卡西尼宇宙尘埃分析仪在土星上的星际尘埃的流动和组成
N Altobelli1, F Postberg2, K Fiege3
1European Space Agency, European Space Astronomy Centre, Madrid, Spain. nicolas.altobelli@sciops.esa.int.
概括
来自当地的星际云的星际尘埃 (ISD) 颗粒被卡西尼航天器分析. 这些尘埃颗粒呈现出同质化的组成, 暗示星际介质中的处理.
科学领域:
- 星球科学
- 宇宙尘埃研究
- 星际介质的组成
背景情况:
- 星际尘埃 (ISD) 是星际介质的凝聚物质.
- 了解ISD的组成可以了解太阳系的过程.
研究的目的:
- 分析在土星系中发现的星际尘埃颗粒的质量分布和元素组成.
- 确定土星上的星际尘埃流量, 并推断当地的星际云中的尘埃属性.
主要方法:
- 使用卡西尼太空船上的宇宙尘埃分析仪对36颗星际尘埃进行现场分析.
- 确定质谱,元素组成和颗粒动态.
主要成果:
- 星际尘埃颗粒在土星系起源于当地的星际云.
- 谷物主要是富含的酸盐和氧化物,含有铁含量.
- 主要的形成岩石的元素 (Mg,Si,Fe,Ca) 在宇宙中大量存在;硫和碳已经耗尽.
- 证据表明星际尘埃颗粒通过星际处理同质化.
结论:
- 在土星上发现的星际尘埃提供了我们当地的星际环境的样本.
- 构成表明星际介质中的重要处理,导致同质化.
- 硫和碳的耗尽可能是处理的星际尘埃的特征.
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