FTIR SPECTROSCOPY OF THE PHOTOREDUCTION OF THE BACTERIOPHEOPHYTIN ELECTRON-ACCEPTOR IN REACTION CENTERS OF RHODOBACTER-SPHAEROIDES AND RHODOPSEUDOMONAS-VIRIDIS

Citation
E. Nabedryk et al., FTIR SPECTROSCOPY OF THE PHOTOREDUCTION OF THE BACTERIOPHEOPHYTIN ELECTRON-ACCEPTOR IN REACTION CENTERS OF RHODOBACTER-SPHAEROIDES AND RHODOPSEUDOMONAS-VIRIDIS, Chemical physics, 194(2-3), 1995, pp. 371-378
Citations number
42
Categorie Soggetti
Physics, Atomic, Molecular & Chemical
Journal title
ISSN journal
03010104
Volume
194
Issue
2-3
Year of publication
1995
Pages
371 - 378
Database
ISI
SICI code
0301-0104(1995)194:2-3<371:FSOTPO>2.0.ZU;2-8
Abstract
The photoreduction of the bacteriopheophytin electron acceptor H-A in reaction centers from Rbodobacter sphaeroides and Rhodopseudomonas vir idis has been monitored by light-induced FTIR difference spectroscopy at 10 degrees C, in the presence of reductant and mediator. The striki ng similarity of the H-A(-)/H-A spectra obtained for Rb. sphaeroides a nd Rps. viridis reflects comparable interactions of the bacteriopheoph ytin electron acceptor with the protein in both reaction centers and i mplies that the photoreduction of H-A affects conserved amino acid res idues. The H-A(-)/H-A spectra are interpreted by comparison with model compound spectra of the anion radicals of bacteriopheophytin a and b, and by analysis of H-1/H-2 isotope effects. The downshift of the 1677 cm(-1) mode in Rb. sphaeroides (1681 cm(-1) in Rps. viridis) reaction centers with respect to the model compound is interpreted in terms of a strongly perturbed 9-keto carbonyl of H-A. This perturbation most p robably originates from hydrogen bonding to Glu L104. At least part of the positive signal at 1591 cm(-1) in Rb. sphaeroides and at 1601 cm( -1) in Rps. viridis is assigned to the 9-keto carbonyl mode of H-A(-). From H-1/H-2 exchange experiments, it is proposed that the (COOH)-H-1 side chain of Glu L104 contributes to the 1745-1735 cm(-1) spectral r ange with the corresponding (COOH)-H-2 signal displaced to lower frequ encies and partly hidden under the 1732 cm(-1) band.