Caves of Mars Project

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THEMIS image of probable cave entrances on Arsia Mons. The pits have been informally named (A) Dena, (B) Chloe, (C) Wendy, (D) Annie, (E) Abby (left) and Nikki, and (F) Jeanne. Mars caves from NASA orbiters.jpg
THEMIS image of probable cave entrances on Arsia Mons. The pits have been informally named (A) Dena, (B) Chloe, (C) Wendy, (D) Annie, (E) Abby (left) and Nikki, and (F) Jeanne.

The Caves of Mars Project was an early 2000s program funded through Phase II[ clarification needed ] by the NASA Institute for Advanced Concepts [1] [2] to assess the best place to situate the research and habitation modules that a human mission to Mars would require. [3] The final report was published in mid 2004. [3]

Contents

Description

A HiRISE image of a lava tube skylight entrance on the Martian volcano Pavonis Mons. Pavonis Mons lava tube skylight crop.jpg
A HiRISE image of a lava tube skylight entrance on the Martian volcano Pavonis Mons.

Caves and other underground structures, including Martian lava tubes, canyon overhangs, and other Martian cavities would be potentially useful for crewed missions, for they would provide considerable shielding from both the elements and intense solar radiation to which a Mars mission would expose astronauts. They might also offer access to minerals, gases, ices, and any subterranean life that the crew of such a mission would probably be searching for. [3]

The program also studied designs for inflatable modules and other such structures that would aid the astronauts to build a livable environment for humans and other Earthian creatures. [3]

Summary of final report

The final report, Human Utilization Of Subsurface Extraterrestrial Environments, [4] is divided into 10 parts.

Project Summary

Section 1 summarizes the entire project and claims that "This project developed a revolutionary system to exploit the novel idea of extraterrestrial cave use" and explaining that two experiments or "Missions" were tested to gather data.

Introduction

Section 2 addresses the question of "why caves [for martian research bases]?" and provides a variety of different answers to the advantages of using caves as a foothold in Martian exploration such as:

This section also contains some speculation on the existence and locations of such caves and what types of caves exist on Mars however it is largely outdated by newer research such as the HiRISE and THEMIS missions.

Enabling Technologies Identification

Section 3 analyses a number of Innovations necessary for the utilization and assigns them a Technology Readiness Level. For example, the innovation "Foamed-in-place Airlocks" are assigned a TRL of 5, while the "Inert Pressurization of Caves" is assigned a TRL of 2.

Essential Tasks Identification

Section 4 describes the steps necessary for cave habitation. These are:

The publication discusses each of these topics in detail and highlights the novel idea of using luminescent bacteria as a lighting backup solution and suggests lighting the habitat using "light piping" technology. The article also discusses skylights and radiation proof glass at length however this is probably due to the lack of advanced solar panels and LED lighting technology available during the publication in 2000.

Demonstration Missions

Section 5 contains information on the "Mouse Mission to Inner Space" (MOMIS) and the Human equivalent, "HUMIS". The idea was to develop preliminary versions of some aspects of a Mars cave habitat such as using argon breathing mixtures and other new life support systems on mouse test subjects. The MOMIS experiment has successfully completed multiple runs however the HUMIS experiment was deemed out of the scope of the investigation and although efforts were made to find test sites, the work done was reflected in a "Cave Astrobiology" exploration-level class at Penn State College during the spring semester of 2004.

Technology Trials

Section 6 covers the different technology tests performed.

First, inflatable habitats were investigated to provide a "shirtsleeve indoor environment" for the astronauts. The article further suggests that if the cave's cross sectional surface area is properly sized, an inflatable cave liner could be placed in the cave and inflated requiring no additional support systems. The article then suggests using a dual-liner system in which an outer liner provides a surface against the cave surface and a pressure seal and an inner liner provides a habitat for the astronauts. Machinery and life support systems could be placed in between the redundant liners. The report also outlines methods of folding, manufacturing, transporting, replacing, and inflating these liners.

Another main topic of this section is the "foamed in place" airlocks. These are designed to be shape-conforming to highly irregular openings along with easy to deploy and leak tight. Their final proposed system is an airlock unit with multiple extending telescoping legs to all of the cave walls. The space between the airlocks and the cave walls are then filled with hardening, spray-able, airtight foam.

Next, the report outlines methods by which an inert pressure atmosphere could be created by pressurizing the gasses present on Mars, particularly Argon. This would allow human scientists only to wear breathing apparatuses and not require full pressure suits. It is suggested that cavernous spaces not be filled with oxygen or other reactive gasses as this would nullify any potential scientific value of the cave along with potentially being harmful to the humans breathing in the atmosphere inside.

