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Argyre Planitia is a plain located within the impact basin Argyre in the southern highlands of Mars. Its name comes from a map produced by Giovanni Schiaparelli in 1877; it refers to Argyre, a mythical island of silver in Greek mythology. Argyre is centered at and lies between 35° and 61° S and 27° and 62° W in the Argyre quadrangle. The basin is approximately wide and drops below the surrounding plains; it is the second deepest impact basin on Mars after Hellas. The crater Galle, located on the east rim of Argyre at , strongly resembles a smiley face. The basin was possibly formed by a giant impact during the Late Heavy Bombardment of the early Solar System, approximately 3.9 billion years ago, and may be one of the best preserved ancient impact basins from that period. Argyre is surrounded by rugged massifs which form concentric and radial patterns around the basin. Several mountain ranges are present, including Charitum and Nereidum Montes.〔http://www.planetary.brown.edu/pdfs/2563.pdf Hiesinger & Head: Topography and morphology of the Argyre Basin, Mars〕 Four large Noachian epoch channels lie radial to the basin. Three of these channels (Surius Valles, Dzígai Valles, and Palacopas Valles) flowed into Argyre from the south and east through the rim mountains. The fourth, Uzboi Vallis, appears to have flowed out from the basin's north rim to the Chryse region and may have drained a lake of melting ice within the basin. A smaller outflow channel named Nia Valles is relatively fresh-looking, and probably formed during the early Amazonian after the major fluvial and lacustrine episodes had finished.〔http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000LPI....31.2033P&link_type=ARTICLE&db_key=AST&high= Parker et al.: Argyre Planitia and the Mars Global Hydrologic Cycle〕 The original basin floor is buried with friable, partially deflated layered material that may be lake sediment. No inner rings are visible; however, isolated massifs within the basin may be remnants of an inner ring.〔 An article written by 22 researchers in Icarus concluded that the impact that formed the Argyre basin probably stuck an ice cap or a thick permafrost layer. Energy from the impact melted the ice and formed a giant lake that eventually sent water to the North. The lakes's volume was equal to that of Earth's Mediterranean Sea. The deepest part of the lake may have taken more than a hundred thousand years to freeze, but with the help of heat from the impact, geothermal heating, and dissolved solutes it may have had liquid water for many millions of years. Life may have developed in this time. This region shows a great deal of evidence of glacial activity with flow features, crevasse-like fractues, drumlines, eskers, tarns, aretes, cirques, horns, U-shaped valleys, and terraces. Because of the shapes of Argyre sinuous ridges, the authors agree with previous publications in that they are eskers. Based on morphometrical and geomorphological analysis of the Argyre eskers and their immediate surroundings, it was suggested that they formed beneath an approximately 2 km thick, stagnant (i.e., stationary) ice sheet around 3.6 billion years ago. This stagnant body of ice might have resembled a Piedmont-style glacier comparable to today's Malaspina Glacier in Alaska. ==Gallery== File:Mars atmosphere 2.jpg|The southern rim of Argyre basin, formed by the Charitum Montes. Adjacent are sinuous ridges, theorized to be glacial eskers. The crater Galle is seen in the background. Image:Argyre basin topo.jpg|MOLA maps showing the geographic context of Argyre. Wikimolaargyre.jpg|MOLA map showing boundaries for Argyre Planitia and other regions File:Gullies in the southern highlands of Mars.jpg|Gullies south of Argyre appear to be unequivocal evidence of water erosion. Image:24808multilevelgullies.jpg|Scene in Argyre quadrangle with gullies, alluvival fans, and hollows, as seen by HiRISE under HiWish program. Enlargements of parts of this image are below. Image:24808multiplefans.jpg|Several levels of alluvial fans, as seen by HiRISE under HiWish program. Locations of these fans are indicated in the previous image. Image:24808smallfan.jpg|Small, well-formed alluvial fan, as seen by HiRISE under HiWish program. Location of this fan is shown in an image displayed above. Image:24808hollows.jpg|Enlargement of above image showing hollows with box showing the size of a football field, as seen by HiRISE under HiWish program. Image:ESP 022685 dunesandgullieslabeled.jpg|Gullies, as seen by HiRISE under HiWish program. Location is Nereidum Montes. Image:Surface features in Argyre.jpg|Surface in Argyre quadrangle as seen by HiRISE, under the HiWish program. This is the image of the surface from a single HiRISE image. The scale bar at the top is 500 meters long. Image:Context image for argyrefeatures.JPG|CTX image showing context for the next image. A group of channels are visible in this image. Image:Close-up of Argyrefeatures.JPG|Close-up of surface in Argyre quadrangle, as seen by HiRISE, under the HiWish program. 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Argyre Planitia」の詳細全文を読む スポンサード リンク
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