Wettability influence on the onset temperature of pool boiling: Experimental evidence onto ultra-smooth surfaces.

In this article we study systematically the effect of wettability on the onset of boiling on the same nanometrically smooth surface. By grafting different monolayers of molecules, we were able to explore the wettability from the equilibrium static contact angle, θ0=0° to θ0=110°, without changing the surface topography. The superheat temperature at the onset of pool boiling was measured and eventually a non-classical trend of TONB as a function of wettability was observed. The nucleation site densities for the different grafting cases were also measured by image analysis. Moreover, we propose a novel theoretical interpretation to this phenomenon linking nucleation and the molecular diffusion coefficient. MD simulation results support this approach.

Influence of the wettability on the boiling onset.

Experimental investigation of pool boiling is conducted in stationary conditions over very smooth bronze surfaces covered by a very thin layer of gold presenting various surface treatments to isolate the role of wettability. We show that even with surfaces presenting mean roughness amplitudes below 10 nm the role of surface topography is of importance. The study shows also that wettability alone can trigger the boiling and that the boiling position on the surface can be controlled by chemical grafting using for instance alkanethiol. Moreover, boiling curves, that is, heat flux versus the surface superheat (which is the difference between the solid surface temperature and the liquid saturation temperature), are recorded and enabled to quantify, for this case, the significant reduction of the superheat at the onset of incipient boiling due to wettability.

Late formation and prolonged differentiation of the Moon inferred from W isotopes in lunar metals.

The Moon is thought to have formed from debris ejected by a giant impact with the early 'proto'-Earth and, as a result of the high energies involved, the Moon would have melted to form a magma ocean. The timescales for formation and solidification of the Moon can be quantified by using 182Hf-182W and 146Sm-142Nd chronometry, but these methods have yielded contradicting results. In earlier studies, 182W anomalies in lunar rocks were attributed to decay of 182Hf within the lunar mantle and were used to infer that the Moon solidified within the first approximately 60 million years of the Solar System. However, the dominant 182W component in most lunar rocks reflects cosmogenic production mainly by neutron capture of 181Ta during cosmic-ray exposure of the lunar surface, compromising a reliable interpretation in terms of 182Hf-182W chronometry. Here we present tungsten isotope data for lunar metals that do not contain any measurable Ta-derived 182W. All metals have identical 182W/184W ratios, indicating that the lunar magma ocean did not crystallize within the first approximately 60 Myr of the Solar System, which is no longer inconsistent with Sm-Nd chronometry. Our new data reveal that the lunar and terrestrial mantles have identical 182W/184W. This, in conjunction with 147Sm-143Nd ages for the oldest lunar rocks, constrains the age of the Moon and Earth to Myr after formation of the Solar System. The identical 182W/184W ratios of the lunar and terrestrial mantles require either that the Moon is derived mainly from terrestrial material or that tungsten isotopes in the Moon and Earth's mantle equilibrated in the aftermath of the giant impact, as has been proposed to account for identical oxygen isotope compositions of the Earth and Moon.

Melting dynamics beneath the tonga-kermadec island arc inferred from (231)Pa-(235)U systematics

Measurement of (231)Pa-(235)U disequilibrium in Tonga-Kermadec island arc lavas (north of New Zealand) permits discrimination of the time scales and mechanisms of fluid addition and partial melting. For Tonga lavas, the ((231)Pa/(235)U) ratios are less than 1 and can be explained by fluid addition from the subducting plate around 60,000 years ago. In contrast, the effects of partial melting overprinted those of fluid addition in the Kermadec lavas resulting in ((231)Pa/(235)U) ratios greater than 1.

Health Initiatives for Youth: a model of youth/adult partnership approach to HIV/AIDS services.

Health Initiatives for Youth (HIFY) in San Francisco, California, is an innovative organization providing health-related services for and by young people funded in part by the Special Projects of National Significance (SPNS) Program. The HIFY Youth Health Initiative (YHI) is composed of eight youth staff and aims to bring about individual and systemic change, enhance the quality of life for human immunodeficiency virus (HIV)-positive and at-risk young people, and increase the responsiveness and youth sensitivity of organizational and community systems. Comprehensive services have been delivered to 136 young men under 25 years, 33.1% of whom are HIV positive, and 164 young women, of whom 12.2% are HIV positive. In addition, thousands of youth and young adults have received lower-intensity services through dozens of educational workshops and presentations. YHI services are implemented through a comprehensive collection of education, training, and support activities that benefit the youth staff who produce them, along with the participants who benefit from the services provided. These activities include a speaker's bureau, health and advocacy trainings, internships, return-to-work and life skills training, publications, and conferences. Regional and national findings suggest that many youth do not yet comprehend their risk for HIV infection or understand the impact of HIV on their community. In direct response to these needs, HIFY programs inform and encourage access to counseling and testing, and provide meaningful access to adolescent care, treatment, and services.