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Article

UVA and UVB Photolysis of Natural and Synthetic Cannabinoids Studied by Online Mass Spectrometry

by
Ambar S. A. Shaikh
,
Kelechi O. Uleanya
,
Kgato P. Selwe
and
Caroline E. H. Dessent
*
Department of Chemistry, University of York, Heslington, York YO10 5DD, UK
*
Author to whom correspondence should be addressed.
Molecules 2026, 31(5), 813; https://doi.org/10.3390/molecules31050813
Submission received: 28 January 2026 / Revised: 19 February 2026 / Accepted: 24 February 2026 / Published: 28 February 2026
(This article belongs to the Special Issue Recent Advances in Cannabis and Hemp Research—2nd Edition)
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Abstract

Cannabinoids are of considerable current interest for use in pharmaceutical and non-medical consumer products. While there have been significant efforts to understand their chemical stability under ambient conditions, only sparse attention has been paid to characterising their photostability. Here, we present UVA (365 nm) and UVB (280 nm) photolysis measurements of eight representative cannabinoids, including natural compounds (THC, CBD, THCA, CBDA), metabolites (THC-COOH, THC-OH), and synthetic analogues (JWH-018, MDMB-FUBINACA). Measurements were performed using a novel online-electrospray mass spectrometry (MS) approach, where online photolysis of cannabinoid solutions was conducted with laser light-emitting diodes. MS detection was used to monitor precursor compound decay and photoproduct formation. Complementary results obtained via UV–Vis spectroscopy of photolysed cannabinoid solutions are also presented. For THC, CBD, THC-COOH, THC-OH, THCA and CBDA, significant photodegradation was observed with 280 nm photolysis, both through the appearance of photoproducts detected by MS and via time-dependent changes in the solution UV–Vis absorption profiles. In contrast, the synthetic cannabinoids (JWH-018 and MDMB-FUBINACA) showed negligible degradation with UVB photolysis, consistent with their relatively low absorbance propensity through the mid-UV region. No significant photodegradation was observed for UVA (365 nm) photolysis of any of the cannabinoids. The results presented here constitute the first directly comparable set of photolysis measurements for key phytocannabinoids.

Graphical Abstract

1. Introduction

Cannabinoids are a class of bioactive chemical compounds that interact with the human endocannabinoid system, exhibiting pharmacological effects. These effects range from psychoactivity to pain relief. Cannabinoid compounds originate either naturally from the Cannabis Sativa plant (phytocannabinoids), or can be produced in laboratories (synthetic cannabinoids) [1]. They have been extensively studied in recent years due to growing interest from the pharmaceutical industry, arising from the potential for developing therapeutic applications to treat nausea and epilepsy [2,3]. Commercially, cannabinoids are also increasingly being incorporated into food, drink and cosmetic products [4,5,6]. Beyond these legal uses, synthetic cannabinoids represent one of the largest classes of new designer drugs, leading to their widescale adoption as custom narcotics [7,8].
Given the growth of cannabinoid usage, it is critical to understand the factors that influence their intrinsic stability. This issue is of importance given that some cannabinoids are known to be inherently unstable and prone to degrading under various environmental conditions [9]. Degradation can occur through several pathways including heat, oxidation, hydrolysis, and light exposure, resulting in reduced functionality and also potential toxicological risks [10,11,12]. Understanding the degradation pathways of cannabinoids is therefore not only important for optimising manufacture and commercial storage procedures, but also for assessing any ecotoxicological risks that arise when cannabinoids are transferred from human consumers into the wider environment [13]. Both natural and synthetic cannabinoids have been detected in aquatic bodies across the globe, and are known to be incompletely transformed by waste-water systems [14,15,16,17].
In this work, we investigate the photostability of a group of representative cannabinoid molecules displayed in Scheme 1. The cannabinoids selected for study include the most common phytocannabinoids [1], along with two synthetic cannabinoids as a contrast to the natural compounds. (The two synthetic cannabinoids were chosen as they have recently been investigated via electrospray ionisation mass spectrometry and higher collisional dissociation [18]). In particular, we are interested in characterising the photoproducts that result following light exposure. There have been a few previous studies of cannabinoid photolysis, but these have been conducted on a small number of individual cannabinoids (THC, CBD and THCOOH) and there has been considerable diversity in the light sources, photolysis wavelengths and photoproduct detection methods employed [19,20,21,22]. It is therefore challenging to compare results for different compounds and obtain a reliable overall picture of the photostability of different natural and synthetic cannabinoids. Furthermore, the previous studies have relied on off-line (manual) sampling following light-induced degradation or storage, an approach that is time-consuming and unsuited to deployment as part of a manufacturing process [23,24,25]. One key point of interest is the difference in photoproduct formation reported in studies of the important, isomeric cannabinoids, THC and CBD: THC was characterised as producing minimal photoproducts, while CBD displays a significantly larger number of photoproducts [26,27]. This is surprising given the similar chemical structures of THC and CBD and warrants further investigation.
Online photolysis with mass spectrometric (MS) detection has been shown to be a facile and reproducible method for surveying photolysis chemistry [28,29,30,31,32], which has been used recently to investigate photolysis of a range of inorganic and organic compounds. Here, it is applied to analyse the photolysis propensity and photoproducts of the Scheme 1 cannabinoids. Single-wavelength laser light-emitting diodes (LEDs) are used as photon sources, allowing us to investigate degradation in both the UVA (365 nm) and UVB (280 nm) at well-defined photoexcitation energies. We have selected 280 nm for the UVA excitation wavelength since it occurs within the UVB absorption bands of cannabinoids such as THC [33]. The UVA wavelength of 365 nm was selected as it lies in the centre of the UVA spectral region. By using this approach, we are able to obtain the first consistent set of measurements which are directly comparable for all the Scheme 1 cannabinoids. We note that while our approach gives photochemical clarity by using two specific excitation wavelengths, the results are not directly transferrable for assessing cannabinoid stability in natural aquatic areas which are exposed to sunlight. Further complementary work, for example coupling on-line MS with a solar simulator light source, is desirable to address this.

