| Nucleic Acids Research | Pages |
The orientation and dynamics of the C2[prime]-OH and hydration of RNA and DNA·RNA hybrids
Introduction
Materials And Methods
Results
Assignments of C2[prime]-OH
Exchange rate constants
Orientation of the C2[prime]-OH
Hydration
Acknowledgements
References
The orientation and dynamics of the C2[prime]-OH and hydration of RNA and DNA·RNA hybrids
ABSTRACT
INTRODUCTION
DNA·RNA hybrids are important biological intermediates involved in transcription, DNA synthesis and reverse transcription (1). They are also formed as translationally inactive products of antisense therapy, and are substrates for the enzyme RNase H. To understand the principles that determine the stability of hybrid duplexes, and thereby improve the design of antisense oligonucleotides, a knowledge of their conformational properties in solution is essential. The conformations of DNA·RNA hybrids are quite different from those of DNA and RNA duplexes at the nucleotide level. They also differ significantly in their global conformations, though they resemble the A-form of RNA more than the B-form of DNA (2-8). Furthermore, the thermodynamic stability of DNA·RNA hybrids, while always lower than that of the homologous RNA duplex, can be either more or less stable than the DNA duplex, depending on the base-composition of the strands (8-10). The thermodynamic stability and solution conformation of nucleic acids also depend on their interaction with ions and water (11-13). Nucleic acids are highly hydrated in aqueous solution (13,14). However, dehydration of DNA causes the conversion from the B-form into the A-form. In contrast, RNA in solution is invariably found in the A-conformation, regardless of the water activity (13). A large contribution to the stability of DNA and RNA duplexes is the favourable enthalpy associated with base-stacking (15), which is greater in the A-form than in the B-form. Hence, there is a strong inter-dependence of the chemical structure, conformation and interactions with water.
The hydroxyl group on the C2[prime] of ribose is likely to have a great influence on the hydration, conformation and thermodynamic stability of RNA compared with DNA. These groups, which line the shallow minor groove of RNA, are expected to be involved in extensive hydrogen bonding interactions with water (16-19). In contrast, the minor groove of A-DNA would be relatively hydrophobic, and therefore potentially destabilised by water. The interplay between conformation and hydration has also been shown in DNA, where the spine of hydration in the narrow minor groove of dAn·dTn sequences is significantly different from that observed in the minor grooves of mixed sequence DNA duplexes (13,14,20-24). However, much less information is available on the hydration of DNA·RNA hybrids. Recently, the hydroxyl protons were observed in a DNA·RNA hybrid by NMR spectroscopy (25). We report here the identification of C2[prime]-OH groups in both RNA and DNA·RNA hybrid duplexes that we have been studying (8,26) and show that there are distinct differences in the behaviour of these protons and how they interact with water for the RNA and DNA·RNA hybrid duplexes.
MATERIALS AND METHODS
DNA and RNA oligonucleotides were synthesised and purified as previously described (8). We have examined the following duplex sequences:
d(GAAGAGAAGC)·d(GCTTCTCTTC) (dR10·dY10), d(GAAGAGAAGC)·r(GCUUCUCUUC) (dR10·rY10), d(GAAGAGAAGC)·r(GCTTCTCTTC) [dR10·rY(T)10], r(GAAGAGAAGC)·-r(GCUUCUCUUC) (rR10·rY10), r(GAAGAGAAGC)·d(GCUUCUCUUC) [rR10·dY(U)10] and r(GAAGAGAAGC)·d(Gp-CpUpUpCpUpCpUpUC) (rR10·dpY10). In dR10·rY(T)10, each RNA uracil base is methylated at the 5-position, in rR10·dY(U)10, each deoxyribose thymidine base is demethylated at the 5-position, and in rR10·dpY10, pN is a pyrimidine base modified at the 5-position with the propyne group (-C[equiv]C-CH3).
1H NMR spectra were recorded at 500 or 600 MHz on a Varian Unity Plus or Unity spectrometer, respectively. Experiments were performed at 5°C in 90% H2O:10% D2O using the Watergate method (27) for suppressing the intense solvent peak. Spectra were recorded at a concentration of ~0.5 mM in 5 mm NMR tubes, or at ~0.15 mM in 8 mm tubes in the case of rR10·rY10 to eliminate aggregation of the solutes at low temperature. Phase-sensitive (28) NOESY and ROESY spectra were typically recorded with mixing times of 50 and 25 ms, respectively, as previously described (19,24). TOCSY spectra were recorded using MLEV-17 (29) with a mixing time of 40-46 ms and a spin-lock strength of 8 kHz. Assignments of the C2[prime]-OH resonances of the RNA strands were achieved where possible using the observed NOEs between these protons and assigned H1[prime] and H2[prime] as previously described (19), and also the scalar coupling to the H2[prime] using TOCSY (29). The assignments of the modified duplexes dR10·rY(T)10, rR10·dY(U)10 and rR10·dpY10 were made using standard techniques as previously described (8) and will be published elsewhere.
