Mars analog habitat

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A Mars analog habitat is one of several historical, existing or proposed research stations designed to simulate the physical and psychological environment of a Martian exploration mission. These habitats are used to study the equipment and techniques that will be used to analyze the surface of Mars during a future crewed mission, and the simulated isolation of the volunteer inhabitants allows scientists to study the medical and psychosocial effects of long-term space missions. They are often constructed in support of extensive Mars analogs (see List of Mars analogs). However, sometimes existing natural places are also valued as Mars analogs. Crewed Mars habitats are featured in most human Mars missions; an alternative may be terraforming or telepresence.

Contents

The ISS has also been described as a predecessor to Mars expedition. In relation to a Mars habitat, it was noted that they are both essentially closed systems. [1]

Scientific motivation

Mars analog habitats are established to prepare astronauts, engineers, and researchers for the future challenges of sending a crewed mission to Mars. These analogs are inhabited by small teams of volunteers and may operate under “Mars-like” conditions for a few days to over a year. Habitats are often located in areas that in some form resemble the environment of Mars, such as polar deserts. While living in the habitats, crew members are mostly isolated from the outside world, survive on a diet of freeze-dried food, and may conduct field experiments while wearing protective space suits. Meanwhile, researchers analyze the crew members’ medical and psychological conditions and study the social and teamwork dynamics of the crew.

Historical missions, experiments, and results

Flashline Mars Arctic Research Station

The FMARS hab in 2009 FMARS 2009 hab.jpg
The FMARS hab in 2009

The Flashline Mars Arctic Research Station (FMARS) was established in 2000 in the territory of Nunavut, Canada. [2] This station is the first Mars analog created by the Mars Society, a space advocacy group established in August 1998. Since the beginning of field operations in April 2001, twelve separate crews (consisting of 6–7 personnel, each) have inhabited the station. While most missions lasted less than a single month, FMARS Crew 11 remained in the Martian simulation for 100 days.

FMARS is guided by three goals set by the Mars Society: to serve as a testbed for human Mars exploration, to serve as a useful research facility at a Mars analog site, and to generate public support for sending humans to Mars. [3] Research conducted by crewmembers while living in the habitat include an analysis of subsurface water detection techniques. Crewmembers set up seismic sensors along the Haughton crater while wearing prototype space suits, then tested how the sensors reacted to mini-earthquakes (produced by a sledgehammer) to produce a three-dimensional subsurface map. [4]

Additional experiments examined how well the FMARS crewmembers could work with an “Earth-based” remote science team. In one example, the remote science team used aerial images to select ten regions of scientific interest for the FMARS crew to explore and analyze. [5] This experiment helped researchers determine more efficient methods of scouting and investigating locations of interest under the communications limitations of a crewed mission to Mars. A study performed on the FMARS crew of July 2009 examined the psychological difficulties faced by crewmembers (especially the effects of isolation from family, conflicts among crewmembers, and diet) as well as the positive effects of problem-solving and exploration. [6]

Mars Desert Research Station

The Mars Society's Mars Desert Research Station MDRS Campus.jpg
The Mars Society's Mars Desert Research Station

The Mars Desert Research Station (MDRS) is the second Mars analog habitat established by the Mars Society. Located on the San Rafael Swell in Utah, the MDRS has been inhabited by 130 individual crews (of roughly 6 members each) between the first field season in December 2001 and the twelfth field season ending in May 2013. [7] Each crew typically remains in the habitat for one or two weeks. MDRS is less focused on the psychosocial aspects of space exploration than FMARS. Instead, crewmembers of MDRS focus on conducting field research in simulated Martian conditions.

The BYU Mars Rover undergoing field tests at the Mars Desert Research Station. BYU Mars Rover 2009-2.jpg
The BYU Mars Rover undergoing field tests at the Mars Desert Research Station.

Several important research results have come out of the MDRS experiments. Crewmembers were able to detect methane in dry desert soils, developing techniques which could detect methane – an important biosignature – in the soil of Mars. [8] Soil and vapor samples from the MDRS habitat were also found to contain significant amounts of methanogens, which were not previously suspected to thrive in a desert environment. [9] This research supported the possibility of microbial life on Mars and demonstrated that crew members could detect such signs of life during an EVA.

