What do we need to know to mine an asteroid?
September 19, 2017

European Planetary Science Congress 2017 Press Notice
Tuesday, 19th September

What do we need to know to mine an asteroid?

The mining of resources contained in asteroids, for use as propellant, building materials or in life-support systems, has the potential to revolutionise exploration of our Solar System. To make this concept a reality, we need to increase our knowledge of the very diverse population of accessible Near Earth Asteroids (NEA). Last year, dozens of the world’s leading asteroid scientists and asteroid mining entrepreneurs came together in Luxembourg to discuss key questions and identify scientific knowledge gaps. A White Paper outlining the results of that discussion, “Answers to Questions from the Asteroid Miners” will be presented at the European Planetary Science Congress (EPSC) 2017 in Riga on Tuesday 19th September by Dr JL Galache and Dr Amara Graps.

“Asteroid mining is this incredible intersection of science, engineering, entrepreneurship and imagination,” says Galache of Aten Engineering. “The problem is, it’s also a classic example of a relatively young scientific field in that the more we find out about asteroids through missions like Hayabusa and Rosetta, the more we realise that we don’t know.”

The aim of the Asteroid Science Intersections with In-Space Mine Engineering (ASIME) 2016 conference on September 21-22, 2016 in Luxembourg City was to provide an environment for the detailed discussion of the specific properties of asteroids, with the engineering needs of space missions that utilise asteroids. Outcomes of ASIME 2016 Conference produced a layered record
of discussions from the asteroid scientists and the asteroid miners to understand each other’s key concerns.

The White Paper covers questions surrounding the need for asteroid surveys in preparing for mining missions, the asteroid’s surface and interior, implications for astrobiology and planetary protection and other questions relating to policy and strategy for developing a roadmap for advancing asteroid in-space resource utilisation.

A number of knowledge gaps were identified: the asteroid miners need access to a map of known NEAs with an orbit similar to the Earth so that they can fine-tune their selection of potential targets. Many objects are – as yet – undiscovered, or very little is known about them, so there is also a need to develop a dedicated NEA discovery and follow-up programme.

Galache explains: “NEAs are usually discovered when they are at their brightest, so our best chance of studying them is by immediately following up detections with further observations to characterise their shape and spectral properties. That needs good quality, relatively large, dedicated telescopes that are available at short notice. We don’t have reliable access to these facilities right now.”

Further studies are needed to understand the link between meteorites and asteroids, and to share data more widely about the composition of meteorites so that more accurate simulant asteroid soils, or “regolith”, can be created. This is important for understanding which asteroids hold which resources, and for preparing for the practical side of a mining mission, such as landing and extraction of material.

“Aside from samples returned from a handful of missions, the only way we can study the composition of asteroids is by analysing light reflected from their surfaces, or by examining fragments that have landed on Earth in the form of meteorites,” says Graps of the University of Latvia and the Planetary Science Institute, Tucson, Arizona. “Both these techniques have limitations. Spectral observations come from the ‘top veneer’ of the asteroid, which has been space weathered and subjected to other kinds of processing. Meteorites are crucial, but they also lack part of the story: fragile constituents of primitive material contained within asteroids may be lost during atmospheric entry. At the moment, our mapping of types of meteorites back to the different classes of parent asteroid is not that robust.”

Three quarters of known asteroids are classed as Carbonaceous or “C-type”, dark, carbon-rich objects. However, most NEAs are from the Silicaceous “S-type” class of asteroids, which are reddish-coloured stony bodies that dominate the inner Asteroid Belt. For asteroid miners looking for water to use in rocket fuel or life support systems, being able to identify the class of asteroid is vital. Carbonaceous chondrite meteorites have been found to contain clay minerals that appear to have been altered by water on their parent body. While these meteorites are thought to be derived from sub-classes of C-type asteroids, there is not an exact match with any single spectral class.

A short-cut to understanding an NEA’s composition could be to identify where in the Solar System they formed and look at the characteristics of their “orbital family”. Thus, another knowledge gap is the link is between the dynamical predictions of where an NEA originates and its actual physical characterisations.

Information is also sparse on the size of grains at the surface of the asteroid. The asteroids Eros and Itokawa have similar spectral signatures and reflectiveness, but rendezvous missions show that they have very different regolith properties. NEAR Shoemaker showed that Eros is covered in fine dust, while Hayabusa revealed that the surface of Itokawa has chunky blocks tens of centimetres in diameter. Comprehensive knowledge of regolith properties at asteroids’ surface and subsurface will be vital for developing strategies for landing and extracting materials. However, as yet, no mission has explored how asteroid regolith might vary with depth.

“Results from ESA’s Rosetta mission showed that the surface of comet 67P/Churyumov Gerasimenko is much denser than its interior. It may be that we’ll find the same thing if we dig down into the regolith of NEAs. But at the moment, we just don’t know,” said Graps.

More work also needs to be done to understand the dynamics of granular material in low-gravity. Studies suggest that granular material can behave as a solid, a liquid or a gas in this environment. This behaviour will be particularly important for asteroids that are rubble-piles, as spacecraft trying to land or drill into these could easily destabilise regolith causing granular flow or avalanches.

