Melis Kant1, Pawel Jaruga1, Erdem Coskun1,2, Samuel Ward3, Alexander D Stark3, Thomas Baumann4, David Becker3, Amitava Adhikary3, Michael D Sevilla3, Miral Dizdaroglu1. 1. Biomolecular Measurement Division, National Institute of Standards and Technology, 100 Bureau Drive, Gaithersburg, Maryland 20899, United States. 2. Institute for Bioscience & Biotechnology Research, University of Maryland, 9600 Gudelsky Way, Rockville, Maryland 20850, United States. 3. Department of Chemistry, Oakland University, 146 Library Drive, Rochester, Michigan 48309, United States. 4. National Superconducting Cyclotron Laboratory, Michigan State University, 640 South Shaw Lane, East Lansing, Michigan 48824, United States.
Abstract
We report on the physicochemical processes and the products of DNA damage involved in Ne-22 ion-beam radiation of hydrated (12 ± 3 H2O/nucleotide) salmon testes DNA at 77 K. Free radicals trapped at 77 K were identified using electron spin resonance (ESR) spectroscopy. The measurement of DNA damage using two different techniques of mass spectrometry revealed the formation of numerous DNA products. Results obtained by ESR spectroscopy showed that as the linear energy transfer (LET) of the ion-beam radiation increases along the beam track, the production of DNA radicals correspondingly increases until just before the Bragg peak is reached. Yields of DNA products along the ion-beam track were in excellent agreement with the radical production. This work is the first to use the combination of ESR spectroscopy and mass spectrometric techniques enabling a better understanding of mechanisms of radiation damage to DNA by heavy ion beams detailing the formation of DNA free radicals and their subsequent products.
We report on the physicochemical processes and the products of DNA damage involved in Ne-22 ion-beam radiation of hydrated (12 ± 3 H2O/nucleotide) salmon testes DNA at 77 K. Free radicals trapped at 77 K were identified using electron spin resonance (ESR) spectroscopy. The measurement of DNA damage using two different techniques of mass spectrometry revealed the formation of numerous DNA products. Results obtained by ESR spectroscopy showed that as the linear energy transfer (LET) of the ion-beam radiation increases along the beam track, the production of DNA radicals correspondingly increases until just before the Bragg peak is reached. Yields of DNA products along the ion-beam track were in excellent agreement with the radical production. This work is the first to use the combination of ESR spectroscopy and mass spectrometric techniques enabling a better understanding of mechanisms of radiation damage to DNA by heavy ion beams detailing the formation of DNA free radicals and their subsequent products.
The ever-increasing
use of ion-beam irradiation, especially with
protons and relatively heavy ions for cancer therapy, and a renewed
interest in extended space missions have resulted in increased interest
in the biological effects of ion beams.[1] The biological effects of ionizing radiation, including low linear
energy transfer (LET) γ- and X-rays and high-LET energetic ion
beams, are largely initiated by damage to the cellular DNA.[2] Radiation damage to DNA by ionizing radiation
can be broadly classified as arising from two effects, direct effects
and indirect effects.[2−6] Damage by direct effects has two components, the first in which
damage is caused by direct ionization of the DNA itself, resulting
in the formation of cation radicals and anion radicals on the DNA
structure.[2−4] A second component of direct effects (called the
quasi-direct effect) results from ionization of the first few water
molecules of solvation (ca. 10–12 H2O/nucleotide).[3,5−7] In this case,
the holes and electrons formed in the solvation shell are efficiently
transferred to DNA, thereby forming additional cation radicals and
anion radicals on the DNA.Indirect damage is mediated by reactive
free radicals formed by
the ionization of the surrounding bulk water, principally •OH, H•, and eaq–.[3,4] These may react with DNA constituents leading to DNA base and 2′-deoxyribose
products, strand breaks, unaltered base release, tandem lesions, 8,5′-cyclopurine-2′-deoxynucleosides,
and interstrand cross-links.[4,8−12] In this current work, the DNA was hydrated (designated by Γ)
to Γ = 12 ± 3 H2O/nucleotide. Thus, no bulk
water is present, and the indirect effect is largely suppressed. As
a result, the direct effects predominate.[3,5−7] Studies indicate that ca. 50% of
the DNA damage in cells is due to direct-type (direct and quasi-direct)
effects.[3]To fully understand the
radiation effects of ion-beam irradiation
on DNA and the spatial arrangement of the damage, the highly heterogeneous
deposition of energy that occurs with energetic ions must be taken
into account.[2,3,13−17] An oft-used model for the energy deposition invokes a track structure
in which the energetic ion, through relatively short-range interactions
with electrons in the target material, ionizes atoms of the target
forming a dense, cylindrical track of ionized atoms called the track
core.[18] The core is the high-LET region
of the track. The electrons that result from these initial ionizations
undergo multiple collisions with atoms in the target, resulting in
further ionizations. Although many electrons stay within the high
energy density core (Figure ) and largely recombine with holes, the most energetic of
them escape from the core as δ-rays and cause further ionizations
in a low-LET region of the track called the penumbra.[18] The energy deposition in the penumbra is very much like
that that occurs with low-LET radiation such as γ-rays and X-rays.[2,3,13−18] The radius of the core and penumbra both increase with energy, and
the penumbra radius is very much larger than that of the core.[18]
Figure 1
PARTRAC simulated track structure for three different
ions (H,
O-16, and He-4), all with energy 6.25 MeV/u. The insets show a high-density
ionization segment of the track (top inset) and a lower density ionization
area (bottom inset), superimposed on schematic DNA segments. Reproduced
from ref (18) with
the permission of the Danish Royal Academy of Science and Letters.
