A pioneering study assesses the feasibility of asteroid mining

Much remains to be known about the chemical composition of small asteroids. Their potential to harbour valuable metals, materials from the early solar system, and the possibility of obtaining a geochemical record of their parent bodies makes them promising candidates for future use of space resources. A team led by researchers from the Institute of Space Studies of Catalonia (IEEC — Institut d’Estudis Espacials de Catalunya) at the Institute of Space Sciences (ICE-CSIC) has analyzed samples of C-type asteroids, carbon-rich minor bodies of the Solar System, progenitors of the carbonaceous chondrites. 

Their findings, published in the Monthly Notices of the Royal Astronomical Society, support the idea that these asteroids can serve as crucial material sources and identify their parent bodies, as well as for planning future missions and developing new technologies for resource exploitation.

Carbonaceous chondrites fall from the sky in a natural way, although with a proportion of 5% regarding the rest of meteorite falls. However, many of them are so fragile that they fragment and are never recovered. Therefore, they are rare and are mainly located in desert regions, such as the Sahara or Antarctica. “The scientific interest in each of these meteorites is that they sample small, undifferentiated asteroids, and provide valuable information on the chemical composition and evolutionary history of the bodies from which they originate,” says Josep M. Trigo-Rodríguez, first author of the study and IEEC astrophysicist at ICE-CSIC.

The scientific team from the IEEC and ICE-CSIC selected, characterised, and provided the asteroid samples, which were analysed using mass spectrometry at the University of Castilla-La Mancha by Professor Jacinto Alonso-Azcárate. This allowed them to determine the precise chemical abundances of the six most common classes of carbonaceous chondrites, fostering the discussion among the scientific community of whether their future extraction would be feasible.

The Asteroids, Comets, and Meteorites research group at ICE-CSIC investigates the physicochemical properties of the materials that make up the surfaces of asteroids and comets and has made numerous contributions in this field over the last decade. “At ICE-CSIC and IEEC, we specialise in developing experiments to better understand the properties of these asteroids and how the physical processes that occur in space affect their nature and mineralogy,” says Trigo-Rodríguez, who leads this group.

Furthermore, for over a decade the group has been involved in selecting and requesting from NASA the several carbonaceous chondrites analysed in this study, as well as devising several experiments with them, since the ICE-CSIC is the international repository for NASA’s Antarctic meteorite collection. “The work now being published is the culmination of that team effort,” he adds.

“Studying and selecting these types of meteorites in our clean room using other analytical techniques is fascinating, particularly because of the diversity of minerals and chemical elements they contain. However, most asteroids have relatively small abundances of precious elements, and therefore the objective of our study has been to understand to what extent their extraction would be viable,” says Pau Grèbol Tomàs, IEEC predoctoral researcher at the ICE-CSIC.

“Although most small asteroids have surfaces covered in fragmented material called regolith—which would facilitate the return of small amounts of samples—developing large-scale collection systems to achieve clear benefits is a very different matter. In any case, it deserves to be explored because the search for resources in space could minimise the impact of mining activities on terrestrial ecosystems,” points out Jordi Ibáñez-Insa, researcher from Geosciences Barcelona (GEO3BCN-CSIC) and co-author of the study.

Given the diversity present in the main asteroid belt, it is crucial to define what types of resources could be found there. According to Trigo-Rodríguez: “They are small and quite heterogeneous objects, heavily influenced by their evolutionary history, particularly collisions and close approaches to the Sun. If we are looking for water, there are certain asteroids from which hydrated carbonaceous chondrites originate, which, conversely, will have fewer metals in their native state. Let’s not forget that, after 4.56 billion years since their formation, each asteroid has a different composition.”

One of the study’s conclusions is that mining undifferentiated asteroids—the primordial remnants of the solar system’s formation considered the progenitor bodies of chondritic meteorites—is still far from viable. On the other hand, the study points to a type of pristine asteroid with olivine and spinel bands as a potential target for mining. A comprehensive chemical analysis of carbonaceous chondrites is essential to identify promising targets for space mining. However, the team states that this effort must be accompanied by new sample-return missions to verify the identity of the progenitor bodies.

“Alongside the progress represented by sample return missions, companies capable of taking decisive steps in the technological development necessary to extract and collect these materials under low-gravity conditions are truly needed. The processing of these materials and the waste generated would also have a significant impact that should be quantified and properly mitigated,” adds Trigo-Rodríguez.

The team is confident of very short-term progress, given that the use of in-situ resources will be a key factor for future long-term missions to the Moon and Mars, reducing dependence on resupply from Earth. In this regard, the authors point out that if water extraction were the goal, water-altered asteroids with a high concentration of water-bearing minerals should be selected. “It sounds like science fiction, but it also seemed like science fiction when the first sample return missions were being planned thirty years ago,” says Pau Grèbol Tomàs.

In an international context, several proposals have been put forward, such as capturing small asteroids that pass close to Earth and placing them in a circumlunar orbit for exploitation. For certain water-rich carbonaceous asteroids, extracting water for reuse seems more viable, either as fuel or as a primary resource for exploring other worlds. “This could also provide science with greater knowledge about certain bodies that could one day threaten our very existence. In the long term, we could even mine and shrink potentially hazardous asteroids so that they cease to be dangerous,” Trigo-Rodríguez concludes.

Press release prepared in collaboration with the Institute of Space Sciences (ICE-CSIC).