![]() ![]() ![]() It uses the pre-Latinized names (" Alpine Valley", etc.), and is numbered in the corner with quadrant numbers, although more detailed maps for the quadrants do not seem to have been distributed with it. This map labels most primary and selected satellite features. Before that, Rükl published a south-up "Skeleton Map of the Moon" at a scale of 1:6000000 (roughly 22.5 in diameter) which was distributed with Kopal's Photographic Atlas of the Moon (1965).The maps in the Hamlyn Atlas were preceded by a set of six Maps of the Lunar Hemispheres, published in 1972, which covered the entire Moon in orthographic views, but in less detail.For example, a little to the left of center, one small crater is shown on the floor of Palus Putredinis, but two more prominent ones to its north are omitted (note : this is the officially unnamed pair of bowl-shaped craters immediately west of NASA's Hill 305, also known as the southern part of the Fresnel Ridge). Not only is the nomenclature not always complete or reliable, but in the process of artistic interpretation certain features are emphasized and others lost. Note that Rükl's map consists essentially of a line-and-shadow rendering of the Lunar Orbiter imagery augmented with some low relief and albedo features interpreted from images with higher and lower sun angle.| class="imageCaption" | Rükl's Atlas map (right) compared to more modern IAU photographic atlas (left) The following image compares a detail from Rükl's Atlas (Sheet 22, right) with the comparable area as seen in the newer Lunar Orbiter-based IAU/USGS on-line Digital Atlas ( Sheet 41, left, much reduced):.The current authorized edition of Rükl's Atlas of the Moon is said to be available from Sky Publishing, although it is reportedly out-of-stock. Reproductions of Rükl's maps can be found on a number of websites.Rükl's maps do not show all IAU-approved satellite feature names (at the time the maps were being prepared, the IAU did not maintain an official list of lettered craters), and in a very few cases his labels are erroneous or ambiguous. In recent years, printed maps of this sort have been somewhat supplanted by electronic products which are generally more flexible, and can be more easily updated to reflect changes in the official nomenclature and avoid inadvertent errors. Rükl uses the traditional system of labeling satellite features by their letters only, placed on the side towards the parent feature after which it is named.Although this is a private publication, Rükl has generally striven to adhere to the IAU nomenclature as closely as possible. Atlas was so strong that he supported the weight of the Universe on his shoulders.Description This series of careful maps of the Moon's nearside and libration zones, created by the former director of the Prague Planetarium, is widely regarded by amateur astronomers as the indispensable observing guide to lunar features. ![]() Atlas was ordered by Zeus to uphold the vault of the sky after the defeat of the Titans. Originally designated S/1980 S28, this moon is named after Atlas, a Titan, and a son of Iapetus. But as many new moons were discovered, scientists began selecting names from more mythologies including Gallic, Inuit, and Norse stories. Moons of Saturn were originally named for Greco-Roman Titans and descendants of the Titans. It orbits 85,544 miles (137,670 km) away from, taking 14.4 hours to complete its trip around the planet. The small, pointy moon has a mean radius of 9.4 miles (15.1 km). Cassini images revealed in 2004 that a temporary faint ring of material with the orbit of Atlas. ![]() Like Pan, Atlas has a distinctive flying saucer shape created by a prominent equatorial ridge not seen on the other small moons of Saturn. OverviewĪtlas is an inner moon of Saturn, orbiting around the outer edge of Saturn's A Ring. Terrile and the Voyager 1 team from photographs taken during its encounter with Saturn. ![]()
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