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从轨道上对火星液态水的全球搜索:现状与未来展望。

The Global Search for Liquid Water on Mars from Orbit: Current and Future Perspectives.

作者信息

Orosei Roberto, Ding Chunyu, Fa Wenzhe, Giannopoulos Antonios, Hérique Alain, Kofman Wlodek, Lauro Sebastian E, Li Chunlai, Pettinelli Elena, Su Yan, Xing Shuguo, Xu Yi

机构信息

Istituto di Radioastronomia, Istituto Nazionale di Astrofisica, Via Piero Gobetti 101, 40129 Bologna, Italy.

School of Atmosphere Sciences, Sun Yat-sen University, 2 Daxue Road, Xiangzhou District, Zhuhai City 519000, China.

出版信息

Life (Basel). 2020 Jul 24;10(8):120. doi: 10.3390/life10080120.

Abstract

Due to its significance in astrobiology, assessing the amount and state of liquid water present on Mars today has become one of the drivers of its exploration. Subglacial water was identified by the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) aboard the European Space Agency spacecraft Mars Express through the analysis of echoes, coming from a depth of about 1.5 km, which were stronger than surface echoes. The cause of this anomalous characteristic is the high relative permittivity of water-bearing materials, resulting in a high reflection coefficient. A determining factor in the occurrence of such strong echoes is the low attenuation of the MARSIS radar pulse in cold water ice, the main constituent of the Martian polar caps. The present analysis clarifies that the conditions causing exceptionally strong subsurface echoes occur solely in the Martian polar caps, and that the detection of subsurface water under a predominantly rocky surface layer using radar sounding will require thorough electromagnetic modeling, complicated by the lack of knowledge of many subsurface physical parameters. Higher-frequency radar sounders such as SHARAD cannot penetrate deep enough to detect basal echoes over the thickest part of the polar caps. Alternative methods such as rover-borne Ground Penetrating Radar and time-domain electromagnetic sounding are not capable of providing global coverage. MARSIS observations over the Martian polar caps have been limited by the need to downlink data before on-board processing, but their number will increase in coming years. The Chinese mission to Mars that is to be launched in 2020, Tianwen-1, will carry a subsurface sounding radar operating at frequencies that are close to those of MARSIS, and the expected signal-to-noise ratio of subsurface detection will likely be sufficient for identifying anomalously bright subsurface reflectors. The search for subsurface water through radar sounding is thus far from being concluded.

摘要

由于其在天体生物学中的重要性,评估如今火星上液态水的数量和状态已成为火星探索的驱动力之一。欧洲航天局的“火星快车”号航天器搭载的火星地下和电离层探测高级雷达(MARSIS),通过分析来自约1.5千米深处、比表面回波更强的回波,识别出了地下冰下的水。这种异常特征的原因是含水物质的相对介电常数高,导致反射系数高。出现如此强回波的一个决定性因素是MARSIS雷达脉冲在火星极冠的主要成分——冷水冰中的低衰减。目前的分析表明,导致地下回波异常强烈的条件仅出现在火星极冠,并且利用雷达探测在主要由岩石构成的表层之下探测地下水体,将需要进行全面的电磁建模,而许多地下物理参数的未知使情况变得复杂。诸如SHARAD等高频雷达探测器无法穿透足够深以探测极冠最厚部分的底部回波。诸如车载探地雷达和时域电磁探测等替代方法无法提供全球覆盖。对火星极冠的MARSIS观测一直受到在机载处理之前需要下行链路数据的限制,但未来几年其观测次数将会增加。计划于2020年发射的中国火星任务“天问一号”将携带一台地下探测雷达,其工作频率与MARSIS接近,预计地下探测的信噪比可能足以识别异常明亮的地下反射体。因此,通过雷达探测寻找地下水体的工作远未结束。

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