Английская Википедия:Colonization of Mars

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An astronaut fixing machine on Mars and another heading back to the base
Artist conception of astronauts working outside, near a large modular habitat

Colonization or settlement of Mars is the theoretical human migration to and establishment of long-term human presence on Mars. The prospect has garnered interest from public space agencies and private corporations and has been extensively explored in science fiction writing, film, and art. Organizations have proposed plans for a human mission to Mars, the first step towards any colonization effort, but thus far no person has set foot on the planet, and there have been no return missions. However, landers and rovers have successfully explored the planetary surface and delivered information about conditions on the ground.

Mars' orbit is close to Earth's orbit and the asteroid belt. While Mars' day and general composition are similar to Earth, the planet is hostile to life. Mars has an unbreathable atmosphere, thin enough that its temperature on average fluctuates between Шаблон:Cvt, yet thick enough to cause planet-wide dust storms. The barren landscape on Mars is covered by fine, toxic dust and intense ionizing radiation. Mars has in-situ resources, such as underground water, Martian soil, and ore, which could be used by colonists. Opportunities to generate electricity via wind, solar, and nuclear power using resources on Mars are poor.

Justifications and motivations for colonizing Mars include curiosity, the potential for humans to provide more in-depth observational research than uncrewed rovers, an economic interest in its resources, and the possibility that the settlement of other planets could decrease the probability of human extinction. Difficulties and hazards include radiation exposure during a trip to Mars and on its surface, toxic soil, low gravity, the isolation that accompanies Mars' distance from Earth, a lack of water, and cold temperatures.

Commitments to researching permanent settlement have been made by public space agencies—NASA, ESA, Roscosmos, ISRO, the CNSA, among others—and private organizations—SpaceX, Lockheed Martin, and Boeing.

Mission concepts and timelines

Since the 20th century, there have been several proposed human missions to Mars both by government agencies and private companies.Шаблон:Vague

Most of the human mission concepts as currently conceived by national governmental space programs would not be direct precursors to colonization. Programs such as those being tentatively planned by NASA, Roscosmos, and ESA are intended solely as exploration missions, with the establishment of a permanent base possible but not yet the main goal. Шаблон:Citation needed

Colonization requires the establishment of permanent habitats that have the potential for self-expansion and self-sustenance. Two early proposals for building habitats on Mars are the Mars Direct and the Semi-Direct concepts, advocated by Robert Zubrin, an advocate of the colonization of Mars.[1]

At the February 2017 World Government Summit, the United Arab Emirates announced a plan to establish a settlement on Mars by 2117, led by the Mohammed bin Rashid Space Centre.[2][3]

Comparisons between Earth and Mars

Atmospheric pressure comparison
Location Pressure
Olympus Mons summit Шаблон:Convert (0.0007 atm)
Mars average Шаблон:Convert (0.006 atm)
Hellas Planitia bottom Шаблон:Convert (0.0114 atm)
Armstrong limit Шаблон:Convert (0.0617 atm)
Mount Everest summit[4] Шаблон:Convert (0.3326 atm)
Earth sea level Шаблон:Convert (1 atm)

Gravity and size

The surface gravity of Mars is just 38% that of Earth. Although microgravity is known to cause health problems such as muscle loss and bone demineralization,[5][6] it is not known if Martian gravity would have a similar effect. The Mars Gravity Biosatellite was a proposed project designed to learn more about what effect Mars' lower surface gravity would have on humans, but it was cancelled due to a lack of funding.[7]

Mars has a surface area that is 28.4% of Earth's, which is only slightly less than the amount of dry land on Earth (which is 29.2% of Earth's surface). Mars has half the radius of Earth and only one-tenth the mass. This means that it has a smaller volume (≈15%) and lower average density than Earth.

Magnetosphere

Due to the lack of a magnetosphere, solar particle events and cosmic rays can easily reach the Martian surface.[8][9][10]

Atmosphere

Atmospheric pressure on Mars is far below the Armstrong limit at which people can survive without pressure suits. Since terraforming cannot be expected as a near-term solution, habitable structures on Mars would need to be constructed with pressure vessels similar to spacecraft, capable of containing a pressure between 30 and 100 kPa. The atmosphere is also toxic as most of it consists of carbon dioxide (95% carbon dioxide, 3% nitrogen, 1.6% argon, and traces totaling less than 0.4% of other gases, including oxygen).

This thin atmosphere does not filter out ultraviolet sunlight, which causes instability in the molecular bonds between atoms. For example, ammonia (NH3) is not stable in the Martian atmosphere and breaks down after a few hours.[11] Also due to the thinness of the atmosphere, the temperature difference between day and night is much larger than on Earth, typically around 70 °C.[12] However, the day/night temperature variation is much lower during dust storms when very little light gets through to the surface even during the day, and instead warms the middle atmosphere.[13]

Water and climate

Water on Mars is scarce, with rovers Spirit and Opportunity finding less than there is in Earth's driest desert.[14][15][16]

The climate is much colder than Earth, with mean surface temperatures between Шаблон:Convert (depending on the season and latitude).[17][18] The lowest temperature ever recorded on Earth was 184 K (−89.2 °C) in Antarctica.

Because Mars is about 52% farther from the Sun, the amount of solar energy entering its upper atmosphere per unit area (the solar constant) is only around 43.3% of what reaches the Earth's upper atmosphere.[19] However, due to the much thinner atmosphere, a higher fraction of the solar energy reaches the surface as radiation.[20][21] The maximum solar irradiance on Mars is about 590 W/m2 compared to about 1000 W/m2 at the Earth's surface; optimal conditions on the Martian equator can be compared to those on Devon Island in the Canadian Arctic in June.[22] Mars' orbit is more eccentric than Earth's, increasing temperature and solar constant variations over the course of the Martian year.Шаблон:Citation needed Mars has no rain and virtually no clouds,Шаблон:Citation needed so although cold, it is permanently sunny (apart from during dust storms). This means solar panels can always operate at maximum efficiency on dust-free days.

