10 research outputs found

    The outer planets - Fly-by prospects

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    The projected benefits of flyby missions to the outer planets are discussed. Possible changes in existing theories of planetary composition as a result of such missions are also discussed

    Exact, E=0, Solutions for General Power-Law Potentials. I. Classical Orbits

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    For zero energy, E=0E=0, we derive exact, classical solutions for {\em all} power-law potentials, V(r)=γ/rνV(r)=-\gamma/r^\nu, with γ>0\gamma>0 and <ν<-\infty <\nu<\infty. When the angular momentum is non-zero, these solutions lead to the orbits (˚t)=[cosμ(th(t)th0(t))]1/μ\r(t)= [\cos \mu (\th(t)-\th_0(t))]^{1/\mu}, for all μν/210\mu \equiv \nu/2-1 \ne 0. When ν>2\nu>2, the orbits are bound and go through the origin. This leads to discrete discontinuities in the functional dependence of th(t)\th(t) and th0(t)\th_0(t), as functions of tt, as the orbits pass through the origin. We describe a procedure to connect different analytic solutions for successive orbits at the origin. We calculate the periods and precessions of these bound orbits, and graph a number of specific examples. Also, we explain why they all must violate the virial theorem. The unbound orbits are also discussed in detail. This includes the unusual orbits which have finite travel times to infinity and also the special ν=2\nu = 2 case.Comment: LaTeX, 27 pages with 12 figures available from the authors or can be generated from Mathematica instructions at end of the fil

    The Structure of Jupiter, Saturn, and Exoplanets: Key Questions for High-Pressure Experiments

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    We give an overview of our current understanding of the structure of gas giant planets, from Jupiter and Saturn to extrasolar giant planets. We focus on addressing what high-pressure laboratory experiments on hydrogen and helium can help to elucidate about the structure of these planets.Comment: Invited contribution to proceedings of High Energy Density Laboratory Astrophysics, 6. Accepted to Astrophysics & Space Science. 12 page

    Nanofluidic transport governed by the liquid/vapour interface

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    Liquid/vapour interfaces govern the behaviour of a wide range of systems but remain poorly understood, leaving ample margin for the exploitation of intriguing functionalities for applications. Here, we systematically investigate the role of liquid/vapour interfaces in the transport of water across apposing liquid menisci in osmosis membranes comprising short hydrophobic nanopores that separate two fluid reservoirs. We show experimentally that mass transport is limited by molecular reflection from the liquid/vapour interface below a certain length scale, which depends on the transmission probability of water molecules across the nanopores and on the condensation probability of a water molecule incident on the liquid surface. This fundamental yet elusive condensation property of water is measured under near-equilibrium conditions and found to decrease from 0.36 ± 0.21 at 30 °C to 0.18 ± 0.09 at 60 °C. These findings define the regime in which liquid/vapour interfaces govern nanofluidic transport and have implications for understanding mass transport in nanofluidic devices, droplets and bubbles, biological components and porous media involving liquid/vapour interfaces.Center for Clean Water and Clean Energy at MIT and KFUPM (Project R10-CW-09
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