Figures
Abstract
Astronauts on a mission to Mars would be exposed for up to 3 years to galactic cosmic rays (GCR) — made up of high-energy protons and high charge (Z) and energy (E) (HZE) nuclei. GCR exposure rate increases about three times as spacecraft venture out of Earth orbit into deep space where protection of the Earth's magnetosphere and solid body are lost. NASA's radiation standard limits astronaut exposures to a 3% risk of exposure induced death (REID) at the upper 95% confidence interval (CI) of the risk estimate. Fatal cancer risk has been considered the dominant risk for GCR, however recent epidemiological analysis of radiation risks for circulatory diseases allow for predictions of REID for circulatory diseases to be included with cancer risk predictions for space missions. Using NASA's models of risks and uncertainties, we predicted that central estimates for radiation induced mortality and morbidity could exceed 5% and 10% with upper 95% CI near 10% and 20%, respectively for a Mars mission. Additional risks to the central nervous system (CNS) and qualitative differences in the biological effects of GCR compared to terrestrial radiation may significantly increase these estimates, and will require new knowledge to evaluate.
Citation: Cucinotta FA, Kim M-HY, Chappell LJ, Huff JL (2013) How Safe Is Safe Enough? Radiation Risk for a Human Mission to Mars. PLoS ONE 8(10): e74988. https://doi.org/10.1371/journal.pone.0074988
Editor: Aaron Alain-Jon Golden, Albert Einstein College of Medicine, United States of America
Received: June 15, 2013; Accepted: August 6, 2013; Published: October 16, 2013
This is an open-access article, free of all copyright, and may be freely reproduced, distributed, transmitted, modified, built upon, or otherwise used by anyone for any lawful purpose. The work is made available under the Creative Commons CC0 public domain dedication.
Funding: This work was supported by the NASA Space Radiation Risk Project, and the University of Nevada Las Vegas. The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript.
Competing interests: The authors have declared that no competing interests exist.
Introduction
In space astronauts are exposed to galactic cosmic rays (GCR) comprised of high-energy protons and high charge (Z) and energy (E) (HZE) nuclei and solar particle events (SPE) comprised largely of low to medium energy protons. As space missions venture away from Earth into deep space, long-term exposures occur leading to important concerns about the risks to astronauts, including discussions on the acceptable risk level. A key component of this concern are the types of radiation that occur in space [1]–[6], which produce distinct types of biological damage from radiation on Earth such as X-rays or gamma-rays. Individual radiation sensitivity and estimating risks at low dose-rates are additional major concerns, while potential interactions between space radiation and microgravity found to be a minor concern [1]. Fatal cancer risk [1]–[6] has been considered the dominant risk for GCR and NASA has developed the NASA Space Cancer Risk (NSCR) model to estimate cancer risks and uncertainties for space missions [5], [6]. NASA's radiation standard limits astronaut exposures to a 3% risk of exposure induced death (REID) evaluated at the upper 95% confidence interval (CI) of the risk estimate [7]. However recent epidemiological analysis of radiation risks for circulatory diseases [8]–[10] shows additional risks, and allow for predictions of REID for circulatory diseases to be included with cancer risk predictions [5], [11], [12]. Risks to the central nervous system (CNS) are also a concern [1], [4], however methods to make quantitative risk estimates of CNS effects have not been developed.
Conjunction class Mars missions [13], [14], where Earth and Mars are in favorable alignments, involve long stays on the martian surface of approximately 540-d with transit times from Earth to Mars and back of about 400-d. Opposition class missions are more variable with launch date, whereby assuming a 60-d Mars surface time can lead to total transit times that vary from 460 to 780-d. In considering radiation risks, the impacts of solar modulation need to be included. GCR organ exposures vary by about 2-fold over the approximately 11-y solar cycle being highest at solar minimum when solar modulation of GCR is weakest [4], [5]. The frequency and size of solar particle events (SPEs) are difficult to predict, however their likelihood of occurrence decreases greatly for a 3-year period about solar minimum [5]. In this paper we make predictions near solar minimum for cancer and circulatory disease and discuss issues related to improving risk estimates and risk reduction for space missions. Predictions for SPEs will be considered in other reports.
