Extraterrestrial oceans may be composed of water or other elements and compounds. The only confirmed large stable bodies of extraterrestrial surface liquids are the lakes of Titan, although there is evidence for the existence of oceans elsewhere in the Solar System. Early in their geologic histories, Mars and Venus are theorized to have had large water oceans. The Mars ocean hypothesis suggests that nearly a third of the surface of Mars was once covered by water, and a runaway greenhouse effect may have boiled away the global ocean of Venus.
Los océanos extraterrestres pueden estar compuestos de agua u otros elementos y compuestos. Los únicos grandes cuerpos estables confirmados de líquidos superficiales extraterrestres son los lagos de Titán, aunque hay evidencia de la existencia de océanos en otras partes del Sistema Solar. Al principio de sus historias geológicas, se teoriza que Marte y Venus tuvieron grandes océanos de agua. La hipótesis del océano de Marte sugiere que casi un tercio de la superficie de Marte estuvo alguna vez cubierta por agua, y un efecto invernadero desbocado puede haber evaporado el océano global de Venus.
Les océans extraterrestres peuvent être composés d'eau ou d'autres éléments et composés. Les seuls grands corps stables confirmés de liquides de surface extraterrestres sont les lacs de Titan, bien qu'il existe des preuves de l'existence d'océans ailleurs dans le système solaire. Au début de leur histoire géologique, Mars et Vénus auraient eu de grands océans aquatiques. L'hypothèse de l'océan de Mars suggère que près d'un tiers de la surface de Mars était autrefois recouverte d'eau, et un effet de serre incontrôlable pourrait avoir fait bouillir l'océan global Vénus.
Außerirdische Ozeane können aus Wasser oder anderen Elementen und Verbindungen bestehen. Die einzigen bestätigten großen stabilen Körper außerirdischer Oberflächenflüssigkeiten sind die Seen von Titan, obwohl es Hinweise auf die Existenz von Ozeanen an anderer Stelle im Sonnensystem gibt. Zu Beginn ihrer geologischen Geschichte wurde angenommen, dass Mars und Venus große Wassermeere hatten. Die Mars-Ozean-Hypothese legt nahe, dass fast ein Drittel der Marsoberfläche einst von Wasser bedeckt war und ein außer Kontrolle geratener Treibhauseffekt den globalen Ozean der Venus weggekocht haben könnte.
Gli oceani extraterrestri possono essere composti da acqua o altri elementi e composti. Gli unici grandi corpi stabili confermati di liquidi superficiali extraterrestri sono i laghi di Titano, sebbene ci siano prove dell'esistenza di oceani in altre parti del Sistema Solare. All'inizio delle loro storie geologiche, si teorizza che Marte e Venere abbiano avuto grandi oceani d'acqua. L'ipotesi dell'oceano di Marte suggerisce che quasi un terzo della superficie di Marte era una volta coperta dall'acqua e un effetto serra in fuga potrebbe aver fatto evaporare l'oceano globale di Venere.
Os oceanos extraterrestres podem ser compostos de água ou outros elementos e compostos. Os únicos grandes corpos estáveis confirmados de líquidos superficiais extraterrestres são os lagos de Titã, embora haja evidências da existência de oceanos em outras partes do Sistema Solar. No início de suas histórias geológicas, teoriza-se que Marte e Vênus tiveram grandes oceanos de água. A hipótese do oceano de Marte sugere que quase um terço da superfície de Marte já foi coberto por água, e um efeito estufa descontrolado pode ter evaporado o oceano global de Vênus.
Внеземные океаны могут состоять из воды или других элементов и соединений. Единственными подтвержденными крупными стабильными телами внеземных поверхностных жидкостей являются озера Титана, хотя есть доказательства существования океанов в других частях Солнечной системы. В начале своей геологической истории предполагается, что Марс и Венера имели большие водные океаны. Гипотеза об океане Марса предполагает, что почти треть поверхности Марса когда-то была покрыта водой, и неконтролируемый парниковый эффект, возможно, испарил глобальный океан Венеры.
地球外の海洋は、水または他の要素と化合物で構成されている可能性があります。 太陽系の他の場所に海が存在するという証拠はありますが、地球外表面液体の確認された大きな安定した物体はタイタンの湖だけです。 火星と金星の地質史の初期には、大きな海があったと理論化されています。 火星の海の仮説は、火星の表面のほぼ3分の1がかつて水で覆われていたことを示唆しており、暴走温室効果が金星の全球海を沸騰させた可能性があります。
地外海洋可能由水或其他元素和化合物組成。 儘管有證據表明太陽係其他地方存在海洋,但唯一確認的大型外星表面液體穩定體是泰坦湖。 在地質歷史的早期,火星和金星被認為擁有廣闊的水域海洋。 火星海洋假說表明,近三分之一的火星表面曾經被水覆蓋,而且失控的溫室效應可能使金星全球海洋沸騰了。
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