Preliminary quantification of the available solar power near the lunar South Pole

被引:2
|
作者
Ross, Amia K. [1 ]
Ruppert, Sephora [1 ,4 ]
Glaeser, Philipp [2 ]
Elvis, Martin [3 ]
机构
[1] Harvard Univ, Harvard Coll, Cambridge, MA 02138 USA
[2] Tech Univ Berlin, Dept Planetary Geodesy, Berlin, Germany
[3] Harvard Univ, Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[4] Stanford Univ, Stanford, CA USA
关键词
Moon; Lunar mining; Lunar tower; Lunar solar power; Resource management; ILLUMINATION; SCIENCE; WATER; MOON;
D O I
10.1016/j.actaastro.2023.06.040
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The lunar South Pole is an area of great interest for human bases and for the mining of water from the nearby permanently shadowed regions (PSRs) that remain below 110 K at all times. To provide power for these ac-tivities, only solar and nuclear fission are currently feasible options. Solar power is nearly continuously available from vertically deployed solar panels from some quite restricted high illumination regions (HIRs) close to the PSRs. One factor in determining the choice between solar and nuclear power sources is an assessment of the total solar power available. If solar power is found to be inadequate, even in a best-case scenario, for the demands of a base or, more challenging, of mining, then nuclear fission will become the only option. Local topography means that the amount of solar power available from the HIRs depends in a non-trivial way on the height of the solar panels deployed. Here we use average illumination maps for a range of heights above the local topography from 2 m to 20 m (for near-term deployment) and up to 2 km (for long-term consideration) to determine the total solar power that is potentially available from the HIRs as a function of time of lunar day. Overshadowing of highly illuminated areas by solar panels placed in sunward locations (at a given time of day) limits the total power to significantly smaller values than the highly illuminated area would suggest. The answers depend on the per-centage illumination demanded by the application. We find that for near-term realizable vertical solar panels (up to 20 m), the upper limit to the time-averaged power available is-55-63 MW at >70% illumination, reducing to-6 MW at >90% illumination. This is sufficient to power thermal mining requirements at a rate of 1600-2450 tonnes/year of water. For the more distant future, for towers up to 2 km in height, a maximum time-averaged power of order 22,000 MW at >70% illumination could be realizable and-15,500 MW at 90% illumination. The variation in generated power with lunar time of day ranges from a factor of 1.1--3. These results suggest that sufficient solar power could be available for currently anticipated base or mining needs. Ensuring this power supply may require careful governance agreements.
引用
收藏
页码:616 / 630
页数:15
相关论文
共 50 条
  • [31] Multibody orbit architectures for lunar south pole coverage
    Grebow, Daniel J.
    Ozimek, Martin T.
    Howell, Kathleen C.
    Folta, David C.
    JOURNAL OF SPACECRAFT AND ROCKETS, 2008, 45 (02) : 344 - 358
  • [32] No evidence for thick deposits of ice at the lunar south pole
    Campbell, Donald B.
    Campbell, Bruce A.
    Carter, Lynn M.
    Margot, Jean-Luc
    Stacy, Nicholas J. S.
    NATURE, 2006, 443 (7113) : 835 - 837
  • [33] SOLAR POWER FOR THE LUNAR NIGHT
    LANDIS, GA
    SPACE MANUFACTURING 7: SPACE RESOURCES TO IMPROVE LIFE ON EARTH, 1989, : 290 - 296
  • [34] Low lunar orbit analysis, determination and selection for soft landing on the lunar south pole
    Floberghagen, R
    Visser, P
    Vasile, M
    12TH INTERNATIONAL SYMPOSIUM ON SPACE FLIGHT DYNAMICS, 1997, 403 : 321 - 326
  • [35] Automated astronaut traverses with minimum metabolic workload: Accessing permanently shadowed regions near the lunar south pole
    Pena-Asensio, Eloy
    Sutherland, Jennifer
    Tripathi, Prateek
    Mason, Kashauna
    Goodwin, Arthur
    Bickel, Valentin T.
    Kring, David A.
    ACTA ASTRONAUTICA, 2024, 214 : 324 - 342
  • [36] A New View of the Lunar South Pole from the Lunar Orbiter Laser Altimeter (LOLA)
    Barker, Michael K.
    Mazarico, Erwan
    Neumann, Gregory A.
    Smith, David E.
    Zuber, Maria T.
    Head, James W.
    Sun, Xiaoli
    PLANETARY SCIENCE JOURNAL, 2023, 4 (09):
  • [37] Quantification of Water Ice in the Hermite-A Crater of the Lunar North Pole
    Calla, O. P. N.
    Mathur, Shubhra
    Gadri, Kishan Lal
    IEEE GEOSCIENCE AND REMOTE SENSING LETTERS, 2016, 13 (07) : 926 - 930
  • [38] Geologic context and potential EVA targets at the lunar south pole
    Gawronska, A. J.
    Barrett, N.
    Boazman, S. J.
    Gilmour, C. M.
    Halim, S. H.
    Harish
    McCanaan, K.
    Satyakumar, A. V.
    Shah, J.
    Meyer, H. M.
    Kring, D. A.
    ADVANCES IN SPACE RESEARCH, 2020, 66 (06) : 1247 - 1264
  • [39] LONG-PERIOD LUNAR TIDES AT THE SOUTH-POLE
    RYDELEK, PA
    KNOPOFF, L
    JOURNAL OF GEOPHYSICAL RESEARCH, 1982, 87 (NB5): : 3969 - 3973
  • [40] Acquisition and tracking for communications between Lunar South Pole and Earth
    Divsalar, Dariush
    Net, Marc Sanchez
    Cheung, Kar-Ming
    2019 IEEE AEROSPACE CONFERENCE, 2019,