彗星81P/Wild 2的矿物学和岩石学核样本
Michael E Zolensky1, Thomas J Zega, Hajime Yano
1Astromaterials Research and Exploration Science, NASA Johnson Space Center, Houston, TX 77058, USA. michael.e.zolensky@nasa.gov
概括
彗星Wild 2的样本显示了颗粒的结构较弱的混合物,表明形成条件多样化和水性变化最小. 一个耐火粒子表明原行星盘中的早期辐射运输.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 彗星科学 彗星科学
背景情况:
- 彗星样本提供了对早期太阳系材料的直接洞察.
- 星尘任务从彗星81P/Wild 2返回了样本,为它的组成提供了独特的窗口.
研究的目的:
- 分析彗星81P/Wild 2的矿物质和组成特征.
- 推断彗星Wild 2的形成条件和演化历史.
主要方法:
- 用先进的显微镜和光谱学分析返回的彗星样本.
- 颗粒大小,矿物成分和化学组合的表征.
主要成果:
- 彗星Wild 2的样本主要由微弱聚合的纳米尺度颗粒组成.
- 较大的颗粒包括铁磁酸盐,Fe-Ni硫化物和Fe-Ni金属.
- 橄烯和烯的广泛组成范围表明了不同的形成位置.
- 限制的硫化物成分和缺少水性相表明水性变化有限.
- 一个耐火粒子暗示了原行星盘内的辐射运输.
结论:
- 野生2彗星是在各种各样的条件下形成的,可能是在原行星盘的不同区域.
- 彗星经历的水性变化很小,甚至没有.
- 耐火材料的存在表明早期太阳系中存在重要的辐射运输过程.
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