OBJECTIVES:
While in Earth orbit, crewmembers are constantly exposed to radiation of solar and galactic origin. Space radiation consists of electrons, protons, heavy particles, single particles of high energy (HZE particles) and secondary radiation, such as bremsstrahlung, neutrons and charged particles created by interactions of primary radiation with nuclei of spacecraft shielding material or the human body. The dosage of each radiation type depends largely on the altitude and inclination of the spacecraft's orbit, effectiveness of the shielding, and solar activity during the mission.
Previous investigations on bacteriophages, bacterial spores, yeast, plant seed, insect embryos, rats, and mice have shown serious effects such as chromosomal damage, cell death, or malfunctions caused by HZE particles passing through the biological material. Irrespective of their rarity, HZE particles represent a considerable risk for humans in space.
The specific effects of HZE particles in humans are not well documented. In ground-based experiments it has been proven that HZE particles induce chromosomal aberrations in human lymphocytes. Thus, this investigation studied chromosomal aberrations in human blood lymphocytes to assess the mutagenic potential of space radiation in man.
Previous investigations were conducted by the same investigator team, using blood from eighteen astronauts and cosmonauts flown on board the Space Shuttle and Mir Space Station. Throughout the study, a postflight increase of chromosomal aberrations in lymphocytes was evident for the long-duration crewmembers. Lymphocytes collected from astronauts and cosmonauts who stayed more than 100 days in Earth orbit showed elevated frequencies of dicentric chromosomes, a typical chromosomal aberration induced by ionizing radiation. In difference to these previous investigations, new multi-color banding fluorescence in situ hybridization (mBAND) and multi-color fluorescence in situ hybrididization (mFISH) techniques were used to analyze the samples.
The compilation of results should provide information about chromosomal aberrations in peripheral lymphocytes of crewmembers exposed to space radiation. The results will enable a better assessment of the genetic risk of humans in space and in consequence, will help to optimize radiation shielding. The data also allows for calculations of aberration frequencies expected during deep-space missions.
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APPROACH:
Blood (10 mL) was drawn before and immediately after spaceflight by venous puncture using heparinized Vacutainer
TM tubes. The whole blood was set up with phytohemaglutin to stimulate the lymphocytes to undergo mitosis. After 48 hours, the cells were stained and prepared for microscopic analysis. Three different staining procedures were performed to assess all types of induced aberrations: (1) Classical Giesma block-staining to score dicentric and ring chromosomes, (2) mFISH to score reciprocal translocations and insertions, and (3) mBAND of a selected chromosome pair to score for inversions and translocations between homologous chromosomes.
Blood draws were scheduled preflight, at L-10 (10 days before launch), and postflight as close to landing as possible (R+0 or R+3, depending on the landing site). Twenty-four crewmembers gave their consent to participate in this study: 11 crewmembers on short-duration Space Shuttle missions, and 13 subjects on long-duration missions of several months on board the International Space Station (ISS).
RESULTS:
This investigation has been performed on ISS Expeditions 6-11. In each Expedition where the experiment has been conducted, preflight and postflight blood samples were drawn from each crewmember. To ensure high-quality results, the blood samples arrived at the Principal Investigator's laboratory in Essen, Germany within 72 hours after collection. Researchers are currently measuring changes in the genetic material and analyzing their significance and will release preliminary conclusions soon. From this study scientists may be able to better assess risk factors for genetic damage in space. Understanding and reducing the risk of radiation is important for safe long-duration travel in space, including stays on the moon and journeys to Mars.
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