Global dust storms are common throughout the year and can cover the entire planet for weeks, blocking sunlight from reaching the surface.[23][24] This has been observed to cause temperature drops of 4 °C for several months after the storm.[25] In contrast, the only comparable events on Earth are infrequent large volcanic eruptions such as the Krakatoa event which threw large amounts of ash into the atmosphere in 1883, causing a global temperature drop of around 1 °C. These dust storms would affect electricity production from solar panels for long periods, and interfere with communications with Earth.[13]

Temperature and seasons

Mars has an axial tilt of 25.19°, similar to Earth's 23.44°. As a result, Mars has seasons much like Earth, though on average they last nearly twice as long because the Martian year is about 1.88 Earth years, despite having a similar rotational period (known as a sol) to an Eartian day (see below). Mars' temperature regime is more similar to Earth's than to any other planet's in the solar system. While generally colder than Earth, Mars can have Earth-like temperatures in some areas and at certain times.

Soil

The Martian soil is toxic due to relatively high concentrations of chlorine and associated compounds, such as perchlorates, which are hazardous to all known forms of life,[26][27] even though some halotolerant microorganisms might be able to cope with enhanced perchlorate concentrations by drawing on physiological adaptations similar to those observed in the yeast Debaryomyces hansenii exposed in lab experiments to increasing NaClO4 concentrations.[28]

Survivability

Plants and animals cannot survive the ambient conditions on the surface of Mars.[29] However, some extremophile organisms that survive in hostile conditions on Earth have endured periods of exposure to environments that approximate some of the conditions found on Mars.

Length of day

The Martian day (or sol) is very close in duration to Earth's. A solar day on Mars is 24 hours, 39 minutes and 35.244 seconds.[30]

Conditions for human habitation

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An expedition-style crewed mission would operate on the surface, but for limited amounts of time.
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Dust is one concern for Mars missions.

Conditions on the surface of Mars are closer to the conditions on Earth in terms of temperature and sunlight than on any other planet or moon, except for the cloud tops of Venus.[31] However, the surface is not hospitable to humans or most known life forms due to the radiation, greatly reduced air pressure, and an atmosphere with only 0.16% oxygen.

In 2012, it was reported that some lichen and cyanobacteria survived and showed remarkable adaptation capacity for photosynthesis after 34 days in simulated Martian conditions in the Mars Simulation Laboratory (MSL) maintained by the German Aerospace Center (DLR).[32][33][34] Some scientists think that cyanobacteria could play a role in the development of self-sustainable crewed outposts on Mars.[35] They propose that cyanobacteria could be used directly for various applications, including the production of food, fuel and oxygen, but also indirectly: products from their culture could support the growth of other organisms, opening the way to a wide range of life-support biological processes based on Martian resources.[35]

Humans have explored parts of Earth that match some conditions on Mars. Based on NASA rover data, temperatures on Mars (at low latitudes) are similar to those in Antarctica.[36] The atmospheric pressure at the highest altitudes reached by piloted balloon ascents (35 km (114,000 feet) in 1961,[37] 38 km in 2012) is similar to that on the surface of Mars. However, the pilots were not exposed to the extremely low pressure, as it would have killed them, but seated in a pressurized capsule.[38]

Human survival on Mars would require living in artificial Mars habitats with complex life-support systems. One key aspect of this would be water processing systems. Being made mainly of water, a human being would die in a matter of days without it. Even a 5–8% decrease in total body water causes fatigue and dizziness and a 10% decrease physical and mental impairment (See Dehydration). A person in the UK uses 70–140 litres of water per day on average.[39] Through experience and training, astronauts on the ISS have shown it is possible to use far less, and that around 70% of what is used can be recycled using the ISS water recovery systems. (For instance, half of all water is used during showers.[40]) Similar systems would be needed on Mars but would need to be much more efficient, since regular robotic deliveries of water to Mars would be prohibitively expensive (the ISS is supplied with water four times per year). Potential access to on-site water (frozen or otherwise) via drilling has been investigated by NASA.[41]

Effects on human health

Шаблон:Main Mars presents a hostile environment for human habitation. Different technologies have been developed to assist long-term space exploration and may be adapted for habitation on Mars. The existing record for the longest consecutive space flight is 438 days by cosmonaut Valeri Polyakov,[42] and the most accrued time in space is 878 days by Gennady Padalka.[43] The longest time spent outside the protection of the Earth's Van Allen radiation belt is about 12 days for the Apollo 17 Moon landing. This is minor in comparison to the 1100-day journey to Mars and back[44] envisioned by NASA for possibly as early as the year 2028. Scientists have also hypothesized that many different biological functions can be negatively affected by the environment of Mars colonies. Due to higher levels of radiation, there are a multitude of physical side-effects that must be mitigated.[45] In addition, Martian soil contains high levels of toxins which are hazardous to human health.

Physical effects

The difference in gravity may negatively affect human health by weakening bones and muscles. There is also risk of osteoporosis and cardiovascular problems. Current rotations on the International Space Station put astronauts in zero gravity for six months, a comparable length of time to a one-way trip to Mars. This gives researchers the ability to better understand the physical state that astronauts going to Mars would arrive in. Once on Mars, surface gravity is only 38% of that on Earth. Microgravity affects the cardiovascular, musculoskeletal and neurovestibular (central nervous) systems. The cardiovascular effects are complex. On Earth, blood within the body stays 70% below the heart, but in microgravity this is not the case due to nothing pulling the blood down. This can have several negative effects. Once entering into microgravity, the blood pressure in the lower body and legs is significantly reduced.[46] This causes legs to become weak through loss of muscle and bone mass. Astronauts show signs of a puffy face and chicken legs syndrome. After the first day of reentry back to earth, blood samples showed a 17% loss of blood plasma, which contributed to a decline of erythropoietin secretion.[47][48] On the skeletal system which is important to support our body's posture, long space flight and exposure to microgravity cause demineralization and atrophy of muscles. During re-acclimation, astronauts were observed to have a myriad of symptoms including cold sweats, nausea, vomiting and motion sickness.[49] Returning astronauts also felt disoriented. Journeys to and from Mars being six months is the average time spent at the ISS. Once on Mars with its lesser surface gravity (38% percent of Earth's), these health effects would be a serious concern.[50] Upon return to Earth, recovery from bone loss and atrophy is a long process and the effects of microgravity may never fully reverse.Шаблон:Citation needed

