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Samarkand Sulci is a region of grooved ter … Samarkand Sulci is a region of grooved terrain on the surface of Saturn's moon Enceladus. The feature is centered at 30.5° North Latitude, 326.8° West Longitude and is approximately 383 kilometers long. Samarkand Sulci consists of three parts. The southern and eastern extensions bound Sarandib Planitia on its western and northern sides, respectively. The northern portions extends into a region of cratered terrain. Using Voyager 2 images, Kargel and Pozio (1996) found that the northern and southern/eastern extensions of this feature are likely distinct features with different origins and ages. The portions surrounding Sarandib Planitia were characterized as sinuous "mountainous ridges" 1-1.5 km in height, and lying within relative topographic lows. Kargel and Pozio (1996) suggested that they might be fold belts, similar to North America's Appalachian Mountains. The northern portion of Samarkand Sulci was found to consist of linear fractures, suggesting that rather than a compressional fold belt, the northern part of Samarkand Sulci may in fact be an extensional rift. Based on analysis of crater counts in both areas of Samarkand Sulci, Kargel and Pozio (1996) suggested that the rift formed before the ridges. Recent images by the Cassini spacecraft show portions of Samarkand Sulci at much higher resolution than in the Voyager 2 images. Numerous parallel ridges are resolved in the southern and eastern extensions of the feature, though some ridges appear chevron shaped. Just as Kargel and Pozio (1996) found parts of this feature lying within topographic lows, sharp scarps bound the ridge belts in several regions. On the far eastern tip of Samarkand Sulci, these scarps begin to converge as the ridge belts disappear, forming narrow canyons. Northern Samarkand Sulci was also observed. This region appears unconsolidated with several craters, like Ahmad and Peri-Banu, appearing to be cross-cut or even flooded by this portion of Samarkand Sulci. Near the southern end of Samarkand Sulci, curious dark patches, 500–750 m across were observed lying along ridge crests. It is possible these spots may be collapse pits. Samarkand Sulci is named after the country ruled over by Shah Zaman, brother of Shahryar, in Arabian Nights.n, brother of Shahryar, in Arabian Nights.
, Рытвины Самарканд (лат. Samarkand Sulci) — система рытвин (рельеф из чередующихся борозд и хребтов) на поверхности Энцелада (спутника Сатурна). Примерные координаты — 30°00′ с. ш. 327°30′ з. д. / 30° с. ш. 327,5° з. д..
, Samarkand Sulci è una regione di Encelado, … Samarkand Sulci è una regione di Encelado, un satellite naturale di Saturno con delle scanalature nel terreno, è situata a 30,5° latitudine nord e 326,8° longitudine ovest ed è lunga 383 chilometri.È stata individuata dalla sonda Voyager 2 e in seguito è stata fotografata dalla sonda Cassini.o è stata fotografata dalla sonda Cassini.
