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The origin and specific features of the martian satellites in the context of the euruption concept
Earth, Moon, and Planets, 1988 The numerous problems related to the origin and evolution of Phobos and Deimos, as well as to specific features of their topography, are readily accounted for in the context of a concept presupposing the possibility of detonation (or burning) of electrolyzed ices.
E. M. Drobyshevski
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Bounded Martian satellite relative motion
Celestial Mechanics and Dynamical Astronomy, 2021zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Guy Marcus, Pini Gurfil
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GETEMME – A Mission to Explore the Martian Satellites and the Limits of Solar System Physics
, 2011 We propose a mission to Mars and its satellites Phobos and Deimos, within the ESA COSMIC VISION program. A spacecraft (S/C) shall deploy retroreflectors on each satellite. These reflectors will act as targets for laser ranging from a Martian orbit for a wide range of science applications in Solar System Dynamics and Fundamental Physics.
Oberst, Jürgen +2 more
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A history of the discovery and positional observation of the Martian satellites; 1877–1977
New Astronomy Reviews, 1978D Pascu
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The motion of the Martian satellites
Celestial Mechanics, 1975An extensive analysis of the motion of Phobos and Deimos from 1877 to 1973 has been fulfilled. The new values of the parameters of the orbital model first developed by Struve have been determined for both satellites. The new sets of the orbital parameters compete with the solutions of similar accuracy found by Wilkins and Sinclair.
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A Comparative Analysis and Study on Martian Satellites
International Journal of Engineering Trends and Technology, 2014The use of satellites in communication systems is very much a fact of everyday life, as is evidenced by the many homes equipped with antennas or dishes used for the reception of satellite television. Satellites offer a number of features not readily available with other means of communication.
Revathy P Nair +2 more
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Dusty Plasma near the Martian Satellite Deimos
Plasma Physics Reports, 2018The formation of dusty plasma in the near-surface layer above the illuminated part of the Deimos, the satellite of Mars, due to photoelectric and electrostatic processes is analyzed. Using a physicomathematical model self-consistently describing the densities of photoelectrons and dust grains above the illuminated part of Deimos, the distribution ...
S. I. Popel +2 more
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