•  
  •  
 

Bulletin of Chinese Academy of Sciences (Chinese Version)

Keywords

tethered dual-satellite system, lunar resources, Earth–Moon material transport, in-situ resource utilization, deep-space exploration strategy

Abstract

Lunar exploration is undergoing a paradigm shift from resource mapping to mechanism identification. Key processes, such as the modulation of volatiles by magnetic anomalies and the contribution of Earth wind to surface hydration, require strictly synchronized observations of magnetic-field gradients, particle fluxes, spectrally detected volatiles, and subsurface hydrogen within the same spatiotemporal window. However, a still-unfilled “near-lunar-surface intermediate layer” gap exists between conventional single-spacecraft orbiters and landed rovers: the capability for multi-altitude, multi-parameter, strictly synchronized process observations. A tethered dual-satellite system, consisting of a main satellite and a subsatellite connected by a 5–10 km short tether, naturally provides a dual-altitude observational baseline and, for the first time, links remote-sensing-based mapping with near-surface mechanism diagnosis into a complete chain of evidence. Its scientific outputs can be organized into three “resource accounts”—primary resources, implanted resources, and usable resources—and further extended to quantitative studies of Earth–Moon material transport. China already possesses the full set of technological elements needed to build a cross-sphere collaborative exploration system integrating satellite orbit, near space, and ground-based observations. The tethered dual-satellite system represents a key node for transferring this capability to the near-lunar-surface environment and constitutes an indispensable diagnostic link between robotic/crewed lunar exploration and the construction of a lunar research station.

First page

1489

Last Page

1499

Language

Chinese

Publisher

Bulletin of Chinese Academy of Sciences

References

[1] Lucey P G, Blewett D T, Jolliff B L. Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images. Journal of Geophysical Research: Planets, 2000, 105(E8): 20297-20305.

[2] Jolliff B L, Wieczorek M A, Shearer C K, et al. New Views of the Moon. Chantilly: Mineralogical Society of America, 2006.

[3] 魏勇, 林红磊, 何飞, 等. 深空探测科技制高点上的新焦点:月球水资源. 中国科学院院刊, 2024, 39(5): 899-906. Wei Y, Lin H L, He F, et al. New frontier in race for deep space exploration: Lunar water resources. Bulletin of Chinese Academy of Sciences, 2024, 39(5): 899-906. (in Chinese)

[4] Wei Y, Zhong J, Hui H, et al. Implantation of Earth’s atmospheric ions into the nearside and farside lunar soil: Implications to geodynamo evolution. Geophysical Research Letters, 2020, 47(3): e2019GL086208.

[5] Baliukin I I, Bertaux J L, Quémerais E, et al. SWAN/SOHO Lyman-α mapping: The hydrogen geocorona extends well beyond the Moon. Journal of Geophysical Research: Space Physics, 2019, 124(2): 861-885.

[6] Pieters C M, Goswami J N, Clark R N, et al. Character and spatial distribution of OH/H₂O on the surface of the Moon seen by M³ on Chandrayaan-1. Science, 2009, 326: 568-572.

[7] Kramer G Y, Besse S, Dhingra D, et al. M³ spectral analysis of lunar swirls and the link between optical maturation and surface hydroxyl formation at magnetic anomalies. Journal of Geophysical Research: Planets, 2011, 116(E9): 2010JE003729.

[8] Wei Y. Planet wind: Planetary evolution dominated by electromagnetic forces. Science China Earth Sciences, 2024, 67(10): 3331-3336.

[9] Ozima M, Seki K, Terada N, et al. Terrestrial nitrogen and noble gases in lunar soils. Nature, 2005, 436: 655-659.

[10] Terada K, Yokota S, Saito Y, et al. Biogenic oxygen from Earth transported to the Moon by a wind of magnetospheric ions. Nature Astronomy, 2017, 1: 26.

[11] Wang H Z, Zhang J, Shi Q Q, et al. Earth wind as a possible exogenous source of lunar surface hydration. The Astrophysical Journal Letters, 2021, 907(2): L32.

[12] Zuber M T, Smith D E, Lehman D H, et al. Gravity recovery and interior laboratory (GRAIL): Mapping the lunar interior from crust to core. Space Science Reviews, 2013, 178(1): 3-24.

[13] Elphic R C, Delory G T, Hine B P, et al. The Lunar atmosphere and dust environment explorer mission. Space Science Reviews, 2014, 185(1): 3-25.

[14] Hemingway D, Garrick-Bethell I. Magnetic field direction and lunar swirl morphology: Insights from Airy and Reiner Gamma. Journal of Geophysical Research: Planets, 2012, 117(E10): 2012JE004165.

[15] Cosmo M L, Lorenzini E C. Tethers in Space Handbook. Cambridge: Smithsonian Astrophysical Observatory, 1997.

[16] 魏勇. 行星科学一级学科建设:“鸿鹄专项”的探索与实践. 科学通报, 2020, 65(14): 1295-1296. Wei Y. Construction of Planetary Science as a first-level scientific discipline: Exploration and practice of Scientific Experiment System in Near Space (SENSE) Program. Chinese Science Bulletin, 2020, 65(14): 1295-1296. (in Chinese)

[17] Li C L, Wang C, Wei Y, et al. China’s present and future lunar exploration program. Science, 2019, 365: 238-239.

Share

COinS