Cargando…

Thermodynamic System Drift in Protein Evolution

Proteins from thermophiles are generally more thermostable than their mesophilic homologs, but little is known about the evolutionary process driving these differences. Here we attempt to understand how the diverse thermostabilities of bacterial ribonuclease H1 (RNH) proteins evolved. RNH proteins f...

Descripción completa

Detalles Bibliográficos
Autores principales: Hart, Kathryn M., Harms, Michael J., Schmidt, Bryan H., Elya, Carolyn, Thornton, Joseph W., Marqusee, Susan
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Public Library of Science 2014
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4227636/
https://www.ncbi.nlm.nih.gov/pubmed/25386647
http://dx.doi.org/10.1371/journal.pbio.1001994
_version_ 1782343841145159680
author Hart, Kathryn M.
Harms, Michael J.
Schmidt, Bryan H.
Elya, Carolyn
Thornton, Joseph W.
Marqusee, Susan
author_facet Hart, Kathryn M.
Harms, Michael J.
Schmidt, Bryan H.
Elya, Carolyn
Thornton, Joseph W.
Marqusee, Susan
author_sort Hart, Kathryn M.
collection PubMed
description Proteins from thermophiles are generally more thermostable than their mesophilic homologs, but little is known about the evolutionary process driving these differences. Here we attempt to understand how the diverse thermostabilities of bacterial ribonuclease H1 (RNH) proteins evolved. RNH proteins from Thermus thermophilus (ttRNH) and Escherichia coli (ecRNH) share similar structures but differ in melting temperature (T(m)) by 20°C. ttRNH's greater stability is caused in part by the presence of residual structure in the unfolded state, which results in a low heat capacity of unfolding (ΔC(p)) relative to ecRNH. We first characterized RNH proteins from a variety of extant bacteria and found that T(m) correlates with the species' growth temperatures, consistent with environmental selection for stability. We then used ancestral sequence reconstruction to statistically infer evolutionary intermediates along lineages leading to ecRNH and ttRNH from their common ancestor, which existed approximately 3 billion years ago. Finally, we synthesized and experimentally characterized these intermediates. The shared ancestor has a melting temperature between those of ttRNH and ecRNH; the T(m)s of intermediate ancestors along the ttRNH lineage increased gradually over time, while the ecRNH lineage exhibited an abrupt drop in T(m) followed by relatively little change. To determine whether the underlying mechanisms for thermostability correlate with the changes in T(m), we measured the thermodynamic basis for stabilization—ΔC(p) and other thermodynamic parameters—for each of the ancestors. We observed that, while the T(m) changes smoothly, the mechanistic basis for stability fluctuates over evolutionary time. Thus, even while overall stability appears to be strongly driven by selection, the proteins explored a wide variety of mechanisms of stabilization, a phenomenon we call “thermodynamic system drift.” This suggests that even on lineages with strong selection to increase stability, proteins have wide latitude to explore sequence space, generating biophysical diversity and potentially opening new evolutionary pathways.
format Online
Article
Text
id pubmed-4227636
institution National Center for Biotechnology Information
language English
publishDate 2014
publisher Public Library of Science
record_format MEDLINE/PubMed
spelling pubmed-42276362014-11-18 Thermodynamic System Drift in Protein Evolution Hart, Kathryn M. Harms, Michael J. Schmidt, Bryan H. Elya, Carolyn Thornton, Joseph W. Marqusee, Susan PLoS Biol Research Article Proteins from thermophiles are generally more thermostable than their mesophilic homologs, but little is known about the evolutionary process driving these differences. Here we attempt to understand how the diverse thermostabilities of bacterial ribonuclease H1 (RNH) proteins evolved. RNH proteins from Thermus thermophilus (ttRNH) and Escherichia coli (ecRNH) share similar structures but differ in melting temperature (T(m)) by 20°C. ttRNH's greater stability is caused in part by the presence of residual structure in the unfolded state, which results in a low heat capacity of unfolding (ΔC(p)) relative to ecRNH. We first characterized RNH proteins from a variety of extant bacteria and found that T(m) correlates with the species' growth temperatures, consistent with environmental selection for stability. We then used ancestral sequence reconstruction to statistically infer evolutionary intermediates along lineages leading to ecRNH and ttRNH from their common ancestor, which existed approximately 3 billion years ago. Finally, we synthesized and experimentally characterized these intermediates. The shared ancestor has a melting temperature between those of ttRNH and ecRNH; the T(m)s of intermediate ancestors along the ttRNH lineage increased gradually over time, while the ecRNH lineage exhibited an abrupt drop in T(m) followed by relatively little change. To determine whether the underlying mechanisms for thermostability correlate with the changes in T(m), we measured the thermodynamic basis for stabilization—ΔC(p) and other thermodynamic parameters—for each of the ancestors. We observed that, while the T(m) changes smoothly, the mechanistic basis for stability fluctuates over evolutionary time. Thus, even while overall stability appears to be strongly driven by selection, the proteins explored a wide variety of mechanisms of stabilization, a phenomenon we call “thermodynamic system drift.” This suggests that even on lineages with strong selection to increase stability, proteins have wide latitude to explore sequence space, generating biophysical diversity and potentially opening new evolutionary pathways. Public Library of Science 2014-11-11 /pmc/articles/PMC4227636/ /pubmed/25386647 http://dx.doi.org/10.1371/journal.pbio.1001994 Text en © 2014 Hart et al http://creativecommons.org/licenses/by/4.0/ This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are properly credited.
spellingShingle Research Article
Hart, Kathryn M.
Harms, Michael J.
Schmidt, Bryan H.
Elya, Carolyn
Thornton, Joseph W.
Marqusee, Susan
Thermodynamic System Drift in Protein Evolution
title Thermodynamic System Drift in Protein Evolution
title_full Thermodynamic System Drift in Protein Evolution
title_fullStr Thermodynamic System Drift in Protein Evolution
title_full_unstemmed Thermodynamic System Drift in Protein Evolution
title_short Thermodynamic System Drift in Protein Evolution
title_sort thermodynamic system drift in protein evolution
topic Research Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4227636/
https://www.ncbi.nlm.nih.gov/pubmed/25386647
http://dx.doi.org/10.1371/journal.pbio.1001994
work_keys_str_mv AT hartkathrynm thermodynamicsystemdriftinproteinevolution
AT harmsmichaelj thermodynamicsystemdriftinproteinevolution
AT schmidtbryanh thermodynamicsystemdriftinproteinevolution
AT elyacarolyn thermodynamicsystemdriftinproteinevolution
AT thorntonjosephw thermodynamicsystemdriftinproteinevolution
AT marquseesusan thermodynamicsystemdriftinproteinevolution