Skip main navigation bar NASA Glenn Research Center
Electro-Physics Branch

[GRC Hanger link to Glenn Research Center Home Page]

[NASA Logo link to NASA national site]

Ultraviolet and Vacuum Ultraviolet Radiation Abstracts


 


Vacuum Ultraviolet Radiation and Atomic Oxygen Durability Evaluation of HST Bi-Stem Boom Thermal Shield Materials

Bellows-type thermal shields were proposed for use on the Hubble Space Telescope (HST) solar array bi-stem booms to reduce the thermal gradient-induced jitter during orbital thermal cycling. Candidate thermal shield materials included aluminized FEP Teflon with and without protective coatings for durability to atomic oxygen (AO) and combined AO and ultraviolet (UV) radiation. NASA Lewis (now Glenn) Research Center performed vacuum ultraviolet (VUV) radiation and AO durability testing of candidate materials as part of an overall program coordinated by NASA Goddard Space Flight Center (GSFC) to evaluate the on-orbit durability of these thermal shield materials.

Coating adhesion problems were observed for samples having AO- and the combined AO/UV-protective coatings which were attributed to exposure to rapid thermal cycling used to simulate thermal cycling on orbit. Such adhesion problems led to production of coating flakes from the material which could pose a significant risk to HST optics if the coated materials were used for the bi-stem boom thermal shields. No serious degradation was observed for the uncoated aluminized Teflon as evaluated by optical microscopy, although atomic force microscopy (AFM) revealed that an embrittled surface layer would build up on the uncoated Teflon surface due to ultraviolet radiation exposure. This embrittled layer was not completely removed by AO erosion. Despite the formation of this embrittled layer, no cracks or particle flakes were produced for the uncoated material upon exposure to VUV and AO.

Uncoated aluminized FEP Teflon was determined to be the most appropriate thermal shield material and was used on the replacement solar arrays installed during the December 1993 First HST Servicing Mission.

[horizontal rule]

Simulated Space Vacuum Ultraviolet (VUV) Exposure Testing for Polymer Films

Vacuum ultraviolet (VUV) radiation of wavelengths between 115 and 200 nm produced by the sun in the space environment can cause degradation to polymer films producing changes in optical, mechanical, and chemical properties. These effects are particularly important for thin polymer films being considered for ultra-lightweight space structures, because, for most polymers, VUV radiation is absorbed in a thin surface layer. NASA Glenn Research Center has developed facilities and methods for long-term ground testing of polymer films to evaluate space environmental VUV radiation effects. VUV exposure can also be used as part of sequential simulated space environmental exposures to determine combined damaging effects. This paper will describe the effects of VUV on polymer films and the necessity for ground testing. Testing practices used at Glenn Research Center for VUV exposure testing will be described including characterization of the VUV radiation source used, calibration procedures traceable to the National Institute of Standards and Technology (NIST), and testing techniques for VUV exposure of polymer surfaces.

[horizontal rule]

International Test Program for Synergistic Atomic Oxygen and VUV Exposure of Spacecraft Materials

Spacecraft in low Earth orbit (LEO) are subject to degradation in thermal and optical performance of components and materials through interaction with atomic oxygen and vacuum ultraviolet radiation which are predominant in LEO. Due to the importance of LEO durability and performance to manufacturers and users, an international test program for assessing the durability of spacecraft materials and components was initiated. Initial tests consisted of exposure of samples representing a variety of thermal control paints and multiplayer insulation materials that have been used in space. Materials donated from various international sources were tested alongside a material whose performance is well known such as Teflon FEP or Kapton H for multiplayer insulation, or Z-93-P for white thermal control paints. The optical, thermal or mass loss data generated during the test was then provided to the participating material supplier. Data was not published unless the participant donating the material consented to the publication. This paper presents a description of the types of test and facilities that have been used for the test program as well as some examples of data that have been generated. The test program is intended to give spacecraft builders and users a better understanding of degradation processes and effects to enable improved prediction of spacecraft performance.

[horizontal rule]

Effects of Vacuum Ultraviolet Radiation on Thin Polyimide Films

This paper describes the vacuum ultraviolet (VUV) radiation durability screening testing of thin (12.7 to 25.4 µm) polyimide films proposed for use on the Next Generation Space Telescope (NGST) sunshield. Materials included in this screening test were Kapton®E, Kapton®HN, Upilex®S, CP1, CP1 with vapor deposited aluminum (VDA) on its back surface, and CP2 with a VDA coating on its back surface. Samples were exposed to approximately 1000 equivalent sun hours (ESH) of VUV radiation and examined for changes in solar absorptance, thermal emittance, ultimate tensile strength, and elongation-to-failure. Changes in solar absorptance were observed for some materials, and additionally, significant changes in spectral reflectance were observed in the ultraviolet to visible wavelength region for all polyimide materials tested. Changes in ultimate tensile strength and elongation at failure were within the experimental uncertainty for all samples. Longer exposures are needed to verify the observed trends and to develop performance predictions for these materials on the NGST sunshield.

[horizontal rule]

Steady Sate Vacuum Ultraviolet Exposure Facility With Automated Calibration Capability

NASA Glenn Research Center at Lewis Field designed and developed a steady state vacuum ultraviolet automated (SSVUVa) facility with in situ VUV intensity calibration capability. The automated feature enables a constant accelerated VUV radiation exposure over long periods of testing without breaking vacuum. This test facility is designed to simultaneously accommodate four isolated radiation exposure tests within the SSVUVa vacuum chamber. Computer-control of the facility for long term continuous operation also provides control and recording of thermocouple temperatures, periodic recording of VUV lamp intensity, and monitoring of vacuum facility status. This paper discusses the design and capabilities of the SSVUVa facility.
[Power & Electric Propulsion Division]
[Privacy Policy and Important Notices
Curator and NASA Official Responsible For Content:  Bruce.A.Banks@grc.nasa.gov 
* an asterisk indicates an external link
Last Updated: 04/14/2006