Mars-500

The Mars-500 mission was a series of experiments conducted between 2007 and 2011 and sponsored by Russia, the European Space Agency, and China. The primary focus of these experiments was to study the effects of long-term isolation on a small crew, so that the psychological difficulties of a voyage to Mars and an extended stay on its surface may be better understood. [10] Three separate missions were performed: a 14-day isolation in November 2007, a 105-day isolation completed in July 2009, and a 520-day isolation from April 2010 to October 2011. Unlike other Mars Analog missions, Mars-500 did not take place in a Mars-like environment, but in a Moscow research institute.

An important focus of the Mars-500 research has been the early diagnosis of “adverse personal dynamics” which would affect cooperation among the crew, as well as the development of methods to overcome such issues. [11] Researchers decided that any sort of psychological support on future missions would need to be tailored to each individual crew member, not just to the group as a whole or to subgroups belonging to different space agencies. Mars-500 also found that most psychological issues were exacerbated by isolation and a lack of stimulus, emphasizing the need to prevent sensory deprivation and boredom.

While female Russian biologist Marina Tugusheva participated in the 2007 experiment, women were reportedly excluded from the 2009 and 2011 missions to prevent issues caused by sexual tension.[ citation needed ] However, given the multinational nature of the crew, special efforts were made to promote efficient interaction among a multicultural crew. [12]

HI-SEAS

The Hawaii Space Exploration Analog and Simulation (HI-SEAS) program is a series of missions organized by Cornell University and the University of Hawai'i at Mānoa. [13] The habitat is located 2,400 meters (8,000ft) above sea level on Mauna Loa on the Big Island of Hawaii. The first HI-SEAS mission ran from April to August 2013, and a series of later missions have followed. [14]

Like other missions, HI-SEAS evaluates the social and psychological status of the crewmembers while they live in isolation and conduct field work in Mars-like environments and conditions. Early missions focused on the diet and nutrition of its crewmembers. In particular, HI-SEAS studied how “food intake in a confined and isolated setting similar to what an astronaut would experience during a mission” affects the moods of the crew members and their interactions with each other. [15] Crew members prepare their own meals using combinations of shelf-stable ingredients and pre-packaged meals and frequently complete surveys to determine their mood, health, and satisfaction with the food. More recent missions have focused on crew composition and communication, with specific focus on in-mission crew interaction and mission debrief technique. [16]

HI-SEAS also undertakes research proposals submitted by outside researchers. As part of this effort, HI-SEAS is testing software which monitors psychological welfare by analyzing text-based communication, so that future astronauts’ limited access to psychiatric help is less of an issue. In addition, HI-SEAS is testing the durability of antimicrobial clothing used daily by the crew members.

CHAPEA

The CHAPEA (Crew Health and Performance Exploration Analog) habitat at NASA's Johnson Space Center will undertake a series of analog missions that will simulate year-long stays on the surface of Mars. Each mission will consist of four crew members living in Mars Dune Alpha, an isolated 1,700 square foot habitat.

CHAPEA Mission 1 began on June 25, 2023, with crew members Kelly Haston, Ph.D (commander), Ross Brockwell (flight engineer), Nathan Jones, M.D. (medical officer), and Anca Selariu, Ph.D (science officer). [17]

Possible future missions

The Flashline Mars Arctic Research Station, Mars Desert Research Station, and HI-SEAS missions are all ongoing. FMARS will launch a one-year mission (Mars Arctic 365) in August 2014. [18] Just as in past missions, Mars Arctic 365 will consist of six volunteers with skills in fields such as geology, biochemistry, microbiology, and engineering, all of whom will conduct field research in Mars-like conditions while in contact with remote support teams. MDRS has scheduled additional short-term missions through May 2014. [19] The Mars Society has planned to establish two more habitats in Mars-like desert locations: the European Mars Analog Research Station in Iceland, and the Australia Mars Analog Research Station in the Australian outback. [20] While these stations were to be built in 2003, neither has moved past the planning stages, and the future of the missions is unclear.

See also

Related Research Articles

The Mars Society is a nonprofit organization that advocates for human Mars exploration and colonization. It was founded by Robert Zubrin in 1998 and its principles are based on Zubrin's Mars Direct philosophy, which aims to make human mission to Mars as lightweight and feasible as possible. The Mars Society aims to generate interest in the Mars program by garnering support from the public and through lobbying. Many Mars Society members and former members are influential in the wider spaceflight community, such as Buzz Aldrin and Elon Musk.

<span class="mw-page-title-main">Mars Desert Research Station</span> Longest-running Mars analog habitat

The Mars Desert Research Station (MDRS) is the largest and longest-running Mars surface research facility and is one of two simulated Mars analog habitats owned and operated by the Mars Society.

