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A soft solid surface on Titan as revealed by the Huygens Surface Science Package

机译:惠更斯表面科学软件包揭示了土卫六上的柔软固体表面

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The surface of Saturn's largest satellite - Titan - is largely obscured by an optically thick atmospheric haze, and so its nature has been the subject of considerable speculation and discussion(1). The Huygens probe entered Titan's atmosphere on 14 January 2005 and descended to the surface using a parachute system(2). Here we report measurements made just above and on the surface of Titan by the Huygens Surface Science Package(3,4). Acoustic sounding over the last 90 m above the surface reveals a relatively smooth, but not completely flat, surface surrounding the landing site. Penetrometry and accelerometry measurements during the probe impact event reveal that the surface was neither hard ( like solid ice) nor very compressible ( like a blanket of fluffy aerosol); rather, the Huygens probe landed on a relatively soft solid surface whose properties are analogous to wet clay, lightly packed snow and wet or dry sand. The probe settled gradually by a few millimetres after landing.
机译:土星最大的卫星土卫六的表面在很大程度上被光学上厚厚的大气雾所遮盖,因此其性质一直是人们进行大量猜测和讨论的主题(1)。惠更斯号探测器于2005年1月14日进入泰坦大气层,并使用降落伞系统下降至地面(2)。在这里,我们报告了由惠更斯表面科学软件包(3,4)在Titan上方和表面进行的测量。在地面上方最后90 m处的声学探测表明围绕着着陆点的表面相对较光滑,但并不完全平坦。探针撞击事件期间的渗透率和加速度测量表明,该表面既不硬(如固体冰),也不易压缩(如蓬松的气溶胶层)。惠更斯探针落在相对较软的固体表面上,其性质类似于湿粘土,轻度堆积的雪以及湿或干沙。探测器着陆后逐渐沉降几毫米。

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