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Zhang JY, Anderson AP. Performance Risks During Surface Extravehicular Activity and Potential Mitigation Using Multimodal Displays. Aerosp Med Hum Perform 2023; 94:34-41. [PMID: 36757234 DOI: 10.3357/amhp.6066.2023] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/09/2023]
Abstract
BACKGROUND: Surface extravehicular activity (sEVA) will be a critical component of future human missions to the Moon. sEVA presents novel risks to astronaut crews not associated with microgravity operations due to fundamental differences in task demands, physiology, environment, and operations of working on the lunar surface. Multimodal spacesuit informatics displays have been proposed as a method of mitigating sEVA risk by increasing operator autonomy.METHODS: A formalized literature review was conducted. In total, 95 journal articles, conference papers, and technical reports were included. Characteristics of U.S. spacesuits were reviewed, ranging from the Apollo A7L to the xEMU Z-2.5. Multimodal display applications were then reviewed and assessed for their potential in aiding sEVA operations.RESULTS: Through literature review 25 performance impairments were identified. Performance impairments caused by the spacesuit represented the greatest number of sEVA challenges. Multimodal displays were mapped to impairments and approximately 36% of performance impairments could be aided by using display interfaces.DISCUSSION: Multimodal displays may provide additional benefits for alleviating performance impairments during sEVA. Utility of multimodal displays may be greater in certain performance impairment domains, such as spacesuit-related impairments.Zhang JY, Anderson AP. Performance risks during surface extravehicular activity and potential mitigation using multimodal displays. Aerosp Med Hum Perform. 2023; 94(1):34-41.
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Stevens A, Kobs Nawotniak S, Garry W, Payler S, Brady A, Miller M, Beaton K, Cockell C, Lim D. Tactical Scientific Decision-Making during Crewed Astrobiology Mars Missions. ASTROBIOLOGY 2019; 19:369-386. [PMID: 30840503 PMCID: PMC6442282 DOI: 10.1089/ast.2018.1837] [Citation(s) in RCA: 6] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/13/2018] [Accepted: 08/19/2018] [Indexed: 05/26/2023]
Abstract
The limitations placed upon human explorers on the surface of Mars will necessitate a methodology for scientific exploration that is different from standard approaches to terrestrial fieldwork and prior crewed exploration of the Moon. In particular, the data transmission limitations and communication latency between Earth and Mars create a unique situation for surface crew in contact with a terrestrial science team. The BASALT research program simulated a series of extravehicular activities (EVAs) in Mars analog terrains under various Mars-relevant bandwidth and latency conditions to investigate how best to approach this problem. Here we discuss tactical decision-making under these conditions, that is, how the crew on Mars interacts with a team of scientists and support personnel on Earth to collect samples of maximum scientific interest. We describe the strategies, protocols, and tools tested in BASALT EVAs and give recommendations on how best to conduct human exploration of Mars with support from Earth-based scientists. We find that even with scientists supporting them, the crew performing the exploration must be trained in the appropriate scientific disciplines in order to provide the terrestrial scientists with enough information to make decisions, but that with appropriate planning and structure, and tools such as a "dynamic leaderboard," terrestrial scientists can add scientific value to an EVA, even under Mars communication latency.
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Affiliation(s)
- A.H. Stevens
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | | | - W.B. Garry
- NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - S.J. Payler
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | - A.L. Brady
- School of Geography and Earth Sciences, McMaster University, Hamilton, Canada
| | - M.J. Miller
- Georgia Institute of Technology College of Engineering, Atlanta, Georgia, USA
| | - K.H. Beaton
- NASA Johnson Space Center, Houston, Texas, USA
| | - C.S. Cockell
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | - D.S.S. Lim
- NASA Ames Research Center, Moffett Field, California, USA
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Miller MJ, Miller MJ, Santiago-Materese D, Seibert MA, Lim DSS. A Flexible Telecommunication Architecture for Human Planetary Exploration Based on the BASALT Science-Driven Mars Analog. ASTROBIOLOGY 2019; 19:478-496. [PMID: 30840502 DOI: 10.1089/ast.2018.1906] [Citation(s) in RCA: 6] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/09/2023]
Abstract
There is a synergistic relationship between analog field testing and the deep space telecommunication capabilities necessary for future human exploration. The BASALT (Biologic Analog Science Associated with Lava Terrains) research project developed and implemented a telecommunications architecture that serves as a high-fidelity analog of future telecommunication capabilities for Mars. This paper presents the architecture and its constituent elements. The rationale for the various protocols and radio frequency (RF) link types required to enable an interdisciplinary field mission are discussed, and the performance results from the BASALT field tests are provided. Extravehicular Informatics Backpacks (EVIB) designed for BASALT and tested by human subjects are also discussed, and the proceeding sections show how these prototype extravehicular activity (EVA) information systems can augment future human exploration. The paper concludes with an aggregate analysis of the data product types and data volumes generated, transferred, and utilized by the ground team and explorers over the course of the field deployments.
