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1.
X-ray fluorescence spectra obtained by the MESSENGER spacecraft orbiting Mercury indicate that the planet's surface differs in composition from those of other terrestrial planets. Relatively high Mg/Si and low Al/Si and Ca/Si ratios rule out a lunarlike feldspar-rich crust. The sulfur abundance is at least 10 times higher than that of the silicate portion of Earth or the Moon, and this observation, together with a low surface Fe abundance, supports the view that Mercury formed from highly reduced precursor materials, perhaps akin to enstatite chondrite meteorites or anhydrous cometary dust particles. Low Fe and Ti abundances do not support the proposal that opaque oxides of these elements contribute substantially to Mercury's low and variable surface reflectance.  相似文献   

2.
The reflectance spectra of the most abundant meteorites, ordinary chondrites, are different from those of the abundant S-type (mnemonic for siliceous) asteroids. This discrepancy has been thought to be due to space weathering, which is an alteration of the surfaces of airless bodies exposed to the space environment. Here we report evidence of space weathering on particles returned from the S-type asteroid 25143 Itokawa by the Hayabusa spacecraft. Surface modification was found in 5 out of 10 particles, which varies depending on mineral species. Sulfur-bearing Fe-rich nanoparticles exist in a thin (5 to 15 nanometers) surface layer on olivine, low-Ca pyroxene, and plagioclase, which is suggestive of vapor deposition. Sulfur-free Fe-rich nanoparticles exist deeper inside (<60 nanometers) ferromagnesian silicates. Their texture suggests formation by metamictization and in situ reduction of Fe(2+).  相似文献   

3.
Site occupancy numbers for ferrous iron, magnesium, and calcium at the Ml and M2 sites in lunar clinopyroxenes are estimated from nuclear gamma-ray resonant absorption spectra of (57)Fe. The cation distribution is ordered; calcium and magnesium prefer M2 and Ml, respectively. The distribution corresponds to an equilibrium at a temperature lower than 680 degrees C. Crystals cleaved and sectioned by diamond-knife ultramicrotomy were examined by high-voltage (200 kv) electron microscopy and diffraction. Uniform 300-to 600-A-wide bands that correspond to single crystal domains were found. Correlation of the bands with magnetic ordering at low temperatures is considered.  相似文献   

4.
Molecular beam epitaxy has been used to grow microcrystalline clusters of gallium arsenide (GaAs) in the size range from 2.5 to 60 nanometers on high-purity, amorphous silica supports. High-resolution transmission electron microscopy reveals that clusters as small as 3.5 nanometers have good crystalline order with a lattice constant equal to that of bulk GaAs. Study of the microcrystallite surfaces by x-ray photoelectron spectroscopy shows that they are covered with a shell (1.0 to 1.5 nanometers thick) of native oxides of gallium and arsenic (Ga(2)O(3) and As(2)O(3)), whose presence could explain the low luminescence efficiency of the clusters. Optical absorption spectra of the supported GaAs are consistent with the blue-shifted band edge expected for semiconductor microcrystallites in the quantum size regime.  相似文献   

5.
硫酸亚铁诱导根表铁膜形成对水稻吸收和转运铜锌的影响   总被引:1,自引:0,他引:1  
通过水培条件下添加硫酸亚铁诱导水稻根表铁膜的形成,利用连二亚硫酸钠-柠檬酸钠-碳酸氢钠(DCB)溶液对根表铁膜进行提取后测定,采用扫描电镜-能谱仪(SEM-EDS)和X射线衍射仪(XRD)等手段对硫酸亚铁诱导产生的根表铁膜进行表征,并分析根表铁膜对水稻吸收铜锌的影响。结果表明,添加硫酸亚铁可以诱导根表铁膜在水稻根系表面产生,未处理的水稻根表Fe含量为731 mg·kg~(-1),80 mg·kg~(-1) Fe~(2+)处理下水稻根表Fe含量为53 562 mg·kg~(-1);SEM-EDS和XRD分析发现大量颗粒状含铁化合物附着于水稻根表。与未经硫酸亚铁处理相比,有根表铁膜水稻的铁膜中,其Cu含量最高增加73.16%,Zn含量最高增加112.10%;水稻根系Cu含量最高降低31.15%,Zn含量最高降低13.02%;水稻茎叶Cu含量最高降低19.50%,Zn含量最高降低25.56%。土壤添加硫酸亚铁可以显著降低水稻对Cu和Zn的吸收与积累。  相似文献   

