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Use of ISS and Artemis as Analogs for Future Mars Missions: A Strategic ViewThe International Space Station (ISS) from its inception has served as a key place for doing research on the effects of microgravity on human physiology and developing mitigations and countermeasures to those effects to enable future exploration. The ISS international partnership is working on periodic modifications to operations so that ISS could be used more effectively as an analog to simulate long-duration crew missions beyond low earth orbit. Ongoing planning includes: (1) demonstration of autonomous medical care with significant communications delay, (2) simulation of other types of operations with communications delay, crew autonomy, or simulated hardware autonomy, and (3) surface operations after the physiological effects of a long transit. Exploration simulations are challenging because there can be operational impacts on nominal ISS activities, but when well-designed can offer a unique degree of fidelity to understand and reduce risks of future missions.

Human spaceflight is entering a new phase where simultaneous operations of multiple platforms can improve the quality of Mars mission simulations beyond what can be done on ISS alone. Artemis offers opportunity to test human operations in a partial gravity and deep space radiation environment, with value for understanding human performance across multiple phases of surface operations: early operations with little surface infrastructure, the ramp up to frequent surface extra-vehicular activity, and if durations in microgravity can be extended, a potential full simulation of a Mars mission.

By developing a strategy that treats all human spaceflight missions in Low Earth Orbit (LEO) and the lunar vicinity as analogs for future Mars missions, human research and technology demonstration can be conducted that is more robust to the limitations of any one analog. This paper will provide the latest integrated strategy being used internationally with updates on the implementation progress and challenges as planning and development continue.
Document ID
20200011530
Acquisition Source
Headquarters
Document Type
Abstract
Authors
Julie A Robinson ORCID
(National Aeronautics and Space Administration Washington D.C., District of Columbia, United States)
Sam Scimemi
(National Aeronautics and Space Administration Washington D.C., District of Columbia, United States)
Michelle Rucker
(Johnson Space Center Houston, Texas, United States)
Michael C Waid
(Johnson Space Center Houston, Texas, United States)
Jennifer Fogarty
(Johnson Space Center Houston, Texas, United States)
William H Paloski ORCID
(Johnson Space Center Houston, Texas, United States)
Oleg Kotov
(Institute of Biomedical Problems Moscow, Russia)
Date Acquired
May 26, 2020
Publication Date
January 28, 2021
Publication Information
Publisher: International Astronautical Federation (IAF)
Subject Category
Spacecraft Design, Testing and Performance
Report/Patent Number
HQ-E-DAA-TN77789
Meeting Information
Meeting: 43rd Committee on Space Research Scientific Assembly (COSPAR)
Location: Sydney
Country: AU
Start Date: January 28, 2021
End Date: February 4, 2021
Sponsors: International Astronautical Federation (IAF)
Funding Number(s)
CONTRACT_GRANT: ISS-IGA-Russia (IBMP)
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
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