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We find that early sea urchin embryos have the capability to induce programmed cell death, or apoptosis, in response to chemical and physical stress. Strongylocentrotus purpuratus embryos (fertilized, 4 cell, 16 cell, 64 cell, and early blastula) were exposed to known cytotoxins, in order to determine when apoptosis occurs naturally and in response to stress. Using cell permeability as an indicator of early stage apoptosis, caspase activation as a mid-stage indicator, and DNA fragmentation as a late stage indicator, we find that during the cleavage stage of embryogenesis apoptosis is almost completely absent. However, a statistically significant (p<0.001) rise in apoptosis in stressed embryos is evident around 24 h after fertilization, during the early blastula stage and shortly after hatching. Before this stage, exposed embryos show no statistically significant increases in apoptosis in comparison to the controls. This pattern of apoptosis in development is similar to that seen in lower vertebrate models in which stress-induced apoptosis occurs only around the mid-blastula transition. We conclude that apoptosis may be used to rid embryos of aberrant or damaged cells in early development, but this response is stage-dependant. Repair, rather than apoptosis, may be utilized during earlier stages, or alternatively, embryos exposed to such stressors may continue development with damaged cells and perhaps damaged DNA. Our continued studies will focus on these alternative hypotheses.  相似文献   
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Several interstellar molecules have been detected toward the highly perturbed B and G clouds associated with the supernova remnant IC 443 via their 3 mm transitions, including N2H+, SiO, SO, CN, HNC, and H13CO+. The (J, K) = (1, 1) and (2, 2) inversion lines of metastable ammonia have also been observed, as well as the J = 3-2 transition of HCO+ at 1.2 mm. Analysis of the (1, 1) and (2, 2) inversion lines of NH3 indicates minimum gas kinetic temperatures of TK = 70 K toward cloud B, and TK = 33 K in cloud G. Modeling of the J = 1-0 and J = 3-2 transitions of HCO+ implies densities greater than 10(5) cm-3 toward both positions. These data clearly show that hot and dense material is present in IC 443, and they suggest the presence of shocks in both regions. A careful analysis of the HCO+ lines indicates that the HCO+ abundance is at most enhanced by factors of a few over that found in cold, quiescent gas. This conclusion contradicts past claims of HCO+ abundance enhancements of several orders of magnitude in the perturbed regions. The N2H+ abundance was also found to be similar to that in cold gas, suggesting that there is no increase in ionization in the clouds. The abundances of SO and CS, as well as CN and NH3, do not appear to differ significantly from those found in cold dark clouds, although chemistry models predict sulfur-containing species to undergo high-temperature enhancements. SiO, however, is found to have an abundance in the perturbed gas 100 times larger than the upper limits observed in the dark cloud TMC 1, a result in agreement with high temperature chemistry models. In addition, the HNC/HCN ratio in both IC 443 B and G was found to be approximately 0.1--far from the ratio of 1 predicted by low-temperature ion-molecule chemistry, but similar to the values observed in clouds where elevated temperatures are present.  相似文献   
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Perennially ice-covered lakes are found in the McMurdo Dry Valleys of southern Victoria Land, Antarctica. In contrast to temperate lakes that have diurnal photic periods, antarctic (and arctic) lakes have a yearly photic period. An unusual feature of the antarctic lakes is the occurrence of O2 at supersaturated levels in certain portions of the water column. Here we report the first sediment O2 profiles obtained using a microelectrode from a perennially ice-covered antarctic lake. Sediment cores collected in January and October 1987 from Lake Hoare in Taylor Valley show oxygenation down to 15, and in some cases, 25 cm. The oxygenation of sediments several centimeters below the sediment-water interface is atypical for lake sediments and may be characteristic of perennially ice-covered lakes. There is a significant difference between the observed January and October sediment O2 profiles. Several explanations may account for the difference, including seasonality. A time-dependent model is presented which tests the feasibility of a seasonal cycle resulting from the long photoperiod and benthic primary production in sediments overlain by a highly oxygenated water column.  相似文献   
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地幔流体及其成矿作用   总被引:8,自引:0,他引:8  
高灵敏度、高精密度、低检出限、多元素同时检测并可提供同位素组成比值信息的等离子体质谱与高空间分辨率的紫外激光采样技术结合 ,可定量地测定单个流体包裹体中常、微量元素含量 ,为成矿流体的研究提供了一个新的研究手段。文中简要地介绍了激光剥蚀电感耦合等离子体质谱 (LA ICP MS)分析仪器的发展 ,结合实验室的研究工作 ,就激光剥蚀池的设计、单个流体包裹体的剥蚀方法、元素的分馏效率、定量校正技术及其在成矿成因物理化学机制研究中的应用等进行评述 ,并阐述单个流体包裹体元素组成的LA ICP MS分析技术存在的局限和发展趋势。  相似文献   
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牙形石作为划分地层的标准化石,具有确切的地层层位和较高的REE含量,并不容易受成岩作用的影响,因此作为研究古海水演化的指示剂引起人们的广泛关注.利用同位素稀释法对扬子克拉通三峡地区寒武纪一三叠纪海相碳酸盐岩中代表古海水化学组成牙形石的Sm/Nd比值进行测定,Sm/Nd比值在0.108-0.348之间,有较大的变化范围.建立Sm/Nd比值随时间的演化曲线,并结合已有沉积地层学和沉积地球化学的成果进行研究,结果表明,古海水Sm/Nd比值变化与海平面升降、古陆块的隆起有明显对应关系,同时,区域性构造运动,如海底地壳拉张产生的幔源组分和地幔柱活动也会影响古海水的Sm/Nd比值.因此,古海水的Sm/Nd比值对海平面的升降、古大陆的风化作用和区域构造事件有指示意义.  相似文献   
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