2. Results

2.1. THC and CBD

Figure 1 displays the UV–Vis absorption spectrum of Δ9-tetrahydrocannabinol, THC, in methanol obtained between 210 and 460 nm. The spectrum was recorded using a 1 × 10−5 M solution of THC in methanol, which provides acceptable absorbance for this molecule. For THC, the UV–Vis spectrum displays three main absorption features, which are labelled I–III on Figure 1, with λmax values of 216, 228 and 276 nm, respectively. It agrees well with a previously reported spectrum [33].
Photolysis at 280 nm of the same THC solution was then performed by irradiating the solution in the UV cuvette for photolysis times from 0 to 120 min. UV–Vis spectra were recorded at regular intervals to identify any changes in the spectral profile. Upon irradiation, the Band I and II features decrease steadily in intensity as a function of photolysis time, indicating light-induced breakdown of THC. A new, broad band (IV) appears at longer wavelengths (λmax = 302 nm). This new feature, which is associated with photoproduct formation, likely comes from the formation of a relatively more conjugated product compared to the reactant. Figure S1 presents the changes in the absorbance intensity at selected absorption wavelengths as a function of photolysis time, clearly illustrating that absorbance at ~302 nm increases upon photolysis.
On-line photolysis with MS detection was then used to identify the THC photoproducts. For consistency with the UV–Vis photolysis experiments, a 1 × 10−5 M THC in methanol solution was used for photolysis in the electrospray syringe. Figure 2a displays the THC electrospray ionisation mass spectra (ESI-MS) obtained prior to irradiation, with Figure 2b and Figure 2c showing the ESI-MS obtained after 30 min of irradiation with 365 and 280 nm, respectively. The precursor ion, produced by deprotonation of THC, i.e., [THC − H]− (m/z 313), is clearly visible prior to irradiation, with the [THC − H]−·THC dimer also prominent (m/z 627). At the solution concentration used here, dimer ions are common in ESI–MS [31,34], but we also note that cannabinoids are known to self-associate into species such as cannabisol and cannabitwinol [35,36,37].
Upon UVA photolysis (365 nm), the precursor ion is largely unaffected (Figure 2b), showing no significant decline in intensity over 30 min, and no significant photoproduct formation. This behaviour is consistent with the low absorbance of THC at wavelengths > 300 nm (Figure 1). In contrast, the [THC − H]− ion decreases dramatically in intensity upon UVB photolysis (280 nm), with a large number of photoproducts produced (Figure 2c). We note the intensity of the [THC − H]−·THC dimer ion also decreases upon photolysis. The most intense photoproduct ions observed are m/z 345, 375, 381, 393, and 511. (Several ions appear with additional +/− 1 or 2 m/z values, consistent with varying numbers of H atoms.) All of these intense product ions have m/z values greater than the precursor ion, and are therefore either produced from photolysis of an aggregate species present in solution prior to ESI [33], or via additive reactions of photoexcited THC. A full list of photoproduct ions is included in Table 1.
Higher collisional dissociation (HCD) was conducted on [THC − H]− (Figure S2) to identify any potential ion-source fragment ions. The most intense HCD product ions observed were m/z 245, 191, 179 and 311. (We note that HCD has been performed on protonated analogues of cannabinoids previously [18,38,39,40].) Importantly, none of the [THC − H]− HCD fragment ions coincide with the identified photoproduct ions, indicating that these are “true” photoproduct ions [41,42,43]. This was checked for all of the cannabinoids studied in this work, and no photoproduct ions reported coincide with HCD fragment ions.
Time-resolved photolysis MS (TRPMS) of THC at 280 nm was performed to provide further insight into the photolysis chemistry (Figure 3). In the Figure 3 data and in all of the TRPMS presented below, photolysis is initiated at t = 3 min (to provide a clear baseline prior to photolysis), and a 1 min transit time exists for the photolysed solution to travel into the MS. The results of photolysis are therefore evident above t = 4 min. Figure 3a shows the time-dependent ion intensities associated with the [THC − H]− precursor ion (m/z 313) and the five most intense photoproduct ions (m/z 381, 511, 375, 393, 345). The [THC − H]− precursor ion intensity decreases smoothly from t = 4–17 min, while the photoproduct ions increase. Notably, several of the photoproducts (m/z 345, 375 and 381) are intermediates, since they have photolysis profiles that peak around 14 min before declining up to 22 min when their intensities plateau. The other group of photoproduct ions, namely m/z 393, 511, rise steadily up to 22 min, indicating that they are photolysis end-products. Figure 3b illustrates the TRPMS results for the group of five photoproducts with the next-highest ion intensities, i.e., m/z 407, 481, 509, 391, and 513. All of these lower-intensity photoproducts display end-product photolysis profiles.
Previous work on THC photolysis has identified limited photoproducts, with the aromatised derivative, cannabinol (CBN), having been reported as the only significant photoproduct [44]. In the current work, numerous other photoproduct ions have been identified, which warrant further study to achieve full structural assignments. Focusing on the major photoproduct ions, m/z 345, 375, 381, and 511, we tentatively assign these as follows: m/z 345 represents the addition of amu 32 to the precursor ion, and therefore likely represents the photoactivated addition of either MeOH or O2 to THC (photoactivated addition of MeOH to CBD has been observed previously [26]); m/z 375 corresponds to the m/z value of the precursor ion of THC-COOH, which appears to be produced from THC via a photoactivated oxidation reaction; and m/z 511 corresponds to the loss of 116 amu from the dimer, consistent with aromatisation of one THC moiety to CBN and the associated loss of the phenol ring and butyl side chain. The m/z 381 fragment can be formed either via the addition of amu 68 to the precursor ion or, more likely, through the loss of 246 amu from the dimer. (Formation from m/z 627 likely occurs through a multistep process, resulting in the eventual loss of the alkyl rings.) Tentative structural assignments of the photoproduct ions are provided in Table S5, with mechanistic schemes for the principal UV-induced transformation pathways for the major photoproducts given in Section S13A.
We next present the comparable results for the THC isomer, cannabidiol CBD. Figure 4 displays the UV–Vis absorption spectrum (210–460 nm, in methanol) of CBD. (A solution of 1 × 10−5 M was studied for consistency with the THC measurements.) The CBD spectrum is notably similar to that of THC (Figure 1), with three main absorption bands I-III with λmax values of 216, 232, and 276 nm, respectively, and agrees well with a previous spectrum [33]. Photolysis at 280 nm was conducted on the CBD solution, with UV–Vis spectra recorded to monitor photolysis (Figure 4). Like THC, the Band I and II features decrease gradually upon irradiation, with a new, broad band appearing at longer wavelengths (λmax = 302 nm). Plots of the changes in the CBD absorbance intensity at selected UV–Vis wavelengths as a function of photolysis time are given in Figure S3. These confirm the similarity of the effects of 280 nm photolysis on the UV–Vis spectral profiles of THC and CBD. (Like THC, the UV–Vis spectrum of CBD is unaffected by 365 nm photolysis.)
CBD and THC are believed to remain in their precursor isomer form in neutral methanol, although they can interconvert under acidic or thermal perturbations [45,46,47]. The highly similar UV–Vis absorption profiles (and photolysis behaviour) of CBD and THC can then be attributed to the two molecules possessing very similar chromophores. Given the similarity of the UV–Vis spectral profiles, it is not possible to assess whether interconversion of the isomers is occurring from these spectra.
To further investigate the nature of 280 nm photolysis of CBD, ESI-MS was conducted on photolysed solutions of CBD, with the results presented in Figure S4. Like THC, no significant CBD photolysis was evident for 365 nm excitation, but extensive 280 nm photolysis was seen. The major 280 nm photofragment ions observed are m/z 359, 345, 375, 363 and 389, with m/z 345 and 375 assigned as for THC, and m/z 359 likely corresponding to oxidation of the m/z 345 species accompanied by the loss of 2H. (Oxidation and dehydrogenation is a common photo-initiated reaction for cannabinoids [19,21,22].) m/z 363 can be assigned to hydrolysis of the m/z 345 product, with m/z 389 corresponding to the addition of a further O atom to m/z 375 species accompanied by the loss of 2H. A full list of CBD photoproduct ions is included in Table 1. Tentative structural assignments of the photoproducts are provided in Table S5, with proposed photochemical reaction pathways (Section S13A).
Figure 5 presents the accompanying TRPMS of CBD, with Figure 5a showing the light-induced depletion of the [CBD − H]− precursor ion (m/z 313), accompanied by the formation of the five most intense photoproducts, while Figure 5b displays the next highest ion intensity products (m/z 391, 407, 477, 479 and 481). Among the photoproducts, m/z 345 exhibits a profile consistent with its identification as an intermediate, with its intensity peaking at ~14 min before declining at longer times. The m/z 359 photoproduct peaks with the m/z 345 ion, but then displays a constant intensity. In contrast, the m/z 363, 375, and 389 ion intensities rise steadily across the photolysis period, plateauing to long photolysis times. All of these ions are stable end products, as are the less intense photoproducts of Figure 5b. Overall, the CBD TRPMS, like those of THC, indicate a mechanistic sequence in which the primary transient intermediate, m/z 345, feeds into a suite of stable higher-mass products.
Comparing the TRPMS results of THC and CBD, depletion of the precursor ion (m/z 313) occurs over a similar timescale (10–20 min). However, THC photolysis leads to more intense transient intermediates (m/z 345 and 381) compared to CBD (m/z 345), and a different set of photoproducts are observed for the two molecules. These differences are significant enough to give us confidence that THC and CBD are not equilibrating to a common solution mixture under the conditions of our study.
Although the photolysis results are distinctive for THC and CBD, the molecules produce many common photoproducts (Table 1), albeit with intensity variation. For example, CBD has more intense product ions with values between m/z 479 and 513, an observation consistent with its known dimerisation under UV exposure [21]. The most notable result to emerge from our comparative study is that it is clear that both THC and CBD produce numerous photoproducts following UVB excitation. This result challenges earlier photolysis studies of THC which identified only a single photolysis pathway [44]. Nonetheless, the overall similarity of their photolysis behaviour is fully consistent with the broad similarity in their geometric and electronic structures.

