Subsidence and thermal history of an inverted Late Jurassic‐Early Cretaceous extensional basin (Cameros,North‐central Spain) affected by very low‐ to low‐grade metamorphism

The Cameros Basin (North Spain) is a Late Jurassic‐Early Cretaceous extensional basin, which was inverted during the Cenozoic. It underwent a remarkable thermal evolution, as indicated by the record of anomalous high temperatures in its deposits. In this study, the subsidence and thermal history of the basin is reconstructed, using subsidence analysis and 2D thermal modelling. Tectonic subsidence curves provide evidence of the occurrence of two rapid subsidence phases during the syn‐extensional stage. In the first phase (Tithonian‐Early Berriasian), the largest accommodation space was formed in the central sector of the basin, whereas in the second (Early Barremian‐Early Albian), it was formed in the northern sector. These rapid subsidence phases could correspond to relevant tectonic events affecting the Iberian Plate at that time. By distinguishing between the initial and thermal subsidence and defining their relative magnitudes, Royden's (1986) method was used to estimate the heat flow at the end of the extensional stage. A maximum heat flow of 60–65 mW/m² is estimated, implying only a minor thermal disturbance associated with extension. In contrast with these data, very high vitrinite reflectance, anomalously distributed in some case with respect to the typical depth‐vitrinite reflectance relation, was measured in the central‐northern sector of the basin. Burial and thermal data are used to construct a 2D thermal basin model, to elucidate the role of the processes involved in sediment heating. Calibration of the thermal model with the vitrinite reflectance (%Ro) and fluid inclusion (FI) data indicates that in the central and northern sectors of the basin, an extra heat source, other than a typical rift, is required to explain the observed thermal anomalies. The distribution of the %Ro and FI values in these sectors suggests that the high temperatures and their distribution are related to the circulation of hot fluids. Hot fluids were attributed to the hydrothermal metamorphic events affecting the area during the early post‐extensional and inversion stages of the basin.     

Genetic Relationships Among One Non-Endemic and Two Endemic Mediterranean Triplefin Blennies (Pisces, Blennioidei)

Abstract. Three triplefin blennies occur sympatrically in the Mediterranean Sea; Tripterygion tripteronotus and T. melanurus are endemic, whereas T. delaisi is also found in the Eastern Atlantic. Although very similar in morphology, ecology and behaviour, some striking differences exist among reproductive strategies. Several authors proposed hypotheses on the evolution of these species. In order to enhance insight into the genetic structure of this genus, an enzyme electrophoretic survey was performed. Samples of 40 to 45 specimens of each species were collected near Calvi (Corsica, France). Twenty-four enzyme loci were analysed, of which 17 appeared polymorphic. T. delaisi showed a high level of average observed heterozygosity (H_o) of 0.140, as opposed to very low levels of 0.009 and 0.021 in T. tripteronotus and T. melanurus , respectively. Nei's genetic distance was 0.21 between T. delaisi and T. tripteronotus , 0.35 between T. delaisi and T. melanurus and 0.45 between T. tripteronotus and T. melanurus . We hypothesise that divergence of these species started before the Pleistocene and that the endemic species survived the Pleistocene glaciations in refugia within the Mediterranean. The possibility that T. tripteronotus and T. delaisi diverged through sympatric speciation is discussed.     

Apollo 12 ropy glasses revisited

Abstract— We analyzed ropy glasses from Apollo 12 soils 12032 and 12033 by a variety of techniques including SEM/EDX, electron microprobe analysis, INAA, and ³⁹Ar-⁴⁰Ar age dating. The ropy glasses have KREEP-like compositions different from those of local Apollo 12 mare soils; it is likely that the ropy glasses are of exotic origin. Mixing calculations indicate that the ropy glasses formed from a liquid enriched in KREEP and that the ropy glass liquid also contained a significant amount of mare material. The presence of solar Ar and a trace of regolith-derived glass within the ropy glasses are evidence that the ropy glasses contain a small regolith component Anorthosite and crystalline breccia (KREEP) clasts occur in some ropy glasses. We also found within these glasses clasts of felsite (fine-grained granitic fragments) very similar in texture and composition to the larger Apollo 12 felsites, which have a ³⁹Ar-⁴⁰Ar degassing age of 800 ± 15 Ma (Bogard et al, 1992). Measurements of ³⁹Ar-⁴⁰Ar in 12032 ropy glass indicate that it was degassed at the same time as the large felsite although the ropy glass was not completely degassed. The ropy glasses and felsites, therefore, probably came from the same source. Most early investigators suggested that the Apollo 12 ropy glasses were part of the ejecta deposited at the Apollo 12 site from the Copernicus impact Our new data reinforce this model. If these ropy glasses are from Copernicus, they provide new clues to the nature of the target material at the Copernicus she, a part of the Moon that has not been sampled directly.     

