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Models of organic-rich surfaces in the outer solar system.

机译:外太阳系中富含有机物的表面的模型。

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摘要

This thesis applies light-scattering theory along with recently-measured optical constants of astronomically-interesting organic materials in an attempt to understand the surfaces of representative organic-rich bodies in the outer Solar System.; The Centaur 5145 Pholus has a visible and near-ir spectrum redder than any other object in the Solar System. Its color can be reproduced by an intraparticle mixture of water ice, Titan tholin, and either astronomical silicate or polymerized hydrogen cyanide. The solar UV flux, combined with surface gardening by micrometeoroids, will convert all carbon-bearing ices to dark organic solids in the top millimeter of Kuiper Belt Objects in {dollar}{lcub}sim{rcub}10sp7{dollar} yrs. Initially red, further irradiation makes the surface more neutral. If impacts expose fresh ice over a large fraction of the object's surface on a similar time scale, an average red color may be retained. The color diversity observed in the Centaur and Kuiper Belt populations thus can be explained by a variation in the average exposure ages of their surfaces.; The dark material on the leading hemisphere of Iapetus has a spectrum that is too generic, lacking in absorption features, to strongly constrain models of its composition; many mixtures of water ice, organics, and/or silicates can reproduce its albedo and spectrum. Several mechanisms have been proposed to explain why one hemisphere of Iapetus is extremely dark while the other hemisphere is very bright, but this thesis finds major flaws in most of them. A scheme postulating a global, several-km-thick layer of dark material covered by a layer of ice {dollar}sim{dollar}1-m thick, but which is excavated on the leading hemisphere, works best.; Finally, the impacts of the fragments of Comet Shoemaker-Levy 9 into Jupiter left behind dark atmospheric blemishes that may be composed of organic matter. The optical constants of the blemish aerosols--as derived by others--are near-perfect matches to Murchison organic residue. The reflectances of the initial impact plumes and the thermal pulse during plume collapse are inconsistent with the blemish aerosols, so the organic matter had to have formed in situ, rather than being cometary debris.
机译:本文将光散射理论与最近测量的对天文学感兴趣的有机材料的光学常数一起应用,以试图了解外部太阳系中典型的富含有机物的物体的表面。半人马座5145 Pholus的可见光谱和近红外光谱比太阳系中的任何其他物体都要红。水冰,泰坦索林和天文硅酸盐或聚合氰化氢的颗粒内混合物可再现其颜色。太阳紫外线通量加上微流星体的表面园艺作用,将在{dollar} {lcub} sim {rcub} 10sp7 {dollar}年内,在柯伊伯带天体的最高毫米处将所有含碳冰转化为深色有机固体。最初呈红色,进一步照射使表面更中性。如果撞击在相似的时间范围内将新鲜的冰暴露在物体表面的很大一部分上,则可能会保留平均红色。因此,在半人马和柯伊伯带种群中观察到的颜色多样性可以用它们表面平均暴露年龄的变化来解释。伊阿佩图斯前半球的深色物质的光谱太笼统,缺乏吸收特性,因此无法强烈限制其组成模型。水冰,有机物和/或硅酸盐的许多混合物可以复制其反照率和光谱。提出了几种机制来解释伊阿佩特斯的一个半球为何如此黑暗而另一半球却非常明亮的现象,但本论文发现其中大多数存在重大缺陷。一种方案是假设一个全球性的,厚达几公里的暗物质层,该层覆盖着一层厚达1米的冰,但该层是在前半球上发掘的,效果最佳。最后,彗星鞋匠征途9碎片撞击木星的过程中留下了可能由有机物组成的深色大气污点。瑕疵气溶胶的光学常数(由其他人得出)与Murchison有机残留物几乎完美匹配。初始撞击羽流的反射率和羽流塌陷期间的热脉冲与微弱的气溶胶不一致,因此有机物必须原位形成,而不是彗星碎屑。

著录项

  • 作者

    Wilson, Peter Derrick.;

  • 作者单位

    Cornell University.;

  • 授予单位 Cornell University.;
  • 学科 Physics Astronomy and Astrophysics.
  • 学位 Ph.D.
  • 年度 1997
  • 页码 244 p.
  • 总页数 244
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;
  • 关键词

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