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Affiliation(s)
| | | | | | - Marc A Seibert
- 4 ASRC Federal Technical Services, NASA SCaN Office, PSE Division, NASA Headquarters, Washington, DC
| | - Darlene S S Lim
- 3 NASA Ames Research Center, Moffett Field, California
- 5 Bay Area Environmental Research Institute/NASA Ames Research Center, Moffett Field, California
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Kobs Nawotniak SE, Miller MJ, Stevens AH, Marquez JJ, Payler SJ, Brady AL, Hughes SS, Haberle CW, Sehlke A, Beaton KH, Chappell SP, Elphic RC, Lim DS. Opportunities and Challenges of Promoting Scientific Dialog throughout Execution of Future Science-Driven Extravehicular Activity. ASTROBIOLOGY 2019; 19:426-439. [PMID: 30840509 PMCID: PMC6442240 DOI: 10.1089/ast.2018.1901] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/06/2018] [Accepted: 10/31/2018] [Indexed: 05/31/2023]
Abstract
Science-driven, human spaceflight missions of the future will rely on regular and interactive communication between Earth- and space-based teams during activity in which astronauts work directly on Mars or other planetary surfaces (extravehicular activity, EVA). The Biologic Analog Science Associated with Lava Terrains (BASALT) project conducted simulated human missions to Mars, complete with realistic one-way light time (OWLT) communication latency. We discuss the modes of communication used by the Mars- and Earth-based teams, including text, audio, video, and still imagery. Real-time communication between astronauts in the field (extravehicular, EV) and astronauts in a communication relay station (intravehicular, IV) was broadcast over OWLT, providing important contextual information to the Science Backroom Team (SBT) in Mission Control. Collaborative communication between the Earth- and Mars-based teams, however, requires active communication across latency via the Mission Log. We provide descriptive statistics of text communication between IV and SBT in a high-fidelity, scientifically driven analog for human space exploration. Over an EVA, the SBT sent an average of ∼23 text messages containing recommendations, requests, and answers to questions, while the science-focused IV crew member (IV2) sent an average of ∼38 text messages. Though patterns varied, communication between the IV and SBT teams tended to be highest during ∼50-150 min into the EVA, corresponding to the candidate sample search and presampling instrument survey phases, and then decreased dramatically after minute ∼200 during the sample collection phase. Generally, the IV2 and SBT used ∼4.6 min to craft a reply to a direct question or comment, regardless of message length or OWLT, offering a valuable glimpse into actual time-to-reply. We discuss IV2-SBT communication within the context of case examples from an EVA during which communication failures affected operations in the field. Finally, we offer recommendations for communication practices for use in future analogs and, perhaps, science-driven human spaceflight.
