彗星C/1999 S4 (LINEAR) 在近日期前和分裂后的成像和光度测量
T L Farnham1, D G Schleicher, L M Woodney
1Department of Astronomy, University of Texas, Austin, TX 78712, USA. farnham@astro.as.utexas.edu
概括
这颗彗星是C/LINEAR彗星.
科学领域:
- 彗星科学是一门彗星科学.
- 天文学 天文学
- 天体物理学 天体物理学
背景情况:
- 彗星C/LINEAR在距离太阳最近 (周日) 之前经历了一次分裂事件.
- 了解彗星的组成和结构完整性对于太阳系进化研究至关重要.
研究的目的:
- 分析C/LINEAR彗星的光度测量和图像.
- 为了确定核的分裂前的大小和组成.
- 确定时间并推断彗星解体的原因.
主要方法:
- 对分手前和后的数据进行光度分析.
- 核成像和旋转状态建模.
- 在尘埃尾部分解后的质量估计.
主要成果:
- 彗星的核在破裂之前的半径至少为0.44公里.
- 与其他彗星相比,彗星C/LINEAR的碳链分子较少.
- 解体始于2000年7月18-19日左右,受到旋转状态的限制.
- 尘埃尾中含有3 x 10^8公斤的分离后质量.
结论:
- 彗星C/LINEAR的大部分原始质量很可能是从1毫米到50米的碎片.
- 彗星的低碳链丰富性可能与其结构上的弱点和破裂有关.
相关概念视频
X-ray Imaging
German physicist Wilhelm Röntgen (1845–1923) was experimenting with electrical current when he discovered that a mysterious and invisible "ray" would pass through his flesh but leave an outline of his bones on a screen coated with a metal compound. In 1895, Röntgen made the first durable record of the internal parts of a living human: an "X-ray" image (as it came to be called) of his wife’s hand. Scientists worldwide quickly began their own experiments with X-rays, and by 1900, X-ray was widely...
Flame Photometry: Lab
In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...


