Many space experiments are scheduled for the International Space Station (ISS). Completion of the ISS will soon become a reality. Astronauts will be exposed to low-level background components from space radiation including heavy ions and other high-linear energy transfer (LET) radiation. For long-term stay in space, we have to protect human health from space radiation. At the same time, we should recognize the maximum permissible doses of space radiation. In recent years, physical monitoring of space radiation has detected about 1 mSv per day. This value is almost 150 times higher than that on the surface of the Earth. However, the direct effects of space radiation on human health are currently unknown. Therefore, it is important to measure biological dosimetry to calculate relative biological effectiveness (RBE) for human health during long-term flight. The RBE is possibly modified by microgravity. In order to understand the exact RBE and any interaction with microgravity, the ISS centrifugation system will be a critical tool, and it is hoped that this system will be in operation as soon as possible.
Key words; space, space radiation, biological effect, high-LET, ISSCharacteristics of space and the composition of space radiation F o r s e v e r a l y e a r s , h u m a n b e i n g s h a v e b e e n residing for long periods in the ISS where many space experiments are scheduled to be performed. In addition, there are proposals for human to travel to Mars. Important characteristics of the environment in space are the presence of microgravity and space radiation. Radiation present in the space environment contains many components including low dose radiation, low dose-rate radiation, and high-LET particles (Table 1). The space environment produces microgravity-and/or space radiation-induced physiological changes in the human body (e.g. calcium release from bone into the urine, loss of muscular power, body fluid shifts, space or airsickness, reduced immunoreactivity and eye flashes).During a long-term stay in space, astronauts will be constantly exposed to space radiation which contains various types of low dose-rate radiation. Space radiation consists of galactic cosmic rays, solar particles and geomagnetically trapped particles (Table 2). A characteristic of galactic cosmic rays is their containing high energy particles with energies over 10 GeV: protons (90%), α-particles (9%) and heavy particles (1%). The origin of galactic cosmic rays is considered to be the explosion of supernovas. Solar particles are primarily protons and electrons with several percent of Review Received: January 4, 2005 Address for correspondence: Dr. Takeo Ohnishi Department of Biology, Nara Medical University School of Medicine, Shijo-cho 840, Kashihara, Nara 634-8521, Japan. E-mail; tohnishi@naramed-u.ac.jp the radiation being composed of α-particles and heavy particles. The sun changes its level of activity during an 11-year-cycle. Solar flares and solar winds, indicators of solar activity, emit large quantities of charged partic...