Methods
We used NASA's models of risks and uncertainties based on recent radio-epidemiology studies of cancer, GCR environmental models, particle transport codes describing the GCR modification by atomic and nuclear interactions in spacecraft and tissue shielding, and models of biological effectiveness of different radiation types [5], [6]. The model [5] includes NASA defined quality factors for solid cancer and leukemia risk estimates for HZE particles, and use of a never-smoker population to represent astronauts. Risk predictions were made for missions near solar minimum using the average of these derived from historical data on sunspot numbers for solar cycles 1 to 24, and fitted to modern data on GCR composition and energy spectra [5], [14], [15]. Transport codes describe the atomic and nuclear interactions of particles including projectile and target nuclei fragmentation and production of light particles (protons, neutrons, helium etc.) [16], [17]. Recent spacecraft such as the International Space Station (ISS) or Orion capsule developed as an exploration mission crew transfer vehicle have an average of about 20 g/cm2 equivalent aluminum shielding, which is used in risk calculations. For the martian surface we use an average shielding thickness of 10 g/cm2 to represent a light surface habitat, and included the martian atmosphere represented by CO2 with a 18 g/cm2 vertical height. Results for the ISS include the trapped protons [18] along with GCR. Previous reports demonstrate that NASA's model agrees with spaceflight dosimetry measurements [5], [18], [19] to within 15%. Organ doses and probability distribution functions (PDF) describing uncertainties in model parameters [5] are summarized in Tables S1 and S2 in File S1, respectively.
Circulatory disease risks included cardiovascular disease (CVD) and ischemic heart disease (IHD) using excess relative risk (ERR) estimates from a recent meta-analysis of studies of atomic bomb survivors, and nuclear workers in several countries [8]. Circulatory disease risk estimates were made using the non-cancer effects dose equivalent for the blood forming system (BFO) based on a distinct relative biological effectiveness (RBE) factor compared [20], [21] to that of cancer estimates, and without the use of a dose and dose-rate reduction effectiveness factor (DDREF). These choices and alternative ones are discussed below. Organ dose equivalents for cancer risk are given in units of Sievert (Sv). For circulatory disease risks because the RBE is distinct from the quality factor (QF), organ dose equivalents are expressed in terms of a different unit, Gray-Equivalent (Gy-Eq) [21]. A detailed description of REID models and uncertainty analysis using Monte-Carlo propagation of uncertainty is described in the Supplementary material and prior report [5].
Results
Calculations of tissue average absorbed doses, non-cancer risk dose equivalent [20], [21], and NASA dose equivalent for leukemia and solid cancer risks [5] were made for up to 100 g/cm2 of aluminum shielding (Fig. 1). GCR doses were not sensitive to shielding amounts due to a near balance in particle loss and production through atomic and nuclear interaction that occur within shielding. Organ specific doses also show small variation (Table S1 in File S1) due to the high energies of GCR and secondary radiation. For SPE's a much larger variation between doses at individual organs occurs [5].
(A) The attenuation of annual GCR organ averaged doses versus depth of aluminum shielding for deep space, the martian surface, and for combined GCR and trapped protons in the ISS orbit. Calculations are for males absorbed dose (D) (mGy), solid cancer and leukemia risks (H) (mSv), and non-cancer effects (G) (mGy-Eq). Calculations on the martian surface consider its atmosphere with an 18 g/cm2 CO2 vertical height.
The distribution spectra of %REID per year for solid cancer versus the GCR descriptive parameter, Z*2/β2, where Z* is a particles effective charge number and β its velocity, is shown in Fig. 2 for average spacecraft shielding conditions. The parameter Z*2/β2 describes the density of the ionization of a particle track more effectively than LET and is used in the NASA quality factor [5]. A prominent peak occurs near 262 corresponding to relativistic iron particles with similar peaks observed for other HZE particles. The contributions at small values of Z*2/β2, which have low biological effectiveness, are increased for ISS due to the trapped protons in the ISS orbit. The martian atmosphere provides some protection from HZE particles, however leads to a buildup of particles at small Z*2/β2 such as protons and pions, and an increased contribution from neutrons.