PARTRAC simulated track structure for three different
ions (H,
O-16, and He-4), all with energy 6.25 MeV/u. The insets show a high-density
ionization segment of the track (top inset) and a lower density ionization
area (bottom inset), superimposed on schematic DNA segments. Reproduced
from ref (18) with
the permission of the Danish Royal Academy of Science and Letters.In this work, we report on the investigation of
physicochemical
processes including the formation of DNA radicals and the resulting
products in DNA upon Ne-22 ion-beam radiation damage at 77 K to hydrated
highly polymerized salmon testes DNA. We used a combination of electron
spin resonance (ESR) spectroscopy to elucidate the DNA radicals formed
(Figure ) and gas
chromatography-tandem mass spectrometry (GC–MS/MS) and liquid-chromatography
tandem mass spectrometry (LC–MS/MS) with isotope dilution to
identify and quantify a plethora of DNA-base damage products including
8,5′-cyclopurine-2′-deoxynucleosides.
Figure 2
Radicals considered in
this work.
Radicals considered in
this work.
Results
Measurement of DNA Radicals
by ESR Spectroscopy
The
aim of this work was to investigate the mechanisms of direct-type
DNA damage by heavy-ion radiation by means of the formation of DNA
free radicals and products using ESR spectroscopy, GC–MS/MS,
and LC–MS/MS. The combined use of these techniques for this
purpose has not been reported previously. Highly polymerized salmon
testes DNA hydrated to Γ= 12 ± 3 H2O/nucleotide
was exposed to Ne-22 ion irradiation at 77 K. DNA radicals trapped
in DNA at 77 K were elucidated using ESR spectroscopy.Figure shows the ESR spectra
from Ne-22 ion-irradiated H2O-hydrated DNA. In earlier
work, we have thoroughly characterized spectra such as these from
both γ-irradiated and ion-beam-irradiated DNA.[2,3,5,6,14−17,20,21] Previous studies indicated that the spectra
are composites that result from at least seven radicals (Figure ). These are three
base radicals, G(−H)•/G•+, C(N3)H•/C•–, and T•–, which originate from ion-radical precursors.
The radiation causes loss of an electron from guanine leading to the
guanine radical cation (G•+), which undergoes reversible
intrabase pair proton transfer from N1 to the N3 of the base-paired
cytosine, forming the neutral free radical G(−H)• and diamagnetic cation C(N3)H+.[2,3,13,38,39] The addition of an electron to cytosine results in
the formation of the free radical C•– which
undergoes reversible protonation at N3, to form the radical C(N3)H•. T•– results from capture
of an electron by thymine.
Figure 3
ESR spectrum, at 77 K, of hydrated [Γ
= (12 ± 3) H2O/nucleotide] salmon testes DNA, using
Ne-22 ion irradiation
at 77 K. The Ne-22 ion energy at the entrance to the sample packet
was 1.14 GeV. The sample number indicates the position in the sample
packet, #1 at the entrance and #5 at the Bragg peak. Doses and LETs
for each spectrum are indicated. Each spectrum is a composite arising
from at least seven radicals (Figure ). The wings of the spectrum for the sample given the
highest dose have been expanded to show line components (indicated
by *) assigned to radicals on the 2′-deoxyribose sugar (Figure ). Three X’s
indicate Fremy Salt resonances, with the central marker at g = 2.0056 and AN = 13.09 G.
ESR spectrum, at 77 K, of hydrated [Γ
= (12 ± 3) H2O/nucleotide] salmon testes DNA, using
Ne-22 ion irradiation
at 77 K. The Ne-22 ion energy at the entrance to the sample packet
was 1.14 GeV. The sample number indicates the position in the sample
packet, #1 at the entrance and #5 at the Bragg peak. Doses and LETs
for each spectrum are indicated. Each spectrum is a composite arising
from at least seven radicals (Figure ). The wings of the spectrum for the sample given the
highest dose have been expanded to show line components (indicated
by *) assigned to radicals on the 2′-deoxyribose sugar (Figure ). Three X’s
indicate Fremy Salt resonances, with the central marker at g = 2.0056 and AN = 13.09 G.The three trapped base radicals form predominantly
in the ion-track
penumbra. This is because in the densely ionized core, base anion
and cation radicals form near one another and Coulombic attractions
drive their fast recombination.[2,3,13] Consequently, DNA-base radicals are not observed in significant
amounts at 77 K in the core.[2,3,13−17] On the other hand, in the sparsely ionized penumbra, about 30% of
the base radicals escape recombination and are trapped at 77 K.[2,3,13−17] The three 2′-deoxyribose radicals (C1′•, C3′•, and C5′•) are formed principally via an ionization-deprotonation
pathway, i.e., fast deprotonation of 2′-deoxyribose
cation radicals before recombination can occur, as part of an oxidative
damage mechanism.[2,3,13−17,20] On the other hand, C3′•dephos is formed by dissociative electron
attachment via the reaction of both radiation-produced
quasi-free electrons and low energy electrons with DNA, possibly through
the agency of excited states, in a reductive damage mechanism.[2,3,13−17,40−44] Most of the 2′-deoxyribose radicals are formed in the track
core, but a small fraction is also formed in the track penumbra.[2,3,13−17] These four 2′-deoxyribose radicals (C1′•, C3′•, C5′•, and C3′•dephos) are uncharged
and not as susceptible to recombination as are the base radicals.[2,3,13−17,20]The relative
amount of the radicals (base vs 2′-deoxyribose)
trapped depends on the LET of the radiation. At higher LETs, more
energy is generally deposited in the core and less in the penumbra,
and the fraction of base radicals found in the cohort of radicals
decreases.[2,3,13−17,20] Analysis of the 2′-deoxyribose
radical cohort using a specific benchmark spectrum for C5′• (Figure S3) indicates that
C5′• constitutes ca. 25%
of the trapped 2′-deoxyribose radicals in ion-beam-irradiated
hydrated DNA.[14] This is highly pertinent
to the formation of the 8,5′-cyclopurine-2′-deoxynucleosides
(see sections entitled “Measurement of DNA Products”
and “Discussion”). Figure shows the measured
yields (μmol/kg) of trapped radicals as the ion beam penetrates
into the sample packet. The seven blue bars in the graph represent
the seven ESR samples in the sample packet. Product yield results,
which were determined for thinner samples along the path than the
ESR samples, indicate that the Bragg peak occurs at about 4.8–5.2
mm in the packet. To construct the two red bars, 98% of the total
yield found in the fifth sample in the packet is imputed to the first ca. 0.4 mm of the sample, in recognition of the fact that
the last ca. 0.9 mm of the sample is unirradiated.
