3-pulse ESEEM and HYSCORE pulse sequences have been used to analyze the secondary electron acceptor semiquinone anion radical (QB-). Photosynthetic reaction centers from Rhodobacter sphaeroides have identical ubiquinone molecules functioning as primary and secondary electron acceptors. The primary quinone radical (QA-) has been extensively studied, and hydrogen bonds have been characterized at both carbonyls. The structure around QB- has received less attention. The O4 carbonyl has been suggested to be hydrogen bonded to the Nδ from a histidine at residue L190. The O1 carbonyl also possesses a hydrogen bond that is weaker than that at O4. OH from serine at L223 is important in the hydrogen bond structure at this carbonyl. However, contributions from surrounding peptide nitrogens are suggested by x-ray structures but have not yet been investigated by EPR methods. Pulsed EPR studies of the QB- radical confirm one strongly coupled nitrogen with NQI frequencies consistent with a histidine Nδ. 3-pulse ESEEM and HYSCORE spectra also contain peaks from a second nitrogen nucleus. A priori knowledge of the origins of these peaks is less clear, but could include contributions from a backbone nitrogen. Additionally, NQI modulation from 14N is sufficiently shallow to observe signals from 2 protons in HYSCORE measurements. These results suggest the possibility that an additional residue contributes to the stability of QB-. Supported by NSF grant MCB 08-18121.