Meteoroid streams: Evidence from meteorites recovered on Earth     

Stephen F. Wolf  Michael E. Lipschutz 《Earth, Moon, and Planets》1995,68(1-3):605-637

The flux of small meteoroids, originating primarily from comets, consists of sporadic, random objects and others whose orbits are related. Here, we summarize data relevant to the question of whether the flux of large meteoroids of asteroidal origin (recoverable as meteorites) also consists of objects with random orbits, as well as coorbital objects. After reviewing some relevant properties of planetary materials, applications of two nuclear techniques - radiochemical neutron activation analysis (RNAA) and accelerator mass spectrometry (AMS) - to this question are discussed. Contents of ten thermally labile trace and ultratrace elements determined by RNAA (Ag, Bi, Cd, Cs, In, Rb, Se, Te, Tl, Zn) act as thermometers for thermal metamorphism in parent sources. These data, together with spectral reflectivity information, establish the nature of surfaces on abundant C-, G-, B- and F-class asteroids. Data for these ten cosmothermometers in H4-6 type ordinary chondrites, when treated by multivariate statistical techniques, demonstrate that a suite chosen by one set of criteria (the circumstances of their fall in May, between 1855 and 1895) is distinguishable by another set, i.e. compositionally, from all other such falls analyzed. Hence, this suite, H Cluster 1, has an average thermal history distinguishable from those of all other falls, demonstrating that near-Earth source regions for H chondrite falls changes rapidly. AMS measurements of cosmogenic³⁶Cl (301 kyr half-life), quantify nominal terrestrial ages for Antarctic H chondrites whose contents of thermometric trace elements were also established by RNAA. While multivariate statistical analysis of RNAA data from Antarctic H chondrites with nominal terrestrial ages 50 kyr are not distinguishable from those of falls, older Antarctic H chondrites are compositionally distinguishable from falls. Assertions that these highly significant compositional differences reflect terrestrial or methodologic causes are refutable. This result argues that near-Earth source regions of H chondrites have changed over a long time, as well. Thus, the Earth receives a highly biased sampling of planetary objects in the Solar System in any one time-period.  相似文献   

Projected changes in area of the Sundarban mangrove forest in Bangladesh due to SLR by 2100     

Andres Payo  Anirban Mukhopadhyay  Sugata Hazra  Tuhin Ghosh  Subhajit Ghosh  Sally Brown  Robert J. Nicholls  Lucy Bricheno  Judith Wolf  Susan Kay  Attila N. Lázár  Anisul Haque 《Climatic change》2016,139(2):279-291

  相似文献   

Dehydration-melting of solid amphibolite at 10 kbar: Textural development,liquid interconnectivity and applications to the segregation of magmas   总被引：14，自引：0，他引：14  

M. B. Wolf  Prof. P. J. Wyllie 《Mineralogy and Petrology》1991,44(3-4):151-179

Summary Anisotropic crystal structures and rock texture control liquid morphology and distribution during dehydration-melting at 10 kbar in solid cylinders of lineated amphibolite (mode: hornblende 70%, plagioclase 30%), sealed in gold capsules, in piston-cylinder runs ranging from 21 days at 850 °C to 4 days at 1000 °C. The shapes of most liquid pockets are crystallographically-controlled, with many corners having angles greater than 60°. Few crystal/liquid triple junctions develop the interfacial energy-controlled dihedral angles (), which form in experiments using finely-ground powders of minerals with poor cleavage. Liquid interconnectivity probably is attained at 875 °C with only 2% liquid, indicating that dihedral angles less than 60° may not be necessary to achieve interconnectivity in partially melted metamorphic rocks. The surfaces between elongated grains in lineated rocks can become pathways for the migration of liquid or the diffusion of components. By 850 °C, hornblende begins to dehydrate at internal nucleation sites, producing a texture of hornblende rims and clinopyroxene cores (generally attributed to hydration of clinopyroxene). Within the temperature interval of 850–900 °C, transient vapor generates layers of low viscosity, H₂O-saturated, granitoid liquid between hornblende and plagiocase crystal faces, potentially capable of segregation if time-temperature relationships are suitable. At higher temperatures the increased liquid fraction is H₂O-undersaturated, with viscosity too high to permit segregation. There is a prospect that segregation of initially hydrous liquids could contribute to the dehydration of low-potassium amphibolites and effectively remove incompatible trace elements during the transition from amphibolite-facies to granulite-facies. Further experiments are needed to study the effects of time and temperature on textures in anisotropic rocks, particularly lineated amphibolites.

