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61.
Abstract Life Investigation For Enceladus (LIFE) presents a low-cost sample return mission to Enceladus, a body with high astrobiological potential. There is ample evidence that liquid water exists under ice coverage in the form of active geysers in the "tiger stripes" area of the southern Enceladus hemisphere. This active plume consists of gas and ice particles and enables the sampling of fresh materials from the interior that may originate from a liquid water source. The particles consist mostly of water ice and are 1-10?μ in diameter. The plume composition shows H(2)O, CO(2), CH(4), NH(3), Ar, and evidence that more complex organic species might be present. Since life on Earth exists whenever liquid water, organics, and energy coexist, understanding the chemical components of the emanating ice particles could indicate whether life is potentially present on Enceladus. The icy worlds of the outer planets are testing grounds for some of the theories for the origin of life on Earth. The LIFE mission concept is envisioned in two parts: first, to orbit Saturn (in order to achieve lower sampling speeds, approaching 2 km/s, and thus enable a softer sample collection impact than Stardust, and to make possible multiple flybys of Enceladus); second, to sample Enceladus' plume, the E ring of Saturn, and the Titan upper atmosphere. With new findings from these samples, NASA could provide detailed chemical and isotopic and, potentially, biological compositional context of the plume. Since the duration of the Enceladus plume is unpredictable, it is imperative that these samples are captured at the earliest flight opportunity. If LIFE is launched before 2019, it could take advantage of a Jupiter gravity assist, which would thus reduce mission lifetimes and launch vehicle costs. The LIFE concept offers science returns comparable to those of a Flagship mission but at the measurably lower sample return costs of a Discovery-class mission. Key Words: Astrobiology-Habitability-Enceladus-Biosignatures. Astrobiology 12, 730-742.  相似文献   
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The delivery of extraterrestrial organic materials to primitive Earth from meteorites or micrometeorites has long been postulated to be one of the origins of the prebiotic molecules involved in the subsequent apparition of life. Here, we report on experiments in which vacuum UV photo-irradiation of interstellar/circumstellar ice analogues containing H(2)O, CH(3)OH, and NH(3) led to the production of several molecules of prebiotic interest. These were recovered at room temperature in the semi-refractory, water-soluble residues after evaporation of the ice. In particular, we detected small quantities of hydantoin (2,4-imidazolidinedione), a species suspected to play an important role in the formation of poly- and oligopeptides. In addition, hydantoin is known to form under extraterrestrial, abiotic conditions, since it has been detected, along with various other derivatives, in the soluble part of organic matter of primitive carbonaceous meteorites. This result, together with other related experiments reported recently, points to the potential importance of the photochemistry of interstellar "dirty" ices in the formation of organics in Solar System materials. Such molecules could then have been delivered to the surface of primitive Earth, as well as other telluric (exo-) planets, to help trigger first prebiotic reactions with the capacity to lead to some form of primitive biomolecular activity.  相似文献   
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INTRODUCTIONIn general,nitrogen launching system[1,2 ] iscomprised of nitrogen cylinder,launching mecha-nism,framework and electrical system,withcompressed Nitrogen as launching energy re-sources.A physical and mathematical model isdeveloped for describing the relations betweenthe detached time and the force,volume,pres-sure,flow,displacement,velocity,acceleration ofnitrogen cylinder and launching mechanism.Thekey technique of NL S is to control detached pa-rameters by changing the press…  相似文献   
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The European Space Agency's ExoMars mission will seek evidence of organic compounds of biological and non-biological origin at the martian surface. One of the instruments in the Pasteur payload may be a Life Marker Chip that utilizes an immunoassay approach to detect specific organic molecules or classes of molecules. Therefore, it is necessary to define and prioritize specific molecular targets for antibody development. Target compounds have been selected to represent meteoritic input, fossil organic matter, extant (living, recently dead) organic matter, and contamination. Once organic molecules are detected on Mars, further information is likely to derive from the detailed distribution of compounds rather than from single molecular identification. This will include concentration gradients beneath the surface and gradients from generic to specific compounds. The choice of biomarkers is informed by terrestrial biology but is wide ranging, and nonterrestrial biology may be evident from unexpected molecular distributions. One of the most important requirements is to sample where irradiation and oxidation are minimized, either by drilling or by using naturally excavated exposures. Analyzing regolith samples will allow for the search of both extant and fossil biomarkers, but sequential extraction would be required to optimize the analysis of each of these in turn.  相似文献   
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介绍在计算机集成信息系统中(CIIS),利用三坐标测量机测量叶片、自适应生成型线图的方法,包括曲线类型、曲线段数、分段点和曲线参数的自适应选择,通过试用对文中提出的方法进行了验证评价.关键词  相似文献   
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日渐明显的是,许多特异意识状态(ASC)和相关问题可以进入科学探索的领域.许多这些主观的状态或现象原先被归类为本质上是宗教的或神秘主义的,因而作为非客观的、非物理性的或不属于普遍的观察而被排除于科学研究之外.这种态度正在改变.首先是因为主观——客观二分法的困境证明了意识的重要性;其次是因为技术的发展使得发现主观状态的生理相关性成为可能——例如,现在可以通过快速眼动和脑电图记录探查和监督做梦.作为这些进展的结果,先前的这些神秘主义主题正转向科学证实和探索的领域.  相似文献   
69.
用甲基丙烯酸甲脂聚合物砼(MMA-PC)修补接缝尚存在许多问题,因此要系统分析MMA-PC的化学性能。介绍了用MMA-PC修补接缝的改进方法,而且反修率极低。  相似文献   
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本文研究脉冲发动机在战术导弹,特别是空空导弹上的应用.因为其飞行任务要求对能量消耗作仔细地监控.一般的中程空空导弹使用助推-主发动机作为动力.除了接近交会之外,发射时导弹雷达导引头并不知道目标.一般的中程空空导弹使用比例导航或者在终段制导使用改进的比例导航,同时为了使导弹在较高的高度飞行以减小阻力,在中段附加了预编程的  相似文献   
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