Choosing Where And How To Extract Water On Mars


This is a Hubble Space Telescope photo of Mars taken when the planet was 50 million miles from Earth on May 12, 2016. Credits: NASA, ESA, the Hubble Heritage Team (STScI/AURA), J. Bell (ASU), and M. Wolff (Space Science Institute)


November 8, 2026

By Eurasia Review


Key Takeaways:

A review in Planet by Xueying Li and colleagues finds that Martian water usability depends on burial depth, material strength, thermal properties and impurities, not water content alone, requiring extraction methods matched to local geology.

Low latitudes mainly hold water in hydrated minerals needing energy-intensive heating, mid-latitudes may offer more accessible pore ice or buried glaciers, and high-latitude ice faces greater operational challenges.

Promising approaches such as in-situ thermal sublimation or Rodwell-type melting must still solve heat transfer, vapor capture, phase-change control under low pressure and impurity management before supporting life support or propellant production.

The suitability of a water resource on Mars depends on more than its water content. Burial depth, material strength, thermal properties, and impurities all influence how readily water can be extracted. For future missions, resource availability and extraction technology must therefore be evaluated together.

In a review published in Planet, Xueying Li and colleagues from Harbin Institute of Technology examine Martian water resources and the technologies proposed for their extraction. The article links the distribution and forms of occurrence of Martian water, together with the properties of water-bearing materials, to the requirements of different extraction methods.

The review examines how water resources and their accessibility vary across Martian latitudes. At low latitudes, water is commonly bound within hydrated minerals and requires heating for extraction, which can be energy-intensive. Mid-latitude regions may contain pore ice, excess ice, and buried glaciers, potentially offering a favorable balance between resource accessibility and operating conditions. High-latitude and polar regions contain extensive ice resources, but present greater environmental and operational challenges.


These differences make the selection of extraction technology highly dependent on local geological conditions. Excavation followed by heating must overcome challenges related to cutting resistance, tool wear, and limited excavation forces under low gravity. In situ thermal sublimation methods can reduce the need for excavation and material handling, but their effectiveness depends on efficient heat transfer and vapor capture.

For relatively pure, massive ice deposits, Rodwell-type systems could enable sustained water extraction through subsurface melting. However, their application on Mars would require controlling water phase changes under low atmospheric pressure, preventing borehole blockage from vapor condensation and refreezing, and managing impurity accumulation.

The review brings together geological observations and engineering considerations to assess the practical extractability of Martian water resources. This integrated perspective helps explain why a method suited to one deposit may perform poorly at another, and why water content alone is insufficient for selecting a suitable extraction site.

Further progress will depend on better characterization of subsurface water resources, more efficient extraction and purification technologies, and experimental validation under representative Martian conditions. Ultimately, these technologies must be integrated into broader resource utilization systems that support life support, propellant production, and long-term surface operations.