Terraforming
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Terraforming or terraformation ("Earth-shaping") is the hypothetical process of deliberately modifying the atmosphere, temperature, surface topography or ecology of a planet, moon, or other body to be similar to the environment of Earth to make it habitable for humans to live on.
The concept of terraforming developed from both
Even if the environment of a planet could be altered deliberately, the feasibility of creating an unconstrained planetary environment that mimics Earth on another planet has yet to be verified. While Venus, Earth, Mars, and even the Moon have been studied in relation to the subject, Mars is usually considered to be the most likely candidate for terraforming. Much study has been done concerning the possibility of heating the planet and altering its atmosphere, and NASA has even hosted debates on the subject. Several potential methods for the terraforming of Mars may be within humanity's technological capabilities, but according to Martin Beech, the economic attitude of preferring short-term profits over long-term investments will not support a terraforming project.[3]
The long timescales and practicality of terraforming are also the subject of debate. As the subject has gained traction, research has expanded to other possibilities including biological terraforming, para-terraforming, and modifying humans to better suit the environments of
History of scholarly study
The astronomer
Sagan also visualized making Mars habitable for human life in an article published in the journal Icarus, "Planetary Engineering on Mars" (1973).[5] Three years later, NASA addressed the issue of planetary engineering officially in a study, but used the term "planetary ecosynthesis" instead.[6] The study concluded that it was possible for Mars to support life and be made into a habitable planet. The first conference session on terraforming, then referred to as "Planetary Modeling", was organized that same year.
In March 1979, NASA engineer and author James Oberg organized the First Terraforming Colloquium, a special session at the Lunar and Planetary Science Conference in Houston. Oberg popularized the terraforming concepts discussed at the colloquium to the general public in his book New Earths (1981).[7] Not until 1982 was the word terraforming used in the title of a published journal article. Planetologist Christopher McKay wrote "Terraforming Mars", a paper for the Journal of the British Interplanetary Society.[8] The paper discussed the prospects of a self-regulating Martian biosphere, and the word "terraforming" has since become the preferred term.[citation needed]
In 1984, James Lovelock and Michael Allaby published The Greening of Mars.[9] Lovelock's book was one of the first to describe a novel method of warming Mars, where chlorofluorocarbons (CFCs) are added to the atmosphere to produce a strong greenhouse effect.
Motivated by Lovelock's book, biophysicist Robert Haynes worked behind the scenes[citation needed] to promote terraforming, and contributed the neologism Ecopoiesis,[10] forming the word from the Greek οἶκος, oikos, "house",[11] and ποίησις, poiesis, "production".[12] Ecopoiesis refers to the origin of an ecosystem. In the context of space exploration, Haynes describes ecopoiesis as the "fabrication of a sustainable ecosystem on a currently lifeless, sterile planet". Fogg defines ecopoiesis as a type of planetary engineering and is one of the first stages of terraformation. This primary stage of ecosystem creation is usually restricted to the initial seeding of microbial life.[13] A 2019 opinion piece by Lopez, Peixoto and Rosado has reintroduced microbiology as a necessary component of any possible colonization strategy based on the principles of microbial symbiosis and their beneficial ecosystem services.[14] As conditions approach that of Earth, plant life could be brought in, and this will accelerate the production of oxygen, theoretically making the planet eventually able to support animal life.
Aspects and definitions
In 1985, Martyn Fogg started publishing several articles on terraforming. He also served as editor for a full issue on terraforming for the Journal of the British Interplanetary Society in 1992. In his book Terraforming: Engineering Planetary Environments (1995), Fogg proposed the following definitions for different aspects related to terraforming:[13]
- Planetary engineering: the application of technology for the purpose of influencing the global properties of a planet.
- insolationor impact flux.
- Terraforming: a process of planetary engineering, specifically directed at enhancing the capacity of an extraterrestrial planetary environment to support life as we know it. The ultimate achievement in terraforming would be to create an open planetary ecosystem emulating all the functions of the biosphere of Earth, one that would be fully habitable for human beings.
Fogg also devised definitions for candidate planets of varying degrees of human compatibility:[15]
- Habitable Planet (HP): A world with an environment sufficiently similar to Earth's as to allow comfortable and free human habitation.
