By David M. Harland
*Brings the tale of the Cassini-Huygens project and their joint exploration of the Saturnian method correct brand new. *Combines a overview of past wisdom of Saturn, its jewelry and moons, together with Titan, with new spacecraft ends up in one convenient quantity. *Provides the most recent and such a lot fabulous pictures, as a way to by no means have seemed sooner than in e-book shape. *Gives a context to let the reader to extra simply savor the flow of discoveries that may be made by way of the Cassini-Huygens project. *Tells the interesting tale of the Huygens spacecraft’s trip to the skin of Titan.
Read or Download Cassini at Saturn: Huygens Results (Springer Praxis Books Space Exploration) PDF
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Additional info for Cassini at Saturn: Huygens Results (Springer Praxis Books Space Exploration)
In 1867 he transported his telescope to the 9,800-foot summit of Mount Etna on Sicily, the tallest volcano in Europe, in order to observe from above most of the tropospheric water vapour, and reported aqueous vapour in Saturn's atmosphere. However, his method involved fitting a prism onto his telescope and making visual comparisons between the planet and the face of the Moon, which was presumed to be arid. Unfortunately, using a micrometer, a visual inspection and documentation of the absorption features along the dispersion could take an hour or more, during which time local atmospheric conditions could easily change, and to make any comparison it was often necessary to wait several hours for the other object to achieve the same elevation, during which time conditions could alter further.
5-inch Northumberland refractor. 5-inch refractor, independently saw two nights later, and again several times during the next week. P. Bond at the Harvard College Observatory noted a line near the inner edge of the `B' ring on 10 October, 11 November and 7 January 1851. Intriguingly, Bond did not see the marking on the `A' ring reported by Lassell and Dawes, and they did not see his line on the `B' ring. W. Tuttle at Harvard noted the `B' ring to be ``minutely subdivided into a great number of narrow rings'', starting close to its inner edge and extending over about one-third of its width, adding that ``the rings and the spaces between them were of equal breadth''.
M. Goldstein of NASA's Jet Propulsion Laboratory used the large spacecraft communications antenna at Goldstone in California as a radar to characterise the surfaces of the Moon, Mars and Venus. F. Lyot made this drawing of Saturn's ring system using the Pic du Midi Observatory's 24-inch refractor during `perfect' seeing using a high magnification and a micrometer to measure the fine detail. Although his contemporaries dismissed such fine structure as illusory, the Voyager missions spectacularly proved him correct.