Space Resources Engineering: Ilmenite Deposits for Oxygen Production on the Moon

Gustavo Jamanca-Lino^{1, 2,}

¹Space Resources Program, Colorado School of Mines, Golden, United States

²FIGMMyG, Universidad Nacional Mayor de San Marcos, Lima, Peru

Cite this paper:
Gustavo Jamanca-Lino. Space Resources Engineering: Ilmenite Deposits for Oxygen Production on the Moon. American Journal of Mining and Metallurgy. 2021; 6(1):6-11. doi: 10.12691/ajmm-6-1-2

Abstract

This decade is an incredible stage in the history of humanity. Man will return to the Moon to stay there. To successfully fulfill this enormous challenge, scientific staff will use the in-situ resources or ISRU, and terrestrial mining industry knowledge to produce prime matters. Oxygen and hydrogen are the crucial resources to obtain water, rocket fuel, and establish commercial activities between the Earth and the Moon. One alternative to produce oxygen is using metallurgical processing of oxide minerals as ilmenite. Also, iron and titanium could be produced from ilmenite to supply a future lunar aerospace industry, making attractive the exploration of this mineral. This paper discusses the ilmenite deposit features in the equator zone's Marias, especially in Mare Tranquillitatis. The author reviews the feasibility of producing oxygen from the ilmenite in a pyrometallurgical process, reviewing the reactions proposed through thermodynamic calculation with the Software HSC Chemistry 6.0 and the regolith sample’s geological data Apollo 11 to verify ore features that can affect the metallurgical behavior. Besides, there is a summary of the challenges to processing ilmenite associated with the degree of liberation. This research aims to clarify the industrial opportunities and challenges to produce oxygen on the Moon as a framework for future process architecture and equipment design.

Keywords:
ISRU space resources space mining lunar ilmenite

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References:

[1]	Moritz, A. F. Mining the Moon, Literary Imagination, 20(1), pp. 39-42, March 2018.
[2]	Rasera, J. N., Cilliers, J. J., Lamamy, J. A., & Hadler, K., The beneficiation of lunar regolith for space resource utilisation: A review, Planetary and Space Science, 186, 104879, Jul. 2020.
[3]	Crawford, Ian A. Lunar resources: A review. Progress in Physical Geography, 39(2), pp.137-167, Feb. 2015.
[4]	NASA, Mare Tranquillitatis, NASA.gov. https://www.nasa.gov/mission_pages/LRO/multimedia/lroimages/lola-20100528-maretranquillitatis.html (Feb.5, 2021).
[5]	Cameron, E., Geology of Mare Tranquillitatis and Its Significance for the Mining of Helium, Technical Report WCSAR-TR-AR3-9006-1, University Wisconsin-Madison, Wisconsin, 1990.
[6]	Anand, M., and Tindle, D. A., Discover Moon Minerals, Open.edu, URL: https://www.open.edu/openlearn/moon-minerals-book (Feb.5, 2021).
[7]	Baugh, T. M., and Osborn, R. G., QuickMAP, Quickmap.lroc.asu.edu URL: https://quickmap.lroc.asu.edu/layers?extent=-90,-24.4852751,90,24.4852751&proj=10&layers=NrBsFYBoAZIRnpEAmAnKgHI2CB2BXAG0MgG8BfAXUrKsqA. (Feb. 5, 2021).
[8]	Taylor, L. A., Cooper, B., McKay, D. S., and Colson, R. O., Oxygen Production on the Moon: Processes for Different Feedstocks. Mining, Metallurgy & Exploration, Vol. 10, No. 1, pp. 43-51, 1993.
[9]	Astromaterials - Acquisition & Curation-Office, 10084. curator.jsc.nasa.gov, URL: https://curator.jsc.nasa.gov/lunar/catalogs/apollo11/10084.pdf. (Cited Feb.5, 2021).
[10]	Heiken, G., Vaniman, D., and French, B. M., Lunar Sourcebook : A User's Guide to the Moon, Cambridge University Press, 1991.
[11]	Wallace, W. T., Taylor, L. A., Liu, Y., Cooper, B. L., McKAY, D. S., Chen, B., and Jeevarajan, A. S., Lunar Dust and Lunar Simulant Activation and Monitoring, Meteoritics & planetary science, Vol. 44, No. 7, pp. 961-970, 2009.
[12]	Korotev, R. L., and Gillis, J. J., A New Look at the Apollo 11 Regolith and KREEP, Journal of geophysical research, Vol. 106, No. E6, pp. 12339-12353, 2001.
[13]	Astromaterials - Acquisition & Curation-Office, 10084. curator.jsc.nasa.gov, https://curator.jsc.nasa.gov/lunar/lsc/10084.pdf (Cited Feb.5, 2021).
[14]	Haramura, H. and Kushiro, Ikuo and Nakamura, Y., Composition of Lunar Fines, Proceedings of the Apollo 11 Lunar Science Conference, Vol. 1, Houston, Texas, pp. 539-540, 1970.
[15]	Fa, W., and Jin, Y., Global Inventory of Helium-3 in Lunar Regoliths Estimated by a Multi-Channel Microwave Radiometer on the Chang-E 1 Lunar Satellite, Kexue Tongbao, Vol. 55, No. 35, pp. 4005-4009, 2010.
[16]	Chambers, J. G., Taylor, L. A., Patchen, A., and McKay, D. S., Quantitative Mineralogical Characterization of Lunar High-Ti Mare Basalts and Soils for Oxygen Production, Journal of geophysical research, Vol. 100, No. E7, p. 14391, 1995.
[17]	Bird M., Duke M., Finkelman R., Sellers G., Woo C., Genesis of Lunar Soil at Tranquillity Base, Proceedings of the Apollo 11 Lunar Science Conference, Vol. 1, Houston, Texas, pp. 347-361, 1970.
[18]	Kong, W. G., Jolliff, B. L., and Wang, A., Ti Distribution in Grain-Size Fractions of Apollo Soils 10084 and 71501, Icarus, Vol. 226, No. 1, pp. 891-897, 2013.
[19]	Adler, I., Walter, L. S., Lowman, P. D., Glass, B. P., French, B. M., Philpotts, J. A., Electron Microprobe Analysis of Apollo 11 Lunar Samples, Proceedings of the Apollo 11 Lunar Science Conference, Vol. 1, Houston, Texas, pp. 87-92, 1970.
[20]	Lino, G. J., Palacios, P., Napan, J. L., & Cornejo, J. (2020). Conceptual design of ARIES rover for water production and resource utilization on the moon. 2020 IEEE Engineering International Research Conference (EIRCON), 1-4.
[21]	Gibson, M. A. & Knudsen, C. W., Lunar Oxygen Production from Ilmenite, Lunar Bases and Space Activities of the 21st Century, Vol. 1 Houston, Texas, pp. 543-550, 1985.
[22]	Lishchuk, V., Koch, P.-H., Ghorbani, Y., and Butcher, A. R., Towards Integrated Geometallurgical Approach: Critical Review of Current Practices and Future Trends, Minerals Engineering, Vol. 145, p. 106072, 2020.
[23]	Manzaneda J. R., Aplicación de microscopía en el procesamiento de minerales por flotación, URL: http://www.lareferencia.info/vufind/Record/PE_c90ec7770f7dc5389 31a55d46e4d650f (Feb. 5, 2021).
[24]	Graf. J. C., Lunar soils grain size catalog, NTRS. URL: https://ntrs.nasa.gov/citations/19930012474 (Feb. 5, 2021).
[25]	Frondel C., Klein C. Jr., Ito J., and Drake J. C., Mineralogical and chemical studies of Apollo 11 lunar fines and selected rocks, Proceedings of the Apollo 11 Lunar Science Conference, Vol. 1, Houston, Texas, pp. 445-474,1970.
[26]	Basu A., Wentworth S. J., and Mckay D. S., Submillimeter grain-size distribution of Apollo 11 soil 10084, Meteorit. Planet. Sci., vol. 36, n°. 1, pp. 177-181, 2001.
[27]	Engelhardt W. V., Arndt J., Müller W. F., and Stöffler D., Shock metamorphism and origin of regolith and breccias at the Apollo 11 and Apollo 12 landing sites, in Proceedings of the Second Lunar Science Conference, Houston, Texas, pp. 833-854, 1971.
[28]	Lovering J. F. and War N. G., Electron-probe microanalyses of minerals and glasses in Apollo 11 lunar samples, Proceedings of the Apollo 11 Lunar Science Conference, Vol. 1, Houston, Texas, pp. 633 -654, 1970.
[29]	Labotka, T. C., Kempa, M. J., White, C., Papike, J. J., & Laul, J. C., The lunar regolith - Comparative petrology of the Apollo sites, Lunar and Planetary Science Conference, 11th, Houston, Texas Vol.2, pp. 1285-1305, 1980.
[30]	Engelhardt W.V., Hurrle, H., & Luft, E., Microimpact-induced changes of textural parameters and modal composition of the lunar regolith. Lunar and Planetary Science Conference, 7th, Houston, Texas, Vol.1, pp. 373-392, 1976.
[31]	King, E. A., Jr., Butler, J. C., & Carman, M. F. Jr., The lunar regolith as sampled by Apollo 11 and Apollo 12: Grain size analyses, modal analyses, and origins of particles, Proceedings of the Second Lunar Science Conference, Houston, Texas, pp. 737-746, 1971.
[32]	Agosto, W., Electrostatic Separation and Sizing of Ilmenite in Lunar Soils Simulants and Samples, Abstracts of Lunar and planetary science XV, p. 1-2, 1984.
[33]	Agosto, W., Electrostatic Concentration of Lunar Soil Minerals, Lunar Bases and Space Activities of the 21st Century, Houston, Texas, Vol. 1.pp.453-464, 1985.
[34]	Arias, V., Rodríguez, C., Ramírez, P., Nonones, E., Salazar, D., Gil, J., Paredes, J., & Jamanca, G. (2012). Aislamiento de bacterias acidófilas a partir del drenaje ácido proveniente de las inmediaciones a las unidades mineras de Julcani y Recuperada, Huancavelica. Revista Del Instituto De Investigación De La Facultad De Ingeniería Geológica, Minera, Metalúrgica Y Geográfica, 15(30), 59-66.
[35]	Arias, V., Anaya, F., Quiñones, J., Salazar, D., Gil, J., & Jamanca, G. (2013). Adaptación del Thiobacillus Ferrooxidans a sustratos conformados con especies de minerales piríticos. Revista Del Instituto De Investigación De La Facultad De Ingeniería Geológica, Minera, Metalúrgica Y Geográfica, 16(31).
[36]	V. Ticllacuri, G. J. Lino, A. B. Diaz and J. Cornejo, “Design of Wearable Soft Robotic System for Muscle Stimulation Applied in Lower Limbs during Lunar Colonization,” 2020 IEEE XXVII International Conference on Electronics, Electrical Engineering and Computing (INTERCON), Lima, Peru, 2020, pp. 1-4.
[37]	M. V. Rivera, J. Cornejo, K. Huallpayunca, A. B. Diaz, Z. N. Ortiz-Benique, A. D. Reina, G. J. Lino and V. Ticllacuri, “Medicina humana espacial: Performance fisiológico y contramedidas para mejorar la salud del astronauta,” Rev. Fac. Med. Humana, vol. 20, no. 2, pp. 303-314, March 2020.