The full GCR spectrum that traverse astronauts in deep space are more biologically damaging compared to the higher energy GCR that occur in low Earth orbit.
Figure 3 shows predictions of the dependence of GCR absorbed dose and solid cancer dose over time from 1950 to 2012. Also shown are times for the 43 largest SPE's out of ∼400 observed since 1950, which corresponds [22] to a lower cutoff for the integral fluence of 100 MeV protons of >106 p/cm2. SPEs with smaller values for 100 MeV integral fluence will have tissue doses below 0.01 Gy for light spacecraft shielding and are not shown. These results show the anti-correlation between GCR and SPE doses that will occur between solar minimum and maximum, respectively. Variation of GCR organ dose equivalents of up to 20% can occur when comparing different solar minimum.
We predicted tissue specific radiation-exposure incidence of cancer (%REIC), and %REID for overall cancer risks for 940-d Mars missions by 45-y old female and male never-smoker (NS) populations (Fig. 4) for heavy shielding. The circulatory disease risks for NS are similar to the U.S. average population (Table 1), which is largely due to NS's longer lifespan, whereby the radiation associated circulatory disease risk up to age 85-y is lower for NS compared to the U.S. population but is similar over all ages. The combined %REID exceeded NASA limits [7] by about 3-fold. Predictions for fatal cancer risk are about 25% higher for females compared to males. For combined cancer and circulatory disease fatal risk, females are about 15% higher risk compared to males. The added contributions to the %REID from circulatory diseases was predicted to increase %REID by about 40% and to reduce the age at exposure dependence on %REID compared to cancer risks alone.
(A) Values are for an average 45-y female never smokers and (B) for an average 45-y male never smokers. Calculations assume 20 g/cm2 and 10 g/cm2 aluminum shielding for transit and martian surface, respectively. PC estimations are for 20 years post mission. All point assessments are bracketed by 95% confidence intervals.
The probability of causation (PC) (also denoted as attributable risk) is a conditional probability used as an indicator of a potential causal relationship between radiation exposure and occurrence of disease in a population. Our predictions (Fig. 4) suggest that a large portion of cancers that would be observed in crews after exploration missions would be attributed to GCR exposure, with PC for leukemia, stomach, colon, lung, bladder, ovarian, and esophageal cancer significant. PC will increase modestly for longer post-mission times for most solid cancers and circulatory diseases, and decrease for leukemia. PC estimates for CVD and IHD were smaller than for many cancers because of the larger background occurrence for these diseases. Estimates for CVD and IHD incidence were not made, since only values ERR for mortality were available from the meta-analysis of Little et al. [8]. However obviously morbidity risks for circulatory diseases would be larger than mortality risk estimates and therefore add substantially to the overall morbidity of astronauts returning from a Mars mission.
The %REID and %REIC for various space missions including 1-year on ISS, 1-year near- Earth asteroid (NEA) mission, and the Mars conjunction and opposition missions were predicted (Fig. 5). Risk was much less on ISS compared to deep space missions, and missions of 1-year on the ISS at solar minimum are within the acceptable risk level for astronauts [7]. In contrast, because the exposure is to all GCR energies and the longer mission duration, exploration missions exceeded NASA's radiation limit by a large amount. The upper 95% CI for the %REIC is estimated near 15% and the inclusion of other significant morbidity as described below, would increase this value to above 20% for returning crew. An improved situation occurs near solar maximum [4], [5] where GCR risks decreased about 2-fold (Fig. 3). At solar maximum there is the mission operations burden to respond to SPE's, which can occur every few months and are difficult to monitor from Earth when Mars is in opposition [4]. Also, the residual dose behind shielding from SPEs will increase REID by a variable amount depending on the SPE size and spectra, and mission operation responses including shielding availability.
(A) Estimates are shown for 45-y old female and (B) male never-smokers. Calculations assume 20 g/cm2 and 10 g/cm2 aluminum shielding for transit vehicle and martian surface habitat, respectively. Error bars reflect the 95% confidence intervals.
