National Academies Press: OpenBook

Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies (1996)

Chapter: Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility

« Previous: Appendix C Beam Sources
Suggested Citation:"Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility." National Research Council. 1996. Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies. Washington, DC: The National Academies Press. doi: 10.17226/5540.
×

D Previous Advice of the National Research Council Regarding the BEVALAC Facility

The Space Studies Board and its Committee on Space Biology and Medicine addressed the following letter to Secretary of Energy James D. Watkins and NASA Administrator Daniel J. Goldin on August 20, 1992.

On May 14, 1992, the Committee on Space Biology and Medicine (CSBM) of the Space Studies Board (SSB) was briefed by the acting director of NASA's Life Sciences Division, Mr. Joseph K. Alexander, concerning various issues and activities in which the division is engaged. Among the issues raised was the impending decommissioning of the BEVALAC at the Lawrence Berkeley Laboratory as outlined in correspondence from Dr. David Hendrie, director of the Department of Energy's Division of Nuclear Physics. Subsequently, the CSBM discussed this issue with the Board at its meeting in Huntsville, Alabama, in June.

The Board and the CSBM are in agreement with a host of advisory committees' recommendations concerning the importance of gaining a better understanding of the biological effects of high Z element (HZE high-energy) particles. 1 Critical to planning for extended human sojourns in deep space is quantitative knowledge about the dose rates and types of radiation that will be encountered and the related biological effects.

The SSB and CSBM are concerned about the closing of the BEVALAC given that there is no alternative facility at which to continue the radiobiological research conducted as part of this country's goal of expanding the human presence in space. This facility is the only accelerator in the United States capable of producing the spectrum of energies required for research concerning the physical and biological effects of the heavy ions that will be encountered during deep-space missions. Providing adequate shielding against radiation and taking other measures to protect astronauts during deep-space travel are directly dependent on information derived from research concerning the biological effects of protons and HZE particles.

It is our understanding that even if funding for an alternative facility were provided today, there would be at least a five-year hiatus before suitable beams could become available. An interruption of the radiobiological research currently under way at the BEVALAC would have a number of deleterious effects on this well-established program that is a critical component of the national goal of human space exploration. Research teams that have been assembled to conduct this work would disperse and transfer to other areas of research. The flow of valuable long-term data derived from the BEVALAC studies would cease. Thus it would be necessary to start all over with new research animals, when another accelerator became available, in order to

1  

 Attachments citing 14 supporting statements drawn from internal NASA and advisory documents and National Research Council reports accompanied the original correspondence; they are here appended to the letter.

Suggested Citation:"Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility." National Research Council. 1996. Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies. Washington, DC: The National Academies Press. doi: 10.17226/5540.
×

obtain data from repeated, increasingly longer periods of exposure—a condition absolutely crucial to this type of research. Finally, losing this capability would seriously damage the research program of the recently established NASA Specialized Center for Research and Training (NSCORT) in Space Radiation Health at Lawrence Berkeley Laboratory and contribute to the loss of expertise in basic radiobiological research—an outcome that would be contrary to the conclusion reached in NASA's Space Radiation Health Program Plan.2

There is an acute need for additional well-trained and well-qualified researchers in space radiation physics and biology. A continuous supply of trained space researchers needs to be developed and adequate numbers of trained personnel need to be available to enable program expansion. (p. 30)

Various heavy-ion facilities exist worldwide that could, theoretically, support the type of space-related research under way at Berkeley. However, the SSB and CSBM have no evidence that any of these facilities could be made available to support NASA's HZE radiation research program. The BNL Booster at Brookhaven National Laboratory has limited capability, and no beam time will be available until a new irradiation facility is built. The Darmstadt accelerator has provisions for cell research but not for animal research, and beam time at the facility is currently oversubscribed by a factor of two. The JINR at Dubna has obsolete equipment, low beam intensity, and beam contamination—significant limiting factors. The Synchrophasotron at Saclay has no provisions for conducting animal or cell research, and at least a year would be required to prepare the facility to provide iron beams. Beams generated at the facility at Geneva are beyond the energy range required by NASA researchers. Finally, the accelerator at Chiba is not yet in operation and will not produce iron ion particles.

Understanding that the NASA-sponsored research at the BEVALAC may be relatively minor in the context of the Department of Energy's (DOE) overall mission, the SSB and CSBM believe that the decision to decommission this facility should be considered in the context of the importance of the BEVALAC to the U.S. space program—one in which DOE plays an increasing role.3 Until a suitable alternative can be provided that supports research related to long-term plans for human space exploration, the SSB and CSBM urge that the BEVALAC remain available to NASA researchers. Given the importance of the radiobiological research conducted at the BEVALAC and its fundamental role in realizing the national goal of human space exploration, the SSB and CSBM strongly recommend that DOE and NASA agree on a means for continuing without interruption the capability now provided by the BEVALAC.