---

Dehydrations-Schmelzen von Amphiboliten bei 10 kbar: Texturelle Entwicklung, Interkonnektivität der Schmelze und Anwendungen auf die Segregation von Magmen

Zusammenfassung Die texturelle Entwicklung von festen Zylindern von Amphibolit (Hornblende 70%, Plagioklas 30%) in Goldkapseln versiegelt, wurde w:rend Dehydrations-Schmelzen bei 10 kbar in einem Piston-Zylinder-Apparat bei Temperaturen von 850°C bis 1000°C für 21 bis 4 Tage untersucht. Die anisotropen Mineralstrukturen und die Gesteinstextur kontrollieren die Morphologie und Verteilung der Schmelze. Diese Parameter sowie der Anteil an Schmelze, bestimmen die Interkonnektivität der Schmelze. Im Gegensatz zu Experimenten, die fein gemahlene Pulver von fast isotropen Mineralen (z.B. Olivin oder Quarz) benützen, scheinen hier die Energieverhältnisse der Kristallstruktur die Energiebeziehungen zwischen den Kristall-Schmelzoberflächen während der texturellen Entwicklung der amphibolitischen Gesteine zu dominieren. Wenige Kristall-Schmelze Triple-Junetions entwickeln zwischen Flächen energie-kontrollierte dihedrale Winkel (). Die Formen der meisten Schmelzeinschlüsse sind kristallographisch kontrolliert und viele Ecken zeigen Winkel, die größer als 60° sind. Die Interkonnektivität der Schmelze wird jedoch eindeutig bei 875° C mit nur 2% Schmelze erreicht und könnte möglicherweise auch bei niedrigeren Temperaturen zustande kommen. Das Vorkommen von dihedralen Winkeln, die kleiner als 60° sind, muß nicht notwendig sein, um Interkonnektivität in teilweis aufgeschmolzenen metamorphen Gesteinen zu erzeugen. Die Oberflächen zwischen gelängten Körnern in Amphiboliten mit Lineation können Wege für die Migration von Schmelzen oder für die Diffussion von Komponenten während teilweisen Aufschmelzens werden. Bei 850° C begann die Dehydration der Hornblende an internen Nukleations-Stellen, unabhängig vom Rest des Gesteins. Zwischen 850° C und 900 °C entsteht so eine Textur von Klinopyroxenen mit Hornblenderändern. Die nicht im Gleichgewicht befindliche Dampfphase, die dabei entsteht, führt zur Bildung von Lagen von wassergesättigter granitoider Schmelze zwischen Hornblende und Plagioklasflächen, mit einer berechneten Viskosität, die gerade niedrig genug ist, um Segregation durch Kompaktion zu ermöglichen. Bei höheren Temperaturen und während längerer Zeiten, wobei mehr Schmelze entsteht, löst sich die Dampfphase in wasseruntersättigter Schmelze, mit einer Viskosität, die zu hoch ist um Segregation in geologisch realistischen Zeiten zu ermöglichen. Die Entwässerung von kalium-armen Gesteinen durch Segregation von ursprünglich wässrigen Schmelzen, die sich in dieser Weise gebildet haben, dürfte beim Amphiboht-Granulit-Übergang eine Rolle spielen.[/ p]

---

---

With 10 Figures  相似文献   

Galaxy morphologies and environment in the Abell 901/902 supercluster from COMBO-17     

K. P. Lane  M. E. Gray  A. Aragón-Salamanca  C. Wolf  K. Meisenheimer 《Monthly notices of the Royal Astronomical Society》2007,378(2):716-722

  相似文献   

Structural analysis of the collar of the Vredefort Dome,South Africa—Significance for impact‐related deformation and central uplift formation     

