paleontology so that testable predictions can be formulated. It is possible that known, systematic changes in the Solar System or Galaxy have had effects on global biology and that these effects have been preserved in the paleontological record.
This paper analyzes the technical feasibility of interstellar communication at infrared frequencies, both in its own right and in comparison with communication at radio frequencies. The analysis considers both the practical and fundamental limits affecting communication over interstellar distances and concludes that for specified transmitter and receiver locations communications at infrared and radio frequencies can be equally effective. On this basis a search for extraterrestrial signals at infrared wavelengths is equally as valid as any planned microwave effort. Work is now in progress to adapt a 10 micrometers heterodyne spectrometer to search for CO2 laser signals from 200 nearby stars.
Temperature measurements of black body most closely fitting solar extraterrestrial spectrum
Characteristics of extraterrestrial ring current system observed by Explorer VI and Pioneer V satellites
Survey of extraterrestrial nonsolar X-radiation by Aerobee rocket measurements
Man-machine system for extraterrestrial surface roving vehicles