Melanoma is a lethal type of skin tumor that has been
linked with
sunlight exposure chiefly in fair-skinned human populations. Wavelengths
from the sun that can reach the earth’s surface include UVA
radiation (320–400 nm) and UVB radiation (280–320 nm).
UVB effectively induces the formation of dimeric DNA photoproducts,
preferentially the cyclobutane pyrimidine dimers (CPDs). The characteristic
UVB signature mutations in the form of C to T mutations at dipyrimidine
sequences are prevalent in melanoma tumor genomes and have been ascribed
to deamination of cytosines within CPDs before DNA polymerase bypass.
However, evidence from epidemiological, animal, and other experimental
studies also suggest that UVA radiation may participate in melanoma
formation. The DNA damage relevant for UVA includes specific types
of CPDs at TT sequences and perhaps oxidative DNA damage to guanine,
both induced by direct or indirect, photosensitization-mediated chemical
and biophysical processes. We summarize the evidence for a potential
role of UVA in melanoma and discuss some of the mechanistic pathways
of how UVA may induce mutagenesis in melanocytes.