Preliminary spectroscopic investigation of a potential Mars analog site: Lake Bagno dell’Acqua, Pantelleria, Italy

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Enrico Bruschini , Marco Ferrari , Cristina Mazzoni , Stefano Fazi , Francesco Latino Chiocci , Ilaria Mazzini , Giovanna Costanzo , Simone De Angelis , Maria Cristina De Sanctis , Francesca Altieri , Jeremy Brossier , Eleonora Ammannito
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Abstract

In this study, we characterize the mineralogy and microbiology of a suite of samples from the Bagno dell’Acqua alkaline (pH ≥ 9) lake in Pantelleria, Italy. The aim of the present characterization is the assessment of the lake as a Martian analog site. Nineteen samples were characterized by a combination of VNIR reflectance spectroscopy, micro-Raman (μ-Raman) spectroscopy, and fluorescence microscopy. In addition, DNA extraction was performed on three selected samples to identify the bacteria phyla and to quantify their abundance. The samples were collected as push cores inside the lake and as loose sediments taken along the eastern and southeastern lake's shore. The samples underwent three thermal cycles (between 343 K and 473 K) to remove excess water and organic matter. The VNIR spectra were measured on each sample after each thermal cycle to check the variation of the spectral features as a function of thermal treatment. The mineralogical content of our push core samples is dominated by the presence of Mg-smectite clays always associated with the remanence of K-feldspars and Ca-carbonates while in the sediments we observe also additional minor phases like pyroxene (aegirine NaFe3+Si2O6), hematite (Fe2O3), anatase (TiO2), and volcanic glass. Two organic phases were detected by μ-Raman spectroscopy. One phase was attributable to carotenoids, in line with the high abundance of Bacterial Phyla that can synthesize these molecules. The second phase appeared to be visually indistinguishable from the inorganic matrix and is therefore attributed to EPS (Extracellular Polymeric Substances) forming a biofilm and extensively observed by fluorescent microscopy. The peculiar chemistry of the waters, the presence of Mg-smectite in the sediments of Lake Bagno dell’Acqua associated with Ca-carbonates and sediments derived by biological activity makes Lake Bagno dell’Acqua a very interesting and promising Martian analog site.

对潜在火星类似点的初步光谱学调查:意大利潘泰勒利亚的巴尼奥德尔阿夸湖
在这项研究中,我们对意大利潘泰勒利亚的 Bagno dell'Acqua 碱湖(pH 值≥ 9)的一系列样本进行了矿物学和微生物学特征描述。本次特征描述的目的是将该湖泊作为火星模拟地点进行评估。通过结合使用近红外反射光谱、微拉曼(μ-Raman)光谱和荧光显微镜,对 19 个样本进行了表征。此外,还对三个选定样本进行了 DNA 提取,以确定细菌门类并量化其丰度。这些样本是在湖内采集的推入式岩心,以及在湖东部和东南部湖岸采集的松散沉积物。样本经过三次热循环(343 K 至 473 K),以去除多余的水分和有机物。在每个热循环之后,都对每个样品进行了近红外光谱测量,以检查光谱特征随热处理的变化情况。推岩心样品的矿物成分主要是镁闪长岩粘土,并伴有钾长石和钙碳酸盐的重现,而在沉积物中,我们还观察到其他小相,如辉石(埃吉林 NaFe3+Si2O6)、赤铁矿(Fe2O3)、锐钛矿(TiO2)和火山玻璃。通过 μ-Raman 光谱法检测到两种有机相。其中一种有机相是类胡萝卜素,这与能够合成这些分子的大量细菌植物相吻合。第二种物质在视觉上与无机基质难以区分,因此被认为是形成生物膜的 EPS(胞外聚合物质),并通过荧光显微镜进行了广泛观察。水的特殊化学性质、巴格诺戴尔阿夸湖沉积物中存在的镁-钠长石、钙碳酸盐和生物活动产生的沉积物,使巴格诺戴尔阿夸湖成为一个非常有趣和有前途的火星模拟地点。
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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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