Metal and Oxide Sublimation from Lunar Regolith: A Kinetics Study

被引:5
|
作者
Shaw, Matthew G. G. [1 ,2 ]
Humbert, Matthew S. S. [1 ]
Brooks, Geoffrey A. A. [1 ]
Rhamdhani, M. Akbar [1 ]
Duffy, Alan R. R. [3 ]
Pownceby, Mark I. I. [2 ]
机构
[1] Swinburne Univ Technol, Sch Engn, Fluid & Proc Dynam Grp, Hawthorn, Vic 3122, Australia
[2] CSIRO Mineral Resources, Bayview Ave Clayton, Clayton, Vic 3168, Australia
[3] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
关键词
ISRU; astrometallurgy; sublimation; evaporation; SRU; THERMODYNAMIC OPTIMIZATION; EVAPORATION; CHEMISTRY; ELEMENT;
D O I
10.3390/min13010079
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
When considering the extraction of metals from lunar regolith for use in space, one reductive method of interest is vacuum thermal dissociation. Given the high vacuum environment on the Moon, the sub-liquidus operation of such a process, i.e., sublimation, warrants investigation. In the current work, the kinetics of the vacuum sublimation of the more volatile major oxides found in the lunar regolith, Na2O, K2O, and FeO, are evaluated. Two distinct factors are accounted for in the current work: the change in the evaporation flux due to temperature; and the reduction in available surface area for evaporation due to sintering of the feedstock. Surface area change due to the sintering of compressed LMS-1 regolith simulant pellets was quantified via a Brunauer-Emmett-Teller analysis. The surface area of the samples was measured to vary from 3.29 m(2)/g in the unsintered sample, to 1.04 m(2)/g in the samples sintered at 800 degrees C, and down to 0.09 m(2)/g in the sample sintered at 1150 degrees C. Evaporation flux was calculated using the Hertz-Knudsen-Langmuir equation using saturated vapor pressures predicted from the FactSage thermochemical package and verified against Knudsen Effusion Mass Spectroscopy data from tests conducted on lunar regolith sample #12022. The combination of these studies resulted in the conclusion that no local maxima in evaporation rate below the melting point was found for the current system, as such the highest rate of sublimation was determined to be 1200 degrees C for all species, at temperatures of 1200 degrees C and above, partial melting of the material occurs. The predicted maximum rate of sublimation for the species Fe, Na, and K at 1200 degrees C was 0.08, 1.38, and 1.02 g/h/g of regolith, respectively. It is noted that significant variation was seen between FactSage predictions of saturated vapor pressures and the measured values. Future work generating detailed thermochemical databases to predict the behavior of complex systems similar in composition to lunar regolith would benefit the accuracy of similar kinetic studies in the future.
引用
收藏
页数:12
相关论文
共 50 条
  • [41] Extraction of Volatiles from Lunar Regolith Using Solar Power
    Frias, Jorge A.
    Shafirovich, Evgeny
    Van Woerkom, Michael
    JOURNAL OF THERMOPHYSICS AND HEAT TRANSFER, 2014, 28 (02) : 343 - 346
  • [42] PETROLOGY OF LUNA-20 REGOLITH FROM LUNAR HIGHLANDS
    CRAWFORD, ML
    WEIGAND, PW
    GEOCHIMICA ET COSMOCHIMICA ACTA, 1973, 37 (04) : 815 - &
  • [43] Kinetics and Optimization of Refractory Metal Alloy Oxidation and Sublimation
    Ratschbacher, Karin
    Luidold, Stefan
    CHEMIE INGENIEUR TECHNIK, 2015, 87 (11) : 1558 - 1568
  • [44] Global survey of lunar regolith depths from LROC images
    Bart, Gwendolyn D.
    Nickerson, Ryan D.
    Lawder, Matthew T.
    Melosh, H. J.
    ICARUS, 2011, 215 (02) : 485 - 490
  • [45] EXAMINATION OF THE KINETICS OF TRANSFER OF HYDROGEN FROM THE OXIDE METAL INTO METAL
    VATOLIN, AN
    SOTNIKOV, AI
    ROGACHEV, VV
    RUSSIAN METALLURGY, 1981, (04): : 28 - 35
  • [46] Rhenium oxide, potassium perrhenate, iron and aluminum hydroxychlorides, barite, and celestine in lunar regolith
    Mokhov, A. V.
    Bogatikov, O. A.
    Kartashov, P. M.
    Gorshkov, A. I.
    Koporulina, E. V.
    Magazina, L. O.
    Ashikhmina, N. A.
    DOKLADY EARTH SCIENCES, 2006, 407 (03) : 460 - 464
  • [47] Rhenium oxide, potassium perrhenate, iron and aluminum hydroxychlorides, barite, and Celestine in lunar regolith
    A. V. Mokhov
    O. A. Bogatikov
    P. M. Kartashov
    A. I. Gorshkov
    E. V. Koporulina
    L. O. Magazina
    N. A. Ashikhmina
    Doklady Earth Sciences, 2006, 407 : 460 - 464
  • [48] THERMODYNAMIC STUDY OF SUBLIMATION OF SELENIUM OXIDE
    PIACENTE, V
    MALASPIN.L
    BARDI, G
    REVUE INTERNATIONALE DES HAUTES TEMPERATURES ET DES REFRACTAIRES, 1969, 6 (01): : 25 - &
  • [49] Magnetic property and paleointenstiy study of the lunar regolith (E21)
    Cai ShuHui
    Qin HuaFeng
    Deng ChengLong
    Liu ShuangChi
    Chen Yi
    He HuaiYu
    Pan YongXin
    ACTA PETROLOGICA SINICA, 2022, 38 (06) : 1832 - 1842
  • [50] X-RAY ELECTRON STUDY OF METALLIC IRON IN LUNAR REGOLITH
    VINOGRAD.AP
    URUSOV, VS
    ZHAVORON.NM
    NEFEDOV, VI
    DOKLADY AKADEMII NAUK SSSR, 1972, 207 (02): : 433 - &