Finally, this section covers a system that would allow communication networks inside caves. This was also tested in a real cave (Robertson's Cave) and future modifications are suggested for increasing bandwidth and signal strength.

Planetary Protection Protocol Development

Section 7 covers the development of a Planetary Protection Protocol and highlights its importance when exploring martian caves and suggests using "sterilized micro-robots" to perform exploration and science.

Education and Outreach

Section 8 contains information on the spinoff science-fair experiments generated from this report and the other outreach impacts that this report and creating it had. This section also outlines educational activities for schools such as a "Find the lava tube activity" and "The Masternauts Program".

Conclusions and references

Sections 9 and 10 conclude the report and cite references for further reading. [3]

Results

The project showed crickets and mice could breathe argon mixtures for extended periods without apparent problems. [3]

The project produced many educational materials, made available through its outreach initiative. [3]

Demonstrated wireless communications within limestone cave system. [3]

See also

Related Research Articles

<span class="mw-page-title-main">Lava tube</span> Natural conduit through which lava flows beneath the solid surface

A lava tube, or pyroduct, is a natural conduit formed by flowing lava from a volcanic vent that moves beneath the hardened surface of a lava flow. If lava in the tube empties, it will leave a cave.

<span class="mw-page-title-main">Colonization of Mars</span> Proposed concepts for human settlements on Mars

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<span class="mw-page-title-main">Human mission to Mars</span> Proposed concepts

The idea of sending humans to Mars has been the subject of aerospace engineering and scientific studies since the late 1940s as part of the broader exploration of Mars. Long-term proposals have included sending settlers and terraforming the planet. Currently, only robotic landers and rovers have been on Mars. The farthest humans have been beyond Earth is the Moon, under the U.S. National Aeronautics and Space Administration (NASA) Apollo program which ended in 1972.

<span class="mw-page-title-main">Suitport</span> Alternative technology to enable extravehicular activity

A suitport or suitlock is an alternative technology to an airlock, designed for use in hazardous environments including in human spaceflight, especially planetary surface exploration. Suitports present advantages over traditional airlocks in terms of mass, volume, and ability to mitigate contamination by—and of—the local environment.

<span class="mw-page-title-main">Space architecture</span> Architecture of off-planet habitable structures

Space architecture is the theory and practice of designing and building inhabited environments in outer space. This mission statement for space architecture was developed at the World Space Congress in Houston in 2002 by members of the Technical Aerospace Architecture Subcommittee of the American Institute of Aeronautics and Astronautics (AIAA). The architectural approach to spacecraft design addresses the total built environment. It is mainly based on the field of engineering, but also involves diverse disciplines such as physiology, psychology, and sociology.

<span class="mw-page-title-main">Mars to Stay</span> Mars colonization architecture proposing no return vehicles

Mars to Stay missions propose that astronauts sent to Mars for the first time should intend to remain there. Unused emergency return vehicles would be recycled into settlement construction as soon as the habitability of Mars becomes evident to the initial pioneers. Mars to Stay missions are advocated both to reduce cost and to ensure permanent settlement of Mars. Among many notable Mars to Stay advocates, former Apollo astronaut Buzz Aldrin has been particularly outspoken, suggesting in numerous forums "Forget the Moon, Let’s Head to Mars!" and, in June 2013, Aldrin promoted a crewed mission "to homestead Mars and become a two-planet species". In August 2015, Aldrin, in association with the Florida Institute of Technology, presented a "master plan", for NASA consideration, for astronauts, with a "tour of duty of ten years", to colonize Mars before the year 2040. The Mars Underground, Mars Homestead Project / Mars Foundation, Mars One, and Mars Artists Community advocacy groups and business organizations have also adopted Mars to Stay policy initiatives.

<span class="mw-page-title-main">Penelope Boston</span> American speleologist

Penelope J. Boston is a speleologist and astrobiologist. She was associate director of the National Cave and Karst Research Institute in Carlsbad, New Mexico, along with founding and directing the Cave and Karst Studies Program at New Mexico Institute of Mining and Technology in Socorro. Among her research interests are geomicrobiology of caves and mines, extraterrestrial speleogenesis, and space exploration and astrobiology generally.

