Stratigraphy and composition of lava flows in Mare Nubium and Mare Cognitum     

Roberto Bugiolacchi  Paul D. Spudis  John E. Guest 《Meteoritics & planetary science》2006,41(2):285-304

Abstract— Three major periods of basaltic activity characterize the infill of the basins. Each of these periods was itself punctuated by discrete phases of widespread magma eruptions: three during both the Late Imbrian Epoch and the early Eratosthenian Period and then two in the late Eratosthenian Period. We found the youngest lavas off the eastern border of the Fra Mauro peninsula and, mantling a much larger area, over most of the central western Nubium basin. Our results place the Nubium/Cognitum basalts in the low‐Ti category (1–5 wt% TiO₂). The data indicate that the majority (?90%) of the mare terrain has iron content between 18 and 22 wt%. In particular, FeO contents tend to concentrate toward two compositional poles, each of ?20 wt%, and a much smaller one of ?15 wt%. These values are typical of nearside lunar maria. To complement our compositional data, we present a census of craters larger than 500 m using Orbiter IV images. The result was a crater count average with frequency 5.6 × 10^?2 km^?2, translating into an inferred mean age of 3300 Ma for the exposed lava flows. By combining lava chemistry with age, we find a possible correlation between the ages of the most prominent flow units and their estimated titanium content, with younger basalts becoming progressively Ti‐richer with time (from 2–3 to 4–5 wt% TiO₂).  相似文献   

Stratigraphy and evolution of basalts in Mare Humorum and southeastern Procellarum     

Terence Hackwill  John Guest  Paul Spudis 《Meteoritics & planetary science》2006,41(3):479-488

Abstract— We have studied the mare basalts of Mare Humorum and southeastern Procellarum (30°W–50°W, 0°–40°S). One hundred and nine basaltic units have been identified from differences in their FeO wt% and TiO₂ wt% content, and variations in crater densities. Crater counting and reference to isotopically dated Apollo samples have provided an age for 33 major units. Some evidence for three distinct periods of volcanic activity has been found. We found that the large unit in the middle of Mare Humorum is the oldest in the basin. This supports the suggestion that the oldest central unit sank causing the lithosphere to bend and create dykes through which lava flowed to produce the outer units. No evidence of a trend in FeO wt% and TiO₂ wt% content against time is found within Mare Humorum. There appears to be no lateral trend of basalts in terms of FeO and TiO₂ wt% over the entire area with time. An increase in FeO content with time is found in the 33 major units and there is some evidence for an increase in TiO₂ in the same units. A correlation between FeO wt% and TiO₂ wt% content is evident when all 109 units are compared. A notable feature of this correlation is a sharp increase in gradient of TiO₂ wt% content when the FeO wt% content rises above about 17%.  相似文献   

Space plasmas and astrophysical plasmas studies interrelation     

Michael Balikhin  Michael Gedalin  Guest Editors 《Planetary and Space Science》2007,55(15):1189

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Resurfacing styles and rates on Venus: assessment of 18 venusian quadrangles     

Ellen R. Stofan  Antony W. Brian  John E. Guest 《Icarus》2005,173(2):312-321

We have quantitatively assessed the resurfacing sources and styles in eighteen mapped venusian quadrangles, about 30% of the venusian surface. Each quadrangle was split into 0.5° by 0.5° boxes, which were then identified as corona materials, large volcano materials (>100 km diameter), intermediate volcano materials (10-100 km), small edifice materials (<10 km), flow materials from rifts or fractures, plains without an identifiable source, impact crater materials and highly deformed materials, or data gaps. We find that coronae resurface approximately 21%, small edifices 22% and large volcanoes about 6% of the surfaces analyzed. Plains with no identifiable source account for an average of 35% of the surface assessed. Small edifices resurface on a scale of 10-100 s of km²; large edifices resurface areas of 10⁴-10⁵ km². Coronae have greatly varying amounts of associated volcanism, with some coronae producing negligible flow deposits and others producing deposits of 10⁴-10⁶ km². The areas identified as plains with no visible source occur on small scales (10² km²) to large scales (> 10⁵ km²). Our results indicate that the majority of plains resurfacing by volcanism can be tied to an identifiable source, that fields of small edifices contribute more to resurfacing than we had anticipated, and that resurfacing styles do not appear to have evolved over the time period represented by the surface geology in the mapped quadrangles. All of the units that we quantified occur throughout the histories of the regions mapped. We favor plains resurfacing to have occurred over at least 100 myr, which implies terrestrially reasonable resurfacing rates.  相似文献   