“Asteroid mining techniques will need to adapt to the low-gravity environment. Possible solutions include cancelling out action-reaction forces by digging in opposite directions at the same time, or by producing a reaction force, such as by strapping a net around the asteroid for robots to grab onto while they dig,” says Galache. “It’s a challenge! But answering the questions posed in this White Paper will be an important first step.”

Further Information

The ASIME 2016 workshop was supported by Europlanet 2020 RI, the Luxembourg Ministry of the Economy, SpaceResources.lu and the European Space Agency.

The thirty ASIME 2016 contributors to the White Paper were: JL Galache, Amara L. Graps (lead author), Philippe Blondel, Grant Bonin, Daniel Britt, Simone Centuori, Marco Delbo, Line Drube, Rene Duffard, Martin Elvis, Daniel Faber, Elizabeth Frank, Simon F. Green, Jan Thimo Grundmann, Henry Hsieh, Akos Kereszturi, Pauli Laine, Anny-Chantal Levasseur-Regourd, Philipp Maier, Philip Metzger, Patrick Michel, Migo Mueller, Thomas Mueller, Naomi Murdoch, Alex Parker, Petr Pravec, Vishnu Reddy, Joel Sercel, Andy Rivkin, Colin Snodgrass, and Paolo Tanga.

The White Paper can be found at: https://arxiv.org/abs/1612.00709

EPSC 2017 abstracts: http://meetingorganizer.copernicus.org/EPSC2017/EPSC2017-985.pdf 


A montage of 17 of the 18 asteroids and comets that have been photographed up close as of August 2014, when Rosetta arrived at comet Churyumov-Gerasimenko. This version is in color and shows the bodies at their correct relative (though not absolute) albedo or brightness. Not included are Vesta or Ceres, both of which are many times larger than Lutetia. Credit: Montage by Emily Lakdawalla. Data from NASA / JPL / JHUAPL / UMD / JAXA / ESA / OSIRIS team / Russian Academy of Sciences / China National Space Agency. Processed by Emily Lakdawalla, Daniel Machacek, Ted Stryk, Gordan Ugarkovic.
Full resolution image: http://planetary.s3.amazonaws.com/assets/images/9-small-bodies/2015/20150313_asteroids_comets_sc_0-000-020_2015_color_lighter.png

Artist’s impression of ESA’s AIM mission encountering asteroid Didymos. Credit: ESA

Science Contacts
Dr JL Galache
Chief Technology Officer
Aten Engineering

Dr Amara Graps
University of Latvia/Planetary Science Institute
+371 28853907

Media Contacts
Anita Heward
EPSC 2017 Press Officer
+44 07756 034243

Livia Giacomini
EPSC 2017 Press Officer

Notes for Editors
EPSC 2017
The European Planetary Science Congress (EPSC) 2017 (www.epsc2017.eu) is taking place at the Radisson Blu Latvija in Riga, from Sunday 17 to Friday 22 September 2017. EPSC is the major European annual meeting on planetary science and in 2017 is hosted for the first time in the Baltic States. Around 800 scientists from Europe and around the world will attend the meeting and will give around 1,000 oral and poster presentations about the latest results on our own Solar System and planets orbiting other stars.

EPSC 2017 is organised by Europlanet and Copernicus Meetings. The Local Organising Committee is led by Baltics in Space, a not-for-profit organisation that is supporting 25 members centred around nine Baltic space facilities for the conference. The meeting is sponsored by Investment and Development Agency of Latvia, the Latvian Ministry of Education and Science, Latvijas Mobilais Telefons, Finnish Meteorological Institute, The Estonia-Latvia programme, The Representation of the European Commission in Latvia, the Planetary Science Institute, Latvijas Universitate and The Division for Planetary Sciences of the AAS.

Details of the Congress and a full schedule of EPSC 2017 scientific sessions and events can be found at the official website:

Since 2005, the Europlanet project has provided European’s planetary science community with a platform to exchange ideas and personnel, share research tools, data and facilities, define key science goals for the future and engage stakeholders, policy makers and European Citizens with planetary science. Europlanet is the parent organisation of the European Planetary Science Congress (EPSC), and the EPSC Executive Committee is drawn from its membership.

The Europlanet 2020 Research Infrastructure (RI) is a €9.95 million project to address key scientific and technological challenges facing modern planetary science by providing open access to state-of-the-art data, models and facilities across the European Research Area. The project was launched on 1st September 2015 and has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 654208. Europlanet 2020 RI is led by the Open University, UK, and has 33 beneficiary institutions from 19 European countries.
Project website: www.europlanet-2020-ri.eu
Outreach website: www.europlanet-eu.org
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Baltics in Space
The philosophy of the nonprofit organization, Baltics in Space, is to “Inventory, Identify, and Integrate” with a sprinkling of Inspiration to build a space product greater than the sum of its parts. The best resource in the space business is people. With an eye to strengthening the triple helix links (Industry, Education, Research), its planned outcomes are integrating Baltic-wide space events, compiling catalogs of skill-sets for prospective users and Baltic space project development with distributed teams and Baltic space education.