The 2% of the yield allocated to the last 0.9 mm of the fifth sample
gives the background yield for this packet. It should be noted here
that the total yield of trapped radicals at the Bragg peak is lower
than that found in the (fourth) pre-Bragg peak sample. In addition,
the small yields beyond the Bragg Peak are expected from beam fragmentation.
Figure 4
Yields
of trapped radicals (77 K) in Ne-22-irradiated, hydrated
[Γ = 12 ± 3 H2O/nucleotide] salmon testes DNA.
Yields in the seven samples used. Only the first five samples in the
packet were irradiated, the fifth only partially. Thus, the Bragg
peak for the Ne-22 ion is located in the fifth sample at ca. 5.2 mm penetration depth. The yield in the fifth sample is recalculated
in recognition of the fact that the beam penetrated only to ca. 5.2 mm into the sample packet, leaving most of the fifth
sample unirradiated. The uncertainties depicted represent the typical ca. 20% variation seen in measuring radical yields.
Yields
of trapped radicals (77 K) in Ne-22-irradiated, hydrated
[Γ = 12 ± 3 H2O/nucleotide] salmon testes DNA.
Yields in the seven samples used. Only the first five samples in the
packet were irradiated, the fifth only partially. Thus, the Bragg
peak for the Ne-22 ion is located in the fifth sample at ca. 5.2 mm penetration depth. The yield in the fifth sample is recalculated
in recognition of the fact that the beam penetrated only to ca. 5.2 mm into the sample packet, leaving most of the fifth
sample unirradiated. The uncertainties depicted represent the typical ca. 20% variation seen in measuring radical yields.Figure shows the
dose response of trapped radicals at 77 K for Ne-22-irradiated DNA.
The three curves shown represent the yields of (a) the four 2′-deoxyribose
radicals treated as a group (ΣdR•), (b) the
three base radicals treated as a group [G(−H)•/G•+ + C(N3)H• + T•–], and (c) the sum of all seven radicals, i.e.,
all of the radicals observed near g = 2.00 (Figure ). Because of unanticipated
handling problems with H2O-hydrated samples, this curve
is constructed from the ESR spectra from pre-Bragg peak samples for
the Ne-22-irradiated DNA samples hydrated with D2O rather
than H2O. We have found that there is little observable
difference between the behavior of D2O- versus H2O-hydrated samples insofar as radical yields are concerned.
Those yield curves which tend to or reach a plateau are fit to eq S2. For the total radical yield, G = 0.13 μmol/J with k = 5.5 × 10–6 Gy–1. The benchmark for the sum
of the 2′-deoxyribose radicals yields G =
0.052 μmol/J; since the fit for the 2′-deoxyribose radicals
is linear, k is zero. The curve for the sum of the base radical yields
is drawn for the eye only. The G-value for the total
trapped radicals at 77 K in similarly prepared and handled γ-irradiated
samples is 0.25 μmol/J.[20] Ne-22 beam-irradiated
samples have a lower G-value than γ-irradiated
samples due to rapid recombination of base radicals in the ion-beam
core, which leads to a diminution in trapped base radicals.
Figure 5
Dose response
of trapped radicals in Ne-22-irradiated D2O-hydrated [Γ
= 12 ± 3 H2O/nucleotide] salmon
testes DNA (77 K). Here, the label ⊙ represents the total radical
yield, “●” represents the sum of sugar radicals,
Σ(C1′• + C3′• + C5′• + C3′•dephos), and the label “○” represents
the sum of base radicals Σ[G(−H)•/G•+ + C(N3H)• + T•–]. Uncertainties are estimates based on typical spin-counting variability.
Dose response
of trapped radicals in Ne-22-irradiated D2O-hydrated [Γ
= 12 ± 3 H2O/nucleotide] salmon
testes DNA (77 K). Here, the label ⊙ represents the total radical
yield, “●” represents the sum of sugar radicals,
Σ(C1′• + C3′• + C5′• + C3′•dephos), and the label “○” represents
the sum of base radicals Σ[G(−H)•/G•+ + C(N3H)• + T•–]. Uncertainties are estimates based on typical spin-counting variability.
Measurement of DNA-Base Damage Products
DNA-base damage
products (Figure )
in the DNA samples were identified and quantified using two different
mass spectrometric techniques. LC–MS/MS with isotope dilution
was used for the measurement of the 8,5′-cyclo-2′-deoxynucleosides, i.e., (5′R)-8,5′-cyclo-2′-deoxyadenosine
(R-cdA), (5′S)-8,5′-cyclo-2′-deoxyadenosine
(S-cdA), (5′R)-8,5′-cyclo-2′-deoxyguanosine
(R-cdG), and (5′S)-8,5′-cyclo-2′-deoxyguanosine
(S-cdG), and the purine-derived lesions 8-hydroxyadenine
(8-OH-Ade) and 8-hydroxyguanine (8-OH-Gua) (also called 8-oxo-Gua)
as their 2′-deoxynucleosides, i.e., 8-hydroxy-2′-deoxyadenosine
(8-OH-dA) and 8-hydroxy-2′-deoxyguanosine (8-OH-dG), respectively.
