Interpretation of discordant ⁴⁰Ar/³⁹Ar age-spectra of mesozoic tholeiites from antarctica     

Robert J Fleck  John F Sutter  David H Elliot 《Geochimica et cosmochimica acta》1977,41(1):15-32

Conventional K-Ar ages of tholeiitic basalts of the Ferrar Group in the central Transantarctic Mountains indicate significant loss of radiogenic ⁴⁰Ar from this unit over much of its outcrop area. Argon loss varies inversely with amount of devitrified matrix in the basalts, which have not been thermally or tectonically disturbed since extrusion. ⁴⁰Ar/¹⁹Ar age-spectra of these tholeiites are generally discordant and indicate significant inhomogeneity in the distribution of radiogenic ⁴⁰Ar with respect to ³⁹Ar, but are distinctly different from release patterns of thermally disturbed samples. Amounts of argon redistribution vary directly with amounts of devitrification and are reflected in progressive modification of the age spectra. A model of redistribution of radiogenic ⁴⁰Ar by devitrification of originally glassy matrix is suggested that is consistent with disturbance of the conventional K-Ar systematics as well as the ⁴⁰Ar/³⁹Ar age-spectra. Samples with substantial redistribution but minor loss of radiogenic argon yield age spectra whose apparent ages decrease from low-temperature to high-temperature steps, similar to those reported for some lunar basalts, breccias, and soils. Modification of all the age spectra is attributed to redistribution of radiogenic ⁴⁰Ar during progressive devitrification, although ³⁹Ar-recoil effects suggested by Turner and Cadogan (1974) may be a factor in some cases. Where devitrification involves most potassium sites within the basalt, ⁴⁰Ar/³⁹Ar age-plateaux may be formed that have no geologic significance.  相似文献   

Isotopic and chemical constraints on the crustal evolution and source signature of Ferrar magmas,north Victoria Land,Antarctica     

Thomas H. Fleming  Kenneth A. Foland  David H. Elliot 《Contributions to Mineralogy and Petrology》1995,121(3):217-236

Isotopic (Nd and Sr) and chemical compositions of the 177 Ma Kirkpatrick Basalt and Ferrar Dolerite from north Victoria Land, Antarctica, are examined in order to address the role of crustal assimilation and the characteristics of their mantle source. Results for the Scarab Peak chemical type (SPCT) that constitutes the flow unit capping the lava sequence [Mg-number, Mg/(Mg+Fe⁺²)=24, MgO=2.4%, SiO₂=57.1%, initial⁸⁷Sr/⁸⁶Sr=0.7087–0.7097, (ε_Nd=−4.3) conform previous reports that attribute variations in the concentrations of the more mobile elements and calculated initial⁸⁷Sr/⁸⁶Sr to mid-Cretaceous alteration and elevated δ¹⁸O to low-temperature interaction with meteoric water. The underlying lavas and the sills that are of the Mt. Fazio chemical type (MFCT) display a much wider range of both chemical and isotopic compositions (Mg-number=40–65, MgO=3.7 7.5%; SiO₂=52.6–58.3%, initial⁸⁷Sr/⁸⁶Sr=0.7087–0.7117, ε_Nd=−5.6 to −4.8). The effects of rock alteration on apparent initial⁸⁷Sr/⁸⁶Sr are demonstrated by large differences between the initial ratio of mineral separates or leached fractions and whole rocks. Cretaceous alteration produced Rb and Sr redistribution within the lava sequence that results in erroneous calculated initial⁸⁷Sr/⁸⁶Sr ratios. These effects are responsible for the large initial⁸⁷Sr/⁸⁶Sr variations previousl7 proposed which, combined with the large range in whole-rock δ¹⁸O, were purported to show very large degrees of crustal assimilation. The variations in ε_Nd are restricted and indicate much smaller degrees of assimilation. The least altered of the MFCT rocks show good chemical and isotopic correlations that can be integrated into a model involving fractionation of pyroxene and plagioclase coupled with assimilation of material similar to early Paleozoic basement. The lower⁸⁷Sr/⁸⁶Sr and higher ε_Nd of the SPCT suggest that they were derived by extensive fractionation of a more primitive, less contaminated, precursor of the MFCT. The most isotopically primitive Ferrar rocks from the region still have a high initial⁸⁷Sr/⁸⁶Sr and low initial¹⁴³Nd/¹⁴⁴Nd; this may reflect either earlier assimilation or an enriched source. The chemical and isotopic similarities, as well as the close geographic correspondence of the Ferrar Group to granitoids produced during the early Paleozoic Ross Orogeny suggest that in either case Ross-type material may have been involved in the development of the enriched isotopic signature. Editorial responsibility: I. Parsons  相似文献   

