Predicting non-functional mutations in protein complexes

POSTER

Abstract

Robust methods to predict the effects of mutation upon protein free energy have many important applications in understanding the consequences of real-time viral evolution. In our research, we seek to develop an effective computational approach for narrowing down the list of viable mutations. We have chosen the bacteriophage $\varphi $X174 as a model to develop this computational approach. Specifically, we focused on mutations within the spike protein, G, located on the viral capsid. Using snapshots generated via molecular dynamics simulations, we predicted the biophysical effects of all possible single mutations within the G protein using FoldX. FoldX has a semi-empirical scoring function that requires a minimum of computational resources, allowing calculation of all possible stability changes to binding and folding among the G pentamer, as well as the binding between protein G and the viral capsid protein, F. We then compared these calculated values to empirically-derived results for a subset of the mutations to protein G. Statistical analysis revealed a relationship between simulated free energy changes and the experimentally-determined viability of the mutation, allowing us to separate viable from nonviable mutants.

Authors

  • Casey Beard

    University of Idaho

  • D. Niroomand

    Gonzaga University, Wabash College, Simon Fraser University, Tel Aviv University, University of Manitoba, Texas A&M University, TRIUMF, University of British Columbia, Caltech, Western Washington University, University of Washington, Whatcom Community College, Smithsonian Astrophysical Observatory, Siena College, University of Idaho, Department of Mechanical Engineering, University of Idaho, Boise State University

  • D. Niroomand

    Gonzaga University, Wabash College, Simon Fraser University, Tel Aviv University, University of Manitoba, Texas A&M University, TRIUMF, University of British Columbia, Caltech, Western Washington University, University of Washington, Whatcom Community College, Smithsonian Astrophysical Observatory, Siena College, University of Idaho, Department of Mechanical Engineering, University of Idaho, Boise State University

  • D. Niroomand

    Gonzaga University, Wabash College, Simon Fraser University, Tel Aviv University, University of Manitoba, Texas A&M University, TRIUMF, University of British Columbia, Caltech, Western Washington University, University of Washington, Whatcom Community College, Smithsonian Astrophysical Observatory, Siena College, University of Idaho, Department of Mechanical Engineering, University of Idaho, Boise State University

  • D. Niroomand

    Gonzaga University, Wabash College, Simon Fraser University, Tel Aviv University, University of Manitoba, Texas A&M University, TRIUMF, University of British Columbia, Caltech, Western Washington University, University of Washington, Whatcom Community College, Smithsonian Astrophysical Observatory, Siena College, University of Idaho, Department of Mechanical Engineering, University of Idaho, Boise State University

  • D. Niroomand

    Gonzaga University, Wabash College, Simon Fraser University, Tel Aviv University, University of Manitoba, Texas A&M University, TRIUMF, University of British Columbia, Caltech, Western Washington University, University of Washington, Whatcom Community College, Smithsonian Astrophysical Observatory, Siena College, University of Idaho, Department of Mechanical Engineering, University of Idaho, Boise State University

  • D. Niroomand

    Gonzaga University, Wabash College, Simon Fraser University, Tel Aviv University, University of Manitoba, Texas A&M University, TRIUMF, University of British Columbia, Caltech, Western Washington University, University of Washington, Whatcom Community College, Smithsonian Astrophysical Observatory, Siena College, University of Idaho, Department of Mechanical Engineering, University of Idaho, Boise State University