, 撒馬爾罕溝是在土星的衛星恩克拉多斯表面上具溝狀的地形之一。這個地點的中心位置在北緯3 … 撒馬爾罕溝是在土星的衛星恩克拉多斯表面上具溝狀的地形之一。這個地點的中心位置在北緯30.5°，西經326.8°，長度大約有383公里。撒馬爾罕溝包括3個部份，它的南部和東部延伸至（Sarandib Planitia）相對的是鄰近它的西側和北側，北部延伸至坑洞的地形。 使用航海家2號的影像，Kargel和Pozio（1996）發現這個地區的北部和南部／或者東部可能有著不同的起源和年齡。圍攏著薩藍迪普低地的部分被描繪成彎曲的"多山的山脊"，相對於低地的高度在1-1.5公里。Kargel和Pozio（1996）認為它們可能是皺褶帶，類似北美洲的阿巴拉契亞山脈。撒馬爾罕溝的北部被發現是包含線性的，被認為是的皺褶，撒馬爾罕溝的北部也許實際上是的。基於對撒馬爾罕溝這兩個地區的坑洞計數，Kargel和Pozio（1996）認為裂口比山脊更早形成。 最近由 卡西尼 太空船拍攝的撒馬爾罕溝影像有著比航海家2號更高的解析度。雖然有些土坎出現山形的形狀，在南部和東部有許多平行土坎延伸的特徵被解晰出來。一如Kargel和Pozio（1996）發現的地形學上的特徵，一些地區的陡坡出現明顯的陡坡帶。在撒馬爾罕溝的最東邊，而這些陡坡開始聚合而土坎坡帶消失，形成狹窄的峽谷。北撒馬爾罕溝也被觀察了，這個地區看上去有幾個坑穴疏鬆的散佈著，像是和，看起來撒馬爾罕溝的這一部分似乎曾經被洪水切割過的。 接近撒馬爾罕溝南端結束處，有些直徑在500-750公尺黑暗的斑塊，被觀察到沿著土坎的冠部橫躺著，這些斑點可能是崩潰的坑穴。 撒馬爾罕溝是以阿拉伯之夜這本書中的國家撒馬爾罕命名的。，這些斑點可能是崩潰的坑穴。 撒馬爾罕溝是以阿拉伯之夜這本書中的國家撒馬爾罕命名的。
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Samarkand Sulci è una regione di Encelado, … Samarkand Sulci è una regione di Encelado, un satellite naturale di Saturno con delle scanalature nel terreno, è situata a 30,5° latitudine nord e 326,8° longitudine ovest ed è lunga 383 chilometri.È stata individuata dalla sonda Voyager 2 e in seguito è stata fotografata dalla sonda Cassini.o è stata fotografata dalla sonda Cassini.
, Samarkand Sulci is a region of grooved ter … Samarkand Sulci is a region of grooved terrain on the surface of Saturn's moon Enceladus. The feature is centered at 30.5° North Latitude, 326.8° West Longitude and is approximately 383 kilometers long. Samarkand Sulci consists of three parts. The southern and eastern extensions bound Sarandib Planitia on its western and northern sides, respectively. The northern portions extends into a region of cratered terrain. Near the southern end of Samarkand Sulci, curious dark patches, 500–750 m across were observed lying along ridge crests. It is possible these spots may be collapse pits.possible these spots may be collapse pits.
, 撒馬爾罕溝是在土星的衛星恩克拉多斯表面上具溝狀的地形之一。這個地點的中心位置在北緯3 … 撒馬爾罕溝是在土星的衛星恩克拉多斯表面上具溝狀的地形之一。這個地點的中心位置在北緯30.5°，西經326.8°，長度大約有383公里。撒馬爾罕溝包括3個部份，它的南部和東部延伸至（Sarandib Planitia）相對的是鄰近它的西側和北側，北部延伸至坑洞的地形。 使用航海家2號的影像，Kargel和Pozio（1996）發現這個地區的北部和南部／或者東部可能有著不同的起源和年齡。圍攏著薩藍迪普低地的部分被描繪成彎曲的"多山的山脊"，相對於低地的高度在1-1.5公里。Kargel和Pozio（1996）認為它們可能是皺褶帶，類似北美洲的阿巴拉契亞山脈。撒馬爾罕溝的北部被發現是包含線性的，被認為是的皺褶，撒馬爾罕溝的北部也許實際上是的。基於對撒馬爾罕溝這兩個地區的坑洞計數，Kargel和Pozio（1996）認為裂口比山脊更早形成。 最近由 卡西尼 太空船拍攝的撒馬爾罕溝影像有著比航海家2號更高的解析度。雖然有些土坎出現山形的形狀，在南部和東部有許多平行土坎延伸的特徵被解晰出來。一如Kargel和Pozio（1996）發現的地形學上的特徵，一些地區的陡坡出現明顯的陡坡帶。在撒馬爾罕溝的最東邊，而這些陡坡開始聚合而土坎坡帶消失，形成狹窄的峽谷。北撒馬爾罕溝也被觀察了，這個地區看上去有幾個坑穴疏鬆的散佈著，像是和，看起來撒馬爾罕溝的這一部分似乎曾經被洪水切割過的。去有幾個坑穴疏鬆的散佈著，像是和，看起來撒馬爾罕溝的這一部分似乎曾經被洪水切割過的。
, Рытвины Самарканд (лат. Samarkand Sulci) — система рытвин (рельеф из чередующихся борозд и хребтов) на поверхности Энцелада (спутника Сатурна). Примерные координаты — 30°00′ с. ш. 327°30′ з. д. / 30° с. ш. 327,5° з. д..
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Samarkand Sulci
, 撒馬爾罕溝
, Рытвины Самарканд
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