2.2. The THC Metabolites (THCOOH and THCOH)

Figure 6 displays the UV–Vis absorption spectrum (210–460 nm) of the THC metabolite THCOOH in methanol. The spectrum is similar to the THC/CBD spectra, with bands assigned with λmax = 218 nm (band I), 230 nm (band II), and 280 nm (band III). Solution-phase 280 nm photolysis was performed from 0 to 120 min, resulting in the band I and II features decreasing steadily in intensity up to 120 min, consistent with light-induced breakdown. A new, broad band again appeared at longer wavelengths with λmax at 302 nm and 354 nm (Bands IV and V). Figure S6 provides plots of the absorbance intensity changes at selected UV–VIS wavelengths as a function of photolysis time, showing that THCOOH degrades more rapidly for 280 nm photolysis than THC or CBD.
The ESI-MS obtained for a solution of THCOOH prior to irradiation and after 30 min of irradiation with 280 and 365 nm LEDs are shown in Figure S7. The precursor ion [THCOOH − H]− (m/z 343) is clearly visible prior to irradiation, with a strong [THCOOH − H]−·THCOOH dimer peak visible at m/z 687. No significant photolysis is observed for 365 nm irradiation (Figure S7b), consistent with THCOOH’s low absorption intensity at 365 nm (Figure 6). In contrast, UVB photolysis (280 nm) results in a dramatic reduction of the precursor ion, accompanied by the formation of numerous photoproducts (Figure S7c). The most intense photofragment ions are m/z 313, 331, 363 and 375. Table S1 provides a full list of THCOOH photofragment ions.
TRPMS results for THCOOH (280 nm) are presented in Figure 7, showing the photolysis profile of the [THCOOH − H]− precursor, along with those of the 10 highest-intensity photoproducts. The [THCOOH − H]− precursor ion (m/z 343) decreases gradually in intensity from 4 to 25 min, with changes in the photoproduct ion intensity occurring up to 30 min. The m/z 363 product is present prior to photolysis but then steadily increases in intensity as the precursor decays, eventually emerging as the major photoproduct. This likely indicates that it is present in the precursor solution as a result of ambient photolysis. m/z 375 is the second highest intensity photoproduct: It increases in intensity rapidly at earlier photolysis time, but then largely plateaus above t = 15 min. The m/z 331 ion displays the profile of a reaction intermediate, as its intensity peaks around t = 13 min. Other ions such as m/z 383, 557, and 625 steadily increase in intensity. The m/z 331 ion was observed previously in hydrolysis of aquatic samples of THCOOH by Boix et al. [48], and assigned to a transformation product associated with the loss of a methyl from the cyclohexanoate ring. In that study, m/z 375 was detected as a photolysis (simulated sunlight) product and corresponds to a +32 Da mass shift relative to the parent ion (m/z 343), consistent with dihydroxylation. The m/z 363 ion represents a +20 Da mass shift and can tentatively be assigned to mono-hydroxylation accompanied by additional hydrogen incorporation. We note that m/z 375 is also consistent with the addition of methanol to the precursor, as with THC and CBD. Tentative structural assignments of the photoproducts are provided in Table S5, with proposed photochemical reaction pathways (Section S13A).
Figure 8 displays the UV–Vis absorption spectra (210–460 nm) of a second THC metabolite THC-OH. The spectrum is again similar to those of THC, CBD and THCOOH although the band II feature is relatively less intense. Features are assigned as follows with Bands I (λmax = 216 nm), II (λmax = 236 nm) and III (λmax = 264 nm). Photolysis at 280 nm was conducted on the THC-OH solution from 0 to 120 min, with the resulting UV–Vis spectra displayed in Figure 8. Light-induced breakdown of THCOH is visible in the reduction of the Band I and II features and the appearance of the new, broad longer wavelength bands with λmax at 304 nm and 344 nm (Bands IV and V). Figure S9 presents the changes in the absorbance intensity as a function of photolysis time at selected wavelengths.
Figure S10 shows the ESI-MS of [THCOH − H]− obtained prior to irradiation, and after 30 min of irradiation with 280 and 365 nm. The precursor ion [THCOH − H]− is visible at m/z 329, along with a strong dimer peak, which is again visible at m/z 659. For UVA photolysis (365 nm), the precursor ion intensity is unaffected and no photoproducts are evident (Figure S10b). In contrast, on UVB photolysis (280 nm), the precursor ion dramatically decreases in intensity, and a large number of photoproducts are evident (Figure S10c). Table S2 provides a full list of the photoproduct ions.
The TRPMS for 280 nm photolysis of [THCOH − H]− is displayed in Figure 9. At times > 4 min, the precursor ion (m/z 329) intensity decreases steadily, concomitant with the formation of a group of photoproducts (m/z 361, 391, 407, 439, 423, 459, 525, and 529). The m/z 361 photoproduct is the dominant photoproduct through most of the photolysis time, peaking as an intermediate photoproduct around 17 min, prior to the end products (e.g., m/z 361, 407, 423) reaching an equilibrium distribution with it at t = 30 min. This corresponds to the addition of 32 amu to the precursor and can therefore again be assigned as resulting from the photoactivated addition of MeOH (or O2) to the cannabinoid. Overall, the ten most intense photoproducts eventually achieve similar product ion intensities, consistent with complex and highly branched photolysis pathways. Tentative structural assignments of the photoproducts are provided in Table S5, with proposed photochemical reaction pathways (Section S13A).