Table 2 shows estimates of the maximum number days in space near solar minimum where NASA's limits are not exceeded for different ages at exposure and demographic variables. Results are for a specific shielding configuration of 20 g/cm2 aluminum, and include comparisons for fatal cancer risk alone or with the additional REID contributions from circulatory diseases. The addition of the circulatory disease risks reduces allowable times in space by two to three months depending on demographic considerations of crew composition. Variations of up to 10% would occur for other shielding designs (materials or additional shielding of a few 10′s of g/cm2). The uncertainties in the risk estimates are large, approaching a 3-fold ratio of the upper 95% CI to the central estimates. Reducing this uncertainty could substantially increase the number of days to stay within NASA's limits.
Discussion
In this paper we made predictions of cancer and circulatory disease risks for space exploration missions to Mars near solar minimum using NASA's recent model developments [5], [6], and results from a recent epidemiological analysis [8] of circulatory disease risks from human exposures to low LET radiation. The combined risk was shown to increase %REID by about 40% from predictions of cancer risk alone. For circulatory disease predictions we used the deterministic effects RBE model recommended by the International Commission on Radiological Protection (ICRP) as our central estimate, which leads to a lower GCR organ averaged equivalent dose compared to solid cancer risk and higher value compared to leukemia risk. One assumption would be that the higher RBE from animal experiments for solid cancers would be the largest RBE that could be expected for circulatory disease risk. In our calculations the ratio for solid cancer to circulatory disease, GCR organ averaged dose equivalent varied between 1.7 and 1.9 for typical different spacecraft shielding amounts. Based on these observations, we used a log-normal distribution with geometric mean, GM = 1 and geometric standard deviation, GSD = 1.35 for the probability distribution function (PDF) representing the uncertainty in the tissue averaged RBE for circulatory disease (Supplementary material).
There are several areas where new information related to the current estimates could lead to reduced uncertainties and perhaps lower risk estimates. Of critical importance is understanding of DDREFs and RBEs for cancer and circulatory risks where data for many tissues are not available for HZE particles at relevant doses and dose-rates [4], [5]. Improved information on specifying tissue specific transfer weights used in applying epidemiology data, and understanding differences in disease rates between model populations would also reduce uncertainties in risk estimates.
Concerns about a possible dose threshold for circulatory disease risks, which is an important consideration for ISS missions [21], should be reduced for a Mars mission because organ doses are above where threshold doses have been estimated [9]. and because we used the meta-analysis results that were based in-part to chronic exposures of radiation workers [8]. For cancer risk predictions a dose and dose-rate reduction effectiveness factor (DDREF) of 1.5 is used for solid cancer estimates based on the BEIR VII report [12], and the recommendations of the National Research Council to NASA [6]. For circulatory disease risk predictions a DDREF is not applied because models were based on meta-analysis of several chronically exposed populations as described by Little et al. [8]. For cancer risks the low value for the DDREF of 1.5 leads to an uncertainty distribution that is skewed towards higher DDREF values and lower REID, which opposes the QF uncertainty estimate which is skewed to higher REID values [5].
The ERR models for circulatory disease do not include gender specific and time dependent factors because analysis suggests these modifiers are weak based on existing data [8]. This is in contrast to cancer risk estimates where more detailed models have been developed which include gender specific estimates, and consideration of age at exposure and time after exposure effects [11], [12]. In addition, cancer risk estimates consider both multiplicative and additive risk models, and uncertainty analysis considers choice for weighting these models [5], [6], [12], [23].
Lifestyle factors for circulatory diseases likely play a major role in considering radiation effects. However, the analysis made by current reports suggest that estimates of ERR do not vary significantly when adjustments for possible lifestyle factors are considered [8]–[10]. The NASA models for never-smokers [5] and US average populations did not lead to very different circulatory disease risks due to a cancellation of the combined effects of lower background rates for NS and their long life-span that leads to additional risks. Estimating uncertainties in radiation estimates due to healthy workers effects and lifestyle factors are important areas for future research.
