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评估作为生物特征的色素:行星环境中色素和色素类似物的非生物/前生物合成。

Evaluating Pigments as a Biosignature: Abiotic/Prebiotic Synthesis of Pigments and Pigment Mimics in Planetary Environments.

机构信息

Lunar and Planetary Institute, Universities Space Research Association, Houston, Texas, USA.

NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.

出版信息

Astrobiology. 2024 Aug;24(8):767-782. doi: 10.1089/ast.2023.0006. Epub 2024 May 20.

Abstract

Pigments serve a multitude of functions in biology including light harvesting for photosynthesis, radiation protection, membrane support, and defense. The ubiquity of pigments-especially within extremophiles found in high-radiation, high-salinity, and dry environments-and their detectability via mission-ready techniques have elevated these molecules as promising targets in the search for evidence of life elsewhere. Moreover, the detection of pigments has been proposed as a "smoking gun" for extraterrestrial life as it has been suggested that these molecules cannot be generated abiotically. However, while pigments may hold promise as a biosignature, current understanding of their possible prebiotic origins remains understudied and uncertain. Better understanding of the abiotic synthesis of pigments is critical for evaluating the biogenicity of any pigment detected during missions, including by the Mars Perseverance rover or from returned samples. Compounding this uncertainty is the broad definition of pigment as it includes any compound capable of absorbing visible light and by itself does not specify a particular chemical motif. While not experimentally verified, there are promising prebiotic routes for generating pigments including hemes, chlorophylls, and carotenoids. Herein, we review the biochemistry of pigments, the inherent assumptions made when searching for these molecules in the field, their abiotic synthesis in industry and prebiotic reactions, prebiotically relevant molecules that can mimic their spectral signatures, and implications/recommendations for future work.

摘要

色素在生物学中具有多种功能,包括光合作用中的光捕获、辐射防护、膜支持和防御。色素的普遍性——尤其是在高辐射、高盐度和干燥环境中发现的极端微生物中——以及通过任务准备技术对其进行检测,使这些分子成为在其他地方寻找生命证据的有前途的目标。此外,由于有人提出这些分子不可能非生物合成,因此色素的检测被认为是外星生命的“确凿证据”。然而,虽然色素可能是生物特征的有力候选者,但目前对其可能的前生物起源的理解仍研究不足且不确定。更好地了解色素的非生物合成对于评估任务中检测到的任何色素的生物成因至关重要,包括火星毅力号漫游车或从返回样本中检测到的色素。使这种不确定性更加复杂的是色素的广泛定义,因为它包括任何能够吸收可见光的化合物,并且本身并不指定特定的化学基序。虽然尚未通过实验验证,但生成色素的前生物途径包括血红素、叶绿素和类胡萝卜素等。本文综述了色素的生物化学、在野外寻找这些分子时所做的固有假设、它们在工业和前生物反应中的非生物合成、能够模拟其光谱特征的前生物相关分子,以及对未来工作的影响/建议。

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