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Coalescence of DNA Double Strand Breaks Induced by Galactic Cosmic Radiation is Modulated by Genetics in 15 Inbred Strains of MiceIn this manuscript we address the challenges associated with the ability to predict radiation sensitivity associated with exposure to either cosmic radiation or X-rays in a population study, by monitoring DNA damage sensing protein 53BP1 forming small nuclear radiation-induced foci (RIF) as a surrogate biomarker of DNA double strand breaks (DSB). 76 primary skin fibroblasts were isolated from 10 collaborative cross strains and five reference inbred mice (C57Bl/6, BALB/CByJ, B6C3, C3H and CBA/CaJ) and exposed to three different charged nuclei of increasing LET (350 MeV/n Si, 350 MeV/n Ar and 600 MeV/n Fe) and X-ray. Our data brings strong evidence against the classic "contact-first" model where DSBs are assumed to be immobile and repaired at the lesion site. In contrast, our model suggests nearby DSBs move into single repair unit characterized by large RIF before the repair machinery kicks in. Such model has the advantage of being much more efficient molecularly but is poorly suited to deal with cosmic radiation, where energy is concentrated along the particle trajectory, inducing a large density of DSBs along each particle track. In accordance with this model, RIF quantification after X-ray exposition showed a saturated dose response for early time points post-irradiation for all strains. Similarly, the high-LET response showed that RIF number matched the number of track per cell, not the number of expected DSB per cell (1). At the temporal level, we noted that the percentage of unrepaired high-LET tracks over a 48 hour time-course increased with LET, confirming that the DNA repair process becomes more difficult as more DSB coalesce into single RIF. There was also good agreement between persistent RIF levels measured in-vitro in the primary skin cultures and survival levels of T-cells and B-cells collected in blood samples from 10 CC strains 24 hours after 0.1 Gy whole-body dose of X-ray. This suggests that persistent RIF 24 hour post-IR is a good surrogate in-vitro biomarker for in-vivo radiation toxicity. Finally, at the genomic level, large differences in repair rates between strains for high-LET allowed us to identify suggestive genetic loci associated with radiation sensitivity. Interestingly, the two highest LETs provided the most strain variation with a common locus on Chromosome 10 highly enriched for DNA repair associated genes we discussed in detail.
Document ID
20180002122
Acquisition Source
Ames Research Center
Document Type
Preprint (Draft being sent to journal)
Authors
Penninckx, Sebastien
(Facultes Univ. Notre-Dame de la Paix Namur, Belgium)
Ray, Shayoni
(Universities Space Research Association Moffett Field, CA, United States)
Staatz, Kevin
(Universities Space Research Association Moffett Field, CA, United States)
Degorre, Charlotte
(Nantes Univ. France)
Guiet, Elodie
(California Univ., Lawrence Berkeley National Lab. Berkeley, CA, United States)
Viger, Louise
(California Univ., Lawrence Berkeley National Lab. Berkeley, CA, United States)
Snijders, Antoine M.
(California Univ., Lawrence Berkeley National Lab. Berkeley, CA, United States)
Mao, Jian-Hua
(California Univ., Lawrence Berkeley National Lab. Berkeley, CA, United States)
Karpen, Gary
(California Univ., Lawrence Berkeley National Lab. Berkeley, CA, United States)
Costes, Sylvain V.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
March 27, 2018
Publication Date
January 1, 2018
Subject Category
Space Radiation
Life Sciences (General)
Report/Patent Number
ARC-E-DAA-TN53515
Funding Number(s)
CONTRACT_GRANT: NNA16BD14C
CONTRACT_GRANT: DE AC02-05CH11231
CONTRACT_GRANT: NNL15AA08I
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Keywords
Radiation-Induced Foci
GWAS
53BP1
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