Preface: The international North Water (NOW) polynya study     

David Barber Guest Editor  Richard Marsden Guest Editor  Peter Minnett Guest Editor 《大气与海洋》2013,51(3)

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‘Applications of X-ray computed tomography in engineering geology’ or ‘looking inside rocks …’     

Patric Jacobs  Veerle Cnudde  Guest Editors 《Engineering Geology》2009,103(3-4):67

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Shoemaker Memorial Issue on the Australian impact record: 1997 – 2005 update     

A. Y. Glikson  P. W. Haines Guest Editors 《Australian Journal of Earth Sciences》2013,60(4-5):475-476

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Introduction: A review of eastern tropical Pacific oceanography     

Paul C. Fiedler  Guest editor  Miguel F. Lavín  Guest editor 《Progress in Oceanography》2006,69(2-4):94

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On the turbulent Prandtl number in the stable atmospheric boundary layer     

Andrey A. Grachev  Edgar L Andreas  Christopher W. Fairall  Peter S. Guest  P. Ola G. Persson 《Boundary-Layer Meteorology》2007,125(2):329-341

This study focuses on the behaviour of the turbulent Prandtl number, Pr _t , in the stable atmospheric boundary layer (SBL) based on measurements made during the Surface Heat Budget of the Arctic Ocean experiment (SHEBA). It is found that Pr _t increases with increasing stability if Pr _t is plotted vs. gradient Richardson number, Ri; but at the same time, Pr _t decreases with increasing stability if Pr _t is plotted vs. flux Richardson number, Rf, or vs. ζ = z/L. This paradoxical behaviour of the turbulent Prandtl number in the SBL derives from the fact that plots of Pr _t vs. Ri (as well as vs. Rf and ζ) for individual 1-h observations and conventional bin-averaged values of the individual quantities have built-in correlation (or self-correlation) because of the shared variables. For independent estimates of how Pr _t behaves in very stable stratification, Pr _t is plotted against the bulk Richardson number; such plots have no built-in correlation. These plots based on the SHEBA data show that, on the average, Pr _t decreases with increasing stability and Pr _t < 1 in the very stable case. For specific heights and stabilities, though, the turbulent Prandtl number has more complicated behaviour in the SBL.  相似文献   

Stresses along the metastable wedge of olivine in a subducting slab: possible explanation for the Tonga double seismic layer   总被引：1，自引：0，他引：1  

A. Guest  G. Schubert 《Physics of the Earth and Planetary Interiors》2004,141(4):253-267

A numerical calculation of the stresses associated with changes in volume during phase transitions of olivine in a descending slab results in a double layer of high shear stress along the metastable olivine wedge in the depth range 350-460 km. Stress in the upper layer is in-plane tensional and stress in the lower layer is down-dip compressional. The modeled stress field agrees with observations of stress in the Tonga double seismic zone. High shear stress also exists in the slab at depths below the metastable wedge. This stress distribution involves down-dip compression and trench-parallel tension, which agrees with about half of the focal mechanisms in the Tonga slab at depths of 460-690 km. The model supports the idea that at least two possible stress release mechanisms for deep earthquakes may act in the Tonga subducting slab. One, transformational faulting, is restricted to the metastable wedge while the other one acts below the metastable wedge.  相似文献