23,459 research outputs found

    Bridging the Gap Between Schools and Non-Formal Science Institutions: Using New York City\u27s Non-Formal Resources to Teach Science

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    Effective science teaching and learning needs to take place in an environment in which the formal and non-formal worlds of science combine their expertise and resources. Science learning and ultimately, scientific literacy for all depends on the teaching that occurs both in schools and in non-formal settings. As we move towards the attainment of scientific literacy for all, it is becoming more imperative that we recognize and utilize the media, industry education programs, non-formal science centers, museums, and other science learning outlets as valuable segments of our nation’s science education infrastructure. This paper describes the context, rationale, and outline of the non-formal science education course developed at New York University under the auspices of New York Collaborative for Excellence in Teacher Preparation (NYCETP) and the subsequently developed non-formal science education specialization

    SO2 on Io: A thermodynamic perspective

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    The presence of condensed SO2 on Io mandates a finite abundance of SO2 vapor which must be present, regardless of plume activity. The absorption of SO2 was measured on particulate sulfur and the equilibrium between absorbed SO2, SO2 vapor, and SO2 ice examined, based upon measurements and simple thermodynamic considerations

    Effect of molecular anisotropy on the intensity and degree of polarization of light scattered from model atmospheres

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    Computations of the intensity, flux, degree of polarization, and the positions of neutral points are presented for models of the terrestrial gaseous and hazy atmospheres by incorporating the molecular anisotropy due to air in the Rayleigh scattering optical thickness and phase matrix. Molecular anisotropy causes significant changes in the intensity, flux and the degree of polarization of the scattered light. The positions of neutral points do not change significantly. When the Rayleigh scattering optical thickness is kept constant and the molecular anisotropy factor is included only in the Rayleigh phase matrix, the flux does not change and the intensity and positions of neutron points change by a small amount. The changes in the degree of polarization are still significant

    CO2: Adsorption on palagonite and the Martian regolith

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    Possible scenarios for the evolution of the Martian climate are discussed. In the interest of determining an upper limit on the absorptive capacity of the Martian regolith, researchers examined the results of Fanale and Cannon (1971, 1974) for CO2 adsorption on nontronite and basalt. There appeared to be a strong proportionality between the capacity of the absorbent and its specific surface area. A model of the Martian climate is given that allows the researchers to make some estimates of exchangeable CO2 abundances

    Atmospheric H2O and the search for Martian brines

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    Abundant martian brines would have important implication for current theories of volatile migration on Mars, since, although the presence of metastable brines is quite plausible, any brine in the reasonably near-surface should be completely depleted on a timescale short in relation to the age of Mars. It is important to determine whether brines exist in the martian subsurface, for the current paradigm for understanding martian volatile regime requires substantial alteration if they are found to exist. It is determined, however, that the prospect for detection of a subsurface brine via atmospheric water vapor measurements is marginal. Four reasons are given for this conclusion
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