Sub-Micrometer Particles Remote Detection in Enceladus’ Plume Based on Cassini’s UV Spectrograph Data

J. Kotlarz, Katarzyna Kubiak, N. Zalewska
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Abstract

Enceladus is the Saturnian satellite is known to have water vapor erupting from its south pole region called „Tiger Stripes”. Data collected by Cassini Ultraviolet Imaging Spectrograph during Enceladus transiting Saturn allow us to estimate water plume absorption from 1115.35–1912.50 Å and compare it to the Mie solutions of Maxwell equations for particles with a diameter in the range from 10 nm up to 2 µm. The best fit performed using Gradient Descent method indicates a presence of sub-micrometer particles of diameters: 120–180 nm and 240–320 nm consistent with Thermofilum sp., Thermoproteus sp., and Pyrobaculum sp. cell sizes present in hydrothermal vents on Earth.
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基于卡西尼号紫外线摄谱仪数据的土卫二羽流中亚微米粒子远程探测
恩克拉多斯是一颗土星卫星,已知其南极区域有被称为 "虎纹 "的水蒸气喷发。卡西尼紫外成像摄谱仪在恩克拉多斯飞越土星时收集的数据使我们能够估算出 1115.35-1912.50 Å 范围内的水羽吸收率,并将其与麦克斯韦方程中直径在 10 纳米到 2 微米之间的粒子的米解法进行比较。使用梯度下降法进行的最佳拟合表明,存在直径为 120-180 纳米和 240-33 微米的亚微米粒子:120-180纳米和240-320纳米,与地球上热液喷口中存在的热纤维菌、热蛋白菌和热杆菌的细胞大小一致。
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