富含的水将形成行星的圆盘与彗星和原恒星结合在一起
John J Tobin1, Merel L R van 't Hoff2, Margot Leemker3
1National Radio Astronomy Observatory, Charlottesville, VA, USA. jtobin@nrao.edu.
Nature
|March 8, 2023
概括
这项研究直接检测了V883 Ori原恒星盘中的气相水,揭示了其在80AU的水雪线. 测量的水
科学领域:
- 天文学与天体物理学
- 星球科学
- 天体化学
背景情况:
- 水对于行星的形成至关重要,它影响了原行星盘中的固体物质生长.
- 由于水的低化温度,水雪线和磁盘中的HDO:H2O比率尚不清楚.
- 以前的估计显示V883 Ori的水雪线在40-120AU之间.
研究的目的:
- 在V883 Ori原行星盘中直接检测气相水.
- 准确确定V883 Ori盘中的水雪线半径和HDO:H2O比率.
- 了解从恒星形成的云层到行星的水分传承.
主要方法:
- 使用先进的观测技术来检测V883奥里盘中的HDO和H2O分子.
- 分析了光谱数据以测量水的空间分布和丰度.
- 计算了盘内的HDO:H2O比率.
主要成果:
- 在V883 Ori盘中直接检测到气相水 (HDO和H2O).
- 测量了一条中平面水雪线半径约为80AU,延伸到160AU.
- 确定盘的HDO:H2O比为 (2.26 ± 0.63) × 10^-3,类似于彗星和超过地球的海洋.
结论:
- 原行星盘直接从母星形成云中继承了水.
- 水被融入冰的物体中,
- 这些发现为太阳系中行星形成和水分发的早期阶段提供了关键的见解.
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