Many small bodies in the solar system, including planetary satellites, comets, and asteroids, have a surface component consisting at least in part of a very low albedo (0.06 or less) solid substance of neutral or red color in the wavelength region 0.3-2.5 microns. Laboratory spectra of organic residues from meteorites and mixtures with hydrous silicates suggest that complex mixtures of complex organic molecules (kerogens) together with aqueous alteration products of igneous minerals may be the source of the dark matter that is distributed so widely throughout the solar system.


    Access

    Access via TIB

    Check availability in my library


    Export, share and cite



    Title :

    Dark matter in the solar system


    Contributors:

    Published in:

    Publication date :

    1987-01-01



    Type of media :

    Miscellaneous


    Type of material :

    No indication


    Language :

    English


    Keywords :


    Dark matter in the solar system

    Cruikshank, Dale P. | Elsevier | 1987


    Dark matter in the outer solar system

    Owen, T. / Cruikshank, D. / De Bergh, C. et al. | NTRS | 1994


    Dark Matter in the Outer Solar System

    Owen, T. / Cruikshank, D. / De Bergh, C. et al. | British Library Conference Proceedings | 1995


    Dark Matter in the Outer Solar System

    Owen, T. | Online Contents | 1995


    Extrasolar solar-sail trajectories and dark matter

    Matloff, Gregory L. | Online Contents | 2014