6.
Occurrence of light saturation in the reaction of thionine (T) with Fe(2+) suggests the existence of T. Fe(2+) complexes practically indistinguishable by their absorption spectra from free thionine; photoreduction seems to occur by electron transfer in such complexes, delayed by more than 10(-5) second after light absorption. Both phenomena must be of general significance.  相似文献   

7.
A reflectance spectrum of Phobos (from 200 to 1100 nanometers) has been compiled from the Mariner 9 ultraviolet spectrometer, Viking lander imaging, and ground-based photometric data. The reflectance of the martian satellite is approximately constant at 5 percent from 1100 to 400 nanometers but drops sharply below 400 nanometers, reaching a value of 1 percent at 200 nanometers. The spectral albedo of Phobos bears a striking resemblance to that of asteroids (1) Ceres and (2) Pallas. Comparison of the reflectance spectra of asteroids with those of meteorites has shown that the spectral signature of Ceres is indicative of a carbonaceous chondritic composition. A physical explanation of how the compositional information is imposed on the reflectance spectrum is given. On the basis of a good match between the reflectance spectra of Phobos and Ceres and the extensive research that has been done to infer the composition of Ceres, it seems reasonable to believe that the surface composition of Phobos is similar to that of carbonaceous chondrites. This suggestion is consistent with the recently determined low density of Mars's inner satellite. Our result and recent Viking noble gas measurements suggest different modes of origin for Mars and Phobos.  相似文献   

8.
Femtosecond time-resolved infrared spectroscopy was used to study the formation of cyclobutane dimers in the all-thymine oligodeoxynucleotide (dT)18 by ultraviolet light at 272 nanometers. The appearance of marker bands in the time-resolved spectra indicates that the dimers are fully formed approximately 1 picosecond after ultraviolet excitation. The ultrafast appearance of this mutagenic photolesion points to an excited-state reaction that is approximately barrierless for bases that are properly oriented at the instant of light absorption. The low quantum yield of this photoreaction is proposed to result from infrequent conformational states in the unexcited polymer, revealing a strong link between conformation before light absorption and photodamage.  相似文献   

9.
Low-field magnetic separation of monodisperse Fe3O4 nanocrystals   总被引:1,自引:0,他引:1  
Magnetic separations at very low magnetic field gradients (<100 tesla per meter) can now be applied to diverse problems, such as point-of-use water purification and the simultaneous separation of complex mixtures. High-surface area and monodisperse magnetite (Fe3O4) nanocrystals (NCs) were shown to respond to low fields in a size-dependent fashion. The particles apparently do not act independently in the separation but rather reversibly aggregate through the resulting high-field gradients present at their surfaces. Using the high specific surface area of Fe3O4 NCs that were 12 nanometers in diameter, we reduced the mass of waste associated with arsenic removal from water by orders of magnitude. Additionally, the size dependence of magnetic separation permitted mixtures of 4- and 12-nanometer-sized Fe3O4 NCs to be separated by the application of different magnetic fields.  相似文献   

10.
Compressibilities of five silicate spinels, including gamma-Mg(2)SiO(4), gamma-Fe(2)SiO(4), Ni(2)SiO(4) and two ferromagnesian compositions, were determined on crystals positioned in the same high-pressure mount. Subjection of all crystals simultaneously to the same pressure revealed differences in compressibility that resulted from compositional differences. Ferromagnesian silicate spinels showed an anomalous 13 percent increase in bulk modulus with increasing iron content, from Mg(2)SiO(4) (184 gigapascals) to Fe(2)SiO(4) (207 gigapascals). This result suggests that ferrous iron and magnesium, which behave similarly under crustal conditions, are chemically more distinct at high pressures characteristic of the transition zone and lower mantle.  相似文献   