The measurement of the pyrimidine-derived lesions, 5-hydroxycytosine
(5-OH-Cyt), thymine glycol (ThyGly), 5,6-dihydrothymine (5,6-diHThy),
5,6-dihydrocytosine (5,6-diHCyt), and 5,6-dihydrouracil (5,6-diHUra),
and purine-derived lesions 4,6-diamino-5-formamidopyrimidine (FapyAde)
and 2,6-diamino-4-hydroxy-5-formamidopyrimidine (FapyGua) was achieved
using GC–MS/MS with isotope dilution. The reason for the use
of GC–MS/MS for the measurement of these products is that this
technique is the best suitable one among available analytical techniques
for this purpose (see the Supporting Information and the cited literature). It should be noted that 5,6-diHUra is
produced to some extent by deamination of 5,6-diHCyt under acidic
conditions (see Experimental section in the Supporting Information). Figure illustrates the structures of these compounds. The yields
of 8,5′-cyclopurine-2′-deoxynucleosides with Ne-22 beam
irradiation along the ion-beam track are shown in Figure . Doses for these samples within
the beam range are shown in Table S1. A
steady increase in the yields was observed up to 4 mm along the radiation
path followed by some decrease up to 5 mm. Afterward, the yields sharply
decreased to slightly above the levels in unirradiated DNA samples
(less than 0.05 lesions/106 DNA bases). The Bragg peak
was likely to be at ca. 5.2 mm of the radiation path
(Figure ). The low
damage levels observed beyond the Bragg peak are likely due to inhomogeneity
in the samples and/or fragmentation of the ion beam. Table S1 in the Supporting Information shows the yields of
8,5′-cyclopurine-2′-deoxynucleosides in Ne-22-irradiated
DNA. In all cases, the yields of the R-diastereomers
were observed to be greater than those of the S-diastereomers
of both cdA and cdG. The R/S-ratios
practically remained constant for all the samples within acceptable
uncertainties (see the average values of the R/S-ratio with the uncertainties in Table S1).
Figure 6
Structures of DNA-base lesions found in Ne-22-irradiated hydrated
DNA.
Figure 7
Yields of 8,5′-cyclopurine-2′-deoxynucleosides
in
Ne-22 beam-irradiated hydrated (Γ = 12 ± 3 H2O/nucleotide) salmon testes DNA (measured by LC–MS/MS with
isotope dilution). The Bragg peak location is judged to be in the
5.0–5.2 mm region. For each of the samples, the yield is calculated
using the full sample mass. However, it should be noted that the sample
containing the Bragg peak may not be uniformly irradiated throughout
the sample depth. Uncertainties are standard deviations. Doses for
those samples within the beam range are shown in Table S1. (A) R-cdA, (B) S-cdA, (C) R-cdG, and (D) S-cdG.
Structures of DNA-base lesions found in Ne-22-irradiated hydrated
DNA.Yields of 8,5′-cyclopurine-2′-deoxynucleosides
in
Ne-22 beam-irradiated hydrated (Γ = 12 ± 3 H2O/nucleotide) salmon testes DNA (measured by LC–MS/MS with
isotope dilution). The Bragg peak location is judged to be in the
5.0–5.2 mm region. For each of the samples, the yield is calculated
using the full sample mass. However, it should be noted that the sample
containing the Bragg peak may not be uniformly irradiated throughout
the sample depth. Uncertainties are standard deviations. Doses for
those samples within the beam range are shown in Table S1. (A) R-cdA, (B) S-cdA, (C) R-cdG, and (D) S-cdG.For comparison, we also measured the yields of
these compounds
in calf thymus DNA γ-irradiated at 10 Gy in N2O-saturated
aqueous solution and in hydrated salmon testes DNA in the solid state
γ-irradiated at room temperature at 20 kGy. Table S2 in the Supporting Information shows the yields in
these samples. The yields in DNA samples γ-irradiated at 10
Gy in N2O-saturated aqueous solution were much greater
than those in hydrated DNA γ-irradiated with 20 kGy at room
temperature. At the highest level of damage, the yields of cdA and
cdG in DNA samples irradiated with Ne-22 ions at 77 K were similar
to those in calf thymus DNA samples γ-irradiated at 10 Gy in
aqueous solutions (compare Tables S1 and S2 in the Supporting Information). In making these comparisons, it
should be pointed out that the radiation chemistry in aqueous solutions
is quite different from that in hydrated DNA in the solid state. One
important distinction is that irradiation of an aqueous solution at
room temperature produces copious amounts of •OH
that in the absence of radical scavengers, migrate to and react with
the DNA.[2−4,13,42] It should be emphasized that the striking difference between the
DNA samples γ-irradiated in aqueous solutions and those γ-irradiated
at room temperature in the solid state or Ne-22 beam-irradiated at
77 K was in the ratios of the R-diastereomers to
the S-diastereomers of both cdA and cdG. The yields
of the S-diastereomers were greater than those of
the R-diastereomers in DNA γ-irradiated in
aqueous solutions, with the R/S ratios
being 0.90 for cdA and 0.73 for cdG (Table S2 in the Supporting Information). In contrast, the R-diastereomers dominated over the S-diastereomers
in hydrated DNA samples γ-irradiated with 20 kGy at room temperature
or Ne-22 beam-irradiated at 77 K with average R/S ratios being greater than 2 for both cdA and cdG (compare Tables S2 and S4 in the Supporting Information).