Signed by

Louis J. Lanzerotti

Chair, Space Studies Board

and

Fred W. Turek

Chair, Committee on Space Biology and Medicine

Excerpts and Recommendations Concerning Biological Effects of Radiation Exposure

It is critical for NASA to formalize agreements to utilize one or more of the federal accelerator facilities, and to assure that those facilities remain in operation until necessary ground-based research is completed.

—Aerospace Medicine Advisory Committee/NASA Advisory Council, Strategic Considerations for Support of Humans in Space and Moon-Mars Exploration Missions, Life Sciences Research and Technology Programs. 1992.

2  

Space Radiation Health Program Plan, Life Support Branch, Life Sciences Division, NASA, Washington, D.C., November 1991.

3  

National Space Policy Directive for Space Exploration Initiative Strategy, Section III, paragraphs c and d, March 13, 1992.

Suggested Citation:"Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility." National Research Council. 1996. Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies. Washington, DC: The National Academies Press. doi: 10.17226/5540.
×

In order to protect crews, to the extent possible, from the various harmful effects of radiation, it is necessary to thoroughly characterize the radiation environment, understand the biological effects of HZE radiation and protons (leading to the establishment of appropriate risk levels and limits for radiation exposure), and accurately predict and provide warning of any increased levels of radiation.

—Discipline Working Group on Radiation Health and Environmental Health, NASA, Space Radiation Health Program Plan. 1991

Determining the long-term medical consequences of exposure to high Z element (HZE) particles present as a component of galactic cosmic radiation (GCR) is critical. The biological hazards associated with HZE particles, i.e., the “late effects,” are not adequately known and may pose unacceptable long-term cancer risks. Exposure can result in life-threatening and life-shortening effects, such as cancer, and other detrimental consequences including cataract formation, mutagenesis, and other tissue damage.

—Aerospace Medicine Advisory Committee/NASA Advisory Council, Strategic Considerations for Support of Humans in Space and Moon-Mars Exploration Missions, Life Sciences Research and Technology Programs. 1992

NASA should make a commitment to support fundamental research on the biological effects of radiation. This support and commitment should take the form of expanding NASA's role in and funding for basic research and of contributing to the necessary facilities, such as the BEVALAC accelerator.

—Life Sciences Strategic Planning Committee, NASA, Exploring the Living Universe—A strategy for Space Life Sciences. 1988

In summary, the highest priorities are for improved dosimetry and for studies of the effects of HZE particles so that the risks of both stochastic effects, such as carcinogenesis, and nonstochastic effects such as CNS damage, can be estimated with confidence.

—National Council on Radiation Protection and Measurements, Guidance on Radiation Received in Space Activities. 1989

One concern requiring further study in this area is the high-energy high-charge component of the cosmic ray flux, which can damage non-dividing cells, including those of the central nervous system.

—National Commission on Space, Pioneering the Space Frontier. 1986

The Space Exploration Initiative requires understanding and management of space radiation hazards. Uncertainties in these radiation effects on cells, tissue and small organisms could be reduced by simulations using the BEVALAC at the Berkeley Radiation Laboratory.

—Synthesis Group, NASA, America at the Threshold. 1991

Reports from the National Research Council.

The availability of HZE particles for experimental radiation biology is extremely limited. The only feasible approach to obtaining the required information is to carry out controlled studies in adequate ground-based facilities.

—Radiobiological Advisory Panel/Space Science Board, Radiobiological Factors in Manned Space Flight. 1967

The availability of a ground-based accelerator capable of producing HZE particles now permits the design of precisely ordered experiments. Such experiments should be supported.

—Committee on Space Biology and Medicine/Space Science Board, A Strategy for Space Biology and Medical Science for the 1980's and 1990's. 1979

Suggested Citation:"Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility." National Research Council. 1996. Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies. Washington, DC: The National Academies Press. doi: 10.17226/5540.
×

It is important to learn more about the relative biological effects of radiation influences, particularly high-Z galactic cosmic rays and solar flare electrons and their relationship to cancer and cataract induction in order to set meaningful guidelines for radiation protection. The question of appropriate shielding in flight is complex and requires further study.

—Committee on Human Exploration of Space/National Research Council, Human Exploration of Space—A Review of NASA's 90-Day Study and Alternatives. 1990

Terrestrial studies of the biological effects of low-level, high-LET irradiation on cell cultures and animals (using particle accelerators) should be expanded, with particular attention paid to the space radiation problem.