Our predictions are incomplete in several aspects. First the qualitative differences in biological damage of HZE particles and secondary neutrons compared to low linear energy transfer (LET) radiation such as X rays or gamma-rays have not been addressed. Our calculations only consider the quantitative differences using quality factors based on experimental studies from particle accelerators simulating GCR components in mice and other small animals, and human cell culture studies. Qualitative differences originate in the much larger energy deposition and distinct spatial distributions of damage in biomolecules, cells and tissues by HZE particles compared to low LET radiation. HZE particles produce complex DNA damage leading to mutations with high frequency [5], [24], [25], and differences in the generation of reactive oxidative species (ROS) or free radicals. These differences result in higher levels of chronic oxidative stress and genomic instability [26].
Non-targeted effects (NTE) [26] include bystander effects, which occur in neighbor cells of damaged cells, and genomic instability, as a delayed effect in the progeny of the initial cells or tissues irradiated. NTEs can lead to non-linear responses at low dose (less than one HZE particle per cell) and higher relative biological effectiveness (RBE) values [27], which would lead to an overall increased cancer REID compared to current estimates. RBE's for tumor induction in mice for iron particles vary greatly with values near 30 obtained for Harderian gland tumors [28] and more than 50 for liver tumors [29]. Understanding possible mechanisms for tumor induction, including NTE's and genomic instability, would help improve approaches to select the RBE's to be used for human risk assessments. An additional concern is the potential earlier appearance and increased lethality of tumors induced by HZE particles and neutrons [28]–[31], which suggests an important qualitative difference not accounted for in current cancer risk estimates for space radiation.
A second area where risk estimates are incomplete is in the inclusion of risks from a range of additional radiation effects occurring at both early and late time points post exposure. These include added components to the circulatory disease risk profile such as increased likelihood for coronary revascularization and myocardial infarction [8]–[10]; risks for other degenerative or premature aging-related endpoints such as earlier appearing cataracts [32], musculoskeletal system effects including osteoporosis and exacerbation of microgravity associated loss of bone strength [33], and respiratory diseases [34].
An expanding body of evidence derived from ground based research using rodent models at particle accelerators that simulate GCR points to a potential risk for disruptions in cognitive performance and memory that may occur within the time scale of an exploration class mission impacting its success [35], [36]. These effects have been observed at low doses of HZE particles (<0.2 Gy) in the hippocampus, striatum and prefrontal cortex, which are correlated with molecular and cellular damage including persistent ROS, altered dopamine expression, apoptosis, neuroinflammation and altered neurogenesis [35]–[40]. A recent observation is acceleration of Alzheimer's disease (AD) pathologies following low dose iron particle exposures in transgenic mice [40]. The substantiation of excess risk for AD by GCR would further increase REID estimates from the current results, and introduce additional morbidity for returning crew.
An important debate surrounds acceptable risks for a Mars mission, which could have historical importance to civilization. Space missions are designed [41] to an aggregate risk for during mission loss of crew (LOC) of less than 1 in 270, with new technology investments expected to reduce LOC to less than 1 in 750. Actual occurrences have led to individual mortality of 0 or 1.6% for the ISS and all NASA programs [42], respectively. The average life-loss for an astronaut of 45-y age at exposure for a radiation induced cancer is estimated at about 15 years for gamma-rays [12], [13] and expected to be higher for HZE particles based on animal studies [28]–[31], or about 2.5 times less than an estimated ∼40 life-loss years for a during mission LOC. For circulatory disease risks, estimated life-loss is a few years smaller compared to solid cancers for low LET [8], [9], however not much is known for high LET radiation. Using the ratio for differences in average life-loss and considering a 4 to 6 person Mars mission crew size, suggests that a 1 to 10 ratio of during mission LOC design criteria to REID limit would be a comparable risk basis. On this basis, the 1 in 270 aggregate risk for during mission LOC is then quite similar to the current 1 in 33 radiation fatality limit at NASA [7], [21], while an aggregate risk goal of 1 in 750 recommended by the NASA Aerospace Safety Advisory Panel [41] would suggest a lower radiation limit should be a future goal for radiation protection. Other considerations are the additional radiation morbidity risk, and ethical considerations that value life at middle or old age, as opposed to considerations of LOC during the mission alone.
