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氨基酸辅料的近紫外光降解机制:天冬氨酸和 Fe(III)形成二氧化碳自由基阴离子。

Near UV Photodegradation Mechanisms of Amino Acid Excipients: Formation of the Carbon Dioxide Radical Anion from Aspartate and Fe(III).

机构信息

Department of Pharmaceutical Chemistry, University of Kansas, 2093 Constant Avenue, Lawrence, Kansas 66047, United States.

出版信息

Mol Pharm. 2024 Mar 4;21(3):1233-1245. doi: 10.1021/acs.molpharmaceut.3c00893. Epub 2024 Feb 13.

DOI:10.1021/acs.molpharmaceut.3c00893
PMID:38350108
Abstract

Carbon dioxide radical anion (CO) is a powerful reducing agent that can reduce protein disulfide bonds and convert molecular oxygen to superoxide. Therefore, the generation of CO can be detrimental to pharmaceutical formulations. Iron is among the most prevalent impurities in formulations, where Fe(III) chelates of histidine (His) can produce CO upon exposure to near-UV light (Zhang and Schöneich, . , 190, 231-241). Here, we monitor by spin-trapping in combination with electron paramagnetic resonance spectroscopy and/or high-performance liquid chromatography-mass spectrometry analysis the photochemical formation of CO for a series of common amino acid excipients, including arginine (Arg), methionine (Met), proline (Pro), glutamic acid (Glu), glycine (Gly), aspartic acid (Asp), and lysine (Lys). Our results indicate that in the presence of Fe(III), Asp, and Glu produce significant yields of CO under photoirradiation with near-UV light. Notably, Asp demonstrates the highest efficiency of CO generation compared with that of the other amino acid excipients. Stable isotope labeling indicates that CO exclusively originates from the α-carboxyl group of Asp. Mechanistic studies reveal two possible pathways for CO formation, which involve either a β-carboxyl radical or an amino radical cation intermediate.

摘要

二氧化碳自由基阴离子(CO)是一种强大的还原剂,可还原蛋白质中二硫键,并将分子氧转化为超氧自由基。因此,CO 的产生可能对药物制剂有害。铁是制剂中最常见的杂质之一,其中组氨酸(His)的 Fe(III)螯合物在近紫外光照射下会产生 CO(Zhang and Schöneich,., 190, 231-241)。在这里,我们通过自旋捕获结合电子顺磁共振波谱和/或高效液相色谱-质谱分析监测了一系列常见氨基酸赋形剂(包括精氨酸(Arg)、蛋氨酸(Met)、脯氨酸(Pro)、谷氨酸(Glu)、甘氨酸(Gly)、天冬氨酸(Asp)和赖氨酸(Lys))的光化学 CO 形成。我们的结果表明,在 Fe(III)存在下,Asp 和 Glu 在近紫外光照射下会产生大量的 CO。值得注意的是,与其他氨基酸赋形剂相比,Asp 表现出最高的 CO 生成效率。稳定同位素标记表明 CO 仅源自 Asp 的α-羧基。机理研究揭示了 CO 形成的两种可能途径,涉及β-羧基自由基或氨基自由基阳离子中间体。

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