2.3. CBDA and THCA

The photolysis behaviour of the carboxylated cannabinoids, tetrahydrocannabinolic acid (THCA) and cannabidiolic acid (CBDA), were investigated using the same approaches as for the cannabinoids and the metabolites. THCA and CBDA are the biosynthetic precursors of THC and CBD, and their additional carboxyl group has been suggested to influence photostability and overall stability under light/heat stress [23,49], so it is useful to fully characterise their photolysis. This pair of molecules are again isomeric.
Figure 10 displays the UV–Vis absorption spectrum of CBDA in methanol, showing three characteristic bands, with the strongest absorption band (I) peaking at λmax ≈ 224 nm, a medium-intensity band (II) at ~260, and a less intense band (III) at ~300 nm. The overall spectral profile is distinctive to those of the cannabinoids presented above due to the electronic influence of the additional aromatic carboxylic acid group. Upon irradiation with 280 nm light over 120 min, all three bands I-III gradually decreased in intensity, while a new broad feature (band IV) emerged at longer wavelengths (λmax~330 nm), consistent with the production of more conjugated photoproducts. Figure S12 presents the changes in the absorbance intensity at selected wavelengths as a function of photolysis time, to complement these qualitative observations.
The ESI-MS of [CBDA − H]− obtained prior to irradiation and after 30 min of irradiation at 280 and 365 nm are shown in Figure 11. The precursor ion [CBDA − H]− is visible at m/z 357, with a strong dimer peak, which is again visible at m/z 715. When CBDA was photolysed at 365 nm, the [CBDA − H]− precursor ion (m/z 357) was observed to remain as the dominant ion over the photolysis time (Figure 11a,b), with the m/z 373, 389, and 403 ions appearing as low-intensity photoproducts. For 280 nm photolysis, modest photolysis was observed, with the precursor ion intensity decreasing gradually over 30 min of photolysis, accompanied by the appearance of several fragment ions, with the m/z 373 fragment being the major photoproduct ion, along with m/z 389 and 403 (Figure 11c,d). m/z 373 corresponds to the addition of amu 16 to the precursor, so can be assigned to the photoactivated addition of O to CBDA. The addition of amu 32 is again evident in production of the m/z 389 ion, indicating the photoactivated addition of MeOH. m/z 403 can be assigned to the addition of amu 32, plus the addition of O with the loss of 2H atoms. Photolysis at 280 nm occurs on the shoulder of Band II, so results in less effective 280 nm photodegradation than for cannabinoids studied above. The corresponding TRPMS of CBDA are shown in Figures S13 and S14 for 365 and 280 nm photolysis. Table S3 provides a full list of the CBDA photoproduct ions. Tentative structural assignments of the photoproducts are provided in Table S5, with proposed photochemical reaction pathways (Section S13A).
Figure 12 shows the absorption spectrum of THCA which was studied in acetonitrile due to poor solubility in methanol. The spectrum is similar to that of CBDA, with a three-band profile (Band I (λmax ≈ 226 nm), band II (λmax~274 nm), and band III (λmax~308 nm)). Photolysis at 280 nm over 120 min produced similar results to CBDA, with decreases in bands I, II and III and a low-intensity, long-wavelength feature emerging at around λmax = 342 nm (band IV) following irradiation. Figure S16 for THCA shows changes in the absorbance intensity at selected wavelengths as a function of photolysis time.
Figure 13 shows the ESI-MS of [THCA − H]− obtained prior to irradiation, and after 30 min of irradiation at 280 and 365 nm. The precursor ion [THCA − H]− is visible at m/z 357, with a strong dimer peak at m/z 715. Photolysis is evident upon 365 nm irradiation (Figure 13a,b), visible via the decrease of the precursor ion and appearance of several, low-intensity photoproducts at m/z 371, 389, and 455. Irradiation at 280 nm also results in photolysis (Figure 13c,d), with production of the m/z 371 fragment ion as the major photoproduct ion, along with m/z 389, 403 and 684. Like CBDA, the extent of 280 nm photolysis is again lower than for the cannabinoids studied above (Section 2.1 and Section 2.2), due to 280 nm excitation occurring in a region of relatively lower absorption intensity.
The corresponding TRPMS of THCA are given in Figures S17 and S18 for 280 and 365 nm photolysis, with Table S4 providing a full list of the photoproduct ions. Tentative structural assignments of the photoproducts are provided in Table S5, with proposed photochemical reaction pathways (Section S13A).

2.4. Synthetic Cannabinoids (JWH-018 and MDMB-FUBINACA)

Across all photolysis experiments, both JWH-018 and MDMB-FUBINACA displayed high photochemical stability, with no evidence of degradation under either 280 nm or 365 nm irradiation. For both molecules, the UV–Vis spectra (Figures S20 and S21) remained essentially unchanged over the full irradiation period, indicating no significant degradation at either 365 or 280 nm. The corresponding time-dependent absorbance plots (Figures S22 and S23) further confirmed this. Consistent with these measurements, ESI-MS (Figures S24 and S25) recorded before and after irradiation for both of the synthetic cannabinoids were effectively identical, with the precursor ions and their characteristic collisional fragment ions displaying stable intensities and no photoproducts appearing. These results demonstrate that both JWH-018 and MDMB-FUBINACA are photostable at 365 and 280 nm, in distinct contrast to natural cannabinoids such as THC and CBD, which readily undergo oxidative and structural transformations under similar irradiation. The photostability of these molecules at these excitation energies can be directly traced to their low absorbances at these wavelengths (Figures S20 and S21).

