Abstract
19F electron-nuclear double resonance (ENDOR) has emerged as an attractive method for determining distance distributions in biomolecules in the range of 0.7-2 nm, which is not easily accessible by pulsed electron dipolar spectroscopy. The 19F ENDOR approach relies on spin labeling, and in this work, we compare various labels’ performance. Four protein variants of GB1 and ubiquitin bearing fluorinated residues were labeled at the same site with nitroxide and trityl radicals and a Gd(iii) chelate. Additionally, a double-histidine variant of GB1 was labeled with a Cu(ii) nitrilotriacetic acid chelate. ENDOR measurements were carried out at W-band (95 GHz) where 19F signals are well separated from 1H signals. Differences in sensitivity were observed, with Gd(iii) chelates providing the highest signal-to-noise ratio. The new trityl label, OXMA, devoid of methyl groups, exhibited a sufficiently long phase memory time to provide an acceptable sensitivity. However, the longer tether of this label effectively reduces the maximum accessible distance between the 19F and the Cα of the spin-labeling site. The nitroxide and Cu(ii) labels provide valuable additional geometric insights via orientation selection. Prediction of electron-nuclear distances based on the known structures of the proteins were the closest to the experimental values for Gd(iii) labels, and distances obtained for Cu(ii) labeled GB1 are in good agreement with previously published NMR results. Overall, our results offer valuable guidance for selecting optimal spin labels for 19F ENDOR distance measurement in proteins.
Original language | English |
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Pages (from-to) | 26921-26932 |
Number of pages | 12 |
Journal | Physical Chemistry Chemical Physics |
Volume | 26 |
Issue number | 42 |
DOIs | |
Publication status | Published Online - 11 Oct 2024 |
Funding
This work was funded by the National Science Foundation USA-Israel Science Foundation program through BSF 2021617 (to DG), and NSF-MCB 2116534 (to AMG), NSF grant CHE 1708773 (to AMG), the NSFC-ISF China-Israel 3559/21 Research Grant Program (to DG) as well as the National Natural Science Foundation of China 22174099 and 21871210 to (to YPL) and made possible, in part, by support from the Helen and Martin Kimmel Institute for Magnetic Resonance Research and the historic generosity of the Harold Perlman Family (DG). We are indebted to Dr Maxx Tessmer and Prof. Stefan Stoll for discussions and help with ChiLife software. Publisher Copyright: © 2024 The Royal Society of Chemistry.
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy
- Physical and Theoretical Chemistry