Nuclear environmental effects on spacecraft thermal control coatings
Effect of nuclear radiation on optical properties of spacecraft thermal control coatings
SEARCH · Engineering Papers
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Effect of nuclear radiation on optical properties of spacecraft thermal control coatings
Metallurgic, thermodynamic, ultrasonic, polymer, and spectroscopic studies in materials science
Oxygen toxicity as result of increased lipid peroxidation - lysosomal enzymes in rats exposed to 100 percent oxygen, and stability of rat liver and brain lysosomes
White coatings for spacecraft, and ultraviolet and proton radiation effects
Mechanical properties and nitrogen tetroxide stress corrosion resistance of Ti-6Al-4V alloy with different heat treatments
High energy particle and electromagnetic space radiation effects on thermal control coating, noting spectral absorptance for various conditions
Interdisciplinary materials research in inorganic nonmetallic materials, metallic solids, polymers, and solid state physics
High energy particle and electromagnetic space radiation effects on thermal control coating, noting spectral absorptance for various conditions
Friction coefficient and wear variations for spacecraft material, due to cold welding or adhesion in space environment, measured in orbital experiment
Test program to determine Martian dust storm effects on solar cells
Simulated solar wind environment effects on zinc oxide/potassium silicate and lanthanum oxide/ potassium silicate spacecraft thermal control coating pigments
Optimum solar cell cover glass systems selected by studying interplanetary space environment effects of proton impact, temperature and concurrent illumination on radiation damage
Subjection of solar cell assemblages to simulated lunar dust storms in wind tunnels
Candidate materials and space environment effects on crystal growth and other solidification processes
Test results indicate that solder coating cells produces protective or deleterious effect, depending on the environment. Major problem for solder coated cells is in control of solder thickness and uniformity. Problem area for non-solder coated cells is not identified.
Accomplishments made during study of coatings are reported. Development of structure/property theory for selecting most appropriate pigments for space vehicle paints is discussed along with improvements made in zinc-oxide pigmented potassium silicate paint.
The results of a study concerned with the effects of the Martian environment on the performance of solar cells are given. The results indicate that the efficiency of a power system composed of solar cells will be greatly reduced when subjected to dust storms such as may occur on Mars. Two factors are responsible for this, (1) accumulation of dust on the protective covers, and (2) damage to covers by pitting, cracking, and chipping. It is recommended that this type of power system not be used on Mars landing vehicles. Experimental procedures are described and results are summarized and damage assessed.
The ATS-F satellite will carry two cesium ion thrusters. Cesium is a material that is not present in the upper atmosphere, and there is concern that the introduction of this material may result in some unexpected behavior. A study has been conducted to assess the magnitude of the effects that are to be expected. No observable effects were found as a result of the study. Consideration was given to the origin and destination of the material and the various reactions that could occur. The origin was considered to be anywhere in space from altitudes of about 100 km upward. The probable short term destination is in the form of cesium ions trapped in the earth's magnetic field or as ions and atoms in the heterosphere. The maximum possible number of cesium atoms in the field of view of an earth based observer is of the order of one million per square centimeter, far too few to be observable by visible, near-visible, or radio-frequency means. Further, no phenomena could be found that would result in the occurance of an observable event.