- Biocompatible Planet (BP): A planet possessing the necessary physical parameters for life to flourish on its surface. If initially lifeless, then such a world could host a biosphere of considerable complexity without the need for terraforming.
- Easily Terraformable Planet (ETP): A planet that might be rendered biocompatible, or possibly habitable, and maintained so by modest planetary engineering techniques and with the limited resources of a starship or robot precursor mission.
Fogg suggests that Mars was a biologically compatible planet in its youth, but is not now in any of these three categories, because it can only be terraformed with greater difficulty.[16]
Habitability requirements
Planetary habitability, broadly defined as the capacity for an astronomical body to sustain life, requires that various geophysical, geochemical, and astrophysical criteria must be met before the surface of such a body is considered habitable. Modifying a planetary surface such that it is able to sustain life, particularly for humans, is generally the end-goal of the hypothetical process of terraforming. Of particular interest in the context of terraforming is the set of factors that have sustained complex, multicellular animals in addition to simpler organisms on Earth. Research and theory in this regard is a component of planetary science and the emerging discipline of astrobiology.
Classifications of the criteria of habitability can be varied, but it is generally agreed upon that the presence of water, non-extreme temperatures, and an energy source put broad constraints on habitability.
In its astrobiology roadmap,
Temperature
The general temperature range for all life on Earth is -20°C to 122°C,
Water
All known life requires water;
Energy
On the most fundamental level, the only absolute requirement of life may be thermodynamic disequilibrium, or the presence of Gibbs Free Energy.[19] It has been argued that habitability can be conceived of as a balance between life's demand for energy and the capacity for the environment to provide such energy.[19] For humans, energy comes in the form of sugars, fats, and proteins provided by consuming plants and animals, necessitating in turn that a habitable planet for humans can sustain such organisms.[23]
Much of earth's biomass (~60%) relies on photosynthesis for an energy source, while a further ~40% is chemotropic.[18] For the development of life on other planetary bodies, chemical energy may have been critical,[18] while for sustaining life on another planetary body in our solar system, sufficiently high solar energy may also be necessary for phototrophic organisms.
Elements
On Earth, life generally requires six elements in high abundance: carbon, hydrogen, nitrogen, oxygen, phosphorus, and sulfur.[20] These elements are considered "essential" for all known life and plentiful within biological systems.[24] Additional elements crucial to life include the cations Mg2+, Ca2+, K+ and Na+ and the anion Cl-.[25] Many of these elements may undergo biologically facilitated oxidation or reduction to produce usable metabolic energy.[24][25]
Preliminary stages
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Terraforming a planet would involve making it fit the habitability requirements listed in the previous section. For example, a planet may be too cold for liquid water to exist on its surface. Its temperature could be raised by adding greenhouse gases to the atmosphere,[26] using orbiting mirrors to reflect more sunlight onto the planet,[27] or lowering the albedo of the planet.[5] Conversely, a planet too hot for liquid water could be cooled down by removing greenhouse gases (if these are present), placing a sunshade in the L1 point to reduce sunlight reaching the planet, or increasing the albedo.[28] Atmospheric pressure is another issue: various celestial bodies including Mars, Mercury and most moons have lower pressure than Earth. At pressures below the
Once conditions become more suitable for
Prospective targets
Mars
In many respects, Mars is the most Earth-like planet in the Solar System.[31][32] It is thought that Mars once had a more Earth-like environment early in its history, with a thicker atmosphere and abundant water that was lost over the course of hundreds of millions of years.[33]
The exact mechanism of this loss is still unclear, though three mechanisms, in particular, seem likely: First, whenever surface water is present, carbon dioxide (CO
2) reacts with rocks to form carbonates, thus drawing atmosphere off and binding it to the planetary surface. On Earth, this process is counteracted when plate tectonics works to cause volcanic eruptions that vent carbon dioxide back to the atmosphere. On Mars, the lack of such tectonic activity worked to prevent the recycling of gases locked up in sediments.[34]
Second, the lack of a
Finally, between approximately 4.1 and 3.8 billion years ago, asteroid impacts during the Late Heavy Bombardment caused significant changes to the surface environment of objects in the Solar System. The low gravity of Mars suggests that these impacts could have ejected much of the Martian atmosphere into deep space.[40]
Terraforming Mars would entail two major interlaced changes: building the atmosphere and heating it.