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Affiliation(s)
| | | | - Adam H. Stevens
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | | | - Samuel J. Payler
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | - Allyson L. Brady
- School of Geography and Earth Sciences, McMaster University, Hamilton, Canada
| | - Scott S. Hughes
- Department of Geosciences, Idaho State University, Pocatello, Idaho, USA
| | - Christopher W. Haberle
- Mars Space Flight Facility, School of Earth and Space Exploration, Arizona State University, Tempe, Arizona, USA
| | | | - Kara H. Beaton
- Biomedical Research and Environmental Science Division (SK), NASA Johnson Space Center, Houston, USA
| | - Steven P. Chappell
- Biomedical Research and Environmental Science Division (SK), NASA Johnson Space Center, Houston, USA
| | | | - Darlene S.S. Lim
- NASA Ames Research Center, Moffett Field, California, USA
- Bay Area Research Institute (BAERI), Moffett Field, California, USA
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Sehlke A, Mirmalek Z, Burtt D, Haberle CW, Santiago-Materese D, Kobs Nawotniak SE, Hughes SS, Garry WB, Bramall N, Brown AJ, Heldmann JL, Lim DS. Requirements for Portable Instrument Suites during Human Scientific Exploration of Mars. ASTROBIOLOGY 2019; 19:401-425. [PMID: 30840506 PMCID: PMC6442242 DOI: 10.1089/ast.2018.1841] [Citation(s) in RCA: 11] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/05/2018] [Accepted: 10/28/2018] [Indexed: 05/31/2023]
Abstract
Human explorers on the surface of Mars will have access to a far wider array of scientific tools than previous crewed planetary exploration missions, but not every tool will be compatible with the restrictions of this exploration. Spectrometers on flyby, orbital, and landed missions are currently used to determine the composition and mineralogy of geological materials of various types and sizes, from small fragments to celestial bodies in the solar system. Handheld spectrometers that are capable of in situ analyses are already used for geological exploration on Earth; however, their usefulness for human exploration missions and how data from multiple handheld instruments could be combined to enhance scientific return must be further evaluated. As part of the Biologic Analog Science Associated with Lava Terrains (BASALT) research project, we incorporated two handheld instruments, a visible-near infrared spectrometer and an X-Ray Fluorescence spectrometer, into simulated Mars exploration missions conducted on basaltic terrains in Idaho and Hawai'i. To understand the data quality provided by these handheld spectrometers, we evaluated their performance under varying conditions of measurement time, distance, angle, atmosphere, and sample matrix, and we compared data quality between handheld instruments and laboratory techniques. Here, we summarize these findings, provide guidelines and requirements on how to effectively incorporate these instruments into human exploration missions to Mars, and posit that future iterations of these instruments will be beneficial for enhancing science returned from human exploration missions.
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Affiliation(s)
| | - Zara Mirmalek
- Kennedy School of Government, Harvard University, Cambridge, Massachusetts
- BAER Institute, Moffett Field, California
| | - David Burtt
- Department of Geosciences, Stony Brook University, Stony Brook, New York
| | | | | | | | - Scott S. Hughes
- Deparment of Geosciences, Idaho State University, Pocatello, Idaho
| | | | - Nathan Bramall
- Leiden Measurement Technology LLC, Sunnyvale, California
| | | | | | - Darlene S.S. Lim
- NASA Ames Research Center, Moffett Field, California
- BAER Institute, Moffett Field, California
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Beaton K, Chappell S, Abercromby A, Miller M, Kobs Nawotniak S, Brady A, Stevens A, Payler S, Hughes S, Lim D. Assessing the Acceptability of Science Operations Concepts and the Level of Mission Enhancement of Capabilities for Human Mars Exploration Extravehicular Activity. ASTROBIOLOGY 2019; 19:321-346. [PMID: 30840507 PMCID: PMC6442237 DOI: 10.1089/ast.2018.1912] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/31/2018] [Accepted: 01/14/2019] [Indexed: 05/31/2023]
Abstract
The Biologic Analog Science Associated with Lava Terrains (BASALT) research project is investigating tools, techniques, and strategies for conducting Mars scientific exploration extravehicular activity (EVA). This has been accomplished through three science-driven terrestrial field tests (BASALT-1, BASALT-2, and BASALT-3) during which the iterative development, testing, assessment, and refinement of concepts of operations (ConOps) and capabilities were conducted. ConOps are the instantiation of operational design elements that guide the organization and flow of personnel, communication, hardware, software, and data products to enable a mission concept. Capabilities include the hardware, software, data products, and protocols that comprise and enable the ConOps. This paper describes the simulation quality and acceptability of the Mars-forward ConOps evaluated during BASALT-2. It also presents the level of mission enhancement and acceptability of the associated Mars-forward capabilities. Together, these results inform science operations for human planetary exploration.