In the case of the other DNA-base lesions including 5,6-dihydropyrimidines,
a similar trend of the yields was observed for Ne-22 beam-radiation
doses at 77 K as was observed for the 8,5′-cyclo-2′-deoxynucleosides. Figures and 9 and Table S3 in the Supporting
Information show the yields of these lesions in DNA samples. The yield
of 5,6-diHCyt represents the total levels of 5,6-diHCyt and 5,6-diHUra
because the latter is formed by deamination of the former by acidic
treatment prior to GC–MS/MS analysis (see Experimental section
in the Supporting Information). Table S4 in the Supporting Information shows
the yields of DNA-base lesions in calf thymus DNA γ-irradiated
at 10 Gy in N2O-saturated aqueous solution and in hydrated
salmon testes DNA γ-irradiated at room temperature to 20 kGy.
In the case of the purine-derived lesions, the yields were somewhat
similar between the two types of DNA samples. In contrast, the yields
of the pyrimidine-derived lesions 5-OH-Cyt and ThyGly were significantly
lower in hydrated DNA than those in DNA γ-irradiated in aqueous
solutions.
Figure 8
Yields of DNA-base products in Ne-22 beam-irradiated hydrated (Γ
= 12 ± 3 H2O/nucleotide) salmon testes DNA. For each
of the samples, the yield is calculated using the full sample mass.
However, it should be noted that the sample containing the Bragg peak
may not be uniformly irradiated throughout the sample depth. Doses
for those samples within the beam range are shown in Table S3 in the Supporting Information. (A) 5-OH-Cyt, (B)
ThyGly, (C) FapyAde, (D) FapyGua (these four products were measured
by GC–MS/MS with isotope dilution), (E) 8-OH-dG, and (F) 8-OH-dA
(these two products were measured by LC–MS/MS with isotope
dilution). Uncertainties are standard deviations.
Figure 9
Yields
of (A) 5,6-diHThy and (B) 5,6-diHCyt in Ne-22 beam-irradiated
hydrated (Γ = 12 ± 3 H2O/nucleotide) salmon
testes DNA (measured by GC–MS/MS with isotope dilution). Uncertainties
are standard deviations.
Yields of DNA-base products in Ne-22 beam-irradiated hydrated (Γ
= 12 ± 3 H2O/nucleotide) salmon testes DNA. For each
of the samples, the yield is calculated using the full sample mass.
However, it should be noted that the sample containing the Bragg peak
may not be uniformly irradiated throughout the sample depth. Doses
for those samples within the beam range are shown in Table S3 in the Supporting Information. (A) 5-OH-Cyt, (B)
ThyGly, (C) FapyAde, (D) FapyGua (these four products were measured
by GC–MS/MS with isotope dilution), (E) 8-OH-dG, and (F) 8-OH-dA
(these two products were measured by LC–MS/MS with isotope
dilution). Uncertainties are standard deviations.Yields
of (A) 5,6-diHThy and (B) 5,6-diHCyt in Ne-22 beam-irradiated
hydrated (Γ = 12 ± 3 H2O/nucleotide) salmon
testes DNA (measured by GC–MS/MS with isotope dilution). Uncertainties
are standard deviations.
Discussion
In
this work, hydrated DNA samples (Γ = 12 ± 3 H2O/nucleotide) were irradiated at 77 K by an initial 1.14 GeV
Ne-22 beam. The ion energy degrades along its path through the stacked
samples and drops to zero at the path end just after the Bragg peak.
Smaller yields found in samples beyond the Bragg peak are in part
a result of fragmentation of the parent ion and the dose delivered
by the fragment ions. ESR spectroscopy was used to determine the yield
of DNA radicals trapped in hydrated DNA samples at 77 K. Subsequently,
upon warming of the same samples, GC–MS/MS and LC–MS/MS
analyses were carried out to identify and quantify resulting DNA products.