Estimates of the exchange rate constant of the C2[prime]-OH with water were made in several ways. First, the degree of saturation was measured by comparing relaxed 1D spectra with and without 3s presaturation of the water resonance. This gives the steady-state magnetisation transfer from water to the C2[prime]-OH, which is determined by the dissociation rate constant and the intrinsic spin-lattice relaxation rate constant of the OH, according to equation 1:
![]() |
1 |
where M is the steady state magnetisation, M0 is the magnetisation in the absence of presaturation, k is the dissociation rate constant and [rho] is the intrinsic spin-lattice relaxation rate constant. To estimate [rho], we calculated a range based on the internuclear distances between the OH and its neighbours using models of the structures (26), according to:
![]() |
2 |
where r is the internuclear distance, J(n[omega]) is the spectral density function and [omega] is the Larmor frequency.
The correlation time was calculated for H2O from the values measured in D2O at 30°C (8) and using the fact that the viscosity of water is ~24% lower than that of D2O, and tabulated values of the viscosity of water at different temperatures (30).
A second estimate of k was obtained from measurements of the linewidth of the OH peaks from OH-H1[prime] cross-peaks in NOESY spectra. The linewidth depends on numerous factors as follows:
![]() |
3 |
where L0 is the intrinsic linewidth, L([Delta]B) is the contribution from magnetic field heterogeneity and limited digital resolution and [Sigma]J is the contribution from unresolved scalar coupling (e.g. to H2[prime]). The intrinsic linewidth was estimated in a manner similar to that described for the spin-lattice relaxation rate constant, L([Delta]B) was estimated as the measured linewidth of DSS in the same spectrum, and [Sigma]J was assumed to be at least 4 Hz on the basis of the observed TOCSY cross-peaks. This calculation should provide an upper limit to the rate constant for exchange with water, as other contributions are not considered, such as fast intermediate exchange among different rotamer states of the hydroxyl group.
A third estimate was obtained by integrating the cross-peaks between OH and water in the NOESY spectra, and normalising them to the sum of the diagonal and cross-peaks volumes. For short mixing times, the exchange cross-peaks depend on mixing time, tm, approximately as:
![]() |
4 |
A fourth estimate was obtained from 1D EXSY experiments (31).
Because of the necessary approximations involved in these calculations, the absolute values of k are unlikely to be very accurate. However, consistency between the methods indicates that the exchange rate constants are determined within reasonable limits.
Simulations of magnetisation transfer between water, OH and H1[prime] were made under a variety of assumptions, namely the exchange rate constant, the spin-lattice relaxation rate constants, and the cross-relaxation rate constant between OH and H1[prime] (i.e. the effects of geometry). For a three-spin system of this kind, analytical expressions can be obtained for the time course of magnetisation transfer, and which then provide a useful guide to the interpretation of the observed results. Additional calculations were made from complete structures using the program NUCFIT (32).
RESULTS
Assignments of C2[prime]-OH
Figure
Figure 1. 1D 1H NMR spectra of rR10·rY10, rR10·dpY10, rR10·dY(U)10, dR10·rY(T)10, dR10·rY10 and dR10·dY10. NMR spectra were recorded at 5°C in H2O as described in Materials and Methods.