<span class="mw-page-title-main">Lunar lava tube</span> Type of natural tunnel on the Moon

Lunar lava tubes are lava tubes on the Moon formed during the eruption of basaltic lava flows. When the surface of a lava flow cools, it hardens and the lava can channel beneath the surface in a tube-shaped passage. Once the flow of lava diminishes, the tube may drain, forming a hollow void. Lunar lava tubes are formed on sloped surfaces that range in angle from 0.4° to 6.5°. These tubes may be as wide as 500 metres (1,600 ft) before they become unstable against gravitational collapse. However, stable tubes may still be disrupted by seismic events or meteoroid bombardment.

Interplanetary contamination refers to biological contamination of a planetary body by a space probe or spacecraft, either deliberate or unintentional.

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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.

<span class="mw-page-title-main">Deep Space Habitat</span> Conceptual design for Mars-bound spaceship

The Deep Space Habitat (DSH) is a series of concepts explored between 2012 and 2018 by NASA for methods to support crewed exploration missions to the Moon, asteroids, and eventually Mars. Some of these concepts were eventually used in the Lunar Gateway program.

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. 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.

<span class="mw-page-title-main">Crewed Mars rover</span> Mars rovers transporting people

Crewed Mars rovers are Mars rovers for transporting people on the planet Mars, and have been conceptualized as part of human missions to that planet.

<span class="mw-page-title-main">Mars habitat</span> Facility where humans could live on Mars

A Mars habitat is a hypothetical place where humans could live on Mars. Mars habitats would have to contend with surface conditions that include almost no oxygen in the air, extreme cold, low pressure, and high radiation. Alternatively, the habitat might be placed underground, which helps solve some problems but creates new difficulties.

<span class="mw-page-title-main">Martian lava tube</span> Volcanic caverns on Mars, believed to form as a result of fast-moving basaltic lava flows

Martian lava tubes are volcanic caverns on Mars that are believed to form as a result of fast-moving, basaltic lava flows associated with shield volcanism. Lava tubes usually form when the external surface of the lava channels cools more quickly and forms a hardened crust over subsurface lava flows. The flow eventually ceases and drains out of the tube, leaving a conduit-shaped void space which is usually several meters below the surface. Lava tubes are typically associated with extremely fluid pahoehoe lava. Gravity on mars is about 38% that of Earth's, allowing Martian lava tubes to be much larger in comparison.

<span class="mw-page-title-main">Mars suit</span> Space suit for the Martian surface

A Mars suit or Mars space suit is a space suit for EVAs on the planet Mars. Compared to a suit designed for space-walking in the near vacuum of low Earth orbit, Mars suits have a greater focus on actual walking and a need for abrasion resistance. Mars' surface gravity is 37.8% of Earth's, approximately 2.3 times that of the Moon, so weight is a significant concern, but there are fewer thermal demands compared to open space. At the surface the suits would contend with the atmosphere of Mars, which has a pressure of about 0.6 to 1 kilopascal. On the surface, radiation exposure is a concern, especially solar flare events, which can dramatically increase the amount of radiation over a short time.

<span class="mw-page-title-main">Space habitat (facility)</span> Facility fulfilling habitational purposes

A space habitat in a basic sense is any facility providing shelter and fulfilling habitational purposes in outer space. It is not to be confused with an extended space settlement, an arrangement of or infrastructure for multiple habitation facilities, in the sense of a space settlement. Space stations or theoretical extraterrestrial stations, such as a Moonbase or Mars habitat, include or are basic space habitats.

Astroland Interplanetary Agency is a Spanish interplanetary agency based in Cantabria, Spain. Astroland operates the first permanent, plug-and -play subsurface analogue station inside a cave of 1.5 km long and 60 meters high in Santander. Astroland is an aerospace startup acting as a research organization, whose main objective is to envision future living capabilities on Mars.

References

  1. Robert Braun; et al. (2009). Appendix E: List and Statistical Analysis of NIAC Grants. National Academies Press. ISBN   978-0-309-14051-5 . Retrieved 2010-06-30.{{cite book}}: |work= ignored (help)
  2. David, Leonard (2005-02-22). "Digging and Sniffing for Life on Mars". Space.com . Retrieved 2010-06-30.
  3. 1 2 3 4 5 6 7 8 Boston, P.; Frederick, G.; Welch, S.; Werker, J.; Meyer, T.R.; Sprungman, B.; Hildreth-Werker, V.; Murphy, D.; Thompson, S.L. (2004), "System Feasibility Demonstrations of Caves and Subsurface Constructed for Mars Habitation and Scientific Exploration" (PDF), USRA Reports, NASA Institute for Advanced Concepts , retrieved 2010-06-30
  4. "Human utilization of subsurface extraterrestrial environments: Final report". Archived from the original on 2021-07-30. Retrieved 2021-06-28.

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