Economic investments to lower radiation risk could have great benefits on Earth in understanding low dose radiation risks after the Fukushima nuclear reactor accident in Japan, or concerns of the risks from diagnostic use of radiation such as CT-scans. Planning missions to avoid solar minimum may be the largest factor to decrease radiation risks (Fig. 3), however such plans could be overcome by mission timeline constraints and limitations in predicting future solar cycle characteristics. Other possible investments to mitigate risks include research on radiation shielding, genetic testing for selection crew at lower risk, and biological countermeasures. However, radiation shielding plays an important role for SPE protection but is not a solution to the GCR risk problem with current launch capabilities which limit shielding mass (Fig. 1). Water or hydro-carbon materials would only provide modest benefits of up to 10% compared to aluminum shielding for GCR [5], [42], [43].
Crew selection for individual radiation sensitivity and biological countermeasures (BCMs) potentially have the highest payoffs in reducing risks, however much more information is needed in these areas [4], [44], [45]. Selecting astronauts against radiation sensitivity [45] could be hampered by a small pool of astronauts and other constraints on crew selection. Of importance is that because population averaged values for overall mortality and morbidity risks could exceed 10% and 20% respectively, individuals of increased sensitivity could be especially vulnerable to GCR based on our current but limited knowledge on radiation sensitivity [44]. This observation should lead to requirements to test potential crew members for DNA damage repair capacity, ROS responses, and susceptibility to specific diseases, and investments in research to develop accurate approaches to do so.
Developing BCMs to GCR pose severe challenges due to the chronic exposure, and the need for protection against high LET radiation, which appear to act through distinct biological mechanisms [1]–[6]. It is not clear that BCMs developed to protect against acute radiation risks from high doses of low LET radiation will be helpful or harmful for GCR [45]. Acute risk BCMs often have unwanted side-effects, and work through the rescue of cells from apoptosis. For GCR such approaches could be untenable for long dietary intake of 940 d and could leave genetically unstable cells available to increase the risks of late effects. For both the development of BCMs and selection of astronauts, a severe challenge is the large number of diseases contributing to the overall risk. This suggests investments are best made in understanding the underlying biological mechanisms that could be applied to reduce uncertainties for many distinct risks. BCM efficacy must be established quantitatively with small uncertainty for GCR, which may be achieved through ground based research at particle accelerators [1]–[6]. Such research should allow for an operational decision to use such BCMs to enable missions projected to exceed risk limits, and would have many benefits on Earth including reducing the health effects from exposure to radiation.
Supporting Information
File S1.
Contains: Supplementary Methods, Supplementary References, Table S1, Table S2.
https://doi.org/10.1371/journal.pone.0074988.s001
(DOCX)
Acknowledgments
Special thanks to Walter Schimmerling, Mark Little, and Joseph Fragola for useful discussions.
Author Contributions
Conceived and designed the experiments: FAC. Performed the experiments: LJC, MYK, FAC. Analyzed the data: FAC, JLH. Contributed reagents/materials/analysis tools: n/a. Wrote the paper: FAC, JLH. N/A.
References
- 1.
National Research Council (1996) Radiation hazards to crews of interplanetary missions: biological issues and research strategies. The National Academies Press, Washington, DC, 1996.
- 2. Cucinotta FA, Schimmerling W, Wilson JW, Peterson LE, Saganti P, et al. (2001) Space radiation cancer risks and uncertainties for Mars missions. Radiation Research 156: 682–688.
- 3. Cucinotta FA, Durante M (2006) Cancer risk from exposure to galactic cosmic rays: implications for space exploration by human beings. The Lancet Oncology 7: 431–435.
- 4.
National Council on Radiation Protection (2006) Information needed to make radiation protection recommendations for space missions beyond low-earth orbit. National Council on Radiation Protection and Measurements Report No. 153, Bethesda MD.
- 5.
Cucinotta FA, Kim MY, Chappell L (2013) Space radiation cancer risk projections and uncertainties- 2012. NASA TP 2013-217375.
- 6.
Committee for Evaluation of Space Radiation Cancer Risk Model, National Research Council (2012) Technical evaluation of the NASA model for cancer risk to astronauts due to space radiation. The National Academies Press, Washington DC.
- 7.
