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Analysis of the structure of HIV-1 protease complexed with a hexapeptide inhibitor. Part II: Molecular dynamic studies of the active site region

โœ Scribed by Maciej Geller; Maria Miller; Stanley M. Swanson; Jacob Maizel


Publisher
John Wiley and Sons
Year
1997
Tongue
English
Weight
130 KB
Volume
27
Category
Article
ISSN
0887-3585

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โœฆ Synopsis


Six models of the catalytic site of HIV-1 protease complexed with a reduced peptide inhibitor, MVT-101, were investigated. These studies focused on the details of protonation of the active site, its total net charge and hydrogen bonding pattern, which was consistent with both the observed coplanar configuration of the acidic groups of the catalytic aspartates (Asp-25 and Asp-125) and the observed binding mode of the inhibitor. Molecular dynamic simulations using AMBER 4.0 indicated that the active site should be neutral. The planarity of the aspartate dyad may be due to the formation of two hydrogen bonds: one between the inner O d1 oxygen atoms of the two catalytic aspartates and another between the O d2 atom of Asp-125 and the nitrogen atom of the reduced peptide bond of the bound inhibitor. This would require two additional protonations, either of both aspartates, or of one Asp and the amido nitrogen atom of Nle-204. Our results favor the Asp-inhibitor protonation but the other one is not excluded. Implications of these findings for the mechanism of enzymatic catalysis are discussed. Dynamic properties of the hydrogen bond network in the active site and an analysis of the interaction energy between the inhibitor and the protease are presented.


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โœ Maria Miller; Maciej Geller; Michael Gribskov; Stephen B. H. Kent ๐Ÿ“‚ Article ๐Ÿ“… 1997 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 294 KB ๐Ÿ‘ 1 views

The structure of a complex between a hexapeptide-based inhibitor, MVT-101, and the chemically synthesized (Aba 67,95,167,195; Aba: L-a-amino-n-butyric acid) protease from the human immunodeficiency virus (HIV-1), reported previously at 2.3 ร… has now been refined to a crystallographic R factor of 15.