Cargando…
The Nuclear Magnetic Resonance of CCCC RNA Reveals a Right-Handed Helix, and Revised Parameters for AMBER Force Field Torsions Improve Structural Predictions from Molecular Dynamics
[Image: see text] The sequence dependence of RNA energetics is important for predicting RNA structure. Hairpins with C(n) loops are consistently less stable than hairpins with other loops, which suggests the structure of C(n) regions could be unusual in the “unfolded” state. For example, previous nu...
Autores principales: | , , , , , |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
American Chemical
Society
2013
|
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3571207/ https://www.ncbi.nlm.nih.gov/pubmed/23286901 http://dx.doi.org/10.1021/bi3010347 |
_version_ | 1782259153911152640 |
---|---|
author | Tubbs, Jason D. Condon, David E. Kennedy, Scott D. Hauser, Melanie Bevilacqua, Philip C. Turner, Douglas H. |
author_facet | Tubbs, Jason D. Condon, David E. Kennedy, Scott D. Hauser, Melanie Bevilacqua, Philip C. Turner, Douglas H. |
author_sort | Tubbs, Jason D. |
collection | PubMed |
description | [Image: see text] The sequence dependence of RNA energetics is important for predicting RNA structure. Hairpins with C(n) loops are consistently less stable than hairpins with other loops, which suggests the structure of C(n) regions could be unusual in the “unfolded” state. For example, previous nuclear magnetic resonance (NMR) evidence suggested that polycytidylic acid forms a left-handed helix. In this study, UV melting experiments show that the hairpin formed by r(5′GGACCCCCGUCC) is less stable than r(5′GGACUUUUGUCC). NMR spectra for single-stranded C(4) oligonucleotide, mimicking the unfolded hairpin loop, are consistent with a right-handed A-form-like helix. Comparisons between NMR spectra and molecular dynamics (MD) simulations suggest that recent reparametrizations, parm99χ_YIL and parm99TOR, of the AMBER parm99 force field improve the agreement between structural features for C(4) determined by NMR and predicted by MD. Evidently, the force field revisions to parm99 improve the modeling of RNA energetics and therefore structure. |
format | Online Article Text |
id | pubmed-3571207 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2013 |
publisher | American Chemical
Society |
record_format | MEDLINE/PubMed |
spelling | pubmed-35712072013-02-14 The Nuclear Magnetic Resonance of CCCC RNA Reveals a Right-Handed Helix, and Revised Parameters for AMBER Force Field Torsions Improve Structural Predictions from Molecular Dynamics Tubbs, Jason D. Condon, David E. Kennedy, Scott D. Hauser, Melanie Bevilacqua, Philip C. Turner, Douglas H. Biochemistry [Image: see text] The sequence dependence of RNA energetics is important for predicting RNA structure. Hairpins with C(n) loops are consistently less stable than hairpins with other loops, which suggests the structure of C(n) regions could be unusual in the “unfolded” state. For example, previous nuclear magnetic resonance (NMR) evidence suggested that polycytidylic acid forms a left-handed helix. In this study, UV melting experiments show that the hairpin formed by r(5′GGACCCCCGUCC) is less stable than r(5′GGACUUUUGUCC). NMR spectra for single-stranded C(4) oligonucleotide, mimicking the unfolded hairpin loop, are consistent with a right-handed A-form-like helix. Comparisons between NMR spectra and molecular dynamics (MD) simulations suggest that recent reparametrizations, parm99χ_YIL and parm99TOR, of the AMBER parm99 force field improve the agreement between structural features for C(4) determined by NMR and predicted by MD. Evidently, the force field revisions to parm99 improve the modeling of RNA energetics and therefore structure. American Chemical Society 2013-01-03 2013-02-12 /pmc/articles/PMC3571207/ /pubmed/23286901 http://dx.doi.org/10.1021/bi3010347 Text en Copyright © 2013 American Chemical Society http://pubs.acs.org This is an open-access article distributed under the ACS AuthorChoice Terms & Conditions. Any use of this article, must conform to the terms of that license which are available at http://pubs.acs.org. |
spellingShingle | Tubbs, Jason D. Condon, David E. Kennedy, Scott D. Hauser, Melanie Bevilacqua, Philip C. Turner, Douglas H. The Nuclear Magnetic Resonance of CCCC RNA Reveals a Right-Handed Helix, and Revised Parameters for AMBER Force Field Torsions Improve Structural Predictions from Molecular Dynamics |
title | The Nuclear Magnetic Resonance of CCCC RNA Reveals
a Right-Handed Helix, and Revised Parameters for AMBER Force Field
Torsions Improve Structural Predictions from Molecular Dynamics |
title_full | The Nuclear Magnetic Resonance of CCCC RNA Reveals
a Right-Handed Helix, and Revised Parameters for AMBER Force Field
Torsions Improve Structural Predictions from Molecular Dynamics |
title_fullStr | The Nuclear Magnetic Resonance of CCCC RNA Reveals
a Right-Handed Helix, and Revised Parameters for AMBER Force Field
Torsions Improve Structural Predictions from Molecular Dynamics |
title_full_unstemmed | The Nuclear Magnetic Resonance of CCCC RNA Reveals
a Right-Handed Helix, and Revised Parameters for AMBER Force Field
Torsions Improve Structural Predictions from Molecular Dynamics |
title_short | The Nuclear Magnetic Resonance of CCCC RNA Reveals
a Right-Handed Helix, and Revised Parameters for AMBER Force Field
Torsions Improve Structural Predictions from Molecular Dynamics |
title_sort | nuclear magnetic resonance of cccc rna reveals
a right-handed helix, and revised parameters for amber force field
torsions improve structural predictions from molecular dynamics |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3571207/ https://www.ncbi.nlm.nih.gov/pubmed/23286901 http://dx.doi.org/10.1021/bi3010347 |
work_keys_str_mv | AT tubbsjasond thenuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT condondavide thenuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT kennedyscottd thenuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT hausermelanie thenuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT bevilacquaphilipc thenuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT turnerdouglash thenuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT tubbsjasond nuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT condondavide nuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT kennedyscottd nuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT hausermelanie nuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT bevilacquaphilipc nuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics AT turnerdouglash nuclearmagneticresonanceofccccrnarevealsarighthandedhelixandrevisedparametersforamberforcefieldtorsionsimprovestructuralpredictionsfrommoleculardynamics |