Search Results - "Scattergood, W."

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    Structural features required for ligand binding to the beta‐adrenergic receptor by Dixon, R. A., Sigal, I. S., Candelore, M. R., Register, R. B., Scattergood, W., Rands, E., Strader, C. D.

    Published in The EMBO journal (01-11-1987)
    “…On the basis of the homology between the amino acid sequences of the beta‐adrenergic receptor (beta AR) and the opsin proteins we have proposed that the ligand…”
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    Journal Article
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    High-temperature shock formation of N2 and organics on primordial Titan by Mckay, Christopher P., Pollack, James B., Borucki, William J., Van Ghyseghem, Hilde T., Scattergood, Thomas W.

    Published in Nature (London) (07-04-1988)
    “…Theoretical models suggest that the initial form of nitrogen in Titan's atmosphere may have been NH3. The possible importance of strong shocks produced during…”
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    Laboratory experiments in the study of the chemistry of the outer planets by Scattergood, T W

    Published in Advances in space research (1987)
    “…The investigation of chemical evolution of bodies in our solar system has, in the past, included observations, theoretical modeling, and laboratory…”
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    Production of organic compounds in plasmas: a comparison among electric sparks, laser-induced plasmas, and UV light by Scattergood, T W, McKay, C P, Borucki, W J, Giver, L P, Van Ghyseghem, H, Parris, J E, Miller, S L

    Published in Icarus (New York, N.Y. 1962) (01-10-1989)
    “…The chemistry in planetary atmospheres that is induced by processes associated with high-temperature plasmas is of broad interest because such processes may…”
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    The role of cometary particle coalescence in chemical evolution by Oberbeck, V. R., Mckay, C. P., Carle, G. C., Valentin, J. R., Scattergood, T. W.

    “…Important prebiotic organic compounds might have been transported to earth in dust or produced in vapor clouds resulting from atmospheric explosions or impacts…”
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    The physical nature of Titan's aerosols: Laboratory simulations by Scattergood, T.W.

    Published in Advances in space research (01-03-1995)
    “…The atmosphere of Titan is known to contain aerosols, as evidenced by the Voyager observations of at least three haze layers. Such aerosols can have…”
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    Laboratory investigations of Mars: chemical and spectroscopic characteristics of a suite of clays as Mars soil analogs by Banin, A, Carle, G C, Chang, S, Coyne, L M, Orenberg, J B, Scattergood, T W

    “…Two major questions have been raised by prior explorations of Mars. Has there ever been abundant water on Mars? Why is the iron found in the Martian soil not…”
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    Exobiology research on Space Station Freedom by Huntington, J.L, Stratton, D.M, Scattergood, T.W

    Published in Advances in space research (01-03-1995)
    “…The Gas-Grain Simulation Facility (GGSF) is a multidisciplinary experiment laboratory being developed by NASA at Ames Research Center for delivery to Space…”
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    High-Temperature Shock Formation of N(2) and Organics on Primordial Titan by McKay, Christopher P, Scattergood, Thomas W, Pollack, James B, Borucki, William J, Van Ghyseghem, Hilde T

    Published in Nature (London) (07-04-1988)
    “…Titan's atmosphere is composed primarily of N2 with a little methane and other organic molecules. But theoretical models suggest that the initial form of…”
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    Gas chromatographic instrumentation for the analysis of aerosols and gases in Titan's atmosphere by Scattergood, T W, Valentin, J R, O'Hara, B J, Kojiro, D R, Carle, C G

    Published in Journal of geophysical research (30-03-1987)
    “…During the next decade or so, NASA, in conjunction with the European Space Agency, plans to send a spacecraft to the Saturnian system so that local studies of…”
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    The physical nature of Titan's aerosol - Laboratory simulations by Scattergood, T W

    Published in Advances in space research (01-03-1995)
    “…The atmosphere of Titan is known to contain aerosols, as evidenced by the Voyager observations of at least three haze layers. Such aerosols can have…”
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    Journal Article
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