Radiation

Dangerous amounts of radiation reach Mars' surface despite it being much further from the Sun compared to Earth. Mars has lost its inner dynamo giving it a weaker global magnetosphere than Earth does. Combined with a thin atmosphere, this permits a significant amount of ionizing radiation to reach the Martian surface. There are two main types of radiation risks to traveling outside the protection of Earth's atmosphere and magnetosphere: galactic cosmic rays (GCR) and solar energetic particles (SEP). Earth's magnetosphere protects from charged particles from the Sun, and the atmosphere protects against uncharged and highly energetic GCRs. There are ways to mitigate solar radiation, but without much of an atmosphere, the only solution to the GCR flux is heavy shielding amounting to roughly 15 centimeters of steel, 1 meter of rock, or 3 meters of water, limiting human colonists to living underground most of the time.[51] Шаблон:Further The Mars Odyssey spacecraft carries an instrument, the Mars Radiation Environment Experiment (MARIE), to measure the radiation. MARIE found that radiation levels in orbit above Mars are 2.5 times higher than at the International Space Station. The average daily dose was about Шаблон:Convert—equivalent to 0.08 Gy per year.[52] A three-year exposure to such levels would exceed the safety limits currently adopted by NASA,[53] and the risk of developing cancer due to radiation exposure after a Mars mission could be two times greater than what scientists previously thought.[54][55] Occasional solar proton events (SPEs) produce much higher doses, as observed in September 2017, when NASA reported radiation levels on the surface of Mars were temporarily doubled, and were associated with an aurora 25-times brighter than any observed earlier, due to a massive, and unexpected, solar storm.[56] Building living quarters underground (possibly in Martian lava tubes) would significantly lower the colonists' exposure to radiation.

Файл:PIA17601-Comparisons-RadiationExposure-MarsTrip-20131209.png
Comparison of radiation doses—includes the amount detected on the trip from Earth to Mars by the RAD on the MSL (2011–2013).[57][58][59]

Much remains to be learned about space radiation. In 2003, NASA's Lyndon B. Johnson Space Center opened a facility, the NASA Space Radiation Laboratory, at Brookhaven National Laboratory, that employs particle accelerators to simulate space radiation. The facility studies its effects on living organisms, as well as experimenting with shielding techniques.[60] Initially, there was some evidence that this kind of low level, chronic radiation is not quite as dangerous as once thought; and that radiation hormesis occurs.[61] However, results from a 2006 study indicated that protons from cosmic radiation may cause twice as much serious damage to DNA as previously estimated, exposing astronauts to greater risk of cancer and other diseases.[62] As a result of the higher radiation in the Martian environment, the summary report of the Review of U.S. Human Space Flight Plans Committee released in 2009 reported that "Mars is not an easy place to visit with existing technology and without a substantial investment of resources."[62] NASA is exploring a variety of alternative techniques and technologies such as deflector shields of plasma to protect astronauts and spacecraft from radiation.[62]

Psychological effects

Due to the communication delays, new protocols need to be developed in order to assess crew members' psychological health. Researchers have developed a Martian simulation called HI-SEAS (Hawaii Space Exploration Analog and Simulation) that places scientists in a simulated Martian laboratory to study the psychological effects of isolation, repetitive tasks, and living in close-quarters with other scientists for up to a year at a time. Computer programs are being developed to assist crews with personal and interpersonal issues in absence of direct communication with professionals on Earth.[63]

Terraforming

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Artist's conception of the process of terraforming Mars as discussed in some works of science fiction

Шаблон:Main Шаблон:See also

Various works of fiction put forward the idea of terraforming Mars to allow a wide variety of life forms, including humans, to survive unaided on Mars' surface. Some ideas of possible technologies that may be able to contribute to the terraforming of Mars have been conjectured, but none would be able to bring the entire planet into the Earth-like habitat pictured in science fiction.[64]

Minimum size of a colony

To be self-sustaining, a colony would have to be large enough to provide all the necessary living services. These include[65]

  • Ecosystem management: producing appropriate gases, controlling air composition pressure and temperature, collecting and producing water, growing food and processing organic wastes.
  • Energy production: this includes extracting methane for vehicles and if photovoltaic cells are used to produce energy this would include the extraction and processing of silicates, to augment or replace any original equipment.
  • Industry: extracting and processing appropriate ores, manufacturing tools and other objects; producing clothes, medicine, glass, ceramics, plastics.
  • Building: even if the base is constructed before arrival, it will need frequent adaptation according to the evolution of the settlement as well as inevitable replacement.
  • Social activities: this includes raising children and educating them, health care, preparing meals, cleaning, washing, organizing the work and making decisions. Time for sport, culture and entertainment can be minimized but not eliminated.

As the number of individuals grows, both activities and objects can be shared between them. Growth also will offset the risks of collapse of the society, caused by sudden deaths, accidents, infertility or inbreeding. But this may not prevent mortal combat between different groups of individuals, or the loss of efficiency due to inappropriate social organization.

