The role of DNA repair by nonhomologous end joining (NHEJ), homologous recombination, spore photoproduct lyase, and DNA polymerase I and genome protection via âŁ/â¤-type small, acid-soluble spore proteins (SASP) in Bacillus subtilis spore resistance to accelerated heavy ions (high-energy charged [HZE] particles) and X rays has been studied. Spores deficient in NHEJ and âŁ/â¤-type SASP were significantly more sensitive to HZE particle bombardment and X-ray irradiation than were the recA, polA, and splB mutant and wild-type spores, indicating that NHEJ provides an efficient DNA double-strand break repair pathway during spore germination and that the loss of the âŁ/â¤-type SASP leads to a significant radiosensitivity to ionizing radiation, suggesting the essential function of these spore proteins as protectants of spore DNA against ionizing radiation.Endospores of the gram-positive bacterium Bacillus subtilis are highly resistant to inactivation by environmental stresses, such as biocidal agents and toxic chemicals, desiccation, pressure and temperature extremes, and high fluences of UV radiation (reviewed in references 44, 45, and 61) and are a powerful biodosimetric system for terrestrial environmental monitoring and astrobiological studies (44). On Earth, understanding extreme spore resistance to ionizing radiation is important in the areas of food preservation, medical sterilization, and decontamination from bioterror attack (4, 17, 47; reviewed in references 42 and 43). Off Earth, spore radiation resistance is important both in space flight and in ground-based simulations, in order to obtain information on the biological damage produced by exposure to space conditions (23,25,26,44). Onboard several spacecraft (Apollo 16, Spacelab 1, LDEF, D2, and FOTON), spores of Bacillus subtilis were exposed to selected parameters of space, such as space vacuum and different spectral ranges of solar UV radiation and cosmic rays, applied separately or in combination (5, 9, 19-21, 23, 24, 26). Especially, the radiation environment on Earth, on Mars, in low-Earth orbit, and in deep space is typified by a wide variety of primary particles covering an extended range of energies. Galactic cosmic rays (GCR) are charged particles that originate from sources beyond our solar system. The distribution of GCR is believed to be isotropic throughout interstellar space. The spectrum of the GCR consists of 98% protons and heavier ions (baryon component) and 2% electrons and positrons (lepton component). The baryon component is composed of 87% protons, 12% helium ions (alpha particles), and the remaining 1% heavy ions of charge 3 from lithium to 92 from uranium. Due to their high abundance, iron ions are highly penetrating, giving them a large potential for radiobiological damage (3,21).While the UV photochemistry of spore DNA and repair of UV damage to DNA during germination are well characterized (34,44,(59)(60)(61), there has been relatively little work on the nature of DNA damage in spores caused by ionizing radiation, the protective role of...