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Access to glacial and subglacial environments in the Solar System by melting probe technology

机译:通过融化探针技术进入太阳系中的冰川和冰川下环境

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A key aspect for understanding the biological and biochemical environment of subglacial waters,on Earth or other planets and moons in the Solar system,is the analysis of material embedded in or underneath icy layers on the surface. In particular the Antarctic lakes (most prominently Lake Vostok) but also the icy crust of Jupiter's moon Europa or the polar caps of Mars require such investigation. One possible technique to penetrate thick ice layers with small and reliable probes is by melting,which does not require the heavy,complex and expensive equipment of a drilling rig. While melting probes have successfully been used for terrestrial applications e.g. in Antarctic ice,their performance in vacuum is different and theory needs confirmation by tests. Thus,a vacuum chamber has been used to perform a series of melting tests in cold (liquid nitrogen cooled) water ice samples. The feasibility of the method was demonstrated and the energy demand for a space mission could be estimated. Due to the high energy demand in case of extraterrestrial application (e.g. Europa or polar caps of Mars),only heating with radioactive isotopes seems feasible for reaching greater depths. The necessary power is driven by the desired penetration velocity (approximately linearly) and the dimensions of the probe (proportional to the cross section). In comparison to traditional drilling techniques the application of a melting probe for exploration of Antarctic lakes offers the advantage that biological contamination is minimized,since the Probe can be sterilized and the melting channel freezes immediately after the probe's passage,inhibiting exchange with the surface layers and the atmosphere. In order to understand the physical and chemical nature of the ice layers,as well as for analysing the underlying water body,a melting probe needs to be equipped with a suite of scientific instruments that are capable of e.g. determining the chemical and isotopic composition of the embedded or dissolved materials.
机译:理解地球上或太阳系中其他行星和卫星上冰川下水域生物和生化环境的一个关键方面是对埋在地表冰层中或之下的物质的分析。特别是南极湖泊(最显着的是沃斯托克湖),但木星的月球欧罗巴结冰的外壳或火星的极地盖帽也需要进行此类调查。用小而可靠的探针穿透厚冰层的一种可能技术是融化,它不需要钻机的笨重,复杂和昂贵的设备。虽然熔解探针已经成功地用于地面应用,例如。在南极冰中,它们在真空中的性能是不同的,理论需要通过试验来证实。因此,已经使用真空室对冷(液氮冷却)水冰样品进行一系列融化测试。证明了该方法的可行性,并可以估算出太空任务的能源需求。由于在外星应用(例如欧罗巴或火星的极地帽)中对能量的需求很高,因此只有用放射性同位素进行加热才能达到更大的深度。所需功率由所需的穿透速度(近似线性)和探针的尺寸(与横截面成比例)驱动。与传统的钻井技术相比,在南极湖泊勘探中使用融化探针的优势在于可将生物污染降至最低,因为可以对探针进行灭菌,融化通道在探针通过后立即冻结,从而抑制了与表层和表面层的交换。气氛。为了了解冰层的物理和化学性质,以及分析下层水体,融化探针需要配备一套科学仪器,例如确定包埋或溶解物质的化学和同位素组成。

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