National Aeronautics and Space Administration (2007) NASA Space flight human system standard volume I; Crew health. NASA STD-3001.
- 8. Little M, Azizova D, Bazyka S, Bouffler SD, Cardis E, et al. (2012) Meta-analysis of circulatory disease from exposure to low-level ionizing radiation and estimates of potential population risks. Environmental Health Perspectives 120: 1503–1511.
- 9. Shimizu Y, Kodama K, Nishi N, Kasagi F, Suyama A, et al. (2010) Radiation exposure and circulatory disease risk: Hiroshima and Nagasaki atomic bomb survivor data, 1950–2003. British Medical Journal 340: b5349
- 10. Darby S, Ewertz M, McGale P, Bennet AM, Blom-Goldman U (2013) Risk of ischemic heart disease in women after radiotherapy for breast cancer. New England Journal of Medicine 368: 986–998.
- 11.
United Nations Scientific Committee on the Effects of Atomic Radiation (2008) Sources and effects of ionizing radiation. UNSCEAR 2008 Report to the General Assembly, with Scientific Annexes, New York: United Nations.
- 12.
BEIR VII, National Academy of Sciences Committee on the Biological Effects of Radiation (2006) Health Risks From Exposure to Low Levels of Ionizing Radiation. Washington DC: National Academy of Sciences Press.
- 13.
National Aeronautics and Space Administration (2009) Human exploration of mars: design reference architecture 5.0. NASA SP 2009-502, Washington DC.
- 14. Badhwar GD, O'Neill PM (1992) An improved model of GCR for space exploration missions. Nuclear Tracks and Radiation Measurements 20: 403–410.
- 15.
O'Neill PM (2010) Badhwar-O'Neill 2010 galactic cosmic ray flux model- Revised. IEEE Transactions in Nuclear Science .57: : 3148 – 3150
- 16. Wilson JW, Townsend LW, Shinn JL, Cucinotta FC, Costen RC (1994) Galactic cosmic ray transport methods, past, present, and future. Advances in Space Research 10: 841–852.
- 17. Cucinotta FA, Kim MY, Schneider SI, Hassler DM (2007) Description of light ion production cross sections and fluxes on the Mars surface using the QMSFRG model. Radiation and Environmental Biophysics 46: 101–106.
- 18.
Cucinotta FA, Kim MY, Willingham V, George KA (2008) Physical and biological organ dosimetry analysis for International Space Station Astronauts. Radiation Research 170: , 127–138
- 19. Zeitlin CJ, Hassler DM, Cucinotta FA, Ehresmann B, Wimmer-Schweingruber RF, et al. (2013) Measurements of energetic particle radiation in transit to Mars on the Mars Science Laboratory. Science 340: 1080–1084.
- 20.
International Commission on Radiation Protection (2003) Relative Biological Effectiveness (RBE), Quality Factor (Q), and Radiation Weighting Factor (wR). ICRP Publication 103.Pergamon.
- 21.
National Council on Radiation Protection and Measurements (2000) Recommendations of dose limits for low earth orbit., NCRP Report 132: Bethesda, MD.
- 22. Kim MY, Hayat MJ, Feiveson AH, Cucinotta FA (2009) Using high-energy proton fluence to improve risk prediction for consequences of solar particle events. Advances in Space Research 44: 1428–1432.
- 23.
National Council on Radiation Protection and Measurements (1997) Uncertainties in fatal cancer risk estimates used in radiation protection. NCRP Report No. 126: Bethesda, MD.
- 24. Goodhead DT (1994) Initial events in the cellular effects of ionizing radiation: clustered damage in DNA. International Journal of Radiation Biology 65: 7–17.
- 25. Cucinotta FA, Nikjoo H, Goodhead DT (2000) Model of the radial distribution of energy imparted in nanometer volumes from HZE particles. Radiation Research 153: 459–468.
- 26. Kadhim M, Salomaa S, Wright E, Hildenbrandt G, Belyakov OV, et al. (2013) Non-targeted effects of ionizing radiation- implications for low dose risk. Mutation Research 752: 84–98.
- 27. Cucinotta FA, Chappell LJ (2010) Non-targeted effects and the dose response for heavy ion tumor formation. Mutation Research 687: 49–53.