Frank Wieland  Roger L. Gibson  Wolf Uwe Reimold 《Meteoritics & planetary science》2005,40(9-10):1537-1554

Abstract— Landsat TM, aerial photograph image analysis, and field mapping of Witwatersrand supergroup meta‐sedimentary strata in the collar of the Vredefort Dome reveals a highly heterogeneous internal structure involving folds, faults, fractures, and melt breccias that are interpreted as the product of shock deformation and central uplift formation during the 2.02 Ga Vredefort impact event. Broadly radially oriented symmetric and asymmetric folds with wavelengths ranging from tens of meters to kilometers and conjugate radial to oblique faults with strike‐slip displacements of, typically, tens to hundreds of meters accommodated tangential shortening of the collar of the dome that decreased from ?17% at a radius from the dome center of 21 km to <5% at a radius of 29 km. Ubiquitous shear fractures containing pseudotachylitic breccia, particularly in the metapelitic units, display local slip senses consistent with either tangential shortening or tangential extension; however, it is uncertain whether they formed at the same time as the larger faults or earlier, during the shock pulse. In addition to shatter cones, quartzite units show two fracture types—a cmspaced rhomboidal to orthogonal type that may be the product of shock‐induced deformation and later joints accomplishing tangential and radial extension. The occurrence of pseudotachylitic breccia within some of these later joints, and the presence of radial and tangential dikes of impact melt rock, confirm the impact timing of these features and are suggestive of late‐stage collapse of the central uplift.  相似文献   

Laser argon dating of melt breccias from the Siljan impact structure,Sweden: Implications for a possible relationship to Late Devonian extinction events     

Wolf U. REIMOLD  Simon P. KELLEY  Sarah C. SHERLOCK  Herbert HENKEL  Christian KOEBERL 《Meteoritics & planetary science》2005,40(4):591-607

Abstract— In earlier studies, the 65‐75 km diameter Siljan impact structure in Sweden has been linked to the Late Devonian mass extinction event. The Siljan impact event has previously been dated by K‐Ar and Ar‐Ar chronology at 342‐368 Ma, with the commonly quoted age being 362.7 ± 2.2 Ma (2 s?, recalculated using currently accepted decay constants). Until recently, the accepted age for the Frasnian/Famennian boundary and associated extinction event was 364 Ma, which is within error limits of this earlier Siljan age. Here we report new Ar‐Ar ages extracted by laser spot and laser step heating techniques for several melt breccia samples from Siljan (interpreted to be impact melt breccia). The analytical results show some scatter, which is greater in samples with more extensive alteration; these samples generally yield younger ages. The two samples with the least alteration yield the most reproducible weighted mean ages: one yielded a laser spot age of 377.2 ± 2.5 Ma (95% confidence limits) and the other yielded both a laser spot age of 376.1 ± 2.8 Ma (95% confidence limits) and a laser stepped heating plateau age over 70.6% ³⁹Ar release of 377.5 ± 2.4 Ma (2 s?). Our conservative estimate for the age of Siljan is 377 ± 2 Ma (95% confidence limits), which is significantly different from both the previously accepted age for the Frasnian/Famennian (F/F) boundary and the previously quoted age of Siljan. However, the age of the F/F boundary has recently been revised to 374.5 ± 2.6 Ma by the International Commission for Stratigraphy, which is, within error, the same as our new age. However, the currently available age data are not proof that there was a connection between the Siljan impact event and the F/F boundary extinction. This new result highlights the dual problems of dating meteorite impacts where fine‐grained melt rocks are often all that can be isotopically dated, and constraining the absolute age of biostratigraphic boundaries, which can only be constrained by age extrapolation. Further work is required to develop and improve the terrestrial impact age record and test whether or not the terrestrial impact flux increased significantly at certain times, perhaps resulting in major extinction events in Earth's biostratigraphic record.  相似文献   

Geochemical and petrographic characteristics of impactites and Cretaceous target rocks from the Yaxcopoil‐1 borehole,Chicxulub impact structure,Mexico: Implications for target composition     

