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SBIR/STTR

Multilayer Polymeric Shielding to Protect Humans from Galactic Cosmic Radiation, Phase II

Completed Technology Project

Project Introduction

Multilayer Polymeric Shielding to Protect Humans from Galactic Cosmic Radiation, Phase II
In Sub-topic X4.01, NASA has identified a need for advanced radiation-shielding materials and structures to protect humans from the hazards of galactic cosmic radiation (GCR) and Solar Energetic Particles (SEP) on long-duration missions, outside the earth's magnetosphere. The radiation species of greatest interest are light ions (particularly protons), heavy ions (such as iron-56) and neutrons. International Scientific Technologies, Inc., in conjunction with the College of William and Mary, in its Phase I program developed lightweight, multi-layered, polymeric shielding against GCR and SEP. The Phase II objectives include analysis and design of single and multi-layered nanocomposite polymeric radiation shields using OLTARIS modeling protocols to supplement the empirical results of Phase I, fabrication of nanocomposite films and multi-layered structures, acquisition of families of test data to determine key parameters of single and multi-layered structures tailored to stopping GCR and SEP, optimization of prototype multi-layered polymeric shields using statistical design and OLTARIS modeling for a range of manned and unmanned NASA applications prior to commercialization in Phase III. The anticipated result of the Phase I and Phase II programs is the development of multi-layered shields with an outer layer of hydrogenous polymeric material for significant dose reduction of incident GCR ions and inner layers of polymeric composites containing additives chosen to moderate and absorb neutrons resulting from fragmentation of incoming heavy ions and to absorb short wavelength electromagnetic radiation resulting from the slowing of the GCR particles and capture of neutrons. The Technology Readiness Level (TRL) at the beginning of Phase II is 4. At the end of Phase II, the TRL will be 5. More »

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