3. Materials and Methods

General: Δ9-tetrahydrocannabinol (THC), 11-nor-9-carboxy-Δ9-tetrahydrocannabinol (THC-COOH-11), and 11-hydroxy-Δ9-tetrahydrocannabinol (THC-OH-11) standards were purchased from Cambridge Bioscience (Cambridge, UK). MDMB-FUBINACA, JWH-018, Cannabidiolic Acid (CBDA), and Tetrahydrocannabinolic acid (2-COOH-THC) were purchased from Sigma Aldrich (Gillingham, UK). All samples were purchased as solutions in methanol except for MDMB-FUBINACA and Tetrahydrocannabinolic acid, which were available only in acetonitrile. HPLC-grade methanol and acetonitrile were used to dilute the standards and were purchased from Fisher Scientific, Inc. (Pittsburgh, PA, USA).
UV–Vis Spectroscopy: Ultraviolet–visible (UV–Vis) spectroscopy measurements were recorded using a Genesys™ 180 Spectrophotometer (ThermoFisher Scientific, Waltham, MA, USA) in double-beam mode at a resolution of 2 nm measuring absorbance from 200 nm to 600 nm. The mounted T-Cube LED diode (part number: M280L6 and M365L2) illuminating light at a wavelength of 280 nm and 365 nm was purchased from Thorlabs (Ely, UK). A T-Cube power supply (part number: LEDD1B) was also purchased from the same supplier. For the UV–Vis photolysis experiment, all molecules were placed in a cuvette (with a cap on to prevent sample evaporation) with a 1 cm path length and approximately 3 mL volume of working solution. The samples were directly irradiated by the LED at different time intervals, using the full intensity (0.5 A for 280 nm and 1.0 A for 365 nm) of the diode. Recordings of the irradiated samples on a UV–Vis spectrometer for THC, CBD, THC-COOH, THC-OH, MDMB-FUBINACA, and JWH-018 were taken at time intervals of 0, 5, 10, 15, 30, 60, and 120 min. For 2-COOH-THC and CBDA, recordings were taken at time intervals of 0, 5, 10, 20, 40, 80, and 120 min after photolysis began. This was to optimise the data collection for the individual systems. Methanol was used as the blank (baseline) solvent for all samples except for MDMB-FUBINACA and THCA acid, where acetonitrile was used (all solution concentrations were 10−5 M). Solutions were stored in amber bottles to prevent photolysis from ambient light sources prior to experiments.
UV Photolysis with Online Mass Spectrometry Detection: Experiments were conducted by allowing LED irradiation to fall on a custom-made quartz-glass syringe (6.82 mm diameter) fitted with a Luer lock tip to allow direct connection to the ESI needle. This represents a modification of a solution-phase photolysis method employed previously [27,30]. The ESI output was introduced into the commercial mass spectrometer under normal operating conditions, and ESI–MS spectra were recorded to probe solution-phase photolysis in real time. The quartz glass used for the syringe was transparent to both UVA and UVB radiation. Ultraviolet irradiation was provided by mounted LED light sources (365 nm, M365L3; 280 nm, M280L6; Thorlabs, Ely, UK), with the LEDs positioned approximately 10–20 mm from the syringe. The maximum LED irradiances (power densities) were approximately 0.1 mW cm−2 at 280 nm and 1.44 mW cm−2 at 365 nm, as specified by the manufacturer at a distance of 200 mm under maximum drive current. Mass spectra acquired during photolysis (“on” spectra) were compared with spectra obtained under identical dark conditions, where the syringe was enclosed in a black box without LED irradiation. Solution concentrations of 1 × 10−5 M were prepared in either methanol or acetonitrile, depending on compound solubility. Full-scan mass spectra were recorded at defined time intervals following initiation of photolysis by switching on the LED. To prevent cross-contamination and eliminate residual signals, the instrument was thoroughly flushed with the appropriate solvent between measurements. All experiments were performed in triplicate to ensure reproducibility.
Mass spectra were recorded using an amaZon SL Dual Funnel Ion Trap Mass Spectrometer (Bruker Daltonics, Bremen, Germany) as described previously [42], with an electrospray ionisation source operating in negative ion mode. The amazon SL is a quadrupole ion trap instrument operating at better than unit mass resolution. Spectra were acquired over a m/z range of 50–800 with enhanced resolution mode enabled. The ion charge control (ICC) target was set to 100,000 with a maximum accumulation times of 200 ms, and spectra were averaged over 15 scans. The syringe-pump flow rate was 0.60 mL/hr. Under these conditions, mass accuracy is typically within ±0.2–0.5 units (ion trap nominal mass accuracy). Higher-energy collisional dissociation (HCD) experiments were performed on an Orbitrap Fusion Tribrid mass spectrometer (Thermo Fisher Scientific, Waltham, MA, USA) equipped with an H-ESI source operating in negative ion mode. Ion source parameters were as follows: spray voltage 3300 V; sheath gas 8 (arb. units); auxiliary gas 2 (arb. units); sweep gas 0; ion transfer tube temperature 300 °C; vaporiser temperature 20 °C; and RF lens 60%. Precursor ions were isolated using the quadrupole mass filter with a 1 m/z isolation window and subjected to HCD activation at fixed collision energy. MS2 spectra were acquired in the ion trap detector (enhanced scan rate) with centroid data processing. Microscan was set to 5, and the AGC target was set to standard with automatic maximum injection time. Precursor ions were isolated using the quadrupole mass filter with a 1 m/z isolation window and subjected to HCD activation under fixed collision energy conditions. MS2 spectra were acquired in the ion trap detector (enhanced scan rate) with centroid data processing.