11.
The reflection spectrum for the integral disk of the planet Mercury was measured and was found to have a constant positive slope from 0.32 to 1.05 micrometers, except for absorption features in the infrared. The reflectivity curve matches closely the curve for the lunar upland and mare regions. Thus, the surface of Mercury is probably covered with a lunar-like soil rich in dark glasses of high iron and titanium content. Pyroxene is probably the dominant mafic mineral.  相似文献   

12.
Femtosecond optical measurement techniques have been used to study the primary photoprocesses in the light-driven transmembrane proton pump bacteriorhodopsin. Light-adapted bacteriorhodopsin was excited with a 60-femtosecond pump pulse at 618 nanometers, and the transient absorption spectra from 560 to 710 nanometers were recorded from -50 to 1000 femtoseconds by means of 6-femtosecond probe pulses. By 60 femtoseconds, a broad transient hole appeared in the absorption spectrum whose amplitude remained constant for about 200 femtoseconds. Stimulated emission in the 660- to 710-nanometer region and excited-state absorption in the 560- to 580-nanometer region appeared promptly and then shifted and decayed from 0 to approximately 150 femtoseconds. These spectral features provide a direct observation of the 13-trans to 13-cis torsional isomerization of the retinal chromophore on the excited-state potential surface. Absorption due to the primary ground-state photoproduct J appears with a time constant of approximately 500 femtoseconds.  相似文献   

13.
Optical absorption spectra have been measured at pressures up to 80 gigapascals (GPa) for the lower-mantle oxide magnesiowüstite (Mg,Fe)O. Upon reaching the high-spin to low-spin transition of Fe2+ at about 60 GPa, we observed enhanced absorption in the mid- and near-infrared spectral range, whereas absorption in the visible-ultraviolet was reduced. The observed changes in absorption are in contrast to prediction and are attributed to d-d orbital charge transfer in the Fe2+ ion. The results indicate that low-spin (Mg,Fe)O will exhibit lower radiative thermal conductivity than high-spin (Mg,Fe)O, which needs to be considered in future geodynamic models of convection and plume stabilization in the lower mantle.  相似文献   

14.
The absorption properties, expressed as a wavelength-dependent imaginary index of refraction, of the Mount St. Helens ash from the 18 May 1980 eruption were measured between 300 and 700 nanometers by diffuse reflectance techniques. The measurements were made for both surface and stratospheric samples. The stratospheric samples show imaginary index values that decrease from approximately 0.01 to 0.02 at 300 nanometers to about 0.0015 at 700 nanometers. The surface samples show less wavelength variation in imaginary refractive index over this spectral range.  相似文献   

15.
【目的】为解决碱性土壤上桑树缺铁黄化问题提供理论依据。【方法】以桑树品种特优2号为试验材料,通过盆栽试验研究施用鸡粪有机肥、硫磺、木质素铁肥对碱性土壤pH值、铁活性及桑树生长、铁素营养的影响。【结果】施用0.670 g/kg硫磺后能明显降低土壤pH值,比对照降低约2个单位。单施硫磺(S2)和硫磺与有机肥混施(S+OF)对桑树生长有明显的促进作用,叶片和茎总重分别比对照增加28.7%和35.9%。施用硫磺(S2)、硫磺与有机肥混施(S+OF)及铁肥与有机肥混施(Fe+OF)均能提高桑树叶片中的活性铁含量。【结论】在碱性土壤中施用硫磺和有机肥能降低土壤pH值,提高土壤中活性铁的含量,促进桑树植株生长,可以作为改善和防治广西地区桑树缺铁黄化的一种较为可行的措施。  相似文献   

16.
【目的】为解决碱性土壤上桑树缺铁黄化问题提供理论依据。【方法】以桑树品种特优2号为试验材料,通过盆栽试验研究施用鸡粪有机肥、硫磺、木质素铁肥对碱性土壤pH值、铁活性及桑树生长、铁素营养的影响。【结果】施用0.670g/kg硫磺后能明显降低土壤pH值,比对照降低约2个单位。单施硫磺(S2)和硫磺与有机肥混施(S+OF)对桑树生长有明显的促进作用,叶片和茎总重分别比对照增加28.7%和35.9%。施用硫磺(S2)、硫磺与有机肥混施(S+OF)及铁肥与有机肥混施(Fe+OF)均能提高桑树叶片中的活性铁含量。【结论】在碱性土壤中施用硫磺和有机肥能降低土壤pH值,提高土壤中活性铁的含量,促进桑树植株生长,可以作为改善和防治广西地区桑树缺铁黄化的一种较为可行的措施。  相似文献   

