Use of suppressive subtractive hybridization and cDNA arrays to discover patterns of altered gene expression in the liver of dihydrotestosterone and 11-ketotestosterone exposed adult male largemouth bass (Micropterus salmoides)     

Blum JL  Knoebl I  Larkin P  Kroll KJ  Denslow ND 《Marine environmental research》2004,58(2-5):565-569

In this study male largemouth bass (LMB) were exposed to the naturally occurring androgens, dihydrotestosterone (DHT) or 11-ketotestosterone (11-KT) in order to identify genes that are differentially regulated by these steroid hormones. Using subtractive hybridization on livers of fish treated with DHT against vehicle control, many novel LMB genes were cloned. These genes were added to our gene library and arrayed. Six genes were up-regulated and five were down-regulated by both androgens. But, each androgen also regulated specific genes. One gene that was identified as a potential androgen marker was spermidine-spermine-N(1)-acetyltransferase that was up-regulated by both androgens. Determining which genes are responsive to natural androgens will help to identify biochemical pathways that are impacted.  相似文献   

Polycyclic aromatic hydrocarbons (PAHs) in Antarctic Martian meteorites, carbonaceous chondrites, and polar ice     

Becker L  Glavin DP  Bada JL 《Geochimica et cosmochimica acta》1997,61(2):475-481

Recent analyses of the carbonate globules present in the Martian meteorite ALH84001 have detected polycyclic aromatic hydrocarbons (PAHs) at the ppm level (McKay et al., 1996). The distribution of PAHs observed in ALH84001 was interpreted as being inconsistent with a terrestrial origin and were claimed to be indigenous to the meteorite, perhaps derived from an ancient martian biota. We have examined PAHs in the Antarctic shergottite EETA79001, which is also considered to be from Mars, as well as several Antarctic carbonaceous chondrites. We have found that many of the same PAHs detected in the ALH84001 carbonate globules are present in Antarctic carbonaceous chondrites and in both the matrix and carbonate (druse) component of EETA79001. We also investigated PAHs in polar ice and found that carbonate is an effective scavenger of PAHs in ice meltwater. Moreover, the distribution of PAHs in the carbonate extract of Antarctic Allan Hills ice is remarkably similar to that found in both EETA79001 and ALH84001. The reported presence of L-amino acids of apparent terrestrial origin in the EETA79001 druse material (McDonald and Bada, 1995) suggests that this meteorite is contaminated with terrestrial organics probably derived from Antarctic ice meltwater that had percolated through the meteorite. Our data suggests that the PAHs observed in both ALH84001 and EETA79001 are derived from either the exogenous delivery of organics to Mars or extraterrestrial and terrestrial PAHs present in the ice meltwater or, more likely, from a mixture of these sources. It would appear that PAHs are not useful biomarkers in the search for extinct or extant life on Mars.  相似文献   

A search for endogenous amino acids in the Martian meteorite EETA79001     

McDonald GD  Bada JL 《Geochimica et cosmochimica acta》1995,59(6):1179-1184

The Antarctic shergottite EETA79001 is believed to be an impact-ejected fragment of the planet Mars. Samples of the carbonate (white druse) and the basaltic (lithology A) components from this meteorite have been found to contain amino acids at a level of approximately 1 ppm and 0.4 ppm, respectively. The detected amino acids consist almost exclusively of the L-enantiomers of the amino acids commonly found in proteins, and are thus terrestrial contaminants. There is no indication of the presence of alpha-aminoisobutyric acid, one of the most abundant amino acids in several carbonaceous chondrites. The relative abundances of amino acids in the druse material resemble those in Antarctic ice, suggesting that the source of the amino acids may be ice meltwater. The level of amino acids in EETA79001 druse is not by itself sufficient to account for the 600-700 ppm of volatile C reported in druse samples and suggested to be from endogenous martian organic material. However, estimates of total terrestrial organic C present in the druse material based on our amino acid analyses and the organic C content of polar ice can account for most of the reported putative organic C in EETA79001 druse.  相似文献   

水压致裂应力测量中破裂重张压的运用     

Rati.  JL 王建军 《地壳构造与地壳应力》1993,(3):25-30

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纵弯压扁褶皱的应变估算     

Rich.  JL 樊光明 《地质科学译丛》1993,10(1):39-40

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科学家们对玻利维亚深震机制取得了进一步的认识     

Wake.  JL 范国胜 《地壳构造与地壳应力》1995,(3):5-7

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弱区域变形期间定位的花岗质岩体的构造特征：...   总被引：1，自引：0，他引：1  

Laga.  JL 牛树银 《国外花岗岩类地质与矿产》1991,(3):12-20

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土壤表面比湿的估计     

Tsen.  JL 陈忠明 《贵州气象》1994,18(1):23-27

要基于最近的实验结果，提出了一个用于数值天气─—气候模式中估计土壤表面湿度的公式。该公式具有十分简洁的形式，且在干、湿土壤状态之间展示出土壤表面比湿的平滑过渡．建议用该公式取代Philip公式。  相似文献   

在海水条件下栽培的喜盐作物     

加拉.  JL 郗金标 《地理译报》1994,13(1):44-48

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The case for planetary sample return missions. 2. History of Mars     

Gooding JL  Carr MH  McKay CP 《Eos》1989,70(31):745, 54-745, 55

Principal science goals for exploration of Mars are to establish the chemical, isotopic, and physical state of Martian material, the nature of major surface-forming processes and their time scales, and the past and present biological potential of the planet. Many of those goals can only be met by detailed analyses of atmospheric gases and carefully selected samples of fresh rocks, weathered rocks, soils, sediments, and ices. The high-fidelity mineral separations, complex chemical treatments, and ultrasensitive instrument systems required for key measurements, as well as the need to adapt analytical strategies to unanticipated results, point to Earth-based laboratory analyses on returned Martian samples as the best means for meeting the stated objectives.  相似文献