By mathematical modelling of the time spent by people on these issues and by keeping things simple, Salotti concludes that the minimum number for a colony on Mars is 110.[65] This is close to other studies of the genetic problems involved in the longer journey to Proxima Centauri b (6,000+ years).[66]

Transportation

Interplanetary spaceflight

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Rendezvous, an interplanetary stage and lander stage come together over Mars
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Mars (Viking 1, 1980)

Mars requires less energy per unit mass (delta V) to reach from Earth than any planet except Venus. Using a Hohmann transfer orbit, a trip to Mars requires approximately nine months in space.[67] Modified transfer trajectories that cut the travel time down to four to seven months in space are possible with incrementally higher amounts of energy and fuel compared to a Hohmann transfer orbit, and are in standard use for robotic Mars missions. Shortening the travel time below about six months requires higher delta-v and an increasing amount of fuel, and is difficult with chemical rockets. It could be feasible with advanced spacecraft propulsion technologies, some of which have already been tested to varying levels, such as Variable Specific Impulse Magnetoplasma Rocket,[68] and nuclear rockets. In the former case, a trip time of forty days could be attainable,[69] and in the latter, a trip time down to about two weeks.[1] In 2016, a University of California, Santa Barbara scientist said they could further reduce travel time for a small robotic probe to Mars down to "as little as 72 hours" with the use of a laser propelled sail (directed photonic propulsion) system instead of the fuel-based rocket propulsion system.[70][71]

During the journey the astronauts would be subject to radiation, which would require a means to protect them. Cosmic radiation and solar wind cause DNA damage, which increases the risk of cancer significantly. The effect of long-term travel in interplanetary space is unknown, but scientists estimate an added risk of between 1% and 19% (one estimate is 3.4%) for males to die of cancer because of the radiation during the journey to Mars and back to Earth. For females the probability is higher due to generally larger glandular tissues.[72]

Landing on Mars

Файл:Mars Lander by Brian McMullin, 1986.jpg
Painting of a landing on Mars (1986)

Mars has a surface gravity 0.38 times that of Earth, and the density of its atmosphere is about 0.6% of that on Earth.[73] The relatively strong gravity and the presence of aerodynamic effects make it difficult to land heavy, crewed spacecraft with thrusters only, as was done with the Apollo Moon landings, yet the atmosphere is too thin for aerodynamic effects to be of much help in aerobraking and landing a large vehicle. Landing piloted missions on Mars would require braking and landing systems different from anything used to land crewed spacecraft on the Moon or robotic missions on Mars.[74]

If one assumes carbon nanotube construction material will be available with a strength of Шаблон:Cvt then a space elevator could be built to land people and material on Mars.[75] A space elevator on Phobos (a Martian moon) has also been proposed.[76]

Phobos as a space elevator for Mars

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Space elevator Phobos
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Earth vs Mars vs Moon gravity at elevation

Phobos is synchronously orbiting Mars, where the same face stays facing the planet at ~6,028 km above the Martian surface. A space elevator could extend down from Phobos to Mars 6,000 km, about 28 kilometers from the surface, and just out of the atmosphere of Mars. A similar space elevator cable could extend out 6,000 km the opposite direction that would counterbalance Phobos. In total the space elevator would extend out over 12,000 km which would be below Areostationary orbit of Mars (17,032 km). A rocket launch would still be needed to get the rocket and cargo to the beginning of the space elevator 28 km above the surface. The surface of Mars is rotating at 0.25 km/s at the equator and the bottom of the space elevator would be rotating around Mars at 0.77 km/s, so only 0.52 km/s of Delta-v would be needed to get to the space elevator. Phobos orbits at 2.15 km/s and the outer most part of the space elevator would rotate around Mars at 3.52 km/s.[76]

Equipment needed for colonization

Colonization of Mars would require a wide variety of equipment—both equipment to directly provide services to humans and production equipment used to produce food, propellant, water, energy and breathable oxygen—in order to support human colonization efforts. Required equipment will include:[1]

Файл:Mars Greenhouse.jpg
Mars greenhouses feature in many colonization designs, especially for food production and other purposes.
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Various technologies and devices for Mars are shown in the illustration of a Mars base.

Basic utilities

In order to function at all the colony would need the basic utilities to support human civilization. These would need to be designed to handle the harsh Martian environment and would either have to be serviceable while wearing an EVA suit or housed inside a human habitable environment. For example, if electricity generation systems rely on solar power, large energy storage facilities will also be needed to cover the periods when dust storms block out the sun, and automatic dust removal systems may be needed to avoid human exposure to conditions on the surface.[25] If the colony is to scale beyond a few people, systems will also need to maximise use of local resources to reduce the need for resupply from Earth, for example by recycling water and oxygen and being adapted to be able to use any water found on Mars, whatever form it is in.

Communication with Earth

Communications with Earth are relatively straightforward during the half-sol when Earth is above the Martian horizon. NASA and ESA included communications relay equipment in several of the Mars orbiters, so Mars already has communications satellites. While these will eventually wear out, additional orbiters with communication relay capability are likely to be launched before any colonization expeditions are mounted.

The one-way communication delay due to the speed of light ranges from about 3 minutes at closest approach (approximated by perihelion of Mars minus aphelion of Earth) to 22 minutes at the largest possible superior conjunction (approximated by aphelion of Mars plus aphelion of Earth). Real-time communication, such as telephone conversations or Internet Relay Chat, between Earth and Mars would be highly impractical due to the long time lags involved. NASA has found that direct communication can be blocked for about two weeks every synodic period, around the time of superior conjunction when the Sun is directly between Mars and Earth,[80] although the actual duration of the communications blackout varies from mission to mission depending on various factors—such as the amount of link margin designed into the communications system, and the minimum data rate that is acceptable from a mission standpoint. In reality most missions at Mars have had communications blackout periods of the order of a month.[81]

A satellite at the Шаблон:L4 or Шаблон:L5 Earth–Sun Lagrangian point could serve as a relay during this period to solve the problem; even a constellation of communications satellites would be a minor expense in the context of a full colonization program. However, the size and power of the equipment needed for these distances make the L4 and L5 locations unrealistic for relay stations, and the inherent stability of these regions, although beneficial in terms of station-keeping, also attracts dust and asteroids, which could pose a risk.[82] Despite that concern, the STEREO probes passed through the L4 and L5 regions without damage in late 2009.

