在Ryugu regolith中,有分子云和流体化学的证据
Maitrayee Bose1, Robert A Root2, Yunbin Guan3
1School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.
Science advances
|July 24, 2024
概括
在Ryugu小行星颗粒中发现的硫化合物揭示了早期太阳系化学的洞察力. 异常的硫同位素表明起源于分子云,扩大了我们对外星有机分子形成的理解.
科学领域:
- 太空化学 太空化学
- 天体生物学 天体生物学
- 行星科学 行星科学
背景情况:
- 小行星Ryugu中硫的化学成分尚未被充分探索.
- 硫化合物可以追踪分子云化学和小体过程.
研究的目的:
- 识别和描述Ryugu粒子中的有机硫和硫酸盐粒.
- 研究这些材料中硫和氧的同位素组成.
- 确定这些化合物的形成和生存条件.
主要方法:
- 对瑞古粒子 (A0070和A0093) 的分析.
- 对硫 (Δ33S) 和氧 (δ17O, δ18O) 的同位素分析.
- 标识有机硫化合物和硫酸盐颗粒.
主要成果:
- 在Ryugu粒子中发现了有机硫和硫酸盐粒.
- 硫酸盐颗粒呈现质量独立的硫同位素分离 (Δ33S = +5 ± 2每毫米).
- 硫酸盐颗粒上的甲类涂层显示异常的同位素 (δ15N = +62 ± 2每毫米).
结论:
- 硫化合物可能在Ryugu的母体上形成并存活在水中变化的过程中.
- 形成条件涉及减少环境,低温和性pH与富含N的有机物.
- 异常的硫,源于分子云中的H2S光解离,在一个延伸的日心区中发现.
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