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Affiliation(s)
- K.H. Beaton
- KBRwyle, Houston, Texas, USA
- NASA Johnson Space Center, Houston, Texas, USA
| | - S.P. Chappell
- KBRwyle, Houston, Texas, USA
- NASA Johnson Space Center, Houston, Texas, USA
| | | | | | | | - A.L. Brady
- School of Geography and Earth Sciences, McMaster University, Hamilton, Ontario, Canada
| | - A.H. Stevens
- European Astronaut Centre, European Space Agency, Cologne, Germany
| | - S.J. Payler
- European Astronaut Centre, European Space Agency, Cologne, Germany
| | - S.S. Hughes
- Department of Geosciences, Idaho State University, Pocatello, Idaho, USA
| | - D.S.S. Lim
- BAER Institute, Moffett Field, California, USA
- NASA Ames Research Center, Moffett Field, California, USA
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Payler S, Mirmalek Z, Hughes S, Kobs Nawotniak S, Brady A, Stevens A, Cockell C, Lim D. Developing Intra-EVA Science Support Team Practices for a Human Mission to Mars. ASTROBIOLOGY 2019; 19:387-400. [PMID: 30840508 PMCID: PMC6442258 DOI: 10.1089/ast.2018.1846] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/26/2018] [Accepted: 09/21/2018] [Indexed: 05/26/2023]
Abstract
During the BASALT research program, real (nonsimulated) geological and biological science was accomplished through a series of extravehicular activities (EVAs) under simulated Mars mission conditions. These EVAs were supported by a Mission Support Center (MSC) that included an on-site, colocated Science Support Team (SST). The SST was composed of scientists from a variety of disciplines and operations researchers who provided scientific and technical expertise to the crew while each EVA was being conducted (intra-EVA). SST management and organization developed under operational conditions that included Mars-like communication latencies, bandwidth constraints, and EVA plans that were infused with Mars analog field science objectives. This paper focuses on the SST workspace considerations such as science team roles, physical layout, communication interactions, operational techniques, and work support technology. Over the course of BASALT field deployments to Idaho and Hawai'i, the SST team made several changes of note to increase both productivity and efficiency. For example, new roles were added for more effective management of technical discussions, and the layout of the SST workspace evolved multiple times during the deployments. SST members' reflexive adjustments resulted in a layout that prioritized face-to-face discussions over face-to-data displays, highlighting the importance of interpersonal communication during SST decision-making. In tandem with these workspace adjustments, a range of operational techniques were developed to help the SST manage discussions and information flow under time pressure.
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Affiliation(s)
- S.J. Payler
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | - Z. Mirmalek
- Kennedy School of Government, Harvard University, Cambridge, Massachusetts, USA
- BAER Institute, Moffett Field, California, USA
| | - S.S. Hughes
- Department of Geosciences, Idaho State University, Pocatello, Idaho, USA
| | | | - A.L. Brady
- School of Geography and Earth Sciences, McMaster University, Hamilton, Canada
| | - A.H. Stevens
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | - C.S. Cockell
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | - D.S.S. Lim
- BAER Institute, Moffett Field, California, USA
- NASA Ames Research Center, Moffett Field, California, USA
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Brady AL, Kobs Nawotniak SE, Hughes SS, Payler SJ, Stevens AH, Cockell CS, Elphic RC, Sehlke A, Haberle CW, Slater GF, Lim DS. Strategic Planning Insights for Future Science-Driven Extravehicular Activity on Mars. ASTROBIOLOGY 2019; 19:347-368. [PMID: 30840500 PMCID: PMC6442241 DOI: 10.1089/ast.2018.1850] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/01/2018] [Accepted: 08/08/2018] [Indexed: 05/26/2023]
Abstract
Short-term and long-term science plans were developed as part of the strategic planning process used by the Biologic Analog Science Associated with Lava Terrains (BASALT) science team to conduct two Mars-simulation missions investigating basalt habitability at terrestrial volcanic analog sites in 2016. A multidisciplinary team of scientists generated and codified a range of scientific hypotheses distilled into a Science Traceability Matrix (STM) that defined the set of objectives pursued in a series of extravehicular activity (EVA) campaigns performed across multiple field deployments. This STM was used to guide the pre-deployment selection of sampling stations within the selected Mars analog sites on the Earth based on precursor site information such as multispectral imagery. It also informed selection of hand-held instruments and observational data to collect during EVA to aid sample selection through latency-impacted interaction with an Earth-based Science Support Team. A significant portion of the pre-deployment strategic planning activities were devoted to station selection, ultimately the locations used for sample collection and EVA planning. During development of the EVAs, the BASALT science team identified lessons learned that could be used to inform future missions and analog activities, including the critical need for high-resolution precursor imagery that would enable the selection of stations that could meet the scientific objectives outlined in the STM.
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Affiliation(s)
- Allyson L. Brady
- School of Geography and Earth Sciences, McMaster University, Hamilton, Canada
| | | | - Scott S. Hughes
- Department of Geosciences, Idaho State University, Pocatello, Idaho
| | - Samuel J. Payler
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | - Adam H. Stevens
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | - Charles S. Cockell
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom
| | | | | | | | - Greg F. Slater
- School of Geography and Earth Sciences, McMaster University, Hamilton, Canada
| | - Darlene S.S. Lim
- NASA Ames Research Center, Moffett Field, California
- Bay Area Environmental Research Institute (BAERI), NASA Research Park, Moffett Field, California
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