1 Dipartimento di Scienze Biologiche, Geologiche e Ambientali, Università di Bologna, Bologna, Italy.
2 Department of Geology, University of Johannesburg, Johannesburg, South Africa.
Astrobiology. 2019 Apr;19(4):553-578. doi: 10.1089/ast.2018.1926. Epub 2019 Jan 17.
The Dallol volcano and its associated hydrothermal field are located in a remote area of the northern Danakil Depression in Ethiopia, a region only recently appraised after decades of inaccessibility due to severe political instability and the absence of infrastructure. The region is notable for hosting environments at the very edge of natural physical-chemical extremities. It is surrounded by a wide, hyperarid salt plain and is one of the hottest (average annual temperature: 36-38°C) and most acidic natural systems (pH ≈0) on Earth. Spectacular geomorphologies and mineral deposits produced by supersaturated hydrothermal waters and brines are the result of complex interactions between active and inactive hydrothermal alteration of the bedrock, sulfuric hot springs and pools, fumaroles and geysers, and recrystallization processes driven by hydrothermal waters, degassing, and rapid evaporation. The study of planetary field analog environments plays a crucial role in characterizing the physical and chemical boundaries within which life can exist on Earth and other planets. It is essential for the definition and assessment of the conditions of habitability on other planets, including the possibility for biosignature preservation and in situ testing of technologies for life detection. The Dallol area represents an excellent Mars analog environment given that the active volcanic environment, the associated diffuse hydrothermalism and hydrothermal alteration, and the vast acidic sulfate deposits are reminiscent of past hydrothermal activity on Mars. The work presented in this paper is an overview of the Dallol volcanic area and its hydrothermal field that integrates previous literature with observations and results obtained from field surveys and monitoring coupled with sample characterization. In so doing, we highlight its exceptional potential as a planetary field analog as well as a site for future astrobiological and exploration programs.
多勒尔火山及其相关的热液场位于埃塞俄比亚北部丹纳基尔洼地的偏远地区,由于数十年的政治不稳定和基础设施的缺乏,该地区一直难以进入,直到最近才被评估。该地区以拥有处于自然物理化学极限边缘的环境而闻名。它被一个宽阔的、极度干旱的盐平原环绕,是地球上最热(年平均温度:36-38°C)和最酸(pH ≈0)的自然系统之一。由过饱和热液水和卤水产生的壮观地貌和矿床是基岩、硫酸温泉和池塘、喷气孔和间歇泉的活跃和不活跃热液蚀变、水热蚀变、脱气和快速蒸发驱动的再结晶过程之间复杂相互作用的结果。对行星场类似环境的研究在确定地球上和其他行星上生命可能存在的物理和化学界限方面起着至关重要的作用。这对于定义和评估其他行星上的可居住性条件至关重要,包括生物特征保存和现场检测生命探测技术的可能性。多勒尔地区是一个极好的火星类似环境,因为活跃的火山环境、相关的弥散热液作用和热液蚀变以及大量的酸性硫酸盐矿床让人联想到火星上过去的热液活动。本文介绍了多勒尔火山地区及其热液场的综合概述,该综述综合了以前的文献以及实地调查和监测结合样本特征描述所获得的观测和结果。通过这样做,我们强调了它作为行星场类似物以及未来天体生物学和探测计划的理想场所的特殊潜力。