Collision orbits in the oblate planet problem

Some of the properties of the oblate planet problem are derived. We use the technique of blowing up the singularity to study the collision orbits. We define some families of them in terms of their asymptotic behavior.     

柴达木盆地西部第四纪气候变化和流域风化

长期以来关于构造隆升、气候变化和大陆化学风化的相互关系存在诸多争议。在气候和构造相互作用典型区域建立高精度大陆化学风化序列是解决上述科学问题的有效途径之一。位于青藏高原东北缘长期封闭的柴达木盆地,其独特的位置和连续的沉积使其成为研究构造隆升、气候变化和大陆化学风化的理想场所。本文以柴达木盆地西部千米深钻SG-1钻孔高质量的连续细粒湖相岩芯为研究对象,使用盐类矿物的硫酸根和钾离子含量、碳酸盐锰含量和硅酸盐化学蚀变指数（CIA）和Nd同位素分析,重建该区第四纪以来湖泊流域气候变化过程和硅酸盐化学风化及可能的物源变化。结果表明柴达木盆地西部第四纪以来流域物源相对稳定,流域整体呈现出气候干旱化、流域硅酸盐风化强度减弱、湖水盐度增加和湖面降低的长期一致性演化过程;上述演化进程在2.2 Ma到2.0 Ma期间短暂加强,在约1.2 Ma和约0.6~0.5 Ma出现逐步加强趋势。过去60万年,柴达木盆地西部在冰期存在的相对高湖面时期与黄土高原粒度指标反映的冬季风减弱阶段可以很好对比。北大西洋海表温度反映的高纬过程是长时间尺度（>105年）驱动柴达木盆地西部气候变化和流域硅酸盐风化强度变化的主要因素;西伯利亚高压系统和西风系统的"跷跷板关系"可能是冰期-间冰期或者更短尺度影响柴达木盆地西部气候变化的主要因素。     

Changes in the ionic composition of a saline lake,Mar Chiquita,Province of Córdoba,Argentina

Mar Chiquita is the largest water-body in Argentina according to area. This ranges from 2,000 km² in dry periods to 5,000 km² in humid ones. Its very high salinity ranged this century from 200 to 300 g/L, but an increase in the average rainfall in the basin since 1973 has led to a rise in lake level and the dilution of its waters to 78 g/L in 1978 and about 30 g/L in the late 1980s. Ionic strength decreased from 6.61 in 1970 to 0.541 in 1986. The composition of the water also changed, with increases in the proportions of sulphate, calcium and magnesium concentrations. The most important processes taking place in solution are calcite and gypsum equilibrium, formation of clay minerals, and sulphate reduction in the interstitial waters of the bottom sediments. The thermodynamic state of the solutions for different years has been obtained. Results show that the solution shifted from gypsum oversaturation in 1970 to gypsum equilibrium in 1978, and to gypsum undersaturation since 1982. A geochemical simulation of the composition of the solution from its origin from mean tributary composition, following a modified Hardie-Eugster model, has been developed using PHRQPITZ. The results agree with empirical observations.     

Orbital Elements of 2004 Perseid Meteoroids Perturbed by Jupiter

Jupiter and Saturn produce important gravitational impulses on meteoroids released by comet 109P/Swift-Tuttle. The meteoroids from this comet once released follow retrograde orbits that during their periodic approaches to these planets (within 1.6 and 0.9 A.U., respectively) are impulsed gaining orbital energy. This perturbation effect is translated into a net inward shift in the node of the perturbed meteoroids. Such geometry with Jupiter occurred in 2004 over a meteoroid trail ejected by this comet during the 1862 A.D. return of the comet to perihelion. In order to study the predicted outburst produced by one-revolution meteoroids, the Spanish Photographic Meteor Network (SPMN) performed an extensive campaign. As a part of this observational effort here are presented 10 accurate meteoroid orbits. We discuss their origin by comparing them with the theoretical orbital elements of the dust trails intercepting the Earth during the 2004 Perseid return.