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Detection of ammonia on Pluto’s surface in a region of geologically recent tectonism

机译:在最近地质构造区域中冥王星表面的氨气探测

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摘要

We report the detection of ammonia (NH3) on Pluto’s surface in spectral images obtained with the New Horizons spacecraft that show absorption bands at 1.65 and 2.2 μm. The ammonia signature is spatially coincident with a region of past extensional tectonic activity (Virgil Fossae) where the presence of H2O ice is prominent. Ammonia in liquid water profoundly depresses the freezing point of the mixture. Ammoniated ices are believed to be geologically short lived when irradiated with ultraviolet photons or charged particles. Thus, the presence of NH3 on a planetary surface is indicative of a relatively recent deposition or possibly through exposure by some geological process. In the present case, the areal distribution is more suggestive of cryovolcanic emplacement, however, adding to the evidence for ongoing geological activity on Pluto and the possible presence of liquid water at depth today.
机译:我们报告了在“新视野”号飞船获得的光谱图像中检测到冥王星表面的氨(NH3),该图像显示了1.65和2.2μm的吸收带。氨气特征在空间上与过去的伸展构造活动区域(维吉尔·福萨(Virgil Fossae))重合,在该区域中H 2 O冰的存在很明显。液态水中的氨会大大降低混合物的凝固点。据信,用紫外线光子或带电粒子照射时,氨化冰在地质上寿命短。因此,在行星表面上存在NH3表示相对较新的沉积或可能通过某些地质过程的暴露。在目前的情况下,面积分布更暗示了冰冷的火山作用,但是,增加了有关冥王星上正在进行的地质活动以及今天深处可能存在液态水的证据。

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