一个行星形成盘中的原始冰被沉重的水暴露出来
Margot Leemker1, John J Tobin2, Stefano Facchini1
1Dipartimento di Fisica, Università degli Studi di Milano, Milan, Italy.
概括
行星形成盘中的水分子是从早期恒星形成阶段继承的. 在V883 Ori盘中的双重化水 (D2O) 提供了强有力的证据证明这种星际起源,将云与彗星联系起来.
科学领域:
- 天体化学是天体化学.
- 行星科学 行星科学
- 星星形成 星星形成
背景情况:
- 水从星际云到行星的旅程对于理解行星的形成和可居住性至关重要.
- 彗星和系外行星中水的起源 (星际遗传与磁盘再处理) 仍然是一个关键问题.
研究的目的:
- 通过分析水同位素比率来研究原行星盘中的水的起源.
- 为了确定水分子是从星际介质中继承的还是在磁盘内重塑的.
主要方法:
- 使用先进的天文技术观测V883 Ori盘.
- 测量双化水 (D2O) 和其他水同位素 (HDO,H2O).
- 观察到的D2O/H2O和D2O/HDO比率与原星和彗星的模型和已知的值进行比较.
主要成果:
- 强有力的证据表明,由于V883 Ori磁盘中D2O水平的提高,导致水的继承.
- 测量的D2O/H2O比率为 (3.2 ± 1.2) × 10^-5,与星际值一致,并且明显高于磁盘再处理的预期值.
- 较重的同位素的高化 (D2O/HDO = (2.3 ± 1.0) × HDO/H2O) 进一步支持遗传假说.
结论:
- 原行星盘中的水冰起源于恒星形成的最早阶段.
- 这项研究提供了冷星际云中的水与彗星和系外行星中发现的水之间的关键联系.
- 这些发现支持了将水送到新生行星的遗传模型.
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