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Methylphosphonate (MP) oligodeoxynucleotides (MPOs) are metabolically stable analogs of conventional DNA containing a methyl group in place of one of the non-bonding phosphoryl oxygens. All 16 possible chiral R(P) MP dinucleotides were synthesized and derivatized for automated oligonucleotide synthesis. These dimer synthons can be used to prepare (i) all-MP linked oligonucleotides having defined R(P) chirality at every other position (R(P) chirally enriched MPOs) or (ii) alternating R(P) MP/phosphodiester backbone oligonucleotides, depending on the composition of the 3'-coupling group. Chirally pure dimer synthons were also prepared with 2'-O-methyl sugar modifications. Oligonucleotides prepared with these R(P) chiral methylphosphonate linkage synthons bind RNA with significantly higher affinity than racemic MPOs.

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The TAR hairpin is an important part of the 5' long terminal repeat of HIV-1 and appears to be recognized by a cellular protein. A 14-base model of the native TAR hairpin 5'-GAGC[CUGGGA]-GCUC-3' (loop bases in square brackets) has been studied by proton, phosphorus, and natural abundance carbon NMR; these results are compared to other published NMR studies of the TAR hairpin. Assignments of all nonexchangeable protons and of all the stem-exchangeable protons have been made, as well as all phosphorus and many carbon resonances. Large J1'2' and J3'4' proton-proton coupling in the C5, G8, and G9 sugars indicate an equilibrium between C2'- and C3'-endo forms; these data show a dynamic loop structure. We see three broad imino resonances that have not been reported before; these resonances are in the right region for unbonded loop imino protons. These peaks suggest the protons are protected from fast exchange with the solvent by the structure of the hairpin loop. Simulated annealing and molecular dynamics with 148 distance constraints, 11 hydrogen bonds, and 84 torsion angle constraints showed a wide variety of structures. Certain trends are evident, such as continuation of the A-form helix on the 3' side of the hairpin loop. The ensemble of calculated structures agree with most chemical modification data.

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Little is known about the folding pathways of RNA. A particularly interesting RNA is L-21 Sca I, a linear form of the self-splicing intron from the precursor of the Tetrahymena thermophila large subunit (LSU) rRNA. Thermal unfolding of L-21 Sca I is studied by UV absorption and chemical mapping in 50 mM Na+ and 10 mM free Mg2+ at pH 7.5. UV melting experiments identify two major transitions with maxima at 65 and 73 degrees C. Chemical mapping at the beginning and middle of the first transition suggests it primarily involves disruption of tertiary structure. Phylogenetic comparisons suggest a potential tertiary interaction between loops L2.1 and L9.1a. Chemical mapping and melting experiments on a truncated form of the intron lacking P9.1a, L-21 Nhe I, are consistent with this hypothesis. The results indicate that increasing temperature disrupts tertiary interactions before disrupting secondary structure. This suggests tertiary interactions are weaker than secondary interactions in this case. These results support an important assumption for RNA structure prediction: that secondary structure dominates the free energy of folding.

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We have determined the structures and thermodynamic stabilities of the wild type Asn-52 and unusually thermostable mutant Ile-52 yeast iso-1-cytochromes c (Das, G., Hickey, D. R. McLendon, D., McLendon, G., and Sherman, F. (1989) Proc. Natl. Acad. Sci. U.S.A. 86, 496-499). Although both structures were similar, Water-166, buried within the wild type protein, is excluded from the Ile-52 mutant, which substantially reorganizes the local hydrogen bonding. Wild type Cys-102 was replaced with alanine or serine to eliminate dimerization in vitro. The Cys-102 (wild type), Ala-102, and Ser-102 proteins were equally stable, whereas the chemically modified Cys-102-SCH3 was less stable. The order of stability observed with replacements at positions 52 and 102 was as follows: Ile-52 Ala-102 greater than Ala-52 Ala-102 greater than Asn-52 Ala-102 ("normal") greater than Gly-52 Ala-102. No significant stabilization was attributed to potential energy interactions expressed as helix-forming propensities of replacements at position 52. A high correlation between differences in free energy changes and transfer free energies suggests hydrophobic interactions are the main factor for enhancing stability in the Ile-52 mutant. Additional possible contributions to the thermostability of the Ile-52 variant are energetic effects due to packing and hydrogen bonding changes surrounding position 52.

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This article describes the latest version of an RNA folding algorithm that predicts both optimal and suboptimal solutions based on free energy minimization. A number of RNA's with known structures deduced from comparative sequence analysis are folded to test program performance. The group of solutions obtained for each molecule is analysed to determine how many of the known helixes occur in the optimal solution and in the best suboptimal solution. In most cases, a structure about 80% correct is found with a free energy within 2% of the predicted lowest free energy structure.

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C IVS is the cyclized form of the intron from the RNA precursor of the Tetrahymena thermophila large subunit (LSU) ribosomal RNA. C IVS was mapped by chemical modification in 1 M Na+, 0.05 M Na+ and 10 mM Mg2+ (Na+/Mg2+), and Na+/Mg2+ with CUCU substrate. The results suggest the secondary structure is similar for all three conditions. Optical melting curves were also measured for C IVS in 1 M Na+ and Na+/Mg2+ and indicate the secondary structures have similar stabilities under both conditions. Computer predictions of secondary structure and stability are in good agreement with observations. The results suggest that many of the approximations used for computer prediction of secondary structure by free energy minimization are reasonable.

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The accuracy of computer predictions of RNA secondary structure from sequence data and free energy parameters has been increased to roughly 70%. Performance is judged by comparison with structures known from phylogenetic analysis. The algorithm also generates suboptimal structures. On average, the best structure within 10% of the lowest free energy contains roughly 90% of phylogenetically known helixes. The algorithm does not include tertiary interactions or pseudoknots and employs a crude model for single-stranded regions. The only favorable interactions are base pairing and stacking of terminal unpaired nucleotides at the ends of helixes. The excellent performance is consistent with these interactions being the primary interactions determining RNA secondary structure.

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Thermodynamic studies of oligoribonucleotides are providing parameters and insights for the fundamental interactions that determine RNA structure. These results can be used to predict the secondary structure of RNA from its sequence. Comparisons of predicted structures with those deduced from phylogenetic data indicate a modest success rate that is improving as more parameters are determined experimentally. Two major fundamental interactions in RNA are stacking and hydrogen bonding. Both contribute similar increments to free-energy changes for associations of oligoribonucleotides. Thus, parameters for stacking and hydrogen bonding will likely be important for predicting the three-dimensional structures of RNAs and for interpreting RNA-RNA associations. Both applications should be important for providing a full understanding of catalysis by RNA.

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Thermodynamic parameters for prediction of RNA duplex stability are reported. One parameter for duplex initiation and 10 parameters for helix propagation are derived from enthalpy and free-energy changes for helix formation by 45 RNA oligonucleotide duplexes. The oligomer sequences were chosen to maximize reliability of secondary structure predictions. Each of the 10 nearest-neighbor sequences is well-represented among the 45 oligonucleotides, and the sequences were chosen to minimize experimental errors in delta GO at 37 degrees C. These parameters predict melting temperatures of most oligonucleotide duplexes within 5 degrees C. This is about as good as can be expected from the nearest-neighbor model. Free-energy changes for helix propagation at dangling ends, terminal mismatches, and internal G X U mismatches, and free-energy changes for helix initiation at hairpin loops, internal loops, or internal bulges are also tabulated.

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