Mare Smythii, located on the equator and east limb of the Moon, has a great variety of scientific and economic uses as the site for a permanent lunar base. Here a complex could be established that would combine the advantages of a nearside base (for ease of communications with Earth and normal operations) with those of a farside base (for shielding a radio astronomical observatory from the electromagnetic noise of Earth). The Mare Smythii region displays virtually the entire known range of geological processes and materials found on the Moon; from this site, a series of field traverses and investigations could be conducted that would provide data on and answers to fundamental questions in lunar geoscience. This endowment of geological materials also makes the Smythii region attractive for the mining of resources for use both on the Moon and in Earth-Moon space. We suggest that the main base complex be located at 0, 90 deg E, within the mare basalts of the Smythii basin; two additional outposts would be required, one at 0, 81 deg E to maintain constant communications with Earth, and and the other, at 0, 101 deg E on the lunar farside, to serve as a radio astronomical observatory. The bulk of lunar surface activities could be conducted by robotic teleoperations under the direct control of the human inhabitants of the base.


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    Titel :

    Geological and geophysical field investigations from a lunar base at Mare Smythii


    Beteiligte:
    Spudis, Paul D. (Autor:in) / Hood, Lon L. (Autor:in)


    Erscheinungsdatum :

    1992-09-01


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch




    Lunar geological field investigations

    Swann, G. A. | NTRS | 1968


    Cracking of lunar mare soil.

    Jaffe, L. D. | NTRS | 1971


    Ages of lunar mare surfaces

    Ronca, L. B. | NTRS | 1971


    Thicknesses of Lunar Mare flow fronts

    Gifford, A. W. / El-Baz, F. | NTRS | 1981


    How thick are lunar mare basalts

    Hoerz, F. | NTRS | 1978