<span class="mw-page-title-main">Devon Island</span> Uninhabited island in Nunavut, Canada

Devon Island is an island in Canada and the largest uninhabited island in the world. It is located in Baffin Bay, Qikiqtaaluk Region, Nunavut, Canada. It is one of the largest members of the Arctic Archipelago, the second-largest of the Queen Elizabeth Islands, Canada's sixth-largest island, and the 27th-largest island in the world. It has an area of 55,247 km2 (21,331 sq mi). The bedrock is Precambrian gneiss and Paleozoic siltstones and shales. The highest point is the Devon Ice Cap at 1,920 m (6,300 ft) which is part of the Arctic Cordillera. Devon Island contains several small mountain ranges, such as the Treuter Mountains, Haddington Range and the Cunningham Mountains. The notable similarity of its surface to that of Mars has attracted interest from scientists.

<span class="mw-page-title-main">Flashline Mars Arctic Research Station</span> Simulated Mars habitat on Devon Island, Nunavut, Canada

The Flashline Mars Arctic Research Station (FMARS) is the first of two simulated Mars habitats located on Devon Island, Nunavut, Canada, which is owned and operated by the Mars Society. The station is a member of the European Union-INTERACT circumarctic network of currently 89 terrestrial field bases located in northern Europe, Russia, US, Canada, Greenland, Iceland, the Faroe Islands, and Scotland as well as stations in northern alpine areas.

<span class="mw-page-title-main">Pascal Lee</span> American planetary scientist

Pascal Lee is co-founder and chairman of the Mars Institute, a planetary scientist at the SETI Institute, and the Principal Investigator of the Haughton-Mars Project (HMP) at NASA Ames Research Center in Mountain View, California. He holds an ME in geology and geophysics from the University of Paris, and a PhD in astronomy and space sciences from Cornell University.

<span class="mw-page-title-main">Haughton–Mars Project</span>

The Haughton–Mars Project (HMP) is an international interdisciplinary field research project being carried out near the Haughton impact crater on Canada's northern Devon Island. Human-centered computing (HCC) studies are aimed at determining how human explorers might live and work on other planetary objects, in particular on Mars. Conducted jointly by SETI and the Mars Institute, the project's goal is to utilize the Mars-like features of Devon Island and the impact crater to develop and test new technologies and field operating procedures, and to study the human dynamics which result from extended contact in close quarters. This knowledge will be used in planning missions by both humans and robots to other terrestrial bodies.

<span class="mw-page-title-main">MARS-500</span> Psychosocial isolation experiment in spaceflight research

The MARS-500 mission was a psychosocial isolation experiment conducted between 2007 and 2011 by Russia, the European Space Agency, and China, in preparation for an unspecified future crewed spaceflight to the planet Mars. The experiment's facility was located at the Russian Academy of Sciences' Institute of Biomedical Problems (IBMP) in Moscow, Russia.

<span class="mw-page-title-main">Desert Research and Technology Studies</span> Field trials of technologies for manned planetary exploration

NASA's Desert Research and Technology Studies is a group of teams which perform an annual series of field trials seeking to demonstrate and test candidate technologies and systems for human exploration of the surface of the Moon, Mars, or other rocky bodies.

Human analog missions are activities undertaken on Earth in various environments to simulate aspects of human missions to other worlds, including the Moon, asteroids, and Mars. These remote field tests are performed in locations that are identified based on their physical similarities to the extreme space environments of a target mission. Such activities are undertaken to test hardware and operational concepts in relevant environments.

<span class="mw-page-title-main">Jonathan Dory</span> Human Systems Integration Lead at NASAs Johnson Space Center

Jonathan Robert Dory is a Human Systems Integration Lead at NASA's Johnson Space Center (JSC) in Houston, Texas. He is Branch Chief of NASA's Habitability and Human Factors Branch, part of the Habitability and Environmental Factors Division at NASA/JSC. Dory supports crew safety and productivity on the International Space Station (ISS) Program by planning and assessing the on-orbit interior configuration of ISS, as well as performing anthropometric analysis of crew tasks. He contributes to the integrated operation of the Space Station while using 3D computer graphics and animation software as part of his daily work. In July 2002, Dory served as an aquanaut on the NASA Extreme Environment Mission Operations 3 crew.

<span class="mw-page-title-main">Vladimir Pletser</span>

Vladimir Pletser is Director of Space Training Operations at Blue Abyss since 2018, where he is in charge of developing astronaut training programs. From 2016 to early 2018, he was a Visiting Professor and Scientific Adviser at the Technology and Engineering Centre for Space Utilization (CSU) of the Chinese Academy of Sciences in Beijing, China. He supported the preparation of scientific experiments in microgravity for the Chinese Tiangong space station and for aircraft parabolic flights. He worked previously from 1985 till early 2016 as a senior Physicist Engineer at the European Space Research and Technology Centre (ESTEC) of ESA.