17.
Reflectance spectra (0.3 to 2.6 micrometers) of 14 C, G, B, and F asteroids and 21 carbonaceous chondrite powders are compared in detail. Only three thermally metamorphosed CM-Cl chondrites that have a weak ultraviolet absorption are shown to have close counterparts among those asteroids. Reflectance spectra of heated Murchison CM2 chondrite are compared with the average C and G type asteroid spectra. Murchison heated at 600 degrees to 1000 degrees C exhibits a similar weak ultraviolet absorption and provides the best analog for those spectra. Comparison of ultraviolet absorption strengths between 160 C, G, B, and F asteroids and carbonaceous chondrites suggests that surface minerals of most of those asteroids are thermally metamorphosed at temperatures around 600 degrees to 1000 degrees C.  相似文献   

18.
打孔塞入法治疗果树缺铁黄叶病   总被引:1,自引:0,他引:1  
为了经济、安全、高效地治疗果树因缺铁而引发的黄叶病,克服目前土壤和叶面施铁疗效差,树干注射复绿剂受季节限制、安全性差、操作复杂的缺陷,选用4类8种含Fe化合物(易溶性二价无机铁盐FeSO4.7H2O和FeCl2.4H2O,易溶性三价无机铁盐Fe2(SO4)3和FeCl3.6H2O,难溶性Fe2O3和FeC2O4,铁络合物Fe(NH4)2(SO4)2.6H2O和FeC6O7H6),在树干上打孔后将其塞入。结果表明,多种含铁化合物都能使果树缺铁黄化病在第6至第7天开始复绿,20d后使已经白化的叶片也能彻底恢复绿色,其中Fe(NH4)2(SO4)2.6H2O最为经济、安全、高效,FeSO4.7H2O次之。  相似文献   

19.
Recrystallization of the solid Cd(10)S(4)(SC(6)H(5))(12) from a solution of pyridine and N, N-di-methylformamide (DMF) results in the formation of the cluster Cd(32)S(14)(SC(6)H(5))(36)-DMF(4) as pale yellow cubes. The structure consists of an 82-atom CdS core that is a roughly spherical piece of the cubic sphalerite lattice approximately 12 angstroms in diameter. The four corners of the lattice are capped by hexagonal wurtzite-like CdS units, which results in an overall tetrahedral cluster approximately 15 angstroms in diameter. This cluster dissolves intact in tetrahydrofuran where its absorption spectrum reveals a sharp peak at 358 nanometers at room temperature and its emission spectra show a strong broad band at 500 nanometers.  相似文献   

20.
The reaction of [Cp*Fe(eta5-P5)] with Cu(I)Cl in solvent mixtures of CH2Cl2/CH3CN leads to the formation of entirely inorganic fullerene-like molecules of the formula [[Cp*Fe(eta5:eta1:eta1:eta1:eta1:eta1-P5)]12[CuCl]10[Cu2Cl3]5[Cu(CH3CN)2]5] (1) possessing 90 inorganic core atoms. This compound represents a structural motif similar to that of C60: cyclo-P5 rings of [Cp*Fe(eta5-P5)] molecules are surrounded by six-membered P4Cu2 rings that result from the coordination of each of the phosphorus lone pairs to CuCl metal centers, which are further coordinated by P atoms of other cyclo-P5 rings. Thus, five- and six-membered rings alternate in a manner comparable to that observed in the fullerene molecules. The so-formed half shells are joined by [Cu2Cl3]- as well as by [Cu(CH3CN)2]+ units. The spherical body has an inside diameter of 1.25 nanometers and an outside diameter of 2.13 nanometers, which is about three times as large as that of C60.  相似文献   

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