Recent work by the University of Strathclyde's Advanced Space Concepts Laboratory, in collaboration with the European Space Agency, has suggested an alternative relay architecture based on highly non-Keplerian orbits. These are a special kind of orbit produced when continuous low-thrust propulsion, such as that produced from an ion engine or solar sail, modifies the natural trajectory of a spacecraft. Such an orbit would enable continuous communications during solar conjunction by allowing a relay spacecraft to "hover" above Mars, out of the orbital plane of the two planets.[83] Such a relay avoids the problems of satellites stationed at either L4 or L5 by being significantly closer to the surface of Mars while still maintaining continuous communication between the two planets.

Robotic precursors

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Astronauts approach Viking 2 lander probe

The path to a human colony could be prepared by robotic systems such as the Mars Exploration Rovers Spirit, Opportunity, Curiosity and Perseverance. These systems could help locate resources, such as ground water or ice, that would help a colony grow and thrive. The lifetimes of these systems would be years and even decades, and as recent developments in commercial spaceflight have shown, it may be that these systems will involve private as well as government ownership. These robotic systems also have a reduced cost compared with early crewed operations, and have less political risk.

Wired systems might lay the groundwork for early crewed landings and bases, by producing various consumables including fuel, oxidizers, water, and construction materials. Establishing power, communications, shelter, heating, and manufacturing basics can begin with robotic systems, if only as a prelude to crewed operations.

Mars Surveyor 2001 Lander MIP (Mars ISPP Precursor) was to demonstrate manufacture of oxygen from the atmosphere of Mars,[84] and test solar cell technologies and methods of mitigating the effect of Martian dust on the power systems.[85]Шаблон:Update after

Before any people are transported to Mars on the notional 2020s Mars transportation infrastructure envisioned by SpaceX, a number of robotic cargo missions would be undertaken first in order to transport the requisite equipment, habitats and supplies.[86] Equipment that would be necessary would include "machines to produce fertilizer, methane and oxygen from Mars' atmospheric nitrogen and carbon dioxide and the planet's subsurface water ice" as well as construction materials to build transparent domes for initial agricultural areas.[87]

Economics

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Iron–nickel meteorite found on Mars' surface (Heat Shield Rock)

As with early colonies in the New World, economics would be a crucial aspect to a colony's success. The reduced gravity well of Mars and its position in the Solar System may facilitate Mars–Earth trade and may provide an economic rationale for continued settlement of the planet. Given its size and resources, this might eventually be a place to grow food and produce equipment to mine the asteroid belt.

Some early Mars colonies might specialize in developing local resources for Martian consumption, such as water and/or ice. Local resources can also be used in infrastructure construction.[88] One source of Martian ore currently known to be available is metallic iron in the form of nickel–iron meteorites. Iron in this form is more easily extracted than from the iron oxides that cover the planet.

Another main inter-Martian trade good during early colonization could be manure.[89] Assuming that life does not exist on Mars, the soil is going to be very poor for growing plants, so manure and other fertilizers will be valued highly in any Martian civilization until the planet changes enough chemically to support growing vegetation on its own.

Solar power is a candidate for power for a Martian colony. Solar insolation (the amount of solar radiation that reaches Mars) is about 42% of that on Earth, since Mars is about 52% farther from the Sun and insolation falls off as the square of distance. But the thin atmosphere would allow almost all of that energy to reach the surface as compared to Earth, where the atmosphere absorbs roughly a quarter of the solar radiation. Sunlight on the surface of Mars would be much like a moderately cloudy day on Earth.[90]

Economic drivers

Space colonization on Mars can roughly be said to be possible when the necessary methods of space colonization become cheap enough (such as space access by cheaper launch systems) to meet the cumulative funds that have been gathered for the purpose.

Although there are no immediate prospects for the large amounts of money required for any space colonization to be available given traditional launch costs,[91] there is some prospect of a radical reduction to launch costs in the 2020s, which would consequently lessen the cost of any efforts in that direction. With a published price of Шаблон:USD per launch of up to Шаблон:Convert payload to low Earth orbit or Шаблон:Convert to Mars,[92] SpaceX Falcon 9 rockets are already the "cheapest in the industry".[93] SpaceX's reusable plans include Falcon Heavy and future methane-based launch vehicles including the Starship. If SpaceX is successful in developing the reusable technology, it would be expected to "have a major impact on the cost of access to space", and change the increasingly competitive market in space launch services.[94]

Alternative funding approaches might include the creation of inducement prizes. For example, the 2004 President's Commission on Implementation of United States Space Exploration Policy suggested that an inducement prize contest should be established, perhaps by government, for the achievement of space colonization. One example provided was offering a prize to the first organization to place humans on the Moon and sustain them for a fixed period before they return to Earth.[95]

Mining the asteroid belts from Mars

Шаблон:See also

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The asteroids of the inner Solar System and Jupiter: The belt is located between the orbits of Jupiter and Mars.
Шаблон:Legend2
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Main Asteroid Belt 42 largest asteroids Шаблон:Legend-line Шаблон:Legend-line Шаблон:Legend-line Шаблон:See also

Since Mars is much closer to the asteroid belt than Earth is, it would take less Delta-v to get to the Asteroid belt and return minerals to Mars. One hypothesis is that the Moons of Mars (Phobos and Deimos) are actually Asteroid captures from the Asteroid belt.[96] 16 Psyche in the main belt could have over $10,000 Quadrillion Dollars worth of minerals. On October 13, 2023,

