Recent developments in space power system meteoroid protection
Meteoroid protection for space power systems
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Meteoroid protection for space power systems
Effect of meteoroid flux velocity distribution and angle of impact on design of spacecraft meteoroid protection systems
Meteoroid protection for space radiators
Meteoroid protection for space radiators, reviewing damage effects from impact and the required armor thickness for varying angles of impact
Multiwall meteoroid protection design in Apollo program, discussing bumper, backup sheet and honeycomb cells insulation
Spacecraft meteoroid protective shield thickness sensitivity relationship to luminous efficiency
Procedure for determination of meteoroid protection requirements for spacecraft structures
Determination of armor thickness necessary for meteoroid protection
Space suit meteoroid protection for extravehicular activity, discussing Gemini and lunar surface EVA suits and bumper concept
Space suit meteoroid protection for extravehicular activity, discussing Gemini and lunar surface EVA suits and bumper concept
Photographic meteor data - significance in design of meteoroid protection for large space vehicles
The high closing speed of 57km/s between the spacecraft and Halley poses special problems in the design of the required meteoroid protection. A double wall structure with a total thickness equal to 0.1 to 1 times the diameter of the largest meteoroid encountered is sufficient to stop that meteoroid. However, the unusually high number of meteoroid impacts on the Halley probe will cause significant erosion of the outer wall so that failure of the second wall is more likely to occur from a small meteoroid passing through a previously created hole in the outer wall and then penetrating the second wall. Calculations of the shielding required based on this failure mode, show that a double wall structure must actually have a total thickness 1.2 to 7.3 times the diameter of the largest meteoroid encountered, depending on the size distribution of the meteoroids.
A study was conducted to determine the configuration and performance of a space tug. Detailed descriptions of the insulation, meteoroid protection, primary structure, and ground support equipment are presented. Technical assessments leading to the concept selection are analyzed. The tug mass properties, reliability, and safety assessments are included.
Various aspects of achieving a low mass heat pipe radiator for the nuclear electric propulsion spacecraft were studied. Specific emphasis was placed on a concept applicable to a closed Brayton cycle power sub-system. Three aspects of inter-related problems were examined: (1) the armor for meteoroid protection, (2) emissivity of the radiator surface, and (3) the heat pipe itself. The study revealed several alternatives for the achievement of the stated goal, but a final recommendation for the best design requires further investigation.
Structural integrity, low thermal conductivity, and meteoroid penetration resistance qualities integrated into common tank wall
A new analysis for designing dual-layer shields is presented which is based on energy and momentum conservation, fundamental electromagnetic radiation physics, and the observation of results of extensive experimental impact studies performed at relatively low velocities (near 7 km/s). An important finding is that most of the kinetic energy of a meteoroid striking a dual-layer shield is expended as radiation at the stagnation zone on the face plate of the underlying structure. Systematic procedures for evaluating the response of shield designs for a given impact threat are described. It is noted that similar applications of the analysis can be employed to support a mathematically rigorous procedure for optimum shield design.
Protection of dissipative heat radiators in electric propulsion systems against meteoritic impacts encountered in space travel
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