Abstract

Nascent proteins fold co-translationally because the folding speed and folding pathways are limited by the rate of ribosome biosynthesis in the living cell. In addition, though full-length proteins can fold all their residues during the folding process, nascent proteins initially fold only with the N-terminal residues. However, the transient structure and the co-translational folding pathway are not well understood. Here we report the atomic structures of a series of N-terminal fragments of the WW domain with increasing amino acid length. Unexpectedly, the structures indicate that the intermediate-length fragments take helical conformations even though the full-length protein has no helical regions. The circular dichroism spectra and theoretical calculations also support the crystallographic results. This suggests that the short-range interactions are more decisive in the structure formation than the long-range interactions for short nascent proteins. In the course of the peptide extension, the helical structure change to the structure mediated by the long-range interactions at a particular polypeptide length. Our results will provide unique information for elucidating the nature of co-translational folding.

Highlights

  • WW35 has a three-stranded beta-sheet structure, as previously reported for the X-ray structure of the full-length WW domain[15] (Fig. 2a,b). These structures can be superimposed with a root-mean-square deviation (RMSD) of 1.14 Å (Supplementary Fig. 3)

  • We found that the intermediate-length fragments of the WW domain form alpha-helical structures

  • These results show that the structures of the nascent proteins are determined by already synthesized polypeptide sequences

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Summary

Introduction

Though WW17 harbors residues 17–20, which form hairpin loop 1 in WW35, their conformations are not identical to WW35 (Fig. 3c,d). This result indicates that the hairpin loop 1 does not form the native-like conformation in the transient structure. In order to obtain structural information for various additional WWX fragments, we collected circular dichroism (CD) spectra (Supplementary Fig. 5a).

Results
Conclusion
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