Exchange rate constants
The exchange cross peaks between the C2[prime]-OH and water in the ROESY spectra demonstrate that the exchange process is relatively slow on the chemical shift time scale. Furthermore, it must be sufficiently slow so as not to bleach out ROEs and NOEs between the C2[prime]-OH and H1[prime] or H2[prime]. Thus, the exchange is much slower than is found for simple sugars. The exchange rate constant for different C2[prime]-OH groups in the various duplexes was estimated as described in the methods, and we find a range from ~10 to 50/s, with the largest rate constants found for the RNA duplex, and the lowest for the rR10·dpY10 duplex (Table 1). These values are an order of magnitude larger than found for the UUCG tetraloop (33), but comparable with the values estimated at 5°C for a DNA·RNA hybrid (25). The exchange rate constants are considerably lower than for a free nucleotide; the C2[prime]-OH was not detected in rUMP under similar solution conditions (A.N.Lane and J.I.Gyi, unpublished results). Furthermore, the 3[prime]-terminal nucleotide of dR10·rY(T)10 showed no hydroxyl cross-peaks, indicating much faster exchange. This C2[prime]-OH cannot hydrogen bond to a 3[prime] residue and must be completely exposed to solvent. Hence, because the minor groove is exposed to solvent, it is probable that the observed relatively low exchange rate constants are due to H-bonding between the C2[prime]-OH and unknown acceptor groups. The likely presence of hydrogen bonding interactions would be expected to result in restricted rotation about the C2[prime]-O2[prime] bond, and to a preference for one of the three rotamer states (see below). The linewidths, measured from cross-sections in the NOESY spectra, reflect the relative exchange rate constants (compare with equation 3). This provides only an upper estimate of k because of unknown contributions from unresolved J-coupling between the C2[prime]-OH and C2[prime]H, which can vary from ~0 to 12 Hz, and the intrinsic linewidth, which we estimate to be of the order of 2-3 Hz. An additional contribution to the linewidth could also arise from exchange among rotamers on the chemical shift timescale. Because the saturation transfer experiments show that most of the linewidth arises from exchange with water (Table 1), this contribution should be small in comparison with the others, but could contribute relatively more to the RNA (broad hydroxyl protons) than to the hybrids. We note also that the apparent linewidths or exchange rate constants (Table 1) do not correlate with thermodynamic stability (8; G.L.Conn, unpublished data).
Figure 2. TOCSY and ROESY spectra of the RNA and DNA·RNA hybrids: assignment of C2[prime]-OH. The spectra were recorded at 5°C and 600 MHz with mixing times of 46 (TOCSY) and 25 ms (ROESY). Positive peaks are in blue, negative peaks are in red. Assignments of the C2[prime]-OH resonances of the RNA strands were achieved where possible using the observed NOEs between these protons and assigned H1[prime] and H2[prime], and also the scalar coupling to the H2[prime] using TOCSY. In each case, the top panel shows the ROESY spectrum, and the bottom panel the analogous region of the TOCSY spectrum. From left to right: rR10·rY10 [ROESY, [tau]m = 25 ms, spectral width (F1/F2) = 10 000 Hz, acquisition times t1 = 0.04 s, t2 = 0.5 s; TOCSY, [tau]m = 46 ms, spectral width (F1/F2) = 10 000 Hz, acquisition times t1 = 0.04 s, t2 = 0.5 s], dR10·rY(T)10 [ROESY, [tau]m = 25 ms, spectral width (F1/F2) = 13 000 Hz, acquisition times t1 = 0.02 s, t2 = 0.5 s; TOCSY, [tau]m = 46 ms, spectral width (F1,F2) = 12 000 Hz, acquisition times t1 = 0.03 s, t2 = 0.5 s], rR10·dpY10 [ROESY, [tau]m = 25 ms, spectral width (F1,F2) = 13 000 Hz, acquisition times t1 = 0.02s, t2 = 0.5 s; TOCSY, [tau]m = 46 ms, spectral width (F1,F2) = 13 000 Hz, acquisition times t1 = 0.02 s, t2 = 0.5 s].
Table 1.
| Duplex | [delta](C2[prime]-OH)/p.p.m. | assignment | L/Hz | kx(L)/s | kx(RY)/s |
| rR10·rY10 | 6.77 | nd | |||
| 6.82 | C15/17 | 26 | <66 | 24 ± 5 | |
| 6.85 | U14 | 26 | <66 | 24 ± 5 | |
| 6.96 | G4,6 | 26 | <66 | 24 ± 5 | |
| dR10·rY10 | 6.86 | U19 | 9.3 | 14 | 12 |
| 6.68 | U14 | 10 | 16 | 12 | |
| adR10·rY(T)10 | 6.64 | U14 | 19 | 44 | 20 |
| 6.78 | U19 | 23 | 56 | 20 | |
| 6.68 | C17/U18 | 15 | 31 | 21 | |
| 6.56,6.62 | nd | 18 | 41 | nd | |
| rR10·dY(U)10 | 6.71 | A2,A3,A7 | 16 | 35 | nd |
| 6.80 | A8 | 15 | 16 | nd | |
| 6.81-6.84 | G1,G4,G6 | 13 | 25 | 38 | |
| 6.88 | G9 | 14 | 28 | 38 | |
| brR10·dpY10 | 6.81 | A2,A5 | 12 | 22 | 24 |
| 6.70 | A3 | 8 | 9.5 | 19 | |
| 6.93 | G4 | 16 | 35 | nd | |
| 6.96 | G6 | 9 | 13 | nd | |
| 6.69 | A7 | 6 | 7 | 19 | |
| 6.74 | A8 | 15 | 35 | 20 |
Orientation of the C2[prime]-OH
Although the ROESY spectrum indicates that the C2[prime]-hydroxyl protons are in slow exchange with the solvent, in the DNA·RNA hybrids they show intense NOEs to both the C2[prime]-H and H1[prime]. This was confirmed by the observation of scalar cross-peaks in a TOCSY recorded with a mixing time of 40 ms, in which clear cross-peaks were obtained between the exchangeable protons in the 6.5-7 p.p.m. range, and the C2[prime]-H, but not H1[prime] (Fig.
