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  • 1
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    Mercury has two permanent thermal bulges. (1968)
    In:  Other Sources
    Details
    Publication Date: 2011-08-12
    Description: Mercury thermal bulges, discussing bulge contribution to dynamic stabilization of Mercury rotation
    Keywords: SPACE SCIENCES
    Format: text
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  • 2
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    Strength of synchronous rotation of the moon. (1967)
    In:  Other Sources
    Details
    Publication Date: 2011-08-11
    Description: Strength of synchronous rotation of moon in terms of upper and lower limits on rotational period, using Runge-Kutta integration
    Keywords: SPACE SCIENCES
    Type: JOURNAL OF GEOPHYSICAL RESEARCH
    Format: text
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  • 3
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    On the figure of the planet Mercury (1969)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Mercury shape estimated with isostatic form of equilibrium controlled by situation near perihelion passage at 3-2 resonance spin rate, discussing solidification thermal effects
    Keywords: SPACE SCIENCES
    Type: ; ADEMIE DES SCIENCES
    Format: text
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  • 4
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    Thermal and tidal effect on the rotation of Mercury (1970)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Thermal tidal friction and gravitation effects on Mercury libration after solidification, noting equilibrium with orbital and rotational periods locked in 3/2 resonant state
    Keywords: SPACE SCIENCES
    Type: ; YSICA STATUS SOLIDI
    Format: text
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  • 5
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    Orientation and resonance locks for satellites in the elliptic orbit. (1972)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: In order to achieve the maximum strength of higher resonance locks for satellites in the elliptic orbit, the condition of satellite orientation during the process of deployment is established. It is shown that for maximum strength locks the axis of the minimum moment of inertia of satellites should point toward the attracting body at plus or minus (5/8) pi and 0 values of the true anomaly f. This condition of deployment is applicable to all cases of resonance rotation regardless of the value of lock number k and orbit eccentricity e.
    Keywords: SPACE SCIENCES
    Type: Celestial Mechanics; 6; Dec. 197
    Format: text
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  • 6
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    Thermal elastic deformations of the planet Mercury. (1972)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: The variation in solar heating due to the resonance rotation of Mercury produces periodic elastic deformations on the surface of the planet. The thermal stress and strain fields under Mercury's surface are calculated after certain simplifications. It is found that deformations penetrate to a greater depth than the variation of solar heating, and that the thermal strain on the surface of the planet pulsates with an amplitude of .004 and a period of 176 days.
    Keywords: SPACE SCIENCES
    Type: Journal of Geophysical Research; 77; Nov. 10
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  • 7
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    Theory of rotation for the planet Mercury. (1965)
    In:  Other Sources
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    Publication Date: 2011-08-11
    Description: Planet Mercury rotation theory, applying motion of rigid system in inverse square field
    Keywords: SPACE SCIENCES
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  • 8
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    A note on the instantaneous rotational velocity of Mercury (1970)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Mercury rotational angular velocity fluctuation in terms of orbital mean motion at different orbit positions
    Keywords: SPACE SCIENCES
    Type: ; YSICA STATUS SOLIDI
    Format: text
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  • 9
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    Satellite Libration on a Elliptical Orbit (1965)
    In:  CASI
    Details
    Publication Date: 2019-05-29
    Description: Librational motion of gravitationally oriented rigid satellite in elliptic orbit studied by canonical transformation
    Keywords: SPACE SCIENCES
    Type: NASA-TM-X-56173
    Format: application/pdf
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  • 10
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    Thermal elastic deformations of the planet Mercury (1971)
    In:  CASI
    Details
    Publication Date: 2019-06-27
    Description: The variation in solar heating due to the resonance rotation of Mercury produces periodic elastic deformations on the surface of the planet. The thermal stress and strain fields under Mercury's surface are calculated after certain simplifications. It is shown that deformations penetrate to a greater depth than the variation of solar heating, and that the thermal strain on the surface of the planet pulsates with an amplitude of 0.004 and a period of 176 days.
    Keywords: SPACE SCIENCES
    Type: NASA-TM-X-65817 , X-553-71-506
    Format: application/pdf
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