在Shoemaker-Levy 9彗星碰撞后,HST对木星的光谱观测
K S Noll1, M A McGrath, L M Trafton
1Space Telescope Science Institute, Baltimore, MD 21218.
概括
哈勃望远镜的观测显示,在木星的平流层中,在G撞击后,发现了新的硫分子和金属. 这表明撞击器深入透,将木星的硫化合物带到了新的高度.
科学领域:
- 行星科学 行星科学
- 频谱学是一种光谱学.
- 大气化学 大气化学
背景情况:
- 木星的平流层组成尚未完全理解.
- 之前的研究缺乏对被撞击的木星大气层的详细分子识别.
研究的目的:
- 为了识别木星的平流层中的分子和原子,在G撞击之后.
- 为了确定撞击器的起源和透深度.
主要方法:
- 利用哈勃太空望远镜的紫外线光谱.
- 分析光谱数据以识别分子和原子物种.
主要成果:
- 确定了至少10种新的分子和原子,包括硫化合物 (S2,CS2,CS,H2S,S+) 和金属 (Mg,Si,Fe).
- 观察到大量的硫 (> 10^14 g) 和金属 (~ 10^7 g).
- 没有发现可检测的含氧分子 (SO2,SO,CO,H2O).
结论:
- 撞击器很可能起源于木星本土的一种含硫母分子.
- 碎片至少透到预测的硫化 (NH4SH) 云层.
- 平流层氨 (NH3) 的存在支持云顶以下的深层碎片透.
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