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马氏锦鳚类色素的光谱特性揭示了蓝物种和品系之间的细微差异。

Spectral Properties of Marennine-like Pigments Reveal Minor Differences Between Blue Species and Strains.

机构信息

Institut des Molécules et Matériaux du Mans, Le Mans Université, Avenue Olivier Messiaen, 72085 Le Mans, France.

Laboratoire Biologie des Organismes, Santé, Environnement, Le Mans Université, Avenue Olivier Messiaen, 72085 Le Mans, France.

出版信息

Molecules. 2024 Nov 6;29(22):5248. doi: 10.3390/molecules29225248.

Abstract

Marennine is the specific bluish pigment produced by the marine diatom Gaillon (Simonsen), responsible for the greening of oysters in France's Atlantic coast. For decades, was considered the only blue diatom and described as such. However, new blue species have been described recently, among which Davidovich, Gastineau, and Mouget (Black Sea, Crimea, Ukraine); Gastineau, Hansen, and Mouget (Mediterranean Sea, southern France) Gastineau, Hansen, and Mouget (West Atlantic Ocean, USA); and one not characterized yet, sp. nov., isolated in Tenerife (Spain). These species produce marennine-like pigments, for which little information is available yet. The present work aims at studying spectral characteristics of these pigments by UV-visible spectrometry, Raman spectrometry, infrared spectrometry, nuclear magnetic resonance, energy-dispersive X-ray spectroscopy, and cyclic voltammetry, and comparing them to those of marennine produced by strains originating from the north Atlantic Ocean (western France and Macaronesia), and north Pacific Ocean (southwestern USA). Results show that marennine produced by strains and marennine-like pigments produced by , , and sp. nov. are quite similar regarding their polysaccharide skeleton, and absorption in the UV-visible, infrared, and Raman regions. The most different marennine-like pigment is produced by but all blue pigments studied so far belong to the same family of organic molecules.

摘要

海胆甲藻素是一种由海洋硅藻 Gaillon(Simonsen)产生的特殊蓝色色素,负责使法国大西洋沿岸的牡蛎变绿。几十年来,它一直被认为是唯一的蓝色硅藻,并以此命名。然而,最近又描述了一些新的蓝色硅藻物种,其中包括:Davidovich、Gastineau 和 Mouget(黑海,克里米亚,乌克兰);Gastineau、Hansen 和 Mouget(地中海,法国南部);Gastineau、Hansen 和 Mouget(西大西洋,美国);以及尚未表征的物种,sp. nov.,分离自西班牙特内里费岛。这些物种产生类似于海胆甲藻素的色素,但目前对此知之甚少。本研究旨在通过紫外可见光谱、拉曼光谱、红外光谱、核磁共振、能量色散 X 射线光谱和循环伏安法研究这些色素的光谱特征,并将其与源自北大西洋(法国西部和马卡罗尼西亚)和北太平洋(美国西南部)的 菌株产生的海胆甲藻素进行比较。结果表明, 菌株产生的海胆甲藻素和 、 和 sp. nov.产生的类似于海胆甲藻素的色素在多糖骨架、紫外可见、红外和拉曼区域的吸收方面非常相似。最不同的类似于海胆甲藻素的色素是由 产生的,但迄今为止研究的所有蓝色色素都属于同一类有机分子。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0620/11596562/5b5a1907e0c8/molecules-29-05248-g001.jpg

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