在NEAR-shoemaker航天器与埃罗斯相遇期间的无线电科学结果
1Navigation and Mission Design Section, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. Department of Terrestrial and Planetary Geodesy, Centre National d'Etudes Spatiales, Toulouse, France. Applied.
概括
研究人员使用航天器数据精确测量了小行星433 Eros的质量和旋转. 这颗小行星433 Eros的旋转稳定,密度均,表明其表面覆盖着石质.
科学领域:
- 行星科学 行星科学
- 小行星动力学 小行星动力学
- 太空飞船任务分析
背景情况:
- 小行星433埃罗斯是一颗近地小行星,是了解小行星形成和演变的重要科学兴趣的目标.
- 之前的研究缺乏对Eros物理性质的精确测量,阻碍了详细的动态和组成分析.
研究的目的:
- 确定小行星433 Eros的精确质量,引力波和旋转状态.
- 为了推断埃罗斯的质量密度和内部结构.
- 分析表面动态和埃罗斯的物质运输潜力.
主要方法:
- 利用了来自近地小行星聚会 (NEAR) -鞋匠航天器的地面多普勒和距离跟踪数据.
- 分析了小行星433 Eros表面地标的图像,以限制其形状和旋转.
主要成果:
- 确定埃罗斯的质量为 (6.687 ± 0.003) x 10^18克,产生一个散装密度为2.67 ± 0.03 g/cm^3.3.
- 建立了Eros的稳定旋转状态,没有可测量的旋转极的自由前行.
- 计算的表面逃逸速度在3.1到17.2m/s之间,表明有 regolith覆盖的表面.
结论:
- 小行星433 Eros具有均的密度分布.
- 动态环境表明有显著的规质覆盖面和物质运输到重力潜力井的潜力.
- 稳定的旋转和确定的物理参数为未来的小行星探索和建模提供了关键数据.
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