Published April 2023 | Version Published + Supplemental Material
Journal Article Open

A Bacterial Form I' Rubisco Has a Smaller Carbon Isotope Fractionation than Its Form I Counterpart

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Lawrence Berkeley National Laboratory
  • 3. ROR icon University of California, Berkeley
  • 4. ROR icon Joint BioEnergy Institute
  • 5. ROR icon Innovative Genomics Institute

Abstract

Form I rubiscos evolved in Cyanobacteria ≥ 2.5 billion years ago and are enzymatically unique due to the presence of small subunits (RbcS) capping both ends of an octameric large subunit (RbcL) rubisco assembly to form a hexadecameric (L8S8) holoenzyme. Although RbcS was previously thought to be integral to Form I rubisco stability, the recent discovery of a closely related sister clade of octameric rubiscos (Form I'; L8) demonstrates that the L8 complex can assemble without small subunits (Banda et al. 2020). Rubisco also displays a kinetic isotope effect (KIE) where the 3PG product is depleted in 13C relative to 12C. In Cyanobacteria, only two Form I KIE measurements exist, making interpretation of bacterial carbon isotope data difficult. To aid comparison, we measured in vitro the KIEs of Form I' (Candidatus Promineofilum breve) and Form I (Synechococcus elongatus PCC 6301) rubiscos and found the KIE to be smaller in the L8 rubisco (16.25 ± 1.36‰ vs. 22.42 ± 2.37‰, respectively). Therefore, while small subunits may not be necessary for protein stability, they may affect the KIE. Our findings may provide insight into the function of RbcS and allow more refined interpretation of environmental carbon isotope data.

Additional Information

© 2023 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). (This article belongs to the Special Issue Future Prospects in Cyanobacterial Synthetic Biology and Biotechnology) We thank Tobias Erb for thoughtful and supportive comments. R.Z.W. was supported by the National Science Foundation Graduate Research Fellowship Program (NSF GRFP). A.K.L., D.M.B., and P.M.S. were supported by a Society in Science–Branco Weiss fellowship from ETH Zürich and a Packard Fellowship from the David Lucile Packard Foundation. W.F.S. and research was supported by NASA Exobiology (80NSSC21K0484), Simons Foundation Collaboration on Origin and Evolution of Life (554187), Schwartz Reisman Collaborative Science Program, Caltech Center for Evolutionary Sciences. Author Contributions. Conceptualization, W.W.F. and P.M.S.; Methodology, R.Z.W., A.K.L., and D.M.B.; Formal Analysis, R.Z.W.; Writing—Original Draft Preparation, R.Z.W.; Writing—Review and Editing, R.Z.W., W.W.F., A.K.L., and P.M.S.; Funding Acquisition, W.W.F. and P.M.S. All authors have read and agreed to the published version of the manuscript. Data Availability Statement. All data used in this study are presented in the supplement. The authors declare no conflict of interest.

Attached Files

Published - biomolecules-13-00596-v2.pdf

Supplemental Material - biomolecules-13-00596-s001.zip

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Additional details

Identifiers

PMCID
PMC10135865
Eprint ID
121396
Resolver ID
CaltechAUTHORS:20230515-138491000.9

Funding

NSF Graduate Research Fellowship
ETH Zürich
David and Lucile Packard Foundation
NASA
80NSSC21K0484
Simons Foundation
554187
Schwartz Reisman Collaborative Science Program
Caltech Center for Evolutionary Science

Dates

Created
2023-05-18
Created from EPrint's datestamp field
Updated
2023-06-30
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS), Caltech Center for Evolutionary Science