Download Dynamic Planet: Mercury in the Context of Its Environment by Pamela Elizabeth Clark PDF
By Pamela Elizabeth Clark
This is an inter-disciplinary e-book masking a number disciplines written to demonstrate the character and dynamic interactions of Mercury with its atmosphere and therefore to be obtainable ( through minimizing discipline-specific jargon) to engineers and scientists in addition to these making plans to be engineers and scientists on the higher point university scholar or ‘educated layman’ point or above.
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Extra resources for Dynamic Planet: Mercury in the Context of Its Environment (2007)(en)(220s)
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Witteborn, D. Cruikshank, Mercury’s feldspar connection mid-IR measurements suggest plagioclase, Adv in Space Research, 19, 1507-1510, 1997. P. L. W. K. L. 5um) observations show heterogeneous composition, presence of intermediate and basic soil types, and pyroxene, Met Plan Sci, 37, 1255 -1268, 2002. , Dynamo generation in Mercury, Nature, 256, 634, 1975. , Applications of liquid state physics to the Earth’s core. Phys. Earth Planet. , 22, 42-52, 1980. , Mercury’s magnetic field: a thermoelectric dynamo?
Safronov, Formation of Mercury and removal of its silicate shell, In Mercury, Eds. Vilas, Chapmen, Matthews (Univ. Arizona Press), pp. 667-669, 1988. , Constitution of terrestrial planets; Phil. Trans. R. Lond. A 303, 287-302, 1981. , G. Colombo, F. Franklin, Secular resonance, solar spin down, and orbit of Mercury, Icarus, 28, 441-452, 1976. Wasson, J. , The building stones of the planets. In Mercury, Eds. Vilas, Chapman, Matthews (Univ. Arizona Press), pp. 622-650, 1988. , Iron/silicate fractionation and the origin of Mercury, Icarus, 35, 99-111, 1978.
What surprises and unresolved issues did the Mariner 10 mission leave in its wake? 2. Compare the MESSENGER and Bepi Colombo missions. How would you improve either mission and what would be the impact on spacecraft resources (mass, power, bandwidth) and cost. 3. Discuss what spatial and temporal resolutions and coverage will be provided by instruments on both missions, and the adequacy and limitations of this instrumentation in revealing the dynamic character of Mercury’s interaction with its environment.