By analyses of ESR spectra recorded at 77 K, we determined the yields
of two separate cohorts of radicals that are responsible for the experimental
spectra: (a) the combined yield of the individual base radicals as
the DNA-base ion radicals (and their conjugate species in prototropic
equilibrium) and (b) the combined yield of the known four radicals
of the 2′-deoxyribose moiety, C1′•, C3′•, C5′•, and
C3′•dephos.[2,3,13−17] C1′•, C3′•, and C5′• are produced by (a) ionization
of 2′-deoxyribose, followed by deprotonation,[2,3,13−17,42] (b) charge and spin
transfer from the excited base cation radicals to 2′-deoxyribose-producing
cation radicals of 2′-deoxyribose, followed by deprotonation,[2,3,13,14,42] and (c) phosphate-to-2′-deoxyribose
hole transfer, followed by deprotonation.[42,43] On the other hand, the formation of C3′•dephos is associated with a radiation-produced low-energy
electron-mediated dissociative electron attachment process.[2,3,13−17,41]Using the trapped
radical yields in Ne-22 beam-irradiated hydrated
DNA samples that were obtained by ESR at 77 K and the physical track
structure model described above, we, in earlier work, developed a DNA Radiation Chemistry Track Structure Model that delineates
the spatial position, within the ion-beam track, of the early free
radicals responsible for the formation of clustered lesions, including
double-strand breaks, and the often mutagenic and/or cytotoxic DNA
products found at room temperature.[2,3,13−17,41] This model posits that the DNA-base
radicals and/or their charged precursors undergo rapid recombination
in the track core and, therefore, the trapped surviving DNA-base radicals
observed at 77 K are formed largely in the track penumbra.[2,3,13−17,41] In contrast, most of
the 2′-deoxyribose radicals that are formed in the core survive
at 77 K.[2] In addition, a small fraction
of the trapped 2′-deoxyribose radicals is formed in the penumbra.[2,3,13−17,41] Therefore, our DNA Radiation Chemistry Track Structure Model posits that
after ion-beam irradiation, most of the trapped DNA-neutral radicals
observed at 77 K form in the core and nearly all the charged base
ion radicals form in the penumbra.[2,3,13−17,41]In this work, the initial
free radicals that are trapped at 77
K in hydrated, anoxic DNA after Ne-22 ion-beam irradiation are investigated
and described, as a variety of potentially mutagenic and/or lethal
products formed when the irradiated samples are warmed to room temperature
and the initial radicals react to form products. Radical yields and
product yields are reported. The likely reactions that lead from the
initial radicals to the products are provided, and the spatial arrangements,
in the ion-beam track, of the initial radicals and the products formed
are described. Finally, the pertinence of these results to various
base lesions including 8,5′-cyclopurine-2′-deoxynucleosides
and 5,6-dihydropyrimidines are presented for the first time. The combination
of ESR spectroscopy and product analyses of Ne-22 ion-beam-irradiated
hydrated DNA has led to the following salient points:The location of maximum damage is found to be just before
the Bragg peak: ESR measurements presented in this work have
shown that as the LET of the ion-beam radiation increases, reaching
a peak at the Bragg peak, at which point the ions come to rest, the
production of cation, anion, and neutral radicals of DNA increases
along the ion-beam track, reaching a maximum in the sample just before
that containing the Bragg peak. With regard to the formation of C3′•dephos (see Figure for its structure), excitations increase
significantly just before and at the Bragg peak relative to the beam
plateau region.[40]This would tend
to increase the probability for the formation of
immediate strand breaks from low-energy electrons (LEEs), which can
involve transient anion excited states.[41−44] It has been shown that C3′•dephos and the phosphoryl radical (DNA–OP(•)O2–), which are the direct
products from a strand break, result from LEEs through the formation
of an excited-state transient negative ion (TNI)[13−17,40−44] and that the concentrations of these radicals are significantly
higher in ion-beam-irradiated samples than in γ-irradiated ones.[13−17] In fact, both are observed in our Ne-22-irradiated DNA/D2O samples. This suggests that increased strand breaks may occur near
the Bragg peak in ion-beam-irradiated DNA. The yields of DNA-base
damage products along the ion-beam track were in excellent agreement
with the radical production. Because the probability of recombination
of DNA radicals in the core increases due to the rise in concentration
of proximate ion radicals, the location of the highest energy deposition,
at the Bragg peak, should show different damage from the plateau region
of the beam. Furthermore, the yields of radicals and products found
at the Bragg Peak are lower than those found in the sample(s) just
before the Bragg Peak. This leads us to conclude that the location
of the maximum damage, insofar as the radicals and products described
here are concerned, is not at the Bragg Peak but just before the peak
in energy deposition and, thereby, the peak in dose. This, we think,
is an important finding of our work. The lower yield at the Bragg
peak is a result of the fact that as the ion slows to a stop at the
Bragg peak, the track “pencils down” to a point, increasing
the concentration of ionizations. This, in turn, increases ion recombination,
thereby significantly lowering the damage yield at the Bragg Peak.We note that the product yields are calculated using the mass of
the whole sample. As noted earlier, the sample containing the Bragg
peak may not have been irradiated for all of its depth and that the
product yield for the irradiated section of the sample
will be higher than that reported for the whole sample. See Figure for a similar effect
in ESR radical yields. Based on the observed yields, this does not
affect the conclusion that pre-Bragg peak samples typically have higher
yields of trapped radicals (77 K) and product yields than the sample
containing the Bragg peak.Yields of purine-derived
DNA-base lesions, i.e., FapyGua,
8-OH-Gua, FapyAde, and 8-OH-Ade: the mechanism of the formation
of the guanine-derived products is shown in Figure . In the first step of this mechanism, G•+ is formed by one-electron oxidation and is in prototropic
equilibrium with G(−H)•, which is dominant
at 77 K.[2,3,13,38,39] Although we could not
precisely determine the yields of trapped G(−H)•/G•+ in Ne-22 ion-beam-irradiated hydrated DNA,
computer deconvolution of the ESR spectra of the first four samples
depicted in Figure indicated that G(−H)•/G•+ comprises ca. 25% of the trapped radicals at 77
K. On the other hand, the yield of products FapyGua and 8-OH-Gua that
originate from G•+ and G(−H)• (Figure ) adds
to 13 ± 2% of the yield of trapped radicals at 77 K. This indicates
that roughly half of the trapped G•+ is converted
to FapyGua and 8-OH-Gua when samples are warmed. Since G•+ and G(−H)• radicals are in prototropic
equilibrium, the complete conversion of G(−H)• to FapyGua and 8-OH-Gua is possible. Figure also shows the mechanism of the formation
of these products by OH– addition (addition of H2O followed by deprotonation) to G•+ giving
rise to the C8–OH-adduct radical of Gua, which then undergoes
one-electron oxidation to yield 8-OH-Gua or one-electron reduction
to yield FapyGua, depending on experimental conditions.[3,4,13,21] The formation of the adenine-derived lesions, 8-OH-Ade and FapyAde,
occurs via analogous pathways from the adenine cation
(A•+) radical. Extensive ESR spectral analyses of
both γ-irradiated and ion-beam-irradiated (at 77 K) hydrated
DNA samples have not led to any observable trapped A•+ radicals at 77 K. Nevertheless, the observed formation of 8-OH-Ade
and FapyAde suggests that A•+ is formed upon Ne-22
ion-beam irradiation at 77 K at about 15% of G•+ levels based on the product yields. These levels are not in sufficient
intensity to be resolved in the ESR spectra.
