![]() ![]() An annotated version of each panorama is also available to assist users with the identification of major geographic features around each Apollo landing site. Lunar surface features captured in the panoramas can be studied using zoom and pan tools. The panoramas are stitched together from individual 70mm Hasselblad frames, each of which is also accessible through this new atlas. These images provide a spectacular boots-on-the-ground view of the lunar landscape. The process of scanning lunar sample images continues and the atlas will grow in the future.Īpollo Surface Panoramas is a digital library of photographic panoramas that the Apollo astronauts took while exploring the Moon's surface. Version 1 of the atlas is being released in August 2009. Links to additional information about each sample are provided for those that have been previously described in The Lunar Sample Compendium and Lunar Sample Catalogs. The atlas contains information about the type of sample (e.g., rock, soil), the lithology (e.g., basalt, norite), and a description of the sample. ![]() LPI’s Lunar Sample Atlas provides an easily accessible library of images of the Apollo samples taken in the Lunar Sample Laboratory, full-color views of the samples in microscopic thin-sections, cutting views and diagrams that illustrate how the samples were subdivided for scientific analyses, and in situ views of the samples on the lunar surface. Furthermore, this tool provides access to additional geographic information and a high-resolution (6 m/pix) Kaguya Terrain Camera (TC) image of each sinuous rille. This atlas provides an interface with which all sinuous rilles can be observed in geographic context with Lunar Reconnaissance Orbiter Camera’s (LROC) Wide Angle Camera (WAC) image mosaics of various hemispheric views of the Moon. LPI’s Atlas of Lunar Sinuous Rilles illustrates 195 lunar sinuous rilles on the nearside and farside of the Moon. The atlas will also continue to grow with products that reflect those initial missions and, thus, should continue to assist the community with "long-term exploration and utilization" of the lunar surface. The content should assist with an initial sequence of missions. To assist the lunar community with those endeavors, the atlas compiles a set of new data products, such as topographic and slope maps, plus other content drawn from LPI's existing collections. LPI's Lunar South Pole Atlas contains a series of maps, images, and illustrations designed to support efforts to explore the lunar south pole, including NASA's plans to land astronauts there by 2024. Atlas and Hercules form a striking pair of craters on the Moon's northeastern limb.Digitized photographic images of the Moon taken from Earth with telescopes, from spacecraft orbiting the Moon, from astronauts and their equipment on the lunar surface, and by spacecraft flying by the Moon, plus digital images taken by spacecraft exploring the Moon. ![]() A further small crater, Hercules E (9 km) breaches the southern crater wall. Directly south of the central peak is Hercules G (13 km). In addition, the floor of the crater has been flooded by lava. In contrast to Atlas, however, the crater's floor is flat, smooth and shows – just visible – the tip of a central peak. Hercules has a diameter of 69 km and, like Atlas, displays terraced inner crater walls. The dark spots probably consist of pyroclastic ash deposits and suggest volcanic activity occurred a long time after the actual impact. The rille system, Rima Atlas, is of volcanic origin (as will all craters of this type), and under high illumination, at least two dark spots are visible on the crater floor (as in the crater Alphonsus). The tip of a central peak is visible and the floor of the crater is rough and fissured. Posidonius and Gassendi are other striking examples.Ītlas has strongly terraced, inner crater walls, which rise 3 km above the crater's floor. ![]() This is shown by an extensive system of rilles on the floor of the crater. The crater Atlas, with a diameter of 87 km, is a conspicuous example of the class of Fractured Floor Craters (FFC). ![]()
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