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Mass Spectrometer Observing Lunar Operations (MSoLo)Introduction: In 2019, the National Aeronautics and Space Administration (NASA) announced that it would seek to have humans return to the moon by 2024 in the hopes of establishing a more sustainable lunar presence by 2028. This goal comes with many challenges, one of upmost importance will be to utilize resources that can be found on the moon. Water, which has been identified in the lunar Polar Regions, will be a key resource for in-situ resource utilization (ISRU), as it is capable of being processed for vehicular fuel, as well as life support systems materials such as oxygen. Upcoming Commercial Lunar Payload Services (CLPS) missions will be critical for these resource assessments.

Methods: A modified commercial off-the-shelf (COTS) mass spectrometer developed at Kennedy Space Center known as MSolo, consisting of a quadrupole mass filter and space rated electronics undergoes testing and modifications in order to study operational parameters to unconventional approaches needed in flight situations. In general, MSolo operates in the 0-100 m/z range with the ability to detect with a faraday cup (FC) or an electron multiplier (EM) for enhanced detection. A crossbeam (XB) ionization source is used.

Preliminary Data: Prior to construction, little information was available on how the MSolo system would perform at lunar like environments, factors such as temperatures (possible fluctuations from 70 to -45 °C), vibrations from launch and their side effects, the general ability to operate while the entire system (hardware and electronic components) were in a vacuum environment, were factors that while know to flight instruments, were something new to a modified COTS system. As components start to warm up, temperature becomes a key factor (ie. heat can no longer escape the electronics as no atmosphere is present), therefore it becomes crucial to find new ways to maintain stable signals and keep the instrument tuned. Calibration itself becomes an important parameter that needs to be performed while maintaining all flight like characteristics. Even the structure itself of MSolo’s sensor needed to be changed to survive the verification parameters needed to be approved for flight. Most important, all the modifications made to the COTS system have to keep the instrument working at the same specifications of the standard commercial systems.

Novel Aspect: Results gathered provide key parameters that will assist to the unconventional mass spectrometry approaches of the upcoming CLPS missions to which MSolo has been selected to.
Document ID
20230007808
Acquisition Source
Kennedy Space Center
Document Type
Presentation
Authors
Roberto Aguilar Ayala
(Kennedy Space Center Merritt Island, Florida, United States)
Matthew L Hancock
(Kennedy Space Center Merritt Island, Florida, United States)
Alexander W Jarnot
(KSC-UB-Generic)
Janine E Captain
(Kennedy Space Center Merritt Island, Florida, United States)
Jacqueline W Quinn
(Kennedy Space Center Merritt Island, Florida, United States)
Date Acquired
May 18, 2023
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 71st ASMS Conference on Mass Spectrometry and Allied Topics
Location: Houston, TX
Country: US
Start Date: June 4, 2023
End Date: June 8, 2023
Sponsors: American Society for Mass Spectrometry
Funding Number(s)
PROJECT: MSolo
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Peer Committee
Keywords
MSolo
Mass Spectrometry
ASMS
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