4. Conclusions

The photolysis profiles of a group of cannabinoids have been studied using a combination of UV–Vis spectroscopy and mass spectrometry, using excitation wavelengths in the UVA and UVB (365 and 280 nm). Inspection of the UV–Vis spectra as a function of photolysis time reveals that all six phytocannabinoids (THC, CBD, THCA, CBDA, THC-COOH, THC-OH) photodegrade with 280 nm excitation, whereas the synthetic cannabinoids (JWH-018, MDMB-FUBINACA) do not. None of the cannabinoids displayed significant photodegradation with 365 nm excitation, consistent with the molecules’ low absorbances at that photon energy. Based on precursor-ion half-lives (tI0/2, where I0 is the initial precursor ion intensity prior to photolysis occurring) derived from TRPMS measurements, THC-COOH photodegrades most rapidly (tI0/2 ≈ 10 min), falling to 50% intensity ~1.3 times faster than THC (tI0/2 ≈ 13 min). THC, CBD (tI0/2 ≈ 15 min), and THC-OH (tI0/2 ≈ 15.5 min) exhibit comparable longer decay times. In contrast, the acidic cannabinoids, THCA and CBDA, do not reach 50% decay within the experimental timeframe (tI0/2 > 30 min), while no measurable photodegradation is observed for JWH-018 and MDMB-FUBINACA.
On-line photolysis coupled with time-resolved mass spectrometry was applied to determine the photoproducts of THC, CBD, THCA, CBDA, THC-COOH, and THC-OH. We found that all of these cannabinoids display numerous photodegradation pathways, although the photoactivated addition of methanol is dominant. Other common degradation pathways include aromatisation, addition of oxygen, and addition/loss of H atoms (H atom loss is a well-known photolytic breakdown pathway for phenol moieties [50,51]). While these general pathways were identified previously in separate photolysis studies of CBD and THCA, our study is the first to provide a comparable study for the set of key cannabinoids, and thus demonstrates the generality of the mechanisms. This insight will be valuable for subsequent toxicological analysis of the photoproducts. Furthermore, our TRPMS results provide direct mechanistic insight into the competing photolysis pathways, indicating that the initial photoactivated addition of methanol commonly acts as an early step that feeds into the formation of multiple secondary photoproducts [26,52]. While structural assignments presented in the current work are tentative, it will be possible to perform further structural characterisation via IRMPD spectroscopy linked to TRPMS in future work [34].
The work presented in this manuscript is motivated by providing fundamental photochemical measurements for the cannabinoids studied. We note that modified photoproducts may be produced in different solvent environments, e.g., pure water, and this should be considered in applying the results here to chemical environments relevant to the natural environment. The extent to which solvent identity affects the observed photoproducts could be tested in future work by conducting TRPMS on solutions where the composition of solvent is varied.
The results for THC and CBD merit further comment. Our results show distinct differences in the photoproduct ions generated on 280 nm photolysis for the two molecules, a result that is not in agreement with earlier results [26,44]. While a prior study of CBD had identified a mix of photoproducts, much earlier work on THC had identified only limited photoproduct formation [44]. The results obtained here are reasonable given the close geometric (and hence electronic) structures of the THC and CBD isomeric pair. Perhaps more interesting, it is notable that despite their similar structures, THC and CBD each produce a distinctive set of photoproducts, particularly in terms of the relative product intensities. This is interesting as it suggests that UV photodissociation of these systems could be used for structure verification [53,54].
The synthetic cannabinoids JWH-018 and MDMB-FUBINACA displayed no significant photolysis under either UVA or UVB irradiation. The molecular structures of these synthetic cannabinoids are strikingly different from the phytocannabinoids, readily explaining the different photolysis behaviour [7]. These differences are important, however, in an environmental context, since photostability is aligned with persistence in the natural environment, indicating that these synthetic cannabinoids will have long residence times in the natural environment [13,14,15,16]. Conversely, the extent of photostability also impacts on the viability of tracking cannabinoids through water systems, a valuable goal for law enforcement. Accurate tracking further requires reliable differentiation between closely related cannabinoid isomers, such as Δ8-THC and Δ9-THC, which has recently been demonstrated using advanced mass spectrometry supported by computational analysis [55]. Our work indicates that tracking natural cannabinoids such as THC will be more challenging than some synthetic cannabinoids [8,15].

Supplementary Materials

The following supporting information can be downloaded at: https://www.mdpi.com/article/10.3390/molecules31050813/s1, Figure S1: Absorbance versus photolysis time measurements for THC obtained from UV–Vis absorption spectra; Figure S2: Higher collision-induced dissociation (HCD) curves for [THC − H]− showing precursor ion dissociation and fragment ion production as a function of HCD energy. Figure S3: Absorbance versus photolysis time measurements for CBD obtained from UV–Vis absorption spectra. Figure S4: ESI-MS spectra of CBD recorded under 365 and 280 nm photolysis conditions; Figure S5: HCD curves for [CBD − H]− showing precursor ion dissociation and fragment ion production as a function of HCD energy. Figure S6: Absorbance versus photolysis time measurements for THC-COOH obtained from UV–Vis absorption spectra; Figure S7: ESI-MS spectra of THC-COOH recorded under 365 and 280 nm photolysis conditions. Figure S8: HCD curves for [THC-COOH − H]− showing precursor ion dissociation and fragment ion production as a function of HCD energy. Figure S9: Absorbance versus photolysis time measurements for THC-OH obtained from UV–Vis absorption spectra; Figure S10: ESI-MS spectra of THC-OH recorded under 365 and 280 nm photolysis conditions. Figure S11: HCD curves for [THC-OH − H]− showing precursor ion dissociation and fragment ion production as a function of HCD energy. Figure S12: Absorbance versus photolysis time measurements for CBDA obtained from UV–Vis absorption spectra; Figures S13 and S14: Time-resolved photolysis mass spectrometry (TRPMS) data for CBDA recorded during 365 and 280 nm photolysis; Figure S15: HCD curves for [CBDA − H]− showing precursor ion dissociation and fragment ion production as a function of HCD energy. Figure S16: Absorbance versus photolysis time measurements for THCA obtained from UV–Vis absorption spectra; Figures S17 and S18: Time-resolved photolysis mass spectrometry (TRPMS) data for THCA recorded during 365 and 280 nm photolysis; Figure S19: HCD curves for [THCA − H]− showing precursor ion dissociation and fragment ion production as a function of HCD energy. Figure S20: UV–Vis absorption spectra monitoring photolysis of JWH-018 and MDMB-FUBINACA; Figure S21: Absorbance versus photolysis time measurements for JWH-018 and MDMB-FUBINACA. Figure S22: ESI-MS spectra of JWH-018 and MDMB-FUBINACA recorded under 365 and 280 nm photolysis conditions. Figure S23: Photograph of the quartz syringe photolysis apparatus used in the experiments; Figure S24: Photograph of the experimental setup used for UV photolysis. Figure S25: UV–Vis absorbance versus wavelength spectra recorded at 0 min for all cannabinoids studied. Figure S26: Picture of the Quartz syringe which is used in the current experiments. Figure S27: Photo of the experimental setup used for UV photolysis. A UV LED shines on the ESI-syringe, allowing the sample to be exposed to light before entering the mass spectrometer. Figure S28. Solution-phase UV–Vis absorption spectra of Cannabinoids at 0 min. Table S1: Comparison of observed m/z fragments from THC-COOH photolysis in negative ESI mode under three conditions: no light (OFF), 280 nm UV irradiation (30 min), and 365 nm UV irradiation (30 min). Table S2: Comparison of observed m/z fragments from THC-OH photolysis in negative ESI mode under three conditions: no light (OFF), 280 nm UV irradiation (30 min), and 365 nm UV irradiation (30 min). Table S3: Comparison of observed m/z fragments from CBDA photolysis in negative ESI mode under three conditions: no light (OFF), 280 nm UV irradiation (30 min), and 365 nm UV irradiation (30 min). Table S4: Comparison of observed m/z fragments from THCA photolysis in negative ESI mode under three conditions: no light (OFF), 280 nm UV irradiation (30 min), and 365 nm UV irradiation (30 min). Table S5: Tentative structural assignments of negative-ion photoproducts observed during photolysis of THC, CBD, THC-COOH, THC-OH, CBDA, and THCA based on measured m/z values and proposed secondary photochemical pathways.

