Main (Martian crater)

http://dbpedia.org/resource/Main_(Martian_crater) an entity of type: Thing

Main es un cráter de impacto en el cuadrángulo Mare Australe de Marte, localizado en las coordenadas 76,6° Sur de latitud y 310.9° Oeste de longitud. Tiene unos 109.0 km de diámetro, y debe su nombre al reverendo Robert Main, nombre aprobado en 1973 por la Unión Astronómica Internacional.​ rdf:langString
Main è un cratere sulla superficie di Marte. Il cratere è dedicato all'astronomo britannico Robert Main. rdf:langString
曼恩陨击坑(Main)是火星南海区的一座撞击坑,其中心坐标位于南纬76.6度、西经310.9度处,直径109公里,该特征取名自十九世纪英国天文学家罗伯特·曼恩(1808年-1878年),1973年被国际天文联合会行星系统命名工作组批准接受。 曼恩陨击坑内地面显示的暗黑部分,是由春季气温上升时膨胀的二氧化碳气体所吹出尘埃而形成。如果有风,一些尘埃会形成细长的条纹。 人们提出了许多想法来解释这些特征,它们可在下面的图片中看到。 这些特征的特写视图通常会显示被称为“蜘蛛”的模糊特征。 rdf:langString
Main is an impact crater on Mars, located in the Mare Australe quadrangle at 76.6°S latitude and 310.9°W longitude. It measures 109.0 kilometers in diameter and was named after Rev. Robert Main. The name was approved in 1973, by the International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN). The floor of Main shows dark portions which are caused by pressurized carbon dioxide blowing dust in the atmosphere in the spring when the temperature goes up. Some of the dust is shaped into streaks if there is a wind. rdf:langString
rdf:langString Main (cráter marciano)
rdf:langString Cratere Main (Marte)
rdf:langString Main (Martian crater)
rdf:langString 曼恩陨击坑
xsd:integer 45374155
xsd:integer 1056260822
rdf:langString Main es un cráter de impacto en el cuadrángulo Mare Australe de Marte, localizado en las coordenadas 76,6° Sur de latitud y 310.9° Oeste de longitud. Tiene unos 109.0 km de diámetro, y debe su nombre al reverendo Robert Main, nombre aprobado en 1973 por la Unión Astronómica Internacional.​
rdf:langString Main is an impact crater on Mars, located in the Mare Australe quadrangle at 76.6°S latitude and 310.9°W longitude. It measures 109.0 kilometers in diameter and was named after Rev. Robert Main. The name was approved in 1973, by the International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN). The floor of Main shows dark portions which are caused by pressurized carbon dioxide blowing dust in the atmosphere in the spring when the temperature goes up. Some of the dust is shaped into streaks if there is a wind. Many ideas have been advanced to explain these features. These features can be seen in some of the pictures below. Close up views of these features often reveal fuzzy features that have been named "spiders."
rdf:langString Main è un cratere sulla superficie di Marte. Il cratere è dedicato all'astronomo britannico Robert Main.
rdf:langString 曼恩陨击坑(Main)是火星南海区的一座撞击坑,其中心坐标位于南纬76.6度、西经310.9度处,直径109公里,该特征取名自十九世纪英国天文学家罗伯特·曼恩(1808年-1878年),1973年被国际天文联合会行星系统命名工作组批准接受。 曼恩陨击坑内地面显示的暗黑部分,是由春季气温上升时膨胀的二氧化碳气体所吹出尘埃而形成。如果有风,一些尘埃会形成细长的条纹。 人们提出了许多想法来解释这些特征,它们可在下面的图片中看到。 这些特征的特写视图通常会显示被称为“蜘蛛”的模糊特征。
xsd:nonNegativeInteger 4142

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