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A Study on the Thermal Extraction of H₂O(S) from Lunar Regolith Simulant Using Concentrated Solar Thermal Technology
A Study on the Thermal Extraction of H₂O(S) from Lunar Regolith Simulant Using Concentrat...
A Study on the Thermal Extraction of H₂O(S) from Lunar Regolith Simulant Using Concentrated Solar Thermal Technology

상세정보

자료유형  
 학위논문 서양
최종처리일시  
20260202105505
ISBN  
9798263327071
DDC  
681.1
저자명  
Farr, Tyler P.
서명/저자  
A Study on the Thermal Extraction of H₂O(S) from Lunar Regolith Simulant Using Concentrated Solar Thermal Technology
발행사항  
[Sl] : Georgia Institute of Technology, 2025
발행사항  
Ann Arbor : ProQuest Dissertations & Theses, 2025
형태사항  
104 p
주기사항  
Source: Dissertations Abstracts International, Volume: 87-05, Section: A.
주기사항  
Advisor: Loutzenhiser, Peter G.
학위논문주기  
Thesis (Ph.D.)--Georgia Institute of Technology, 2025.
초록/해제  
요약The focus of this research was to determine the feasibility of using concentrated solar thermal (CST) technology as a method for extracting H2O from H2O(s) deposits on the lunar surface. The potential source of lunar H2O(s), found in the permanently shadowed regions (PSR), and related extraction using solar thermal energy constitute the focal points of this investigation. The research leverages CST technology, supplemented by an indirect solar receiver (ISR) for optimal heat transfer, to explore H2O extraction. Initial investigations examined H2O(v) transport through Lunar Mare Simulant (LMS-1) and Lunar Highland Simulant (LHS-1), yielding a diffusion model indispensable for in-situ resource utilization (ISRU) technology development. A specialized Concentrated Lunar and Rapid Kinetics (CLARK) reactor was designed, built, and used to replicate lunar surface conditions, allowing for concentrated irradiation of simulant packed beds from a high-flux solar simulator (HFSS). The experiments were conducted with varying levels of key factors, including the use of a copper indirect solar receiver, various packing densities, and adjusting the irradiation to study the impacts and interactions on the sublimation. Alongside the experimental work, preliminary work on transient computational models are presented, simulating the heat and mass transfer phenomena and providing valuable insights for optimizing the system design. Advanced X-ray tomography scans were used to develop detailed 3D packed bed models. The models were developed for future Monte Carlo simulations to evaluate reflective and absorptive properties and for a lattice Boltzmann model to analyze flow dynamics. This work sets the foundation for detailed simulations and further analysis of thermal and mass transfer processes. These investigations confirm the viability of solar thermal energy in extracting H2O(v) from lunar regolith simulants, laying the foundation for future research into lunar regolith H2O thermal extraction, a crucial endeavor for sustainable long-term space exploration.
일반주제명  
Mirrors
일반주제명  
Design
일반주제명  
Moon
일반주제명  
Sun
기타저자  
Georgia Institute of Technology.
기본자료저록  
Dissertations Abstracts International. 87-05A.
전자적 위치 및 접속  
로그인 후 원문을 볼 수 있습니다.

MARC

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■020    ▼a9798263327071
■035    ▼a(MiAaPQ)AAI32308024
■035    ▼a(MiAaPQ)GeorgiaTech78748
■040    ▼aMiAaPQ▼cMiAaPQ
■0820  ▼a681.1
■1001  ▼aFarr,  Tyler  P.
■24512▼aA  Study  on  the  Thermal  Extraction  of  H₂O(S)  from  Lunar  Regolith  Simulant  Using  Concentrated  Solar  Thermal  Technology
■260    ▼a[Sl]▼bGeorgia  Institute  of  Technology▼c2025
■260  1▼aAnn  Arbor▼bProQuest  Dissertations  &  Theses▼c2025
■300    ▼a104  p
■500    ▼aSource:  Dissertations  Abstracts  International,  Volume:  87-05,  Section:  A.
■500    ▼aAdvisor:  Loutzenhiser,  Peter  G.
■5021  ▼aThesis  (Ph.D.)--Georgia  Institute  of  Technology,  2025.
■520    ▼aThe  focus  of  this  research  was  to  determine  the  feasibility  of  using  concentrated  solar  thermal  (CST)  technology  as  a  method  for  extracting  H2O  from  H2O(s)  deposits  on  the  lunar  surface.  The  potential  source  of  lunar  H2O(s),  found  in  the  permanently  shadowed  regions  (PSR),  and  related  extraction  using  solar  thermal  energy  constitute  the  focal  points  of  this  investigation.  The  research  leverages  CST  technology,  supplemented  by  an  indirect  solar  receiver  (ISR)  for  optimal  heat  transfer,  to  explore  H2O  extraction.  Initial  investigations  examined  H2O(v)  transport  through  Lunar  Mare  Simulant  (LMS-1)  and  Lunar  Highland  Simulant  (LHS-1),  yielding  a  diffusion  model  indispensable  for  in-situ  resource  utilization  (ISRU)  technology  development.  A  specialized  Concentrated  Lunar  and  Rapid  Kinetics  (CLARK)  reactor  was  designed,  built,  and  used  to  replicate  lunar  surface  conditions,  allowing  for  concentrated  irradiation  of  simulant  packed  beds  from  a  high-flux  solar  simulator  (HFSS).  The  experiments  were  conducted  with  varying  levels  of  key  factors,  including  the  use  of  a  copper  indirect  solar  receiver,  various  packing  densities,  and  adjusting  the  irradiation  to  study  the  impacts  and  interactions  on  the  sublimation.  Alongside  the  experimental  work,  preliminary  work  on  transient  computational  models  are  presented,  simulating  the  heat  and  mass  transfer  phenomena  and  providing  valuable  insights  for  optimizing  the  system  design.  Advanced  X-ray  tomography  scans  were  used  to  develop  detailed  3D  packed  bed  models.  The  models  were  developed  for  future  Monte  Carlo  simulations  to  evaluate  reflective  and  absorptive  properties  and  for  a  lattice  Boltzmann  model  to  analyze  flow  dynamics.  This  work  sets  the  foundation  for  detailed  simulations  and  further  analysis  of  thermal  and  mass  transfer  processes.  These  investigations  confirm  the  viability  of  solar  thermal  energy  in  extracting  H2O(v)  from  lunar  regolith  simulants,  laying  the  foundation  for  future  research  into  lunar  regolith  H2O  thermal  extraction,  a  crucial  endeavor  for  sustainable  long-term  space  exploration.
■590    ▼aSchool  code:  0078.
■650  4▼aMirrors
■650  4▼aDesign
■650  4▼aMoon
■650  4▼aSun
■690    ▼a0389
■71020▼aGeorgia  Institute  of  Technology.
■7730  ▼tDissertations  Abstracts  International▼g87-05A.
■790    ▼a0078
■791    ▼aPh.D.
■792    ▼a2025
■793    ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17360316▼nKERIS▼z이  자료의  원문은  한국교육학술정보원에서  제공합니다.

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