Table 2.
| Cross-peak intensities | |||||
| Duplex | C2[prime]-OH-H2[prime] | C2[prime]-OH-H1[prime] | H1[prime]-H2O | AH2-H2O | H6/H8-H2O |
| rR10·rY10 | m/s | m | 0/w | w | w |
| rR10·dY(U)10 | s | m | 0/w | 0 | 0/w |
| rR10·dpY10 | s | s | w/m | m | m |
| dR10·rY(T)10 | s | s | w/m | m | m |
| dR10·rY10 | s | s | w | m | m |
| dR10·dY10 | - | - | 0/w | m | m |
The pattern of NOEs in the DNA duplex is quite different from that observed in the hybrid duplexes (Table 2). The DNA duplex has no C2[prime]-OH, so that NOEs involving these protons are not present. This is further supporting evidence that the NOEs observed in the RNA-containing duplexes involve the hydroxyl protons. In the RNA decamer, NOEs were observed between the C2[prime]-OH and the H2[prime] (and a strong exchange cross-peak with water) and between the C2[prime]-OH and the H1[prime]. The pattern of NOEs is different than previously observed in an RNA oligomer having a mixed sequence (19), and distinct thermodynamic and conformational properties (34).
Figure 3. Model adenosine nucleotide showing a superimposition of the three favoured rotamers of C2[prime]-OH. The torsion angle labelled [phis] refers to that formed between O2[prime]H and H2[prime]. The rotation is about the bond C[prime]-O2[prime].
Molecular models of the RNA duplexes and the DNA·RNA hybrids show that there are three stable rotamers for rotation about the C2[prime]-O2[prime] bond (Fig.
The presence of the C2[prime]-OH-H2[prime] TOCSY cross-peaks, and the strong NOE or ROE between C2[prime]-OH and H1[prime] for all of the DNA·RNA hybrids and the RNA duplex (Fig.
Hydration
In addition to the obvious chemical and conformational differences between DNA and RNA duplexes, the pattern of hydration of non-exchangeable protons is also different. We have therefore examined some aspects of hydration of these duplexes using NMR. Figure
Water-base proton NOEs and ROEs show that the major groove is accessible to solvent. The methyl groups of thymine, where present, showed positive NOEs, indicating a short (<0.3 ns) correlation time. This probably reflects the rapid reorientation of the methyl group. The methyl of the propyne group in rR10·dpY10 also showed positive NOEs and ROEs at the water frequency. Thus, the major groove in both the DNA·RNA hybrids and the DNA duplex is accessible to water. Figure
In both the DNA duplex and the DNA·RNA hybrids, significant negative NOEs and positive ROEs were found between water and the Ade H2 in the minor groove (Fig.
Figure 4. Cross-sections through NOESY and ROESY spectra. NOESY (NY) and ROESY (RY) spectra were recorded at 5°C, 600 MHz with mixing times of 50 and 25 ms respectively. The cross-sections are taken at the water frequency, along the F2 dimension. Cross peaks show interaction of solute protons with water via dipolar interactions or chemical exchange. Protons in red are in the major groove, those in blue are in the minor groove, and exchangeable protons, with the exception of C2[prime]OH, are shown in black. Water-H1[prime] NOEs are complicated by the exchange between the C2[prime]-OH and water. Because a strong ROE was observed between the C2[prime]-OH and the H1[prime] (Fig. Figure 5. Simulated ROE time courses in the absence and presence of exchange with solvent. Time courses were calculated analytically for a three-spin system comprising water, C2[prime]-OH and H1[prime] assuming exponential relaxation of the water resonance. The curves shown were calculated for different values of the exchange rate constant (k) and the cross-relaxation constant for C2[prime]-OH-H1[prime] ([sigma]). [rho]w (water), [rho]1[prime] (H1[prime]) and [rho]OH (C2[prime]-OH) were set to 1, 7 and 12/s based on calculations as described in Materials and Methods. The magnetisation has been normalised to that of the cytosine H5-H6 cross peak calculated for standard A-RNA. [cir], [sigma] = 0.4/s and k = 5/s; [bull], [sigma] = 2.4/s and k = 5/s; [squ], [sigma] = 0.4/s and k = 25/s; [squf], [sigma] = 2.4/s and k = 25/s; [diams], [sigma] = 0.4/s and k = 50/s; z, [sigma] = 2.4/s and k = 50/s. The DNA·RNA hybrids show interactions with water that have characteristics in common with both the DNA duplex and the RNA duplex. In the major groove, the accessibility to water in the hybrids is more similar to the DNA duplex than to the RNA duplex. The minor groove also shows evidence of relatively stable hydration around the Ade C2H, comparable with that in the DNA duplex. The C2[prime]-OH has a preferred orientation, and interacts directly with water. In the RNA duplex, access to water or its kinetic stability in the major groove is less than in the DNA duplex or the DNA·RNA hybrids. However, the C2[prime]-OH also has a preferred orientation (though not necessarily as stable as that in the hybrids), and interacts directly with the water.