Six-color photometry of lapetus,Titan, Rhea,Dione and Tethys     

M. Noland  J. Veverka  D. Morrison  D.P. Cruikshank  A.R. Lazarewicz  N.D. Morrison  J.L. Elliot  J. Goguen  J.A. Burns 《Icarus》1974,23(3):334-354

Six-color photometric observations made during Saturn's 1972/73 opposition enable us to separate the solar phase and orbital phase contributions to the observed light variations of Iapetus, Titan, Rhea, Dione and Tethys. Titan shows no orbital variations, but has phase coefficients which range from negligible values in the infrared to 0.014mag/deg in the ultraviolet. Rhea has a bright leading side, a light curve amplitude of about 0.2mag, which increases toward short wavelengths, and surprisingly large phase coefficients, which increase from 0.025mag/deg in the red to 0.037mag/deg in the ultraviolet. Combined with other available information, this behavior suggests a very porous, texturally complex surface layer. Dione also has a leading side which is a few tenths of a magnitude brighter than the trailing side, but the light curve amplitude has little wavelength dependence and the phase coefficients are significantly smaller than those of Rhea, suggesting a less intricate surface texture. The leading side of Tethys is probably a few tenths of a magnitude brighter than the trailing side. Our Iapetus observations generally supplement the earlier work by Millis. The phase coefficients of the bright (trailing) side are typically ～0.03mag/deg and are not strongly wavelength dependent; the dark (leading) side coefficients are large (～0.05 mag/deg) and increase at shorter wavelengths, indicating a very porous and intricate surface texture. The light curve amplitude shows a slight increase at shorter wavelengths, suggesting an increasing contrast between the dark and bright materials. The spectral reflectance curves we derive for the satellites are in agreement with the spectrophotometry of McCord, Johnson, and Elias.  相似文献   

Chemical and isotopic variations in an iron-rich lava flow from the Kirkpatrick Basalt,north Victoria Land,Antarctica: implications for low-temperature alteration   总被引：4，自引：0，他引：4  

Thomas H. Fleming  David H. Elliot  Lois M. Jones  John R. Bowman  Mary A. Siders 《Contributions to Mineralogy and Petrology》1992,111(4):440-457

Chemical and isotopic (Sr, O, H) variations have been examined in an iron-rich lava flow of the Kirkpatrick Basalt from the Mesa Range in north Victoria Land, Antarctica. The flow is homogeneous with respect to the less mobile elements, whereas variations observed in K, Na, Si, Fe, and Rb result largely from alteration of glassy matrix material. Whole-rock Rb–Sr isotope data fall along a poorly-defined 103 Ma array attributed to secondary mobilization of Rb during the mid-Cretaceous. Alteration at that time is suggested by paleomagnetic data and would also account for discordant K–Ar dates. Whole-rock ¹⁸O values vary from +5.8 to +8.2 and a plagioclase separate has a ¹⁸O value of +5.6, reflecting the original composition of the magma. The range of ¹⁸O values for the whole-rock samples results from low-temperature alteration occurring primarily in the Jurassic and/or mid-Cretaceous. Whole-rock D values (-201 to -243) are markedly depleted, approaching equilibrium with modern meteoric water. In light of these data, variable Sr and O isotopic ratios in the underlying sequence of flows, previously interpreted in terms of an assimilation-fractionation model, may largely reflect post-magmatic alteration.  相似文献   

Location of Viking 1 Lander on the surface of Mars     

Elliot C. Morris  Kenneth L. Jones  Jan P. Berger 《Icarus》1978,34(3):548-555

A location of the Viking 1 Lander on the surface of Mars has been determined by correlating topographic features in the lander pictures with similar features in the Viking orbiter pictures. Radio tracking data narrowed the area of search for correlating orbiter and lander features and an area was found on the orbiter pictures in which there is good agreement with topographic features on the lander pictures. This location, when plotted on the 1:250,000 scale photomosaic of the Yorktown Region of Mars (U.S. Geological Survey, 1977) is at 22.487°N latitude and 48.041°W longitude.  相似文献   

Lunar Occultation of Saturn II. The normal reflectances of Rhea,Titan, and Iapetus     

J.L. Elliot  E.W. Dunham  J. Veverka  J. Goguen 《Icarus》1978,35(2):237-246

An inversion procedure to obtain the reflectance of the central region of a satellite's disk from lunar occultation data is presented. The scheme assumes that the limb darkening of the satellite depends only on the radial distance from the center of the disk. Given this assumption, normal reflectances can be derived that are essentially independent of the limb darkening and the diameter of the satellite. The procedure has been applied to our observations of the March 1974 lunar occultation of Tethys, Dione, Rhea, Titan, and Iapetus. In the V passband we derive the following normal reflectances: Rhea (0.97±0.20), Titan (0.24±0.03), Iapetus, bright face (0.60±0.14). For Tethys and Dione the values derived have large uncertainties, but are consistent with our result for Rhea.  相似文献   

Lunar occultation of Saturn: III. How big is Iapetus?     

