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The persistence of a chlorophyll spectral biosignature from Martian evaporite and spring analogues under Mars-like conditions

机译:类火星条件下火星蒸发物和春季类似物的叶绿素光谱生物特征的持久性

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摘要

Spring and evaporite deposits are considered two of the most promising environments for past habitability on Mars and preservation of biosignatures. Manitoba, Canada hosts the East German Creek (EGC) hypersaline spring complex, and the post impact evaporite gypsum beds of the Lake St. Martin (LSM) impact. The EGC complex has microbial mats, sediments, algae and biofabrics, while endolithic communities are ubiquitous in the LSM gypsum beds. These communities are spectrally detectable based largely on the presence of a chlorophyll absorption band at 670 nm; however, the robustness of this feature under Martian surface conditions was unclear. Biological and biology-bearing samples from EGC and LSM were exposed to conditions similar to the surface of present day Mars (high UV flux, 100 mbar, anoxic, CO_2 rich) for up to 44 days, and preservation of the 670 nm chlorophyll feature and chlorophyll red-edge was observed. A decrease in band depth of the 670 nm band ranging from ∼16 to 80% resulted, with correlations seen in the degree of preservation and the spatial proximity of samples to the spring mound and mineral shielding effects. The spectra were deconvolved to Mars Exploration Rover (MER) Pancam and Mars Science Laboratory (MSL) Mastcam science filter bandpasses to investigate the detectability of the 670 nm feature and to compare with common mineral features. The red-edge and 670 nm feature associated with chlorophyll can be distinguished from the spectra of minerals with features below ∼1000 nm, such as hematite and jarosite. However, distinguishing goethite from samples with the chlorophyll feature is more problematic, and quantitative interpretation using band depth data makes little distinction between iron oxyhydroxides and the 670 nm chlorophyll feature. The chlorophyll spectral feature is observable in both Pancam and Mastcam, and we propose that of the proposed EXOMARS Pancam filters, the PHYLL filter is best suited for its detection.
机译:对于过去在火星上的可居住性和生物特征的保存,春季和蒸发岩沉积物被认为是两个最有希望的环境。加拿大马尼托巴省拥有东德河(EGC)高盐泉综合体,以及圣马丁湖(LSM)撞击后的撞击后蒸发石膏床。 EGC复合体具有微生物垫,沉积物,藻类和生物纤维,而内生石块群落在LSM石膏床中无处不在。这些群落在很大程度上是根据670 nm处叶绿素吸收带的存在进行光谱检测的。然而,该功能在火星表面条件下的鲁棒性尚不清楚。将来自EGC和LSM的生物学和生物学样本暴露于与当今火星表面相似的条件(高紫外线通量,100 mbar,缺氧,富含CO_2)长达44天,并保留了670 nm的叶绿素特征和观察到叶绿素红边。 670 nm谱带的谱带深度从约16%降低到80%,与保存程度,样品与春季土墩的空间接近性以及矿物屏蔽效果相关。将光谱分别解卷到火星探测漫游者(MER)Pancam和火星科学实验室(MSL)Mastcam科学滤光带通上,以研究670 nm特征的可检测性并与常见的矿物特征进行比较。与叶绿素有关的红边和670 nm特征可以与特征在〜1000 nm以下的矿物(如赤铁矿和黄钾铁矾)的光谱区分开。但是,将针铁矿与具有叶绿素特征的样品区分开来会遇到更多问题,并且使用能带深度数据进行定量解释几乎不会区分羟基氧化铁和670 nm叶绿素特征。在Pancam和Mastcam中均可观察到叶绿素光谱特征,我们建议在提出的EXOMARS Pancam滤光片中,PHYLL滤光片最适合于其检测。

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