Figure 10
Formation of FapyGua
and 8-OH-Gua from the guanine cation radical,
G•+.
Formation of FapyGua
and 8-OH-Gua from the guanine cation radical,
G•+.Moreover, Gua has the
lowest one-electron reduction potential (E7 = midpoint
potential = 1.29 V4) and the lowest
ionization energy among the DNA bases; as a consequence, the hole
localizes on Gua.[2−8,13,38−40,42] These properties of
Gua also explain the yields of FapyGua and 8-OH-Gua being much greater
than those of FapyAde and 8-OH-Ade in DNA samples that were Ne-22
ion-beam-irradiated at 77 K (Tables S3 and S4 in the Supporting Information). However, runs of Ade (i.e., sequences such as AAA) in DNA would likely have trapped A•+ which would account for the modest levels of products found for
Ade.Formation of R-cdA, S-cdA, R-cdG, and S-cdG in Ne-22 beam-irradiated hydrated DNA: the 2′-deoxyribose radical, C5′• (Figure ), has been
detected previously in hydrated DNA exposed to γ- and ion-beam
radiations.[13,14] Using a benchmark ESR spectrum
for C5′• (Figure S3 in the Supporting Information), it was estimated that C5′• makes up ca. 25% (ion-beam-irradiated)
to ca. 40% (γ-irradiated) of the 2′-deoxyribose
radicals (ΣdR•) trapped at 77 K.[14] Since, for each ESR sample, the yield of 2′-deoxyribose
radicals, as determined by spectral deconvolution using the ΣdR
benchmark spectrum can be estimated (Figure ), the yield of C5′• could also be estimated. Once formed, C5′• can undergo several reactions: (a) unaltered base release along
with strand break formation,[3,4,45] (b) 8,5′-intramolecular cyclization followed by one-electron
oxidation, leading to the formation of R-cdA, S-cdA, R-cdG, and S-cdG,[8−10] and (c) cross-link production.[4,8−13] When compared with the measured yields of 8,5′-cyclopurine-2′-deoxynucleosides
[Σ(R-cdA + S-cdA + R-cdG + S-cdG)], it is found that approximately
(4.1 ± 1.1)% of the trapped C5′• reacts
to form these products. The reactions leading to the formation of R-cdA and S-cdA from C5′• radicals in DNA are shown in Figure . The formation of R-cdG
and S-cdG occurs via analogous reactions.
It should be pointed out that R-cdA, S-cdA, R-cdG, and S-cdG were identified
in ion-beam-irradiated DNA at 77 K for the first time in this work.
Figure 11
Reactions
leading from the C5′• of 2′-deoxyadenosine
to R-cdA and S-cdA.
Reactions
leading from the C5′• of 2′-deoxyadenosine
to R-cdA and S-cdA.Our results show that for R-cdA, S-cdA, R-cdG, and S-cdG
measured
in DNA samples γ-irradiated in aqueous solutions and in irradiated
cells at ambient temperature,[9] the yields
of the S-diastereomers were found to be greater than
those of the R-diastereomers. This was confirmed
in the present work for the yields of cdG and cdA in DNA γ-irradiated
in aqueous solutions (Table S2 in the Supporting
Information). However, hydrated DNA samples of Ne-22 ion-irradiated
at 77 K or γ-irradiated at room temperature exhibited greater
yields of the R-diastereomers than those of the S-diastereomers for both cdA and cdG (Tables S1 and S4 in the Supporting Information). This is quite
an interesting phenomenon which is due to a stereoisomeric effect
on the formation of the covalent bond between C5′• of 2′-deoxyribose and C8 of Ade or Gua in the same nucleoside
in the hydrated DNA vs that of DNA in solution. Our
ESR studies established that the conformations of C5′• in γ-irradiated hydrated DNA and in ion-beam-irradiated DNA
are quite similar.[13,14] This finding explains our observation
of greater yields of R-diastereomers than those of
the S-diastereomers for both cdA and cdG in hydrated
DNA samples either γ-irradiated at room temperature or Ne-22
beam-irradiated at 77 K.Based on these results, the R/S ratio of 8,5′-cyclopurine-2′-deoxynucleosides
may
be diagnostic for the direct or indirect effect of ionizing radiations.
In addition, recent theoretical calculations[46] predict that the R/S ratio of
the radicals (Figure ) leading to the formation of the R and S forms of cdG is ca. 2, and the corresponding R/S ratio of the diamagnetic product cdG
is ca. 0.3. These results predict the trend observed
in Table S2 and suggest that the R/S ratio of the radicals is maintained
in the hydrated DNA in forming the diamagnetic cdG.Formation of pyrimidine-derived lesions, ThyGly and 5-OH-Cyt: the hydration (OH– addition, i.e., H2O addition followed by deprotonation) of pyrimidine
cation radicals or their deprotonated forms, i.e., T•+/T(−H)• and C•+/C(−H)•, gives rise to 5-OH-adduct
radicals,[47] the oxidation of which results
in the formation of ThyGly and CytGly, respectively, as shown in Figure .[4,8,48] The dehydration of CytGly leads
to 5-OH-Cyt.[4,8,48] Extensive
analyses of ESR spectra of both γ-irradiated and ion-beam-irradiated
hydrated DNA in the literature and in our results in Figure do not indicate the existence
of any observable line components due to any trapped pyrimidine cation
radicals at 77 K.[2−4,13,38−40,42] In fact, there is compelling
evidence that any pyrimidine cation radicals that are initially formed
in irradiated DNA quickly undergo hole transfer to guanine to form
G•+.[2−4,13,38−40,42] This indicates that
the initial step shown in Figure , the addition of water to the pyrimidine cation radical,
occurs on a relatively fast time scale, before completion of the hole
transfer away from the cation radical can occur (ca. 10 ps).[41] Water residents in the major
and minor grooves of the DNA, with a residence time of ca. 1 ns,[49] are likely candidates for this
initial step. The identification of ThyGly and 5-OH-Cyt attests to
the formation of T•+ and C•+ in
Ne-22 beam-irradiated hydrated DNA (Figure ). The fact that the yields of these products
in Ne-22 beam-irradiated hydrated DNA are much lower than those of
Gua-derived lesions (Table S3) may point
to the fast hole transfer from T•+ and C•+ to Gua.[2−4,13,38−40,42]
Figure 12
Formation of ThyGly
from the thymine cation radical, T•+, and formation
of 5-OH-Cyt from the cytosine cation radical, C•+.