Terrestrial analogue sites are places on Earth with assumed past or present geological, environmental or biological conditions of a celestial body such as the Moon or Mars. Analogue sites are used in the frame of space exploration to either study geological or biological processes observed on other planets, or to prepare astronauts for surface extra-vehicular activity.

The Austrian Space Forum (OeWF) is an expert organization in the field of analogue research, which researches how humans can prepare on Earth for astronautical exploration of other planets. Since the AustroMars mission in 2006, OeWF has been involved in analog research, developing space suit simulators and also conducting astronautical simulations on Earth. The resulting data is available to researchers from a wide range of disciplines in the Multi-Mission Science Data Archive

Angelo Vermeulen is a Belgian space systems researcher, biologist and artist. In 2009 he co-founded SEADS, an international transdisciplinary collective of artists, scientists, engineers, and activists Its goal is to reshape the future through critical inquiry and hands-on experimentation. Biomodd is one of their most well-known art projects and consists of a worldwide series of co-created interactive art installations in which computers coexist with internal living ecosystems. For the last ten years, he has been collaborating with the European Space Agency’s MELiSSA program on biological life support for space and in 2013 he was crew commander of one of the NASA-funded HI-SEAS Mars mission simulations in Hawai'i. Currently, he works at Delft University of Technology on advanced concepts for interstellar exploration. His work proposes a bio-inspired design approach to deal with the unpredictability inherent to interstellar travel. He is a Senior TED Fellow and was selected in 2017 as one of the Top 5 Tech Pioneers from Belgium by the newspaper De Tijd.

<span class="mw-page-title-main">HI-SEAS</span> Analog habitat for human spaceflight to Mars

The Hawaii Space Exploration Analog and Simulation (HI-SEAS) is an analog habitat for human spaceflight to Mars currently operated by the International MoonBase Alliance. HI-SEAS is located in an isolated position on the slopes of the Mauna Loa volcano on the island of Hawaii. The area has Mars-like features and an elevation of approximately 8,200 feet (2,500 m) above sea level. The first HI-SEAS study was in 2013 and NASA's Human Research Program continues to fund and sponsor follow-up studies. The missions are of extended duration from four months to a year. Its missions place HI-SEAS in the company of a small group of analogs that are capable of operating very long duration missions in isolated and confined environments, such as Mars500, Concordia, and the International Space Station.

<span class="mw-page-title-main">Psychological and sociological effects of spaceflight</span>

Psychological and sociological effects of space flight are important to understanding how to successfully achieve the goals of long-duration expeditionary missions. Although robotic spacecraft have landed on Mars, plans have also been discussed for a human expedition, perhaps in the 2030s, or as early as 2024 for a return mission.

The International Lunar Exploration Working Group(ILEWG) is a public forum sponsored by the world's space agencies to support "international cooperation towards a world strategy for the exploration and utilization of the Moon - our natural satellite" (International Lunar Workshop, Beatenberg (CH), June 1994).

<span class="mw-page-title-main">Darlene Lim</span> NASA geobiologist and exobiologist

Darlene Sze Shien Lim is a NASA geobiologist and exobiologist who prepares astronauts for scientific exploration of the Moon, Deep Space and Mars. Her expertise involves Mars human analog missions, in which extreme landscapes like volcanoes and Arctic deserts serve as physical or operational substitutes for various planetary bodies. She has become a leading public figure for Mars exploration, having presented her missions publicly at academic institutions and public events around the world. She has also discussed her work for various media groups such as NPR, The New York Times, and The Washington Post.

Tamarack "Tam" R. Czarnik is an American medical researcher, notable for space advocacy and academic studies of human physiology in extreme environmental conditions. Czarnik is especially known for his scientific contributions to space medicine as well as a better understanding of such phenomena as ebullism and uncontrolled decompression. He is the author of a number of publications in the domain of bioastronautics including "Ebullism at 1 million feet: Surviving Rapid/Explosive Decompression" and "Medical emergencies in space". Czarnik was at the origin of the Mars Society Chapter foundation in Dayton, Ohio, and also served as the chapter's first Chair. From 2001 to 2011, Czarnik served in several missions as Medical Director for the Mars Society's FMARS and MDRS, simulated Mars habitats.

References

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