Author Contributions

Conceptualisation, C.E.H.D.; methodology, C.E.H.D., A.S.A.S. and K.O.U.; investigation, A.S.A.S., K.P.S. and K.O.U.; formal analysis, A.S.A.S. and K.O.U.; resources, C.E.H.D.; data curation, A.S.A.S.; writing—original draft preparation, A.S.A.S.; writing—review and editing, C.E.H.D., A.S.A.S., K.P.S. and K.O.U.; supervision, C.E.H.D. and K.O.U. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

Data is available from the research data repository of the University of York at https://doi.org/10.15124/1e81a765-1fb4-435c-83d4-8b55fc7417b6 (accessed on 19 February 2026).

Acknowledgments

We thank Abigail Mortimer for constructing the quartz syringe used in the experiments. A.S.A.S gratefully acknowledges the Department of Chemistry for providing a Wild Doctoral Scholarship. The York Centre of Excellence in Mass Spectrometry, used for the HRMS work, was created thanks to a major capital investment through Science City York, supported by Yorkshire Forward with funds from the Northern Way Initiative, and has more recently received additional support from the Engineering and Physical Sciences Research Council and Biotechnology and Biological Sciences Research Council.

Conflicts of Interest

The authors declare no conflicts of interest.

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Molecules 31 00813 sch001
Scheme 1. Structures, chemical formulae and exact masses (parenthesis) of the cannabinoids studied in this work, namely (a) Δ9-tetrahydrocannabinol (THC), (b) cannabidiol (CBD), (c) 11-nor-9-carboxy-Δ9-tetrahydrocannabinol (THCOOH), (d) 11-hydroxy-Δ9-tetrahydrocannabinol (THCOH), (e) Cannabidiolic Acid (CBDA), (f) Tetrahydrocannabinolic acid (THCA), (g) MDMB-FUBINACA, and (h) JWH-018.
Scheme 1. Structures, chemical formulae and exact masses (parenthesis) of the cannabinoids studied in this work, namely (a) Δ9-tetrahydrocannabinol (THC), (b) cannabidiol (CBD), (c) 11-nor-9-carboxy-Δ9-tetrahydrocannabinol (THCOOH), (d) 11-hydroxy-Δ9-tetrahydrocannabinol (THCOH), (e) Cannabidiolic Acid (CBDA), (f) Tetrahydrocannabinolic acid (THCA), (g) MDMB-FUBINACA, and (h) JWH-018.
Molecules 31 00813 sch001
Molecules 31 00813 g001
Figure 1. Solution-phase UV–Vis absorption spectra of THC in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Figure 1. Solution-phase UV–Vis absorption spectra of THC in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Molecules 31 00813 g001
Molecules 31 00813 g002
Figure 2. (a) Photolysis OFF and (b,c) photolysis ON ESI MS of THC obtained in negative ion mode. (b,c) displays the ESI-MS obtained with 365 and 280 nm photolysis, respectively. The [THC − H]− precursor ion is visible at m/z 313, indicated by *.
Figure 2. (a) Photolysis OFF and (b,c) photolysis ON ESI MS of THC obtained in negative ion mode. (b,c) displays the ESI-MS obtained with 365 and 280 nm photolysis, respectively. The [THC − H]− precursor ion is visible at m/z 313, indicated by *.
Molecules 31 00813 g002
Molecules 31 00813 g003
Figure 3. ESI-MS ion intensities (negative ion mode) for 280 nm photolysis of solution-phase THC displayed as a function of time: (a) displays the ion intensities for the precursor ion, [THC − H]−, with the five most intense photoproduct ions, with (b) showing the next five most intense photoproduct ions. Photolysis is initiated at t = 3 min and there is a 1 min lead time for the solution to reach the MS.
Figure 3. ESI-MS ion intensities (negative ion mode) for 280 nm photolysis of solution-phase THC displayed as a function of time: (a) displays the ion intensities for the precursor ion, [THC − H]−, with the five most intense photoproduct ions, with (b) showing the next five most intense photoproduct ions. Photolysis is initiated at t = 3 min and there is a 1 min lead time for the solution to reach the MS.
Molecules 31 00813 g003
Molecules 31 00813 g004
Figure 4. Solution-phase UV–Vis absorption spectra of CBD in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Figure 4. Solution-phase UV–Vis absorption spectra of CBD in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Molecules 31 00813 g004
Molecules 31 00813 g005
Figure 5. ESI-MS ion intensities (negative ion mode) for 280 nm photolysis of solution-phase CBD displayed as a function of time. (a) Displays the ion intensities for the precursor ion, [CBD − H]−, with the five most intense photoproduct ions, with (b) showing the next five most intense photoproduct ions. Photolysis is initiated at t = 3 min and there is a 1 min lead time for the solution to reach the MS.
Figure 5. ESI-MS ion intensities (negative ion mode) for 280 nm photolysis of solution-phase CBD displayed as a function of time. (a) Displays the ion intensities for the precursor ion, [CBD − H]−, with the five most intense photoproduct ions, with (b) showing the next five most intense photoproduct ions. Photolysis is initiated at t = 3 min and there is a 1 min lead time for the solution to reach the MS.
Molecules 31 00813 g005
Molecules 31 00813 g006
Figure 6. Solution-phase UV–Vis absorption spectra of THCOOH in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Figure 6. Solution-phase UV–Vis absorption spectra of THCOOH in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Molecules 31 00813 g006
Molecules 31 00813 g007
Figure 7. ESI-MS ion intensities (negative ion mode) for 280 nm photolysis of solution-phase THCOOH displayed as a function of time, showing the decrease in the precursor ion [THCOOH − H]− (m/z 343) and the increase in the 10 most intense photoproduct ions. Photolysis is initiated at t = 3 min and there is a 1 min lead time for the solution to reach the MS.