Martin G. Tuchscherer  Wolf Uwe Reimold  Christian Koeberl  Roger L. Gibson 《Meteoritics & planetary science》2005,40(9-10):1513-1536

Abstract— We present major and trace element data as well as petrographic observations for impactites (suevitic groundmass, bulk suevite, and melt rock particles) and target lithologies, including Cretaceous anhydrite, dolomite, argillaceous limestone, and oil shale, from the Yaxcopoil‐1 borehole, Chixculub impact structure. The suevitic groundmass and bulk suevite have similar compositions, largely representing mixtures of carbonate and silicate components. The latter are dominated by melt rock particles. Trace element data indicate that dolomitic rocks represented a significant target component that became incorporated into the suevites; in contrast, major elements indicate a strong calcitic component in the impactites. The siliceous end‐member requires a mafic component in order to explain the low SiO₂ content. Multicomponent mixing of various target rocks, the high alteration state, and dilution by carbonate complicate the determination of primary melt particle compositions. However, two overlapping compositional groups can be discerned—a high‐Ba, low‐Ta group and a high‐Fe, high‐Zn, and high‐Hf group. Cretaceous dolomitic rocks, argillaceous limestone, and shale are typically enriched in U, As, Br, and Sb, whereas anhydrite contains high Sr contents. The oil shale samples have abundances that are similar to the North American Shale Composite (NASC), but with a comparatively high U content. Clastic sedimentary rocks are characterized by relatively high Th, Hf, Zr, As, and Sb abundances. Petrographic observations indicate that the Cretaceous rocks in the Yaxcopoil‐1 drill core likely register a multistage deformation history that spans the period from pre‐ to post‐impact. Contrary to previous studies that claimed evidence for the presence of impact melt breccia injection veins, we have found no evidence in our samples from a depth of 1347–1348 m for the presence of melt breccia. We favor that clastic veinlets occur in a sheared and altered zone that underwent intense diagenetic overprint prior to the impact event.  相似文献   

Glacial-isostatic Adjustment and the Viscosity Structure Underlying the Vatnajökull Ice Cap,Iceland     

Kevin Fleming  Zdeněk Martinec  Detlef Wolf 《Pure and Applied Geophysics》2007,164(4):751-768

We examine the dependence of glacial-isostatic adjustment (GIA) due to changes in the Vatnajökull Ice Cap, Iceland, on the underlying viscosity structure. Iceland offers a unique case study for GIA research, with a thinner elastic lithosphere underlain by a low-viscosity zone or asthenosphere, as opposed to regions such as Fennoscandia or North America described by a thicker lithosphere, while not necessarily featuring an asthenosphere.A laterally homogeneous spherical earth model is used consisting of an elastic lithosphere, a viscoelastic asthenosphere, a viscoelastic upper and lower mantle and a fluid core. We examine the response of the earth model to three ice models with circular plans and cross-section profiles based on the assumption of perfectly plastic material, but with different load histories. These are: (1) A history where the ice cap grows from a AD 900 minimum to a maximum at 1890, followed by a uniform decrease until 1991, continuing to the present day at an average rate based on recent mass-balance measurements, (2) a history that is the same as the first, except for constant ice volumes prior to 1890, and (3) a history that is again the same as the first model, except that the post-1991 changes correspond to the measured mass-balance values. We first compare the response to each ice model using typical earth-model parameters for Iceland presented in the literature. We then undertake a parameter-space search, where we assess the importance of lithosphere thickness, asthenosphere viscosity and basal asthenosphere depth, to predicted vertical-displacement rates, and compare them to rates determined from GPS measurements obtained from campaigns conducted between 1991 and 1999.The earth-viscosity structure that provides the optimum predictions with respect to the GPS-derived vertical-displacement rates consists of an elastic lithosphere with a thickness of between 20 and 30 km, an asthenosphere viscosity between 1 and 2 × 10¹⁸ Pa s, and a basal asthenosphere depth between 250 km and possibly greater than 400 km. We find that the very low asthenosphere viscosity values of ca. 10¹⁷ Pa s sometimes suggested in the literature are not necessary to account for the rapid vertical-displacement rates observed, which are the result of the contemporary decrease in the mass of the ice cap not considered previously.  相似文献   

