Apatite and associated minerals in ferromanganese crusts from the Magellan Seamounts

The phosphate fraction extracted from a combined technological sample of ferromanganese crusts obtained from the Magellan Seamounts (Northwest Pacific) was studied with analytical electron microscopic methods. The material examined is represented by small rock fragments composed of well crystallized calcium phosphate with pores filled in with Mn oxides consisting largely of vernadite. The rock hosts crystallized barite aggregates, disseminated ultramicroscopic cubic pyrite crystals, filamentous halloysite aggregates, and assemblages of finely dispersed REE minerals represented by cerianite and parisite, which incrust the surface of apatite or are dispersed in the phosphatic matrix. The presence of the latter minerals shows that some REE related to the phosphatic phase do not enter the apatite lattice, which might influence the general pattern of the REE distribution in bulk samples     

Issue of the relationship between primary productivity of organic carbon in ocean and phosphate accumulation (Holocene-Late Jurassic)

By analogy with the present-day ocean, the primary productivity of paleoceans can be reconstructed using calculations based on the content of organic carbon in sediments and their accumulation rates. Results of calculations based on literature data show that the primary productivity of organic carbon, the mass of phosphorus involved in the process, and the content of phosphorus in oceanic waters were relatively stable in the Mesozoic and Late Mesozoic. Prior to precipitation on the seafloor together with the biogenic detritus, the dissolved phosphorus could repeatedly be involved in the biogeochemical cycle. Therefore, only less than 0.1% of phosphorus is retained in bottom sediments. The bulk phosphorus accumulation rate in oceanic sediments is partly consistent with the calculated primary productivity. Some epochs of phosphate accumulation also coincide with maximums of primary productivity and minimums of the fossilization coefficient of organic carbon. The latter fact can testify to episodes of the acceleration of organic matter mineralization and the release of phosphorus from sediments, leading to increase in the phosphorus reserve in paleoceans and phosphate accumulation in some places.     

The Composition of Phosphatized Bones in Recent Sediments

Mineral and chemical compositions of bone phosphate were studied in two samples from the outer Namibian shelf sediments composed of fish skull fragments and whale ribbon. Fossilization of bones is accompanied by the accumulation of lithogenic components, iron, sulfur, rare earth and other trace elements (Ni, Cu, Co, Cd, Mo, La, Ce, Th, U, and others), whereas the organic and mineral carbon content decreases. The evolution of bone phosphate during fossilization consists in transition from primary hydroxylapatite to a gel-type material, which subsequently becomes globular and crystallizes as fluorcarbonate-apatite crystallites. Additionally, some authigenic minerals, including both relatively widespread minerals (pyrite, uraninite, and coffinite) and rare minerals (graphite and calcium and germanium oxides) are formed in the bones. A considerable proportion of uranium in bones consists of uranium minerals, which also contain rare earth elements.     

Helioseismic models of the sun with a low heavy element abundance

Helioseismology and neutrino experiments probing the internal structure of the Sun have yieldedmuch information, such as the adiabatic elasticity index, density, and sound speed in the convective and radiative zones, the depth of the convective zone, and the flux of neutrinos from the core. The standard model of the Sun does not adequately reproduce these characteristics, with models with low heavy element contents (mass fraction of metals Z = 0.013 in the convective zone) deviating from the helioseismic data appreciably more strongly than models with high heavy element contents (Z = 0.018). However, a spectroscopic low Z value is supported by studies reconstructing the Γ ₁ profile in the adiabatic part of the convective zone based on the oscillation frequencies. Models of the convective zone show a good agreement precisely for low Z values. This study attempts to construct a model for the Sun with low Z that satisfies the helioseismic constraints. This model requires changes in the p + p reaction cross section and the opacities in the radiative zone. In our view, the helioseismic result for the mass concentrated in the convective zone testifies that the p + p reaction cross section or the electron-screening coefficient in the solar core must be increased by several percent over the current values. This requires a comparatively small correction to the opacities (by less than 5%), in order to obtain a solar model with low Z that is in agreement with the results of helioseismology and the observed solar neutrino fluxes.     

A New Improved System of Orbital Elements for Comet 35P/Herschel–Rigollet

The results of determination of orbital elements of comet 35P/Herschel–Rigollet on the basis of the angular measurements in two observed apparitions are presented. An analysis of the problem showed some essential peculiarities, which have not been taken into account previously and have inhibited its solution. The estimates of the accuracy of the obtained solution showed that the new system of orbital elements of the comet allows one to predict its motion most accurately.