The trail of water and the delivery of volatiles to habitable planets

The trail of water and the delivery of volatiles to habitable planets
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水的踪迹和挥发物向宜居行星的输送

DOI：
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发表时间：
2019
期刊：
影响因子：
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通讯作者：
Ke Zhang
Ke Zhang
中科院分区：
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文献类型：
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作者：
K. Pontoppidan;A. Banzatti;E. Bergin;G. Blake;S. Brittain;M. Gerin;P. Goldsmith;Q. Kral;D. Leisawitz;D. Lis;M. McClure;S. Milam;G. Melnick;J. Najita;Karin Oberg;M. Richter;C. Salyk;M. Wiedner;Ke Zhang

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水是我们理解行星形成和挥发物向其表面传递的基础。然而，我们目前还没有能够全面观测它的设施，需要一个在25-600微米范围内运行的寒冷的天基天文台来解决有关行星及其水的起源的基本问题。
Water is fundamental to our understanding of the formation of planets and the delivery of volatiles to their surfaces. Yet, we currently have no facilities capable of comprehensively observing it. A cold, space-based observatory operating at 25-600 micron is needed to address fundamental questions about the origin of planets and their water.