STAGES: the Space Telescope A901/2 Galaxy Evolution Survey     

Meghan E. Gray  Christian Wolf  Marco Barden  Chien Y. Peng  Boris Häußler  Eric F. Bell  Daniel H. McIntosh  Yicheng Guo  John A. R. Caldwell  David Bacon  Michael Balogh  Fabio D. Barazza  Asmus Böhm  Catherine Heymans  Knud Jahnke  Shardha Jogee  Eelco van Kampen  Kyle Lane  Klaus Meisenheimer  Sebastian F. Sánchez  y Taylor  Lutz Wisotzki  Xianzhong Zheng  David A. Green  R. J. Beswick  D. J. Saikia  Rachel Gilmour  Benjamin D. Johnson  Casey Papovich 《Monthly notices of the Royal Astronomical Society》2009,393(4):1275-1301

We present an overview of the Space Telescope A901/2 Galaxy Evolution Survey (STAGES). STAGES is a multiwavelength project designed to probe physical drivers of galaxy evolution across a wide range of environments and luminosity. A complex multicluster system at   z ∼ 0.165  has been the subject of an 80-orbit F606W Hubble Space Telescope (HST) /Advanced Camera for Surveys (ACS) mosaic covering the full     span of the supercluster. Extensive multiwavelength observations with XMM–Newton , GALEX, Spitzer , 2dF, Giant Metrewave Radio Telescope and the 17-band COMBO-17 photometric redshift survey complement the HST imaging. Our survey goals include simultaneously linking galaxy morphology with other observables such as age, star formation rate, nuclear activity and stellar mass. In addition, with the multiwavelength data set and new high-resolution mass maps from gravitational lensing, we are able to disentangle the large-scale structure of the system. By examining all aspects of an environment we will be able to evaluate the relative importance of the dark matter haloes, the local galaxy density and the hot X-ray gas in driving galaxy transformation. This paper describes the HST imaging, data reduction and creation of a master catalogue. We perform the Sérsic fitting on the HST images and conduct associated simulations to quantify completeness. In addition, we present the COMBO-17 photometric redshift catalogue and estimates of stellar masses and star formation rates for this field. We define galaxy and cluster sample selection criteria, which will be the basis for forthcoming science analyses, and present a compilation of notable objects in the field. Finally, we describe the further multiwavelength observations and announce public access to the data and catalogues.  相似文献   

Bayesian photometric redshifts with empirical training sets     

Christian Wolf 《Monthly notices of the Royal Astronomical Society》2009,397(1):520-533

We combine in a single framework the two complementary benefits of  χ²  template fits and empirical training sets used e.g. in neural nets:  χ²  is more reliable when its probability density functions (PDFs) are inspected for multiple peaks, while empirical training is more accurate when calibration and priors of query data and training set match. We present a  χ²  empirical method that derives PDFs from empirical models as a subclass of kernel regression methods, and apply it to the Sloan Digital Sky Survey Data Release 5 sample of >75 000 quasi-stellar objects, which is full of ambiguities. Objects with single-peak PDFs show <1 per cent outliers, rms redshift errors <0.05 and vanishing redshift bias. At   z > 2.5  , these figures are two times better. Outliers result purely from the discrete nature and limited size of the model, and rms errors are dominated by the intrinsic variety of object colours. PDFs classed as ambiguous provide accurate probabilities for alternative solutions and thus weights for using both solutions and avoiding needless outliers. E.g. the PDFs predict 78.0 per cent of the stronger peaks to be correct, which is true for 77.9 per cent of them. Redshift incompleteness is common in faint spectroscopic surveys and turns into a massive undetectable outlier risk above other performance limitations, but we can quantify residual outlier risks stemming from size and completeness of the model. We propose a matched  χ²  error scale for noisy data and show that it produces correct error estimates and redshift distributions accurate within Poisson errors. Our method can easily be applied to future large galaxy surveys, which will benefit from the reliability in ambiguity detection and residual risk quantification.  相似文献