Formation of ThyGly
from the thymine cation radical, T•+, and formation
of 5-OH-Cyt from the cytosine cation radical, C•+.Formation of pyrimidine-derived
lesions 5,6-diHThy and
5,6-diHCyt: the mechanisms of the formation of 5,6-diHThy
and 5,6-diHCyt are shown in Figure . These products originate with the pyrimidineanion
radicals, T•– and C•–, which are formed by one-electron addition to Thy and Cyt, respectively,
and which are part of the trapped radical cohort observed at 77 K
(Figures , 4, and 5). It should be mentioned
that 5,6-diHThy and 5,6-diHCyt have been identified previously in
γ-irradiated hydrated DNA.[50] They
were identified in ion-beam-irradiated DNA at 77 K for the first time
in this work. The yields of 5,6-diHCyt are 6–9 times those
of 5,6-diHThy in the irradiated samples. Analysis of the percentages
of C(N3)H•/C•– and T•– in Ne-22-irradiated hydrated DNA, at 77 K,
indicated that the yields of C(N3)H•/C•–were higher than T•– yields, consistent
with the finding of higher yields of 5,6-diHCyt relative to 5,6-diHThy.
Figure 13
Formation
of 5,6-diHThy from the thymine anion radical, T•–, and formation of 5,6-diHCyt from the cytosine anion radical, C•–.
Formation
of 5,6-diHThy from the thymine anion radical, T•–, and formation of 5,6-diHCyt from the cytosine anion radical, C•–.Spatial positioning
of 8,5′-cyclopurine-2′-deoxynucleosides
and DNA-base lesions in the ion-beam track: based on the
ESR spectroscopy results, it is possible to suggest the spatial positioning,
in the ion track, of the products discussed in this work. R-cdA, S-cdA, R-cdG, and S-cdG are all thought to originate from C5′• (Figure ), which
is largely formed in the ion-beam core, which indicates that the cyclized
products are largely located in the core. These helix-distorting tandem
lesions are repaired by nucleotide excision repair and, if not repaired,
can lead to adverse biological effects such as reducing transcription,
blocking replication. They are also highly mutagenic, leading to G
→ A and A → G transitions and G → T and A →
T transversions.[10,34,51] The formation of C5′• radicals in the small
volume of the ion-beam core is likely to lead to the formation of
damage clusters and an increased difficulty in repair of the resulting
8,5′-cyclopurine-2′-deoxynucleosides, especially in
clustered damage sites, which, in turn, suggests an increase in the
cytotoxicity of these lesions in ion-beam-irradiated DNA, relative
to low-LET radiation. Furthermore, owing to the large amount of energy
deposited in the low volume core, clustered damage along the track
core is an expected result.[52] Unlike the
8,5′-cyclopurine-2′-deoxynucleosides, the DNA-base lesions
originate from DNA-base radicals, which are formed almost entirely
in the beam penumbra. Through both intra- and intertrack interactions,
these products may also contribute to the formation of damage clusters.
It is often conjectured that the dose in the penumbra decreases as
1/r2 from the center of the track, thus
significant amounts of energy are deposited in the penumbra close
to the core. DNA-base lesions formed near or in the core can, in a
single track, also contribute to damage cluster formation. The DNA-base
lesions identified in Ne-22 beam-irradiated DNA possess highly mutagenic
and cytotoxic effects.[53−55] All these DNA-base damage products may contribute
to the mutagenic and cytotoxic effects of high-LET ion-beam irradiations in vivo.[56]In summary,
this work is the first to use the combination of ESR
spectroscopy, LC–MS/MS and GC–MS/MS, and to report the
formation of DNA products that had not been reported previously in
DNA ion-beam-irradiated at 77 K. Our results show that both DNA radicals
and DNA-base damage products formed via both oxidative
and reductive pathways (e.g., Figure ) increase along the track until just before
the Bragg peak is reached; in addition, the DNA radical and product
yields are reduced at the Bragg Peak. This work thus enables a better
understanding of the mechanisms of radiation damage to DNA along the
ion-beam track in terms of the formation of DNA radicals, the stable
products that are formed from the radicals, and the location of products
in the ion track.
Experimental Section
The experimental
part is divided in sections, viz., (a) the materials
used, (b) hydrated DNA sample preparation,[14−17,19−21] (c) Ne-22 ion-beam and γ-irradiation (Figures S1 and S2, eqs S1 and S2),[20−24] (d) electron spin resonance (ESR) spectroscopy and computer analyses,[14−17,19−21] and (e) measurements
of DNA lesions.[25−37] All these are described in the Supporting Information.