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Updated: May 13, 2026

The Lambda Select cII Mutation Detection System
Published on: April 26, 2018
Solar-UV-signature mutation prefers TCG to CCG: extrapolative consideration from UVA1-induced mutation spectra in
Hironobu Ikehata1, Jun Kumagai, Tetsuya Ono
1Department of Cell Biology, Tohoku University Graduate School of Medicine, Sendai, Japan. ikehata@med.tohoku.ac.jp
Abstract:
UVA1 exerts its genotoxicity on mammalian skin by producing cyclobutane pyrimidine dimers (CPDs) in DNA and preferentially inducing solar-UV-signature mutations, C → T base substitution mutations at methylated CpG-associated dipyrimidine (Py-mCpG) sites, as demonstrated previously using a 364 nm laser as a UVA1 source and lacZ-transgenic mice that utilize the transgene as a mutational reporter. In the present study, we confirmed that a broadband UVA1 source induced the same mutation profiles in mouse epidermis as the UVA1 laser, generalizing the previous result from a single 364 nm to a wider wavelength range of UVA1 (340-400 nm). Combined with our previous data on the mutation spectra induced in mouse epidermis by UVB, UVA2 and solar UVR, we proved that the solar-UV-signature mutation is commonly observed in the wavelength range from UVB to UVA, and found that UVA1 induces this mutation more preferentially than the other shorter wavelength ranges. This finding indicates that the solar-UV-signature mutation-causing CPDs, which are known to prefer Py-mCpG sites, could be produced with the energy provided by the longer wavelength region of UVR, suggesting a photochemical reaction through the excitation of pyrimidine bases to energy states that can be accomplished by absorption of even low-energy UVR. On the other hand, the lower proportions of solar-UV-signature mutations observed in the mutation spectra for UVB and solar UVR indicate that the direct photochemical reaction through excited singlet state of pyrimidine bases, which can be accomplished only by high-energy UVR, is also involved in the mutation induction at those shorter wavelengths of UVR. We also found that the solar-UV signature prefers 5'-TCG-3' to 5'-CCG-3' as mutational target sites, consistent with the fact that UVA induces CPDs selectively at thymine-containing dipyrimidine sites and that solar UVR induces them preferably at Py-mCpG sites. However, the mutation spectrum in human p53 gene from non-melanoma skin cancers shows the opposite preference for 5'-CCG-3' sites. This apparent discrepancy in the site preference seems to result from the lack of 5'-TCG-3' sites mutable to missense mutations on the nontranscribed strand of human p53 gene, which should be evolutionally acquired under selective pressure from the sun.
Insights
UVA1 radiation causes DNA mutations in skin, particularly at CpG sites. This study confirms UVA1
Area of Science:
- Genetics and Molecular Biology
- Dermatology
- Photochemistry
Background:
- UVA1 radiation is known to cause genotoxicity in mammalian skin.
- Previous studies identified cyclobutane pyrimidine dimers (CPDs) and specific C→T mutations at methylated CpG sites (Py-mCpG) as key genotoxic effects of UVA1.
- Transgenic mice with the lacZ gene have been used as a reporter system to study UV-induced mutations.
Purpose of the Study:
- To confirm that a broadband UVA1 source induces similar mutation profiles in mouse epidermis as a previously used UVA1 laser.
- To generalize findings across a wider UVA1 wavelength range (340-400 nm).
- To compare mutation spectra induced by UVA1 with those from UVB, UVA2, and solar UVR to understand wavelength-dependent mutagenic mechanisms.
Main Methods:
- Utilized a broadband UVA1 source and lacZ-transgenic mice to analyze mutation profiles in mouse epidermis.
- Compared mutation spectra from UVA1 with previously established data for UVB, UVA2, and solar UVR.
- Analyzed mutation signatures, including base substitutions and target site preferences (e.g., 5'-TCG-3' vs. 5'-CCG-3').
Main Results:
- A broadband UVA1 source confirmed the UVA1 laser's findings, inducing solar-UV-signature mutations (C→T at Py-mCpG sites) across the 340-400 nm range.
- UVA1 preferentially induced solar-UV-signature mutations compared to UVB and UVA2.
- The study observed a preference for 5'-TCG-3' over 5'-CCG-3' mutation sites for UVA1, aligning with CPD formation at thymine-containing sites, but noted a discrepancy with human p53 mutations.
Conclusions:
- The solar-UV-signature mutation is common across UVB to UVA wavelengths, with UVA1 showing a higher preference.
- CPDs responsible for these mutations can be generated by longer UVA wavelengths, suggesting photochemical reactions involving excited pyrimidine bases.
- Differences in mutation site preference between mouse models and human p53 mutations may be due to evolutionary selective pressures and site availability.
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