NASlaunchedAthe Psyche oiter, which is set to reach the asteroid d by August 20dy.[97] 511 Davida could have $27 quadrillion Dollars worth of minerals and resources.[98] Using the moon Phobos to launch spacecraft is energetically favorable and a useful location from which to dispatch missions to main belt asteroids.[99] Mining the asteroid belt from Mars and its moons could help in the colonization of Mars.[100][101][102]

Possible locations for settlements

Файл:Pavonis Mons lava tube skylight crop.jpg
Cropped version of a HiRISE image of a lava tube skylight entrance on the Martian volcano Pavonis Mons

Poles

It has been proposed to set up a first base at a Martian pole, which would allow access to water.[103]

Caves

Шаблон:See also Caves would naturally provide a degree of insulation from Martian hazards for humans on the planet.[104] These hazards include radiation, impactor events, and the wide range in temperatures on the surface.[104]

Mars Odyssey found what appear to be natural caves near the volcano Arsia Mons. It has been speculated that settlers could benefit from the shelter that these or similar structures could provide from radiation and micrometeoroids. Geothermal energy is also suspected in the equatorial regions.[105]

A team of researchers which presented at Geological Society of America Connects 2022 identified some 139 caves worth exploring as potential shelters.[104] Each was within Шаблон:Convert of a location ideal for use as a landing site and had been imaged in high-resolution by HiRISE.[104]

Lava tubes

Several possible Martian lava tube skylights have been located on the flanks of Arsia Mons. Earth based examples indicate that some should have lengthy passages offering complete protection from radiation and be relatively easy to seal using on-site materials, especially in small subsections.[106]

Hellas Planitia

Hellas Planitia is the lowest lying plain below the Martian geodetic datum. The atmospheric pressure is relatively higher in this place when compared to the rest of Mars.

Planetary protection

Шаблон:See also Robotic spacecraft to Mars are required to be sterilized, to have at most 300,000 spores on the exterior of the craft—and more thoroughly sterilized if they contact "special regions" containing water,[107][108] otherwise there is a risk of contaminating not only the life-detection experiments but possibly the planet itself.

It is impossible to sterilize human missions to this level, as humans are host to typically a hundred trillion microorganisms of thousands of species of the human microbiome, and these cannot be removed while preserving the life of the human. Containment seems the only option, but it is a major challenge in the event of a hard landing (i.e. crash).[109] There have been several planetary workshops on this issue, but with no final guidelines for a way forward yet.[110] Human explorers would also be vulnerable to back contamination to Earth if they become carriers of microorganisms should Mars have life.[111]

Ethical, political and legal challenges

It is unforeseen how the first human landing on Mars will change the current policies regarding the exploration of space and occupancy of celestial bodies. In the 1967 United Nations Outer Space Treaty, it was determined that no country may take claim to space or its inhabitants. Since the planet Mars offers a challenging environment and dangerous obstacles for humans to overcome, the laws and culture on the planet will most likely be very different from those on Earth.[112] With Elon Musk announcing his plans for travel to Mars, it is uncertain how the dynamic of a private company possibly being the first to put a human on Mars will play out on a national and global scale.[113][114] NASA had to deal with several cuts in funding. During the presidency of Barack Obama, the objective for NASA to reach Mars was pushed to the background.[115] In 2017, president Donald Trump promised to return humans to the Moon and eventually Mars,[116] and increased the NASA budget by $1.1 billion,[117] to mostly focus on development of the new Space Launch System.[118][119]

Colonialism

Шаблон:Main Space colonization in general has been discussed as continuation of imperialism and colonialism,[120] especially regarding Mars colonial decision making and reasons for colonial labor[121] and land exploitation have been questioned with postcolonial critique. Seeing the need for inclusive[122] and democratic participation and implementation of any space and Mars exploration, infrastructure, or colonialization, many have called for dramatic sociological reforms and guarantees to prevent racism, sexism, and other forms of prejudice.[123]

The narrative of space exploration as a "New Frontier" has been criticized as unreflected continuation of settler colonialism and manifest destiny, continuing the narrative of colonial exploration as fundamental to the assumed human nature.[124][125][126]

The predominant perspective of territorial colonization in space has been called surfacism, especially comparing advocacy for colonization of Mars opposed to Venus.[127][128]

Файл:NASA Artemis Gateway logo.png
The logo and name of the Lunar Gateway references the St. Louis Gateway Arch, associating Mars with the American frontier.[129]

Dangers to pregnancy

One possible ethical challenge that space travelers might face is that of pregnancy during the trip. According to NASA's policies, it is forbidden for members of the crew to engage in sex in space. NASA wants its crew members to treat each other like coworkers would in a professional environment. A pregnant member on a spacecraft is dangerous to all those aboard. The pregnant woman and child would need additional nutrition from the rations aboard, as well as special treatment and care. The pregnancy would impinge on the pregnant crew member's duties and abilities. It is still not fully known how the environment in a spacecraft would affect the development of a child aboard. It is known however that a fetus would be more susceptible to solar radiation in space, which would likely have a negative effect on its cells and genetics.[130] During a long trip to Mars, it is likely that members of craft may engage in sex due to their stressful and isolated environment.[131]

Advocacy

Файл:Buzz Aldrin.jpg
Buzz Aldrin, the Apollo 11 astronaut and second person to set foot on the Moon, has recommended human Mars missions.

Mars colonization is advocated by several non-governmental groups for a range of reasons and with varied proposals. One of the oldest groups is the Mars Society who promote a NASA program to accomplish human exploration of Mars and have set up Mars analog research stations in Canada and the United States. Mars to Stay advocates recycling emergency return vehicles into permanent settlements as soon as initial explorers determine permanent habitation is possible.