Figure 7. ESI-MS ion intensities (negative ion mode) for 280 nm photolysis of solution-phase THCOOH displayed as a function of time, showing the decrease in the precursor ion [THCOOH − H]− (m/z 343) and the increase in the 10 most intense photoproduct ions. Photolysis is initiated at t = 3 min and there is a 1 min lead time for the solution to reach the MS.
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Molecules 31 00813 g008
Figure 8. Solution-phase UV–Vis absorption spectra of THCOH in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Figure 8. Solution-phase UV–Vis absorption spectra of THCOH in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Molecules 31 00813 g008
Molecules 31 00813 g009
Figure 9. ESI-MS ion intensities (negative ion mode) for 280 nm photolysis of solution-phase THCOH displayed as a function of time, showing the decrease in the precursor ion [THCOH − H]− (m/z 329) and the increase in the 10 most intense photoproduct ions. Photolysis is initiated at t = 3 min and there is a 1 min lead time for the solution to reach the MS.
Figure 9. ESI-MS ion intensities (negative ion mode) for 280 nm photolysis of solution-phase THCOH displayed as a function of time, showing the decrease in the precursor ion [THCOH − H]− (m/z 329) and the increase in the 10 most intense photoproduct ions. Photolysis is initiated at t = 3 min and there is a 1 min lead time for the solution to reach the MS.
Molecules 31 00813 g009
Molecules 31 00813 g010
Figure 10. Solution-phase UV–Vis absorption spectra of CBDA in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Figure 10. Solution-phase UV–Vis absorption spectra of CBDA in MeOH obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
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Molecules 31 00813 g011
Figure 11. (a) Photolysis OFF and (b) photolysis ON ESI mass spectra of CBDA obtained in negative ion mode, with 365 nm photolysis. (c) Photolysis OFF and (d) photolysis ON ESI mass spectra of CBDA obtained in negative ion mode, with 280 nm photolysis. The [CBDA − H]− precursor ion is visible at m/z 357, marked by *.
Figure 11. (a) Photolysis OFF and (b) photolysis ON ESI mass spectra of CBDA obtained in negative ion mode, with 365 nm photolysis. (c) Photolysis OFF and (d) photolysis ON ESI mass spectra of CBDA obtained in negative ion mode, with 280 nm photolysis. The [CBDA − H]− precursor ion is visible at m/z 357, marked by *.
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Molecules 31 00813 g012
Figure 12. Solution-phase UV–Vis absorption spectra of THCA in ACN obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Figure 12. Solution-phase UV–Vis absorption spectra of THCA in ACN obtained following irradiation at 280 nm over 0–120 min. The arrows indicate the changes in the UV spectral bands upon photolysis.
Molecules 31 00813 g012
Molecules 31 00813 g013
Figure 13. (a) Photolysis OFF and (b) photolysis ON ESI-MS of THCA obtained in negative ion mode, with photolysis at 365 nm. (c) Photolysis OFF and (d) photolysis ON ESI-MS of THCA obtained in negative ion mode, with photolysis at 280 nm. The [THCA − H]− precursor ion is visible at m/z 357, indicated by *.
Figure 13. (a) Photolysis OFF and (b) photolysis ON ESI-MS of THCA obtained in negative ion mode, with photolysis at 365 nm. (c) Photolysis OFF and (d) photolysis ON ESI-MS of THCA obtained in negative ion mode, with photolysis at 280 nm. The [THCA − H]− precursor ion is visible at m/z 357, indicated by *.
Molecules 31 00813 g013
Table 1. Comparison of observed m/z fragments from THC and CBD photolysis in methanol with negative ion mode ESI under three conditions: no light (OFF), 280 nm UV light (30 min), and 365 nm UV light (30 min). ✓ indicates that the ion is observed, ✗ that it is not observed. The precursor ion (m/z 313) is indicated by *. (Very strong (vs), strong (s), and weak (w)).
Table 1. Comparison of observed m/z fragments from THC and CBD photolysis in methanol with negative ion mode ESI under three conditions: no light (OFF), 280 nm UV light (30 min), and 365 nm UV light (30 min). ✓ indicates that the ion is observed, ✗ that it is not observed. The precursor ion (m/z 313) is indicated by *. (Very strong (vs), strong (s), and weak (w)).
m/zTHC_No PhotTHC_280 nmTHC_365 nmCBD_No PhotCBD_280 nmCBD_365 nm
113✓✓ (s)✗✗✓ (s)✓
179✓ a✗✓ a✓ a✗✓ a
191✓ a✗✓ a✗✗✗
207✗✓ (s)✗✗✓ (s)✓
245✓ a✗✓ a✓ a✗✓ a
253✓✓ (s)✗✗✓ (s)✓
289✓✓ (s)✓✗✓ (vs)✓
311✓ a✗✓ a✓ a✗✓ a
313 *✓ (vs)✗✓ (vs) ✓ (vs)✗✓ (vs)
345✗✓ (vs)✗✗✓ (vs)✗
359✗✓ (w)✗✗✓ (vs)✗
363✗✓ (w)✗✗✓ (vs)✗
375✗✓ (vs)✗✗✓ (vs)✗
381✗✓ (vs)✗✗✓ (w)✗
389✗✓ (w)✗✗✓ (vs)✗
391✗✓ (s)✗✗✓ (s)✗
393✗✓ (vs)✗✗✓ (w)✗
407✗✓ (s)✗✗✓ (s)✗
477✗✓ (w)✗✗✓ (s)✗
479✗✓ (w)✗✗✓ (s)✗
481✗✓ (s)✗✗✓ (s)✗
509✗✓ (s)✗✗✓ (w)✗
511✗✓ (vs)✗✗✓ (w)✗
513✗✓ (s)✗✗✓ (w)✗
627 ✓ (vs)✗✓ (vs)✓ (vs)✗✓ (vs)
a Present as a strong fragment at 20% HCD (Figures S2 and S5).
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Shaikh, A.S.A.; Uleanya, K.O.; Selwe, K.P.; Dessent, C.E.H. UVA and UVB Photolysis of Natural and Synthetic Cannabinoids Studied by Online Mass Spectrometry. Molecules 2026, 31, 813. https://doi.org/10.3390/molecules31050813

AMA Style

Shaikh ASA, Uleanya KO, Selwe KP, Dessent CEH. UVA and UVB Photolysis of Natural and Synthetic Cannabinoids Studied by Online Mass Spectrometry. Molecules. 2026; 31(5):813. https://doi.org/10.3390/molecules31050813

Chicago/Turabian Style

Shaikh, Ambar S. A., Kelechi O. Uleanya, Kgato P. Selwe, and Caroline E. H. Dessent. 2026. "UVA and UVB Photolysis of Natural and Synthetic Cannabinoids Studied by Online Mass Spectrometry" Molecules 31, no. 5: 813. https://doi.org/10.3390/molecules31050813

APA Style

Shaikh, A. S. A., Uleanya, K. O., Selwe, K. P., & Dessent, C. E. H. (2026). UVA and UVB Photolysis of Natural and Synthetic Cannabinoids Studied by Online Mass Spectrometry. Molecules, 31(5), 813. https://doi.org/10.3390/molecules31050813

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