DNA damage formation, DNA repair, and survival after exposure of DNA repair-proficient and nucleotide excision repair-deficient human lymphoblasts toUVA1 and UVB
Tm. Runger et al., DNA damage formation, DNA repair, and survival after exposure of DNA repair-proficient and nucleotide excision repair-deficient human lymphoblasts toUVA1 and UVB, INT J RAD B, 76(6), 2000, pp. 789-797
Purpose: The comet assay has been used to visualize DNA damage in single ce
lls after exposure to UV light. These comets are commonly thought to reflec
t transient, repair-induced DNA breaks. The goal of the work presented here
was to further characterize the nature of UV-induced comets and to further
elucidate DNA damage formation by different wavelengths of ultraviolet lig
ht.
Materials and methods: Detailed dose-response and time-course experiments w
ith comet formation were carried out with normal and nucleotide excision re
pair (NER)-deficient xeroderma pigmentosum (XP) lymphoblasts. Irradiation w
as carried out with low, intermediate, or high doses of UVAl or UVB, comet
formation was observed, cell survival and viability were determined, and UV
-induced apoptosis was measured.
Results: All responses were dose-dependent. With the intermediate dose of U
VAl, a pronounced comet formation was observed without subsequent growth in
hibition. Raising levels of porphyrins, which act as photosensitizers, by p
reincubation with 5-amino-levulinic acid increased comet formation with UVA
, but not with UVB. UVAl-sensitivity and comet formation in XP cells was no
t significantly different from the normal cells. With UVB no comet formatio
n was seen without subsequent apoptotic cell death. XP cells exhibited the
known UVB-hypersensitivity, but their comet formation was not significantly
different from that of normal cells.
Conclusions: The findings are compatible with the hypothesis that UV-induce
d comets represent transient repair-induced DNA breaks. Both, the NER of di
mers and the base excision repair of oxidative DNA modifications are though
t to contribute to comet formation.