ACKNOWLEDGEMENTS
This work was supported by the MRC and Oswel Research Products Ltd. GLC gratefully acknowledges a Royal Society of Edinburgh Caledonian Research Fellowship.
REFERENCES
This article has been cited by other articles:
This page is run by Oxford University Press, Great Clarendon Street, Oxford OX2 6DP, as part of the OUP Journals
Comments and feedback: www-admin{at}oup.co.uk
Last modification: 16 Jun 1998
Copyright©Oxford University Press, 1998.
![]()
CiteULike
Connotea
Del.icio.us What's this?
![]()
![]()

![]()
![]()
![]()
S. Nozinovic, B. Furtig, H. R. A. Jonker, C. Richter, and H. Schwalbe
High-resolution NMR structure of an RNA model system: the 14-mer cUUCGg tetraloop hairpin RNA
Nucleic Acids Res.,
November 11, 2009;
(2009)
gkp956v1.
[Abstract]
[Full Text]
[PDF]
![]()
![]()
![]()

![]()
![]()
![]()
J. I. Gyi, D. Gao, G. L. Conn, J. O. Trent, T. Brown, and A. N. Lane
The solution structure of a DNA{middle dot}RNA duplex containing 5-propynyl U and C; comparison with 5-Me modifications
Nucleic Acids Res.,
May 15, 2003;
31(10):
2683 - 2693.
[Abstract]
[Full Text]
[PDF]
![]()
![]()
![]()

![]()
![]()
![]()
L. R. Comolli, N. B. Ulyanov, A. M. Soto, L. A. Marky, T. L. James, and W. H. Gmeiner
NMR structure of the 3' stem-loop from human U4 snRNA
Nucleic Acids Res.,
October 15, 2002;
30(20):
4371 - 4379.
[Abstract]
[Full Text]
[PDF]
![]()
![]()
![]()

![]()
![]()
![]()
M. R. Valentine and J. Termini
Kinetics of formation of hypoxanthine containing base pairs by HIV-RT: RNA template effects on the base substitution frequencies
Nucleic Acids Res.,
March 1, 2001;
29(5):
1191 - 1199.
[Abstract]
[Full Text]
[PDF]
![]()
![]()
![]()

![]()
![]()
![]()
S.-T. Hsu, M.-T. Chou, and J.-W. Cheng
The solution structure of [d(CGC)r(aaa)d(TTTGCG)]2: hybrid junctions flanked by DNA duplexes
Nucleic Acids Res.,
March 15, 2000;
28(6):
1322 - 1331.
[Abstract]
[Full Text]
[PDF]
![]()
This Article ![]()
![]()
Abstract
![]()
Print PDF (908K)
![]()
Alert me when this article is cited
![]()
Alert me if a correction is posted
![]()
Services ![]()
![]()
Email this article to a friend
![]()
Similar articles in this journal
![]()
Similar articles in ISI Web of Science
![]()
Similar articles in PubMed
![]()
Alert me to new issues of the journal
![]()
Add to My Personal Archive
![]()
Download to citation manager
![]()
Search for citing articles in:
ISI Web of Science (26)
![]()
Request Permissions ![]()
Commercial Re-use Guidelines
for Open Access NAR Content
![]()
Google Scholar ![]()
![]()
Articles by Gyi, J. I.
![]()
Articles by Brown, T.
![]()
Search for Related Content
![]()
PubMed ![]()
![]()
PubMed Citation
![]()
Articles by Gyi, J. I.
![]()
Articles by Brown, T.
![]()
Social Bookmarking ![]()
![]()
What's this?