—Life Sciences Task Group, Space Studies Board, Space Science in the Twenty-First Century—Imperatives for the Decades 1995 to 2015—Overview and Life Sciences. 1988

Planning for extended human sojourns in space mandates that we have quantitative knowledge about the dose rates and the types of radiation that will be encountered. Similarly, the effects of the different types of radiation encountered in space, especially deep space, must be defined quantitatively. Much of the necessary radiobiology research can be carried out on Earth with defined radiation sources.

—Committee on Space Biology and Medicine/Space Studies Board, Assessment of Programs in Space Biology and Medicine. 1991

One way to maximize the return on investment in research is through various modes of cooperative research, with foreign partners, private concerns, and between federal agencies…. [An] example for collaboration between federal agencies [is] facilities supported by the Department of Energy such as the BEVALAC, which has the capability of providing for study of very high-Z particles and their biological effects.

—Space Studies Board, Priorities in Space Life Sciences Research, testimony by Space Studies Board Member Robert A. Moser to the House Budget Committee Task Force on Defense, Foreign Policy and Space, April 28, 1992

Improved measurements of cross sections and better modeling of heavy-ion interactions, particularly for the yield and spectra of neutrons and other secondary particles generated in the shielding material, are also required. NASA currently helps support the BEVALAC heavy-ion accelerator and some cross-section studies. However, the BEVALAC has been threatened with closure, thus endangering some of the enabling research on both cross-section measurements and the long-term biological effects of ionizing radiation.

—Committee on Human Exploration/Space Studies Board, Scientific Prerequisites for the Human Exploration of Space. 1993

Suggested Citation:"Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility." National Research Council. 1996. Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies. Washington, DC: The National Academies Press. doi: 10.17226/5540.
×
Page 72
Suggested Citation:"Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility." National Research Council. 1996. Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies. Washington, DC: The National Academies Press. doi: 10.17226/5540.
×
Page 73
Suggested Citation:"Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility." National Research Council. 1996. Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies. Washington, DC: The National Academies Press. doi: 10.17226/5540.
×
Page 74
Suggested Citation:"Appendix D Previous Advice of the National Research Council Regarding the BEVALAC Facility." National Research Council. 1996. Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies. Washington, DC: The National Academies Press. doi: 10.17226/5540.
×
Page 75
Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies Get This Book
×
 Radiation Hazards to Crews of Interplanetary Missions: Biological Issues and Research Strategies
Buy Paperback | $47.00 Buy Ebook | $37.99
MyNAP members save 10% online.
Login or Register to save!
Download Free PDF

NASA's long-range plans include possible human exploratory missions to the moon and Mars within the next quarter century. Such missions beyond low Earth orbit will expose crews to transient radiation from solar particle events as well as continuous high-energy galactic cosmic rays ranging from energetic protons with low mean linear energy transfer (LET) to nuclei with high atomic numbers, high energies, and high LET. Because the radiation levels in space are high and the missions long, adequate shielding is needed to minimize the deleterious health effects of exposure to radiation.

The knowledge base needed to design shielding involves two sets of factors, each with quantitative uncertainty—the radiation spectra and doses present behind different types of shielding, and the effects of the doses on relevant biological systems. It is only prudent to design shielding that will protect the crew of spacecraft exposed to predicted high, but uncertain, levels of radiation and biological effects. Because of the uncertainties regarding the degree and type of radiation protection needed, a requirement for shielding to protect against large deleterious, but uncertain, biological effects may be imposed, which in turn could result in an unacceptable cost to a mission. It therefore is of interest to reduce these uncertainties in biological effects and shielding requirements for reasons of mission feasibility, safety, and cost.

READ FREE ONLINE

  1. ×

    Welcome to OpenBook!

    You're looking at OpenBook, NAP.edu's online reading room since 1999. Based on feedback from you, our users, we've made some improvements that make it easier than ever to read thousands of publications on our website.

    Do you want to take a quick tour of the OpenBook's features?

    No Thanks Take a Tour »
  2. ×

    Show this book's table of contents, where you can jump to any chapter by name.

    « Back Next »
  3. ×

    ...or use these buttons to go back to the previous chapter or skip to the next one.

    « Back Next »
  4. ×

    Jump up to the previous page or down to the next one. Also, you can type in a page number and press Enter to go directly to that page in the book.

    « Back Next »
  5. ×

    Switch between the Original Pages, where you can read the report as it appeared in print, and Text Pages for the web version, where you can highlight and search the text.

    « Back Next »
  6. ×

    To search the entire text of this book, type in your search term here and press Enter.

    « Back Next »
  7. ×

    Share a link to this book page on your preferred social network or via email.

    « Back Next »
  8. ×

    View our suggested citation for this chapter.

    « Back Next »
  9. ×

    Ready to take your reading offline? Click here to buy this book in print or download it as a free PDF, if available.

    « Back Next »
Stay Connected!