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Рытвины Арран (лат. Harran Sulci) — система рытвин (рельеф из чередующихся борозд и хребтов) на спутнике Сатурна — Энцеладе.
, Gli Harran Sulci sono una struttura geologica della superficie di Encelado.
, Harran Sulci is a region of grooved terrai … Harran Sulci is a region of grooved terrain on the surface of Saturn's moon Enceladus. The feature is centered at 26.7° North Latitude, 237.6° West Longitude and is approximately 276 kilometers long. Harran Sulci bounds Diyar Planitia to the north and east. Using Voyager 2 images, Kargel and Pozio (1996) characterized Harran Sulci as consisting of 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. Recent images by the Cassini spacecraft show of Harran Sulci at much higher resolution than in the Voyager 2 images. The feature has a convex cross-section with numerous ridges running down the length of the feature. Like Samarkand Sulci, tall scarps facing the feature separate the surrounding cratered terrain to the north, and Diyar Planitia to the south, from Harran Sulci. Near the western end of the feature, two deep fracture were observed running perpendicular to Harran. Similar, but smaller, fractures are seen running perpendicular to Samarkand Sulci, suggesting that a period of extension accompanies the later stages of formation (or occurs after formation) of these ridge belts. Harran Sulci is named after the city in Arabian Nights where Khudadad's father ruled.bian Nights where Khudadad's father ruled.
, 哈爾蘭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26 … 哈爾蘭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26.7°，西經237.6° West，長約276公里。哈爾蘭溝的北邊和東邊與迪亞爾低地相鄰接。 使用航海家2號的影像，Kargel和Pozio（1996）Kargel and Pozio (1996) 哈爾蘭溝被描繪成包含彎曲的"多山的山脊"，相對於低地的高度在1-1.5公里。Kargel和Pozio（1996）認為它們可能是褶皺帶，類似北美洲的阿巴拉契亞山脈。 最近由 卡西尼 太空船拍攝的哈爾蘭溝影像有著比航海家2號更高的解析度。多數的土坎在外觀上有突起的橫斷面在長度的方向連接著，就像撒馬爾罕溝一樣，高聳的陡坡地形分散著面對環繞著的坑穴，從哈爾蘭溝的北部到迪亞爾低地的南部。靠近地形西方的終點，觀察到兩條深邃的裂口垂直的穿越哈爾蘭溝。在撒馬爾罕溝也觀測到相似、但是較小的裂縫，被認為是在這些土坎帶形成週期的後期階段（或在形成以後）發生的。 哈爾蘭溝的名字來自於一千零一夜的的父親所掌管的城市。期階段（或在形成以後）發生的。 哈爾蘭溝的名字來自於一千零一夜的的父親所掌管的城市。
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Рытвины Арран (лат. Harran Sulci) — система рытвин (рельеф из чередующихся борозд и хребтов) на спутнике Сатурна — Энцеладе.
, Gli Harran Sulci sono una struttura geologica della superficie di Encelado.
, Harran Sulci is a region of grooved terrai … Harran Sulci is a region of grooved terrain on the surface of Saturn's moon Enceladus. The feature is centered at 26.7° North Latitude, 237.6° West Longitude and is approximately 276 kilometers long. Harran Sulci bounds Diyar Planitia to the north and east. Using Voyager 2 images, Kargel and Pozio (1996) characterized Harran Sulci as consisting of 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. to North America's Appalachian Mountains.
, 哈爾蘭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26 … 哈爾蘭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26.7°，西經237.6° West，長約276公里。哈爾蘭溝的北邊和東邊與迪亞爾低地相鄰接。 使用航海家2號的影像，Kargel和Pozio（1996）Kargel and Pozio (1996) 哈爾蘭溝被描繪成包含彎曲的"多山的山脊"，相對於低地的高度在1-1.5公里。Kargel和Pozio（1996）認為它們可能是褶皺帶，類似北美洲的阿巴拉契亞山脈。 最近由 卡西尼 太空船拍攝的哈爾蘭溝影像有著比航海家2號更高的解析度。多數的土坎在外觀上有突起的橫斷面在長度的方向連接著，就像撒馬爾罕溝一樣，高聳的陡坡地形分散著面對環繞著的坑穴，從哈爾蘭溝的北部到迪亞爾低地的南部。靠近地形西方的終點，觀察到兩條深邃的裂口垂直的穿越哈爾蘭溝。在撒馬爾罕溝也觀測到相似、但是較小的裂縫，被認為是在這些土坎帶形成週期的後期階段（或在形成以後）發生的。 哈爾蘭溝的名字來自於一千零一夜的的父親所掌管的城市。期階段（或在形成以後）發生的。 哈爾蘭溝的名字來自於一千零一夜的的父親所掌管的城市。
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Harran Sulci
, Рытвины Арран
, 哈爾蘭溝
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