Thetis regio
WebTo the south of Thetis Regio in Aphrodite lies Artemis (see Figure 3-14), one of the most enigmatic features on Venus. Magellan will begin mapping Artemis in late November 1990. Artemis is a large circular feature about 2,600 kilometers (1,616 miles) in diameter, with relatively raised topography surrounded by a deep narrow trough. WebJan 26, 2004 · The Diana Chasma quadrangle (V–37), an equatorial region between 0° to 25° S. and 150° to 180° E. that encompasses ~8,400,000 km 2, is broadly divided into southern Rusalka Planitia in the north, eastern Aphrodite Terra in the central region, and unnamed regions to the south. Geologic mapping constrains the temporal and spatial relations ...
Thetis regio
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WebIts western extremity consists of two large curving ridges that partially surround a broad circular region of low-lying rugged terrain. Most of Aphrodite is formed by two broad … WebThe highland terrain in southeast Thetis Regio consists of a series of thrust faults and conjugate graben that would usually be classified as tesserae. Unusually, this small area …
WebFor Thetis Regio, crustal thicknesses may exceed 50 km. The thickened crust of Thetis Regio may also have been rifted and embayed by plains forming lavas. The lavas appear … WebRestaurants near Twantay, Yangon Region: See Tripadvisor traveller reviews of dining near Twantay and search by cuisine, price, location, and more.
WebThe region (25º-0º N., 150º-180º E.) is framed by the crustal plateau Thetis Regio to the southwest, the coronae of the Diana-Dali chasmata complex to the south, and volcanic rise Atla Regio to the west. Regions to the north, and the quadrangle itself, are part of the vast lowlands, which cover four-fifths of the surface of Venus. WebInternational Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN)
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WebThe highland terrain in southeast Thetis Regio consists of a series of thrust faults and conjugate graben that would usually be classified as tesserae. Unusually, this small area … my old vhs tapes 87-03 and moreWeb[1] The highland terrain in southeast Thetis Regio consists of a series of thrust faults and conjugate graben that would usually be classified as tesserae. Unusually, this small area … old roman recipesWebA 400-km-scale strike-slip zone near the boundary of Thetis Regio, Venus. 2003 • George Tuckwell. Download Free PDF ... valuesare found aroundthe marginsof Ovda and Thetis Tominim/zetheeffectsof theformertypeof mismatchon our Regiones,in westernAphrodite,andnearArtemisChasma. evaluation,theVenera15/16mapof tessera … old roman provincesWebVenus. In this paper a small region of Thetis Regio, south-east of the main block, is demonstrated to be an area of more recent tesserae formation that may offer an insight … my old walletold roman paintings of womenWebThetis Regio V-36 0-25° S 120-150° E Diana Chasma V-37 0-25° S 150-180° E Stanton V-38 0-25° S 180-210° E Taussig V-39 0-25° S 210-240° E Galindo V-40 0-25° S 240-270° E Phoebe Regio: V-41 0-25° S 270-300° E Navka Planitia V-42 0-25° S 300-330° E Carson V-43 0-25° S 330-360° E Kaiwan Fluctus old roman ruler crosswordWebMar 1, 2012 · This study is based on the results of photogeologi cal mapping of the Thetis Regio (Burba, 1988) on Venus: map V 36, 0°-25° S, 120°-150° E (Basilevsky and Head, … old roman road iter