Venus
Terraforming Venus requires two major changes: removing most of the planet's dense 9 MPa (1,300 psi; 89 atm) carbon dioxide atmosphere, and reducing the planet's 450 °C (842 °F) surface temperature.[44][28] These goals are closely interrelated because Venus's extreme temperature may result from the greenhouse effect caused by its dense atmosphere.
Venus's atmosphere currently contains little oxygen, so an additional step would be to inject breathable O2 into the atmosphere. An early proposal for such a process comes from
An additional step noted by Martin Beech includes the injection of water and/or hydrogen into the planetary atmosphere;[3] this step follows after sequestering CO2 and reducing the mass of the atmosphere. In order to combine hydrogen with O2 produced by other means, an estimated 4*1019 kg of hydrogen is necessary; this may need to be mined from another source, such as Uranus or Neptune.[3]
Moon
Although the gravity on Earth's Moon is too low to hold an atmosphere for geological spans of time, if given one, it would retain it for spans of time that are long compared to human lifespans.[46][30] Landis[30] and others[47][48] have thus proposed that it could be feasible to terraform the moon, although not all agree with that proposal.[49] Landis estimates that a 1 PSI atmosphere of pure oxygen on the Moon would require on the order of two hundred trillion tons of oxygen, and suggests it could be produced by reducing the oxygen from an amount of lunar rock equivalent to a cube about fifty kilometers on an edge. Alternatively, he suggests that the water content of "fifty to a hundred comets" the size of Halley's comet would do the job, "assuming that the water doesn't splash away when the comets hit the moon."[30] Likewise, Benford calculates that terraforming the moon would require "about 100 comets the size of Halley's."[47]
Mercury
This section needs additional citations for verification. (March 2021) |
Despite being much smaller than Mars, Mercury has an escape velocity only slightly less than that of Mars due to its higher density and could, if a magnetosphere prevents atmospheric stripping, hold a nitrogen/oxygen atmosphere for millions of years.
To provide one atmosphere of pressure, roughly 1.1×1018 kilograms of gas would be required;[51] or a somewhat lower amount if lower pressure is acceptable. Water could be delivered from the outer solar system. Once this water has been delivered, it would split the water into its constituent oxygen and hydrogen molecules, possibly using a photo-catalytic dust, with the hydrogen rapidly being lost to space. At an oxygen pressure of 0.2-0.3 bar, the atmosphere would be breathable and nitrogen may be added as required to allow for plant growth in the presence of nitrates.
Temperature management would be required, due to the equilibrium average temperature of ~159 Celsius. However, millions of square kilometers at the poles have an average temperature of 0-50 Celsius, or 32-122 Fahrenheit (i.e., an area the size of Mexico at each pole with habitable temperatures). The total habitable area could be even larger if the planetary albedo were increased from 0.12 to ~0.6, potentially increasing the habitable area. Roy proposes that the temperature could be further managed by decreasing the solar flux at Mercury to near the terrestrial value by solar sails reflecting sunlight. He calculates that 16 to 17 million sails, each with an area of one square kilometer would be needed.[51]
Earth
It has been recently proposed[
Other bodies in the Solar System
Other possible candidates for terraforming (possibly only partial or paraterraforming) include large moons of Jupiter or Saturn (Europa, Ganymede, Callisto, Enceladus, Titan), and the dwarf planet Ceres.
The moons are covered in ice, so heating them would make some of this ice sublimate into an atmosphere of water vapour, ammonia and other gases.
Challenges to terraforming the moons include their high amounts of ice and their low gravity.[55][56] If all of the ice were fully melted, it would result in deep moon-spanning oceans, meaning any settlements would have to be floating (unless some of the ice was allowed to remain, to serve as land).[55][56] Low gravity would cause atmospheric escape over time and may cause problems for human health. However, atmospheric escape would take place over spans of time that are long compared to human lifespans, as with the Moon.[30]
One proposal for terraforming Ceres would involve heating it (using orbital mirrors, detonating thermonuclear devices or colliding small asteroids with Ceres), creating an atmosphere and deep ocean.[59] However, this appears to be based on a misconception that Ceres' surface is icy in a similar way to the gas giant moons. In reality, Ceres' surface is "a layer of mixed ice, silicates and light strong phases best matched by hydrated salts and clathrates".[60] It is unclear what the result of heating this up would be.
