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From the Department of Pathology,*
Johns Hopkins
Hospital, Baltimore, Maryland; the Department of
Pathology,
University of Maryland, Baltimore,
Maryland; Department of Laboratory Medicine and
Pathology,
Mayo Clinic, Rochester, Minnesota;
and the Department of Medicine,§
University of
California San Diego, La Jolla, California
| Abstract |
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| Introduction |
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| Materials and Methods |
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Immunohistochemistry
For immunohistochemical studies, paraffin-embedded specimens were sectioned at 4 µm, deparaffinized, and treated for antigen enhancement by either limited protein digestion or steaming (20 minutes at 80°C). Slides were then incubated at room temperature with antibodies to EGFR (monoclonal, 1:15; Zymed, South San Francisco, CA) or p53 (monoclonal, 1:250; Dako Co., Carpenteria, CA). Antibody was detected using the avidin-biotin complex method and diaminobenzidine as the chromogen. p53 staining of nuclei was graded in the region of greatest staining for each tumor as 3+ (>50% of nuclei), 2+ (>20% and <50%), 1+ (>0 and <20%), or absent. Intensity of cytoplasmic and cell membrane immunoreactivity for EGFR was graded as absent, mild, moderate, or strong.
DNA Isolation
For each paraffin-embedded block containing tumor, corresponding H&E slides were reviewed to ensure that DNA was isolated from tissue containing at least 90% tumor. Ten unstained histological sections containing neoplastic tissue, each 10 µm thick, were cut from paraffin blocks, deparaffinized in xylene, octane, or Histoclear, and scraped into microcentrifuge tubes containing 300 µl of a mixture consisting of 3 mmol/L Tris (pH 7.5), 0.2 mmol/L EDTA, 1 mg/ml proteinase K, 0.5% Tween 20, and 0.05% sodium dodecyl sulfate (SDS). Samples were incubated at 58°C for 5 hours, and fresh proteinase K/Tween 20/SDS was added for a minimum of 12 hours. Following protein digestion, samples were incubated at 95°C for 10 minutes. Samples were assessed for purity and DNA concentration spectrophotometrically at 260 and 280 nm.
PCR/Sequencing of Exons 58 of p53
Purified genomic DNA (100 ng) was PCR amplified in a 50-µl reaction containing 50 mmol/L KCl, 10 mmol/L Tris (pH 8.3), 1.5 mmol/L MgCl2, 1.0 µl 10 mmol/L dNTPs (2.5 mmol/L each dATP, dCTP, dGTP, and dTTP), 1.0 U Taq polymerase (Sigma, St. Louis, MO), and 0.4 µmol/L forward and reverse primers. Primers were designed to flank each exon and include the intron-exon junctions. One of the primers in each pair was 5'-biotinylated to allow for purification of single-stranded template for sequencing using a streptavidin-coated magnetic bead protocol.17 DNA was denatured at 94°C for 10 minutes. Thermocycler conditions were set for 30 cycles at 94°C for 30 seconds each, an empirically determined, optimal annealing temperature for each primer pair for 30 seconds and at 72°C for 30 seconds. A final extension step was 72°C for 7 minutes. The annealing temperatures and primer pairs for each exon were as follows: exon 5, 58°C for primer set Sarker 5U + Koga 5L-Bio, or 62°C for primer set 5U-Bio + 5L; exon 6, 66°C for Ohgaki 6U + 6L-Bio or 64°C for Ohgaki 6U-Bio + Sakar 6L; exon 7, 66°C for Vogel 7U + Sakar 7L-Bio or 62°C for 7U + 7L; and exon 8, 60°C for both 8U + 8L-Bio or 8U-Bio + Sakar 8L.18-21 Sequencing was performed using Sequenase v. 2.0 and dideoxy-chain termination methods incorporating 35S-dATP, as previously described.17 Internal primers were used for sequencing reactions and were annealed at 60°C. Labeling mix (dGTP) was diluted 1:10 and buffer supplemented with manganese was used in all reaction mixes. Sequencing was duplicated in the forward direction and confirmed in the reverse direction for each exon.
PCR/Sequencing of PTEN
One microliter of the DNA isolates were amplified in 50-µl
reactions containing the following: 20 pmol/L forward and reverse
primers (see Table 1
for primer sequences and annealing temperatures),
200 µmol/L each dNTP, 1.5 mmol/L MgCl2, 50
mmol/L KCl, 10 mmol/L Tris-HCl (pH 8.3), 0.001% gelatin, 5% DMSO, and
1.25 units Amplitaq Gold (Perkin-Elmer, Foster City, CA). Reactions
were carried out in a Perkin-Elmer 9600 thermocycler using the
following conditions: 95°C hold for 9 minutes, followed by 50 cycles
of 95°C for 30 seconds, 55°C or 48°C for 30 seconds, 72°C for 1
minute, followed by a 10-minute hold at 72°C. Forty microliters of
each PCR product were treated with 40 U exonuclease I and 8 U shrimp
alkaline phosphatase (PCR Product Pre-Sequencing kit, Amersham,
Arlington, IL) by incubating at 37°C for 15 minutes, then at
80°C for 15 minutes. Approximately 100 ng of the treated PCR products
were then sequenced using 2 pmol/L of forward or reverse primer and
Thermosequenase kit (Amersham). Cycle sequencing conditions were 95°C
for 20 seconds, 58°C for 30 seconds, and 72°C for 1 minute for 30
cycles. Reactions were quenched, denatured at 95°C for 2 minutes, and
electrophoresed through a 6% polyacrylamide gel with 15% formamide
and 7 mol/L urea. Gels were dried for 1 hour and exposed to film
overnight.
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A 190-bp segment of the K-ras gene was amplified using primers K-ras-F (5'-ACTGAATATAAACTTGTGGTAGTTGGAG) and K-ras-R (5'-TCATGAAAATGGTCAGAGAAACC). PCR reactions containing 1x Gene Amp PCR buffer (Perkin-Elmer), 400 µmol/L dNTPs, 0.8 µmol/L K-ras-F, 0.8 µmol/L K-ras-R, and 1.5 U Taq polymerase (Life Technologies, Gaithersburg, MD) were amplified using 32 cycles of 30 seconds at 94°C, 30 seconds at 56°C, and 45 seconds at 72°C, followed by a 1-minute extension at 72°C. The resulting PCR products were evaluated on 2% ethidium bromide-stained agarose gels. Confirmed PCR products were purified for direct sequencing by treatment with 10.0 U Exonuclease I and 2.0 U Shrimp Alkaline Phosphatase (Amersham) at 37°C for 15 minutes, followed by a brief incubation at 80°C for 15 minutes. The purified PCR products were directly sequenced using the ThermoSequenase radiolabeled terminator cycle sequencing kit (Amersham) according to manufacturer's instructions. Products of the cycle sequencing reactions were resolved on 6% acrylamide-8 mol/L urea denaturing gels. Gels were fixed in a solution of 5% methanol and acetic acid, dried, and subjected to radiography.
Differential PCR of EGFR
PCR amplifications (Perkin-Elmer apparatus) were carried out in a final volume of 25 µl as previously described.22 Each reaction mixture contained 0.150.20 µg of template, 10 mmol/L Tris-Cl (pH 8.3), 50 mmol/L KCI, 1.5 mmol/L MgCl2, 0.001% gelatin (w/v), 200 µmol/L dNTPs, 0.05 µmol/L oligonucleotide primers for reference and target gene, and 0.0625 U AmpliTaq DNA polymerase (Perkin-Elmer, Norwalk, CT). PCR cycles were carried out as follows: 92°C for 2 minutes; cycles 15 at 97°C for 30 seconds, 53°C for 1 minute, and 72°C for 1 minute; cycles 625 or 630 at 95°C for 1 minute, 53°C for 1 minute, and 72°C for 1 minute; and a final extension after the last cycle at 72°C for 10 minutes. After PCR, the entire reaction product was electrophoresed on a 2% agarose gel and stained with ethidium bromide. Fragments from X174-HaeIII digested DNA (Promega, Madison, WI) were used as markers to document amplification of appropriately sized fragments. Gels were photographed using the Gel-doc 1000 photodocumentation system (Bio-Rad, Philadelphia, PA) and resulting images were quantitatively analyzed using Molecular Analyst software. This method of differential PCR used with appropriate controls has demonstrated 100% concordance with slot blot analysis for EGFR amplification in a series of astrocytic neoplasms.22
Primers for EGFR used in this study (sense, AGCCATGCCCGCATTAGCTC; antisense, AAAGGAATGCAACTTCCCAA) amplify a 110-bp genomic fragment corresponding to bases 39014010 of the cDNA sequence. The reference primers for the detection of increased EGFR gene dosage amplify a 70-bp genomic fragment from the ß-globin gene (sense, TGACTCCTGAGGAGAAGTCTGC [cDNA bases 164186]; antisense, TCACCACCAACTTCATCACGT [cDNA bases 212233]), and a 79-bp fragment of the cystic fibrosis gene (sense, GGCACCATTAAAGAAATATCATCTT [cDNA bases 16301655]; antisense, GTTGGCATGCTTTGATGACGCTTC [cDNA bases 16851708]), respectively.
Quantitive PCR Analysis of p16 and MTAP
Quantitative PCR assays were performed using primers from p16 exon 1 and MTAP exon 8 with an MTAP pseudogene as reference, as described previously.23 MTAP is located approximately 100 kb telomeric to p16 on chromosome 9p and encodes methylthioadenosine phosphorylase. Amplification was carried out in a total volume of 50 µl containing 100 ng of genomic DNA, 1x PCR buffer (10 mmol/L Tris-HCl (pH 8.3), 50 mmol/L KCl, 1.5 mmol/L MgCl2, 0.01% gelatin), 200 µmol/L of each dNTP including 80 µmol/L digoxigenin-labeled dUTP (Boehringer Mannheim, Indianapolis, IN), 150 ng each of sense and anti-sense primers, and 2.5 units of Taq DNA polymerase (AMITaq Gold; Perkin-Elmer, Foster City, CA). Following incubation at 94°C for 5 minutes, 26 cycles were performed consisting of 94°C denaturation (1 minute), 64°C annealing (1 minute), and 72°C extension (1 minute).
Aliquots of the PCR products were resolved on 2% agarose gels (Gibco,
Grand Island, NY) for qualitative purposes. The remaining PCR products
were subjected to purification through QiaQuick Spin Columns (Qiagen
Inc., Chatsworth, CA) to remove unincorporated primers. After binding
the PCR products to a 96-well enzyme-linked immunosorbent assay plate
coated with streptavidin, the incorporated digoxigenin-dUTP in the PCR
products was detected with enzyme-linked immunosorbent assay. To
construct calibration curves, PCR assays were carried out in parallel
using standard DNA templates that contained mixtures of p16-negative,
MTAP-negative Jurkat leukemic cells and normal human diploid fibroblast
DNA (WI-38) in varying proportions. The optical density reading of each
sample was used to determine the status of p16 exon 1 or MTAP exon 8 by
calculating the relative gene dosage (Dp16 and
DMTAP) as follows:
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represent the tumor optical density readings
of p16 exon 1, MTAP exon 8, and the MTAP pseudogene, respectively, and
Np16, Nmtap8, and
N
represent the normal fibroblast optical
density readings of p16 exon 1, MTAP exon 8, and the MTAP pseudogene,
respectively.23
Dp16 and
DMTAP values were plotted as standard curves for
determination of relative gene doses in primary tumor samples.
Homozygous deletion of p16 or MTAP genes was defined as a relative gene
dosage less than 30%. | Results |
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Complete genomic DNA sequence analysis of exons 58 of the p53 gene revealed a single point mutation in one of nine tumors sequenced. This tumor was a glioblastoma multiforme that occurred in the suprasellar region of an 18-year-old female who had been radiated 11 years earlier following incomplete resection of a craniopharyngioma. No associated low grade astrocytoma was noted histologically. The point mutation was a G-to-A transition within codon 285 (exon 8) that results in an amino acid substitution from glutamic acid to lysine. Sequencing in the reverse direction confirmed the mutation. Each of the other eight tumors contained wild-type p53 sequence within exons 58.
Three of nine tumors had strong (3+) diffuse nuclear immunoreactivity for p53 protein, while two had weak (1+) diffuse nuclear staining. Four tumors had no immunoreactivity for p53. The point mutation in the p53 gene was present in a tumor that had distinct but weak (1+) nuclear immunoreactivity for p53 protein.
EGFR Amplification
Multiplex PCR of eight tumor specimens revealed preferential
amplification of the EGFR fragment compared to both ß-globin and
cystic fibrosis reference in two tumors, T309 and T312 (Figure 2)
. A breast tumor cell line (MDA-468;
ATCC), a glioblastoma cell line (SK-MG3), and an epidermoid carcinoma
cell line (A-431; ATCC), each containing known EGFR amplification,
showed significantly increased bands of amplified EGFR gene compared to
references and served as positive controls.22
In six of
the astrocytic tumors, no evidence of increased EGFR band intensity was
seen over the reference level.
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Seven of the nine radiation-induced astrocytomas provided DNA
suitable for deletion analyses of both the p16 and MTAP genes. Relative
gene dosages (Dp16 or
DMTAP) of p16 and MTAP for each tumor are listed
in Table 3
. Two of the tumors (T308 and T311) had homozygous deletions
that included both exon 1 of p16 and exon 8 of MTAP. These genes are
located approximately 100 kb apart on chromosome 9p21, suggesting that
these two tumors had large deletions of this region of the chromosome.
One tumor (T307) had a deletion that encompassed the MTAP gene but not
p16.
PTEN
All nine tumors contained wild-type sequence of exons 19 of the PTEN gene. No mutations or deletions were noted.
K-ras Proto-oncogene
Wild-type sequence in the region of K-ras proto-oncogene containing codons 12 and 13 was present in all eight tumors tested. No activating point mutations were identified.
| Discussion |
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With a few exceptions, the spectrum of genetic alterations that we found in radiation-induced gliomas were similar to those described in spontaneous high grade astrocytic tumors (ie, glioblastoma multiforme) of the primary or de novo type.24,25 Specifically, both p16 deletions and EGFR amplifications were more common in the de novo pathway of GBM formation, in which tumors arise without a well-defined low-grade precursor lesion.26 We detected EGFR amplifications in two of eight tumors and p16 deletions in two of seven tumors. Although the number of neoplasms analyzed was small, we found a slightly lower percentage of EGFR and p16 alterations in radiation-induced tumors than have been reported for de novo GBMs. In larger series of astrocytic neoplasms, EGFR amplifications have been noted in approximately 10% of anaplastic astrocytomas and 40% of glioblastomas,10,11 whereas p16 homozygous deletions have been detected in 4060% of malignant gliomas.14,23 Homozygous p16 deletions are more common in GBMs with EGFR amplification than in those without EGFR amplification.27 One study found that 71% of GBMs with EGFR amplification also had homozygous p16 deletions.27 Within the present series, p16 deletions and EGFR amplifications did not occur in the same neoplasms. This finding may suggest some molecular genetic differences between radiation-induced and spontaneous astrocytomas, but analysis of a larger series will be required to address this more completely.
In the two tumors with p16 deletions, the MTAP gene, located 100 kb telomeric to p16 and encoding methylthioadenosine phosphorylase, was codeleted, indicating a sizable deletion involving chromosome 9p. In one tumor, the MTAP gene was deleted but the p16 gene was not. This genotype has been noted in other spontaneous astrocytomas and may suggest that another tumor suppressor gene is present on chromosome 9 telomeric to p16.23
Only one of the nine tumors had a p53 mutation detected by direct sequence analysis. p53 mutations have been noted in both progression and primary lesions, but occur with higher frequency in the former. They are thought to represent an early genetic alteration in the progression pathway of GBMs and are therefore common in low grade astrocytomas as well as in high grade tumors that have evolved from a lower grade.16,25 The tumor in the present series that contained the p53 point mutation was a GBM at clinical presentation, with no histological evidence of an associated lower grade precursor lesion. In keeping with previous studies that have concluded that p53 mutations and EGFR amplification are statistically exclusive events, we did not detect any p53 mutations in tumors that had EGFR amplification.
We did not detect any mutations of the PTEN tumor suppressor gene in the nine tumors that were sequenced. Mutations in PTEN are relatively common in infiltrating astrocytic neoplasms, and have been described in both the de novo and progression pathway of GBMs. They are more common in de novo GBMs and occur in approximately 2530% of these high grade tumors.12,28,29 Although the absence of PTEN mutations is these radiation-induced tumors is somewhat surprising, the number of cases analyzed in our series was small.
Unlike some experimental, radiation-induced malignancies, the radiation-induced astrocytic tumors in this series did not harbor activating K-ras mutations in codons 12 or 13. These mutations are a relatively common tumorigenic event in spontaneous neoplasms of the colon, pancreas, lung, and other organs, but are not common in primary brain tumors.30 The only report of a K-ras mutation in a primary brain tumor is that of an activating point mutation in codon 12 in a pediatric primitive neuroectodermal tumor (PNET) that occurred 9 years after radiation therapy for acute lymphoblastic leukemia involving the CNS.8 Two other radiation-induced PNETs in the same report did not contain K-ras mutations. Our data do not support a role for activating point mutations in K-ras in the development of radiation-induced astrocytic tumors.
The astrocytic tumors that arose following radiation therapy were all high grade at clinical presentation, and contained primarily molecular genetic alterations similar to those reported for the de novo pathway of GBMs. In this regard, radiation-induced tumors are distinct from infiltrating astrocytic neoplasms that arise spontaneously. In general, de novo GBMs occur in patients in their sixth or seventh decades, whereas GBMs that progress from low-grade precursors occur in patients in their third and fourth decades.31,32 These radiation-induced gliomas occurred in patients of all ages, but particularly in patients less than 30 years old (66%) who had received radiation therapy as children. Although the low number of patients in this study precludes a statistical analysis, a recent review of the literature concluded that radiation-induced gliomas are nearly all high grade at clinical presentation and that they occur in a younger patient population than would be expected for de novo high grade gliomas.3 In addition, almost all radiation-induced gliomas are astrocytic in their differentiation (ie, not oligodendroglial or ependymal).
Another unique feature of these tumors is their anatomical distribution. Although radiation-induced astrocytic tumors occur most often in the temporal and frontal lobes, they also occur at sites that are not typical for spontaneous infiltrating gliomas. For example, spontaneous high grade astrocytomas of the suprasellar region and cerebellum are rare, yet they have been noted in our series and in other reports of radiation-induced gliomas.3 It has also been suggested that radiation-induced gliomas may be more likely to be multifocal.33 This feature is unlikely to be specific, because multifocal spontaneous high grade gliomas have been well-documented, and it is unclear if multifocal lesions are more frequent following radiation therapy. All of the lesions in the present series were solitary.
In this set of astrocytomas, we did not find any specific or unique mutations, such as base pair deletions in tumor suppressor genes, that might help distinguish radiation-induced tumors from spontaneous ones. Base pair deletions result from the misrepair of double-stranded DNA breaks, a type of DNA damage that occurs following high-dose ionizing radiation.34,35 Other types of DNA injury do not result in double-strand breaks, and single-strand breaks are repaired without the introduction of base pair deletions. Because of this, base pair deletions could potentially represent a marker for DNA damage caused by radiation. One such homozygous 3-bp deletion in exon 7 of the p53 gene was recently described in a radiation-induced glioblastoma.7 In our DNA sequence analyses of nine radiation-induced astrocytic tumors, which included exons 19 of the PTEN gene, exons 58 of the p53 gene, and a short segment of the K-ras gene, we found no evidence of base pair deletions that might be specific for radiation-associated DNA damage. On the basis of our results, it appears that base pair deletions are not a frequent or consistent finding in radiation-induced astrocytic tumors, at least in the genes that we have analyzed.
Only a small percentage of patients who receive CNS radiation therapy will develop subsequent gliomas. One study suggests that the cumulative risk for developing a second brain tumor after radiation therapy for pituitary adenoma is 1.9% over the course of 20 years, and of these only a subset will be gliomas.5 Outside of the well-known but rare genetic syndromes of radiation sensitivity (eg, ataxia telangiectasia, hereditary retinoblastoma, xeroderma pigmentosa, and others), little is known regarding the susceptibility of individuals within the general population to radiation-induced tumorigenesis.36 In vitro studies of radiation-induced chromatid damage in peripheral blood lymphocytes have demonstrated that relative genetic instability may be a risk factor for the development of spontaneous malignancies, including gliomas.37 Similar studies may be helpful in assessing susceptibility to radiation-induced neoplasia.38
| Footnotes |
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Supported in part by National Institutes of Health grants CA 64928, CA 64976, and CA 55728.
D. Connolly's current address: Department of Pathology, University of Michigan, Ann Arbor, MI.
Accepted for publication February 3, 1999.
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radiation. Science 1984, 225:1159-1162
, and epidermal growth factor and their expression in human gliomas in vivo. Cancer Res 1991, 51:2164-2172This article has been cited by other articles:
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