J. Veverka  J. Burt  J.L. Elliot  J. Goguen 《Icarus》1978,33(2):301-310

By considering both the orbital lightcurve of Iapetus and data obtained during the March 30, 1974, occultation of the satellite by the Moon, we obtain information about the brightness distribution on the bright face of Iapetus and derive an accurate value for the satellite's radius. From the observed orbital lightcurve we find that the trailing face of Iapetus must consist predominantly of a single bright material with an effective limb-darkening parameter of k = 0.62_?0.12^0.10. Given this result the occultation observations imply a radius of 718_?78⁺⁸⁷ km. If the patchy albedo model proposed by Morrison et al. represents the surface of Iapetus accurately (as far as the relative albedo distribution is concerned) then the radius of Iapetus is 724 ± 60 km. Both estimates are consistent with the radiometric radius of 835 (+50, ?75) km derived by Morrison et al. Combining our results with the value of 0.60 ± 0.14 for the normal reflectance (in V) of the material at the center of the bright face derived by Elliot et al. we find that the normal reflectance of the dark side material is 0.11_?0.03^+0.04. These values are higher than the corresponding values of 0.35 and 0.05 quoted by Morrison et al.  相似文献   

Investigation of Thulium and Other Rare Earth Element Mass Fractions in NIST SRM 1632a Bituminous Coal Reference Material by Quadrupole ICP‐MS          下载免费PDF全文

Elliot Roth  Tracy L. Bank  Evan Granite 《Geostandards and Geoanalytical Research》2018,42(2):263-269

Inductively coupled plasma‐mass spectrometry after lithium metaborate fusion and digestion was used to measure the rare earth element (REE) mass fractions of several reference materials including NIST SRM 1632a, a historical bituminous Pennsylvania seam coal. While most of the REE mass fractions measured in this study were consistent with the published consensus data, the measured mass fraction of thulium for NIST SRM 1632a was consistently lower compared with the published data. Chondrite normalisation of the published consensus data for NIST SRM 1632a produced a positive thulium anomaly (Tm = 1.78), which is inconsistent with a terrestrial source of sediment. Normalisation of REE mass fractions collected in this study produced no significant Tm anomaly (Tm = 0.93), which agrees with the sedimentary depositional environment of coal. Therefore, a revised mass fraction of 0.16 mg kg^?1 Tm in NIST SRM 1632a is recommended.  相似文献   

Assessing water contamination risk from vegetation fires: Challenges,opportunities and a framework for progress          下载免费PDF全文

Joao P. Nunes  Stefan H. Doerr  Gary Sheridan  Jonay Neris  Cristina Santín  Monica B. Emelko  Uldis Silins  Peter R. Robichaud  William J. Elliot  Jacob Keizer 《水文研究》2018,32(5):687-694

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Improving watershed management practices in humid regions          下载免费PDF全文

Fasikaw A. Zimale  Seifu A. Tilahun  Tigist Y. Tebebu  Christian D. Guzman  Linh Hoang  Elliot M. Schneiderman  Eddy J. Langendoen  Tammo S. Steenhuis 《水文研究》2017,31(18):3294-3301

In many parts of the world, watershed management practices have been extremely effective. However, implementation of soil and water conservation technologies in the humid African highlands, while beneficial in the short term, were remarkably unsuccessful in the long term. Insights from community knowledge perspectives have revealed that alternative methods are needed. Although conservation practices are designed to conserve water in semi‐arid areas, safely draining excess water is needed in humid areas. The objective of this paper is to review current watershed management approaches used in humid regions as exemplified by those used in Ethiopian highlands and then based on these findings propose more effective practices. Although current government sponsored practices primarily protect the hillsides, direct run‐off is generated from areas that become saturated on valley bottoms near rivers and on specific parts of the hillsides with degraded soils (or with highly permeable surface soils) and with perched water tables on slowly permeable horizons at shallow depths. In these areas, direct run‐off is increasing with deforestation and the soil degradation, demanding additional drainage ways that evolve in the form of gullies. Therefore, watershed management interventions for erosion control should prioritize revegetation of degraded areas, increasing sustainable infiltration, and rehabilitating gullies situated at saturated bottomlands.  相似文献