Other possibilities
Biological terraforming
Many proposals for planetary engineering involve the use of genetically engineered bacteria.[61][62]
As synthetic biology matures over the coming decades it may become possible to build designer organisms from scratch that directly manufacture desired products efficiently.[63] Lisa Nip, Ph.D. candidate at the MIT Media Lab's Molecular Machines group, said that by synthetic biology, scientists could genetically engineer humans, plants and bacteria to create Earth-like conditions on another planet.[64][65]
Gary King, microbiologist at Louisiana State University studying the most extreme organisms on Earth, notes that "synthetic biology has given us a remarkable toolkit that can be used to manufacture new kinds of organisms specially suited for the systems we want to plan for" and outlines the prospects for terraforming, saying "we'll want to investigate our chosen microbes, find the genes that code for the survival and terraforming properties that we want (like radiation and drought resistance), and then use that knowledge to genetically engineer specifically Martian-designed microbes". He sees the project's biggest bottleneck in the ability to genetically tweak and tailor the right microbes, estimating that this hurdle could take "a decade or more" to be solved. He also notes that it would be best to develop "not a single kind of microbe but a suite of several that work together".[66]
DARPA is researching the use of photosynthesizing plants, bacteria, and algae grown directly on the Mars surface that could warm up and thicken its atmosphere. In 2015 the agency and some of its research partners created an software called DTA GView − a 'Google Maps of genomes', in which genomes of several organisms can be pulled up on the program to immediately show a list of known genes and where they are located in the genome. According to Alicia Jackson, deputy director of DARPA's Biological Technologies Office, they have developed a "technological toolkit to transform not just hostile places here on Earth, but to go into space not just to visit, but to stay".[67][68][69][70]
Paraterraforming
Also known as the "world house" concept, para-terraforming involves the construction of a habitable enclosure on a planet that encompasses most of the planet's usable area.[71] The enclosure would consist of a transparent roof held one or more kilometers above the surface, pressurized with a breathable atmosphere, and anchored with tension towers and cables at regular intervals. The world house concept is similar to the concept of a domed habitat, but one which covers all (or most) of the planet.
Potential targets for paraterraforming include Mercury, the Moon, Ceres and the gas giant moons.[72]
Adapting humans
It has also been suggested that instead of or in addition to terraforming a hostile environment humans might adapt to these places by the use of genetic engineering, biotechnology and cybernetic enhancements.[73][74][75][76][77] This is known as pantropy.
Issues
Ethical issues
There is a philosophical debate within
On the pro-terraforming side of the argument, there are those like
The opposing argument posits that terraforming would be an unethical interference in nature, and that given humanity's past treatment of Earth, other planets may be better off without human interference.[citation needed] Still others strike a middle ground, such as Christopher McKay, who argues that terraforming is ethically sound only once we have completely assured that an alien planet does not harbor life of its own; but that if it does, we should not try to reshape it to our own use, but we should engineer its environment to artificially nurture the alien life and help it thrive and co-evolve, or even co-exist with humans.[82] Even this would be seen as a type of terraforming to the strictest of ecocentrists, who would say that all life has the right, in its home biosphere, to evolve without outside interference.
Economic issues
The initial cost of such projects as planetary terraforming would be massive, and the infrastructure of such an enterprise would have to be built from scratch. Such technology has not yet been developed, let alone financially feasible at the moment. John Hickman has pointed out that almost none of the current schemes for terraforming incorporate economic strategies, and most of their models and expectations seem highly optimistic.[83]
In popular culture
Terraforming is a common concept in
A related concept from science fiction is xenoforming – a process in which aliens change the Earth or other planets to suit their own needs, already suggested in the classic The War of the Worlds (1898) of H.G. Wells.[85]
See also
- Astrobotany – Study of plants grown in spacecraft
- Climate engineering, also known as Geoengineering – Deliberate and large-scale intervention in the Earth's climate system
- Colonization of Mars – Proposed concepts for human settlements on Mars
- Colonization of Venus – Proposed colonization of the planet Venus
- Desert greening – Process of man-made reclamation of deserