UVA and UVB elicit distinct mutational signatures in melanoma

It is difficult to discern the relative contributions of ultraviolet-A (UVA; 320-400nm) and ultraviolet-B (UVB; 280-320nm) radiation to human melanoma development. Here, we compared the tumorigenic consequences of a single UVA or UVB exposure in mouse models predisposed to Braf- or Nras-mutant melanoma. Exposures approximated the amount of UVA or UVB energy contained in ∼40 minutes of summer sunlight. While UVA accelerated melanoma onset in a subset of mice, UVB universally reduced tumor latency and induced gene mutations relevant to the human disease. Genomic analyses uncovered distinct mutational signatures specific to each UV spectrum. The UVB-specific signature was biased for mutations on the untranscribed DNA strand and closely mirrored mutational signatures enriched in human cutaneous melanoma. The UVA-specific signature mimicked SBS51, a mutational signature found in human uveal melanoma. Distinctions in the trinucleotide patterns of the UVA and UVB signatures suggest that cytosine deamination plays a key role in UVB-mediated melanomagenesis.