首页> 外文期刊>Icarus: International Journal of Solar System Studies >Evidence for surface water ice in the lunar polar regions using reflectance measurements from the Lunar Orbiter Laser Altimeter and temperature measurements from the Diviner Lunar Radiometer Experiment
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Evidence for surface water ice in the lunar polar regions using reflectance measurements from the Lunar Orbiter Laser Altimeter and temperature measurements from the Diviner Lunar Radiometer Experiment

机译:利用农历轨道激光高度计和拆分月球辐射计试验的月球轨道激光高度计和温度测量的射击率测量的地表水冰的证据

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We find that the reflectance of the lunar surface within 5 degrees of latitude of the South Pole increases rapidly with decreasing temperature, near similar to 110 K, behavior consistent with the presence of surface water ice. The North polar region does not show this behavior, nor do South polar surfaces at latitudes more than 5 degrees from the pole. This South pole reflectance anomaly persists when analysis is limited to surfaces with slopes less than 10 degrees to eliminate false detection due to the brightening effect of mass wasting, and also when the very bright south polar crater Shackleton is excluded from the analysis. We also find that south polar regions of permanent shadow that have been reported to be generally brighter at 1064 nm do not show anomalous reflectance when their annual maximum surface temperatures are too high to preserve water ice. This distinction is not observed at the North Pole. The reflectance excursion on surfaces with maximum temperatures below 110 K is superimposed on a general trend of increasing reflectance with decreasing maximum temperature that is present throughout the polar regions in the north and south; we attribute this trend to a temperature or illumination-dependent space weathering effect (e.g. Hemingway et al., 2015). We also find a sudden increase in reflectance with decreasing temperature superimposed on the general trend at 200 K and possibly at 300 K. This may indicate the presence of other volatiles such as sulfur or organics. We identified and mapped surfaces with reflectances so high as to be unlikely to be part of an ice-free population. In this south we find a similar distribution found by Hayne et al. (2015) based on UV properties. In the north a cluster of pixels near that pole may represent a limited frost exposure. (C) 2017 Elsevier Inc. All rights reserved.
机译:我们发现,在南极的5度纬度范围内的月球表面的反射率随着温度的降低而增加,与110 k相似,与表面水冰的存在一致。北极地区没有显示出这种行为,也没有南极表面在纬度超过5度。这种南极反射率异常仍然存在,当分析限制为小于10度的斜坡的表面,以消除由于大量浪费的效果亮起而消除伪检测,并且当非常明亮的南极火山口Shackleton被排除在分析之外。我们还发现,当其年度最大表面温度过高时,据报道,据报道,据报道的永久阴影在1064纳米通常无法展示异常的反射率,不能保持水冰。北极未观察到这种区别。在110 k以下的最大温度的表面上的反射速度偏移叠加在增加反射率的一般趋势,随着南北地区的整个极地地区的最大温度降低;我们将这种趋势归因于温度或照明依赖空气风化效果(例如Hemingway等,2015)。我们还发现反射率的突然增加,降低温度叠加在200 k的一般趋势上,并且可能在300K时呈现。这可能表明存在其他挥发物如硫或有机物。我们识别和映射表面,这非常高,不太可能成为无冰群的一部分。在这个南方,我们发现Hayne等人发现了类似的分布。 (2015)基于UV属性。在北部,杆附近的像素簇可以代表有限的霜冻曝光。 (c)2017年Elsevier Inc.保留所有权利。

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