首页> 外文期刊>Icarus: International Journal of Solar System Studies >Oceans on Mars: The possibility of a Noachian groundwater-fed ocean in a sub-freezing martian climate
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Oceans on Mars: The possibility of a Noachian groundwater-fed ocean in a sub-freezing martian climate

机译:火星上的海洋:在冻结火星气候中Noachian地下水喂水的可能性

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The Noachian climate of Mars is thought by many to have been "warm and wet", characterized by a global mean annual temperature (MAT) > 273 K and abundant rainfall infiltrating into the groundwater system. In this "warm and wet" scenario, when the groundwater system was in contact with the surface in the northern lowlands, a groundwater-fed ocean could form. In contrast, 1-dimensional climate models and 3-dimensional general circulation models (GCMs) are unable to reproduce long-lived, continuous "warm and wet" conditions due to the influence of the faint young Sun when considering a pure CO2-H2O atmosphere; these models instead predict "cold and icy" conditions, characterized by MAT similar to 225 K and water trapped as snow and ice in the southern highlands. Furthermore, a kilometers-thick globally continuous cryosphere is predicted in this "cold and icy" scenario, precluding direct connection of the groundwater system and the surface, and disfavoring a Noachian northern lowlands ocean. However, global MAT values lack information about regional and seasonal temperature variations, which may vary significantly from global MAT. In this work, we explore whether regional or seasonal temperature variations could permit the formation of a Noachian ocean in a climate with global MAT < 273 K. We use a combination of a 3D climate model and a 1D thermal model to determine the climatic conditions in which the required criteria for groundwater release could be met: (1) temperatures above 273 K, required for there to be no cryosphere preventing the groundwater from being released onto the surface, and (2) a sufficiently large groundwater reservoir, required for the groundwater table to intersect the surface. Our results suggest that the formation of a groundwater-fed ocean does not require a continuous and long-lived "warm and wet" climate with global MAT > 273 K. If the long-lived Noachian global MAT was > 255 K (similar to 30 K above the nominal ambient "cold and icy" climate
机译:Mars的Noachian气候被许多人认为“温暖湿润”,其特点是全球平均年度温度(垫子)> 273 k和充足的降雨渗透到地下水系统中。在这种“温暖和潮湿的”情景中,当地下水系统与北部低地的表面接触时,地下水喂养的海洋可以形成。相比之下,由于微弱的幼小阳光在考虑纯二氧化碳-H2O气氛时,1维气候模型和三维通用循环模型(GCMS)无法再现长寿,连续的“温暖和潮湿”的条件;这些模型代替预测“冷和冰冷”的条件,其特征在于垫子,南部高地作为雪和冰困难的225 k和水。此外,在这种“冷酷和冰冷”的情景中预测了一公里厚的全球连续冰冻层,排除地下水系统和地面的直接连接,以及不憎恶Noachian Northern Leglands海洋。然而,全球垫子值缺乏有关区域和季节性温度变化的信息,这可能与全球垫子显着变化。在这项工作中,我们探讨了区域或季节性温度变化是否可以在具有全球垫子的气候中形成一个Noachian海洋<273 K.我们使用3D气候模型和1D热模型的组合来确定气候条件可以满足地下水释放所需标准:(1)在273 k以上的温度,没有冰区所需的,防止地下水释放到表面上,(2)地下水所需的足够大的地下水储层。表格与表面相交。我们的研究结果表明,地下水喂养的海洋的形成不需要连续和长期的“温暖和潮湿”的气候与全球垫子> 273 k。如果长寿的Noachian全球垫子> 255 k(类似于30高于标称环境“冷酷和冰冷”的气候

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