Elon Musk founded SpaceX with the long-term goal of developing the technologies that will enable a self-sustaining human colony on Mars.[113][132] Richard Branson, in his lifetime, is "determined to be a part of starting a population on Mars. I think it is absolutely realistic. It will happen... I think over the next 20 years," [from 2012] "we will take literally hundreds of thousands of people to space and that will give us the financial resources to do even bigger things".[133]

Author Robert Zubrin has been a major advocate for Mars exploration and colonization for many years. He is a member of the Mars society and has authored several fiction and nonfiction books about the subject. In 1996 he wrote The Case for Mars: The Plan to Settle the Red Planet and Why We Must. He continues to advocate for Mars and space exploration with his most recent book being The Case for Space: How the Revolution in Spaceflight Opens Up a Future of Limitless Possibility.

In June 2013, Buzz Aldrin, American engineer and former astronaut, and the second person to walk on the Moon, wrote an opinion, published in The New York Times, supporting a human mission to Mars and viewing the Moon "not as a destination but more a point of departure, one that places humankind on a trajectory to homestead Mars and become a two-planet species".[134] 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.[135]

There are critics of the project of Mars colonization. American political scientist Daniel Deudney has argued that a fully developed Mars colony represents an existential threat to humans remaining on Earth. His book, Dark Skies: Space Expansionism, Planetary Geopolitics, and the Ends of Humanity, challenges the widespread view among advocates that a Mars colony would be friendly to the interests of humans still on Earth.[136] According to Deudney, this is merely an assumption based on the largely unexamined claim that a future Mars colony will be a straightforward extension of civilization on Earth, rather than a completely new kind of civilization with distinct goals, values, fears and desires.

In fiction

Шаблон:Main

A few instances in fiction provide detailed descriptions of Mars colonization. They include:

Interactive Mars map

Шаблон:Mars map

See also

Шаблон:Div col

Шаблон:Div col end

References

Шаблон:Reflist

Further reading

External links

Шаблон:Commons category Шаблон:Wikibooks Шаблон:Wikiversity Шаблон:Spoken Wikipedia

Шаблон:Human missions to Mars Шаблон:Mars Шаблон:Space colonization Шаблон:Portal bar

