Published March 6, 2023 | Version Supplemental Material + Submitted
Discussion Paper Open

Bacterial Form I' rubisco has 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) that cap 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 enzyme complex assembles 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

The copyright holder for this preprint is the author/funder, who has granted bioRxiv a license to display the preprint in perpetuity. It is made available under a CC-BY-NC-ND 4.0 International license. Data Availability Statement. All data used in this study are presented in the supplement. The authors have declared no competing interest.

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Identifiers

Eprint ID
120128
Resolver ID
CaltechAUTHORS:20230316-182052000.9

Dates

Created
2023-03-22
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