- 28. Alpen EL, Powers-Risius P, Curtis SB, DeGuzman R (1993) Tumorigenic potential of high-Z, high-LET charged particle radiations. Radiation Research 88: 132–143.
- 29. Weil MM, Bedford JS, Bielefeldt-Ohmann H, Ray AF, Gernik PC, et al. (2009) Incidence of acute myeloid leukemia and hepatocellular carcinoma in mice irradiated with 1 GeV/nucleon 56Fe ions. Radiation Research 172: 213–219.
- 30. Grahn D, Lombard LS, Carnes BA (1992) The comparative tumorigenic effects of fission neutrons and Cobalt-60 γ rays in B6CF1 mouse. Radiation Research 129: 19–36.
- 31.
Datta K, Suman S, Kallakury BV, Fornace Jr AJ (2013) Heavy ion radiation exposure triggered higher intestinal tumor frequency and greater β-catenin activation than γ radiation in APC Min/+ mice. PLoS One 8: e59295.
- 32. Chylack LT Jr, Feiveson AH, Peterson LE, Tung WH, Marak LJ, et al. (2012) NASCA report 2: Longitudinal study of relationship of exposure to space radiation and risk of lens opacity. Radiation Research 178: 25–32.
- 33. Alwood JS, Yumoto K, Mojarrab R, Limoli CL, Almeida EA, et al. (2010) Ion irradiation and unloading effects on mouse lumbar vertebral microarchitecture, mechanical properties and tissue stresses. Bone 47: 248–255.
- 34. Ozasa K, Shimizu Y, Suyama A, Kasagi F, Soda M, et al. (2012) Studies of the mortality of atomic bomb survivors, Report 14, 1950–2003: an overview of cancer and noncancer diseases. Radiation Research 177: 229–243.
- 35. Joseph JA, Hunt WA, Rabin BM, Dalton TK (1992) Possible “accelerated striatal aging” induced by 56Fe heavy-particle irradiation: implications for manned space flights. Radiation Research 130: 88–93.
- 36. Haley GE, Yesier L, Olsen RH, Davis MJ, Johnson LA, et al. (2013) Early effects of whole body 56Fe irradiation on hippocampul function in C57Bl/6J mice. Radiation Research 179: 590–596.
- 37. Britten RA, Davis LK, Johnson AM, Keeney S, Siegel A, et al. (2012) Low (20 cGy) doses of 1 GeV/u (56)Fe—particle radiation lead to a persistent reduction in the spatial learning ability of rats. Radiation Research 177: 146–151.
- 38. Rola R, Fishman K, Baure J, Rosi S, Lamborn KR, et al. (2008) Hippocampal neurogenesis and neuroinflammation after cranial irradiation with (56)Fe particles. Radiation Research 169: 626–632.
- 39.
Cherry JD, Liu B, Frost JL, Lemere CA, Williams JP, et al.. (2012) Galactic cosmic radiation leads to cognitive impairment and increased Aβ plaque accumulation in a mouse model of Alzheimer's disease. PLoS One 7(12); e53275.
- 40.
National Aeronautics and Space Administration (2013) The astronaut fact book. NASA http://www.nasa.gov/pdf/740566main_current.pdf.
- 41.
Aerospace Safety Advisory Panel (2010) Annual Report for 2010. http://oiir.hq.nasa.gov/asap/documents/2010_ASAP_Annual_Report.pdf.
- 42. Badhwar GD, Cucinotta FA (2000) A comparison on depth dependence of dose and linear energy transfer spectra in aluminum and polyethylene. Radiation Research 153: 1–8.
- 43. Durante M, Cucinotta FA (2011) The physical basis for radiation protection in space travel. Reviews of Modern Physics 83: 1245–1281.
- 44.
National Council on Radiation Protection and Measurements (2011) Potential impact of individual genetic susceptibility and previous radiation exposure on radiation risks for astronauts. NCRP Report 167, Bethesda, MD.
- 45. Durante M, Cucinotta FA (2008) Heavy ion carcinogenesis and human space exploration. Nature Reviews Cancer 8: 465–472.