Шаблон:Use American English

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  1. ↑ 1,0 1,1 1,2 Шаблон:Cite book
  2. ↑ Шаблон:Cite web
  3. ↑ Шаблон:Cite web
  4. ↑ Шаблон:Cite journal
  5. ↑ Шаблон:Cite magazine
  6. ↑ Шаблон:Cite web
  7. ↑ Шаблон:Cite web
  8. ↑ Шаблон:Cite web
  9. ↑ Шаблон:Cite news
  10. ↑ Шаблон:Cite journal
  11. ↑ Шаблон:Cite news
  12. ↑ Шаблон:Cite web
  13. ↑ 13,0 13,1 Шаблон:Cite web
  14. ↑ Шаблон:Cite web
  15. ↑ Шаблон:Cite journal
  16. ↑ Шаблон:Cite web
  17. ↑ Шаблон:Cite web
  18. ↑ Шаблон:Cite web
  19. ↑ Шаблон:Cite journal
  20. ↑ Шаблон:Cite book
  21. ↑ Шаблон:Cite journal
  22. ↑ Шаблон:Cite web
  23. ↑ Шаблон:Cite book
  24. ↑ Шаблон:Cite web
  25. ↑ 25,0 25,1 Шаблон:Cite journal
  26. ↑ Шаблон:Cite web
  27. ↑ Шаблон:Cite web
  28. ↑ Шаблон:Cite journal
  29. ↑ Шаблон:Cite web
  30. ↑ Шаблон:Cite book Extract of page 600 Шаблон:Webarchive
  31. ↑ Шаблон:Cite web
  32. ↑ Шаблон:Cite web
  33. ↑ Шаблон:Cite journal
  34. ↑ Шаблон:Cite web
  35. ↑ 35,0 35,1 Шаблон:Cite journal
  36. ↑ Шаблон:Cite web
  37. ↑ Шаблон:Cite web
  38. ↑ Шаблон:Cite web
  39. ↑ Шаблон:Cite web
  40. ↑ Mui, K. W., Wong, L. T., & Law, L. Y. (2007). Domestic water consumption benchmark development for Hong Kong. Building Services Engineering Research & Technology, 28(4), 329.
  41. ↑ Шаблон:Cite news
  42. ↑ Шаблон:Cite news
  43. ↑ Шаблон:Cite news
  44. ↑ Шаблон:Cite web
  45. ↑ Шаблон:Cite news
  46. ↑ Шаблон:Cite journal
  47. ↑ Aubert AE, Beckers F, Verheyden B. Cardiovascular function and basics of physiology in microgravity. Acta Cardiologica 2005;60(2):129-151.
  48. ↑ Williams D, Kuipers A, Mukai C, Thirsk R. Acclimation during space flight: effects on human physiology. CMAJ : Canadian Medical Association journal = journal de l’Association medicale canadienne 2009;180(13):1317-1323.
  49. ↑ Heer M, Paloski WH. Space motion sickness: Incidence, etiology, and countermeasures. Autonomic Neuroscience 2006;129(1):77-79.
  50. ↑ Шаблон:Cite news
  51. ↑ Шаблон:Cite web
  52. ↑ Шаблон:Cite web
  53. ↑ Real Martians: How to Protect Astronauts from Space Radiation on Mars. Шаблон:Webarchive Moon To Mars. NASA. 30 September 2015. Quote: "[...] a trip to interplanetary space carries more radiation risk than working in low-Earth orbit, said Jonathan Pellish, a space radiation engineer at Goddard."
  54. ↑ Study: Collateral Damage from Cosmic Rays Increases Cancer Risk for Mars Astronauts Шаблон:Webarchive. University of Nevada, Las Vegas (UNLV). May 2017.
  55. ↑ "Non-Targeted Effects Models Predict Significantly Higher Mars Mission Cancer Risk than Targeted Effects Models." Francis A. Cucinotta, and Eliedonna Cacao. Nature, Scientific Reports, volume 7, Article number: 1832. 12 May 2017.Шаблон:Doi
  56. ↑ Шаблон:Cite web
  57. ↑ Шаблон:Cite journal
  58. ↑ Шаблон:Cite journal
  59. ↑ Шаблон:Cite news
  60. ↑ Шаблон:Cite web
  61. ↑ Шаблон:Cite book
  62. ↑ 62,0 62,1 62,2 Шаблон:Cite web
  63. ↑ Шаблон:Cite web
  64. ↑ Шаблон:Cite web
  65. ↑ 65,0 65,1 Шаблон:Cite journal
  66. ↑ Шаблон:Cite journal
  67. ↑ Шаблон:Cite web
  68. ↑ Шаблон:Cite web
  69. ↑ Шаблон:Cite web
  70. ↑ Шаблон:Cite web
  71. ↑ Starlight: Directed Energy for Relativistic Interstellar Missions. Шаблон:Webarchive UCSB Experimental Cosmology Group. Accessed on 9 November 2019.
  72. ↑ Шаблон:Cite web
  73. ↑ Шаблон:Cite web
  74. ↑ Шаблон:Cite web
  75. ↑ Шаблон:Cite web
  76. ↑ 76,0 76,1 Шаблон:Cite conference
  77. ↑ Шаблон:Cite news
  78. ↑ Шаблон:Cite news
  79. ↑ Шаблон:Cite journal
  80. ↑ Шаблон:Cite web
  81. ↑ Шаблон:Cite journal
  82. ↑ Шаблон:Cite web
  83. ↑ Шаблон:Cite web
  84. ↑ Шаблон:Cite journal Paper presented at Mars 2001: Integrated Science in Preparation for Sample Return and Human Exploration, Lunar and Planetary Institute, Oct. 2–4 1999, Houston, TX.
  85. ↑ Шаблон:Cite web Presented at Concepts and Approaches for Mars Exploration, July 18–20, 2000 Houston, Texas.
  86. ↑ Шаблон:Cite AV media
  87. ↑ Шаблон:Cite news
  88. ↑ Шаблон:Cite journal
  89. ↑ Lovelock, James and Allaby, Michael, "The Greening of Mars" 1984
  90. ↑ Шаблон:Cite web
  91. ↑ Шаблон:Cite web
  92. ↑ Шаблон:Cite web
  93. ↑ Шаблон:Cite news
  94. ↑ Шаблон:Cite news
  95. ↑ Шаблон:Cite web
  96. ↑ Шаблон:Cite web
  97. ↑ Шаблон:Cite web
  98. ↑ Шаблон:Cite web
  99. ↑ Шаблон:Cite journal
  100. ↑ Шаблон:Cite web
  101. ↑ Шаблон:Cite web
  102. ↑ Шаблон:Cite web
  103. ↑ Шаблон:Cite journal
  104. ↑ 104,0 104,1 104,2 104,3 Шаблон:Cite news
  105. ↑ Шаблон:Cite journal
  106. ↑ Шаблон:Cite web
  107. ↑ Queens University Belfast scientist helps NASA Mars project Шаблон:Webarchive "No-one has yet proved that there is deep groundwater on Mars, but it is plausible as there is certainly surface ice and atmospheric water vapour, so we wouldn't want to contaminate it and make it unusable by the introduction of micro-organisms."
  108. ↑ COSPAR PLANETARY PROTECTION POLICY Шаблон:Webarchive (20 October 2002; As Amended to 24 March 2011)
  109. ↑ When Biospheres Collide – a history of NASA's Planetary Protection Programs Шаблон:Webarchive, Michael Meltzer, May 31, 2012, see Chapter 7, Return to Mars – final section: "Should we do away with human missions to sensitive targets"
  110. ↑ Johnson, James E. "Planetary Protection Knowledge Gaps for Human Extraterrestrial Missions: Goals and Scope." (2015) Шаблон:Webarchive
  111. ↑ Safe on Mars page 37 Шаблон:Webarchive "Martian biological contamination may occur if astronauts breathe contaminated dust or if they contact material that is introduced into their habitat. If an astronaut becomes contaminated or infected, it is conceivable that he or she could transmit Martian biological entities or even disease to fellow astronauts, or introduce such entities into the biosphere upon returning to Earth. A contaminated vehicle or item of equipment returned to Earth could also be a source of contamination."
  112. ↑ Szocik, Konrad, Kateryna Lysenko-Ryba, Sylwia Banaś, and Sylwia Mazur. "Political and Legal Challenges in a Mars Colony." Space Policy (2016): n. pag. Web. 24 Oct. 2016.
  113. ↑ 113,0 113,1 Шаблон:Cite news
  114. ↑ Commercial Space Exploration: Ethics, Policy and Governance, 2015. Print.
  115. ↑ Шаблон:Cite web
  116. ↑ Шаблон:Cite web
  117. ↑ Шаблон:Cite web
  118. ↑ Шаблон:Cite web
  119. ↑ Шаблон:Cite web
  120. ↑ Шаблон:Cite news
  121. ↑ Шаблон:Cite web
  122. ↑ Шаблон:Cite web
  123. ↑ Шаблон:Cite web
  124. ↑ Шаблон:Cite web
  125. ↑ Шаблон:Cite web
  126. ↑ Шаблон:Cite web
  127. ↑ Шаблон:Cite web
  128. ↑ Шаблон:Cite news
  129. ↑ Шаблон:Cite web
  130. ↑ Minkel, JR. "Sex and Pregnancy on Mars: A Risky Proposition." Space.com. Space.com, 11 Feb. 2011. Web. 09 Dec. 2016.
  131. ↑ Шаблон:Cite journal
  132. ↑ Шаблон:Cite web
  133. ↑ Шаблон:Cite web
  134. ↑ Шаблон:Cite news
  135. ↑ Шаблон:Cite news
  136. ↑ Шаблон:Cite book
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