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Statements

Subject Item
dbr:Marius_Hills
rdf:type
yago:Idea105833840 yago:Abstraction100002137 yago:Content105809192 yago:Concept105835747 yago:PsychologicalFeature100023100 yago:WikicatGeologicalFeaturesOnTheMoon yago:Property105849040 yago:Cognition100023271 yago:Feature105849789
rdfs:label
Marius Hills 馬利厄斯丘陵 Collines Marius Marius Mendixkak
rdfs:comment
Les collines Marius sont une région de (en) situé dans l'océan des Tempêtes sur la face visible de la Lune. Ces dômes lunaires seraient formés de laves beaucoup plus visqueuses que celles qui ont formé la mer lunaire. Ce dômes dont 200 à 500 m de haut. Les collines tiennent leur nom du cratère proche de 41 km de diamètre à proximité nommé Marius. Cette région représente la plus grande concentration de formations volcaniques sur la Lune. Marius Mendixkak Ilargiko Oceanus Procellarum ean kokatutako domo bolkaniko multzo bat da. Uste denez ilargi-itsasoen sorrerarekin batera laba biskotsuagoak sortu zituen. Gutxi gora behera 200 eta 500 metro arteko altuera dute. Euren izena 41 kilometrora dagoen hartzen dute. Ilargiko ezaugarri bolkanikoen kontzentraziorik altuena hemen ematen da. 馬利厄斯丘陵是月球的風暴洋中一系列的火山熔岩穹丘之一。這些圓形的頂被認為是由熔岩形成的,比那些形成海的熔岩更具粘性。這些圓頂的平均高度約為200-500米(660-1,640英尺)。馬利厄斯丘陵的名字來自附近直徑為41公里(25英里)的隕石坑馬利厄斯。。這些丘陵顯示了月球表面火山地形最集中的地區。 The Marius Hills are a set of volcanic domes located in Oceanus Procellarum on Earth's Moon. The domes are thought to have formed from lavas fairly more viscous than those that formed lunar mares. These domes average approximately 200–500 m (660–1,640 ft) in height. The Marius Hills take their name from the nearby 41 km (25 mi) diameter crater Marius. These hills represent the highest concentration of volcanic features on the Moon.
foaf:depiction
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dbo:abstract
Marius Mendixkak Ilargiko Oceanus Procellarum ean kokatutako domo bolkaniko multzo bat da. Uste denez ilargi-itsasoen sorrerarekin batera laba biskotsuagoak sortu zituen. Gutxi gora behera 200 eta 500 metro arteko altuera dute. Euren izena 41 kilometrora dagoen hartzen dute. Ilargiko ezaugarri bolkanikoen kontzentraziorik altuena hemen ematen da. Domo, kono eta kanal bolkanikoen ugaritasuna dago eskualde honetan. Lunar Reconnaissance Orbiter sateliteak bertan ere lurrazpiko laba hodi bat izan daitekeenaren sarrera aurkitu zuen, zapaia kolapsatu zela ikusiz. Zulo horren luzera 80 eta 88 metro artean kalkulatzen da, eta bere zabalera ehunka metrokoa dela kalkulatu da. Etorkizunean emango balitz, erradiaziotik babesteko lekua izan liteke. 馬利厄斯丘陵是月球的風暴洋中一系列的火山熔岩穹丘之一。這些圓形的頂被認為是由熔岩形成的,比那些形成海的熔岩更具粘性。這些圓頂的平均高度約為200-500米(660-1,640英尺)。馬利厄斯丘陵的名字來自附近直徑為41公里(25英里)的隕石坑馬利厄斯。。這些丘陵顯示了月球表面火山地形最集中的地區。 Les collines Marius sont une région de (en) situé dans l'océan des Tempêtes sur la face visible de la Lune. Ces dômes lunaires seraient formés de laves beaucoup plus visqueuses que celles qui ont formé la mer lunaire. Ce dômes dont 200 à 500 m de haut. Les collines tiennent leur nom du cratère proche de 41 km de diamètre à proximité nommé Marius. Cette région représente la plus grande concentration de formations volcaniques sur la Lune. The Marius Hills are a set of volcanic domes located in Oceanus Procellarum on Earth's Moon. The domes are thought to have formed from lavas fairly more viscous than those that formed lunar mares. These domes average approximately 200–500 m (660–1,640 ft) in height. The Marius Hills take their name from the nearby 41 km (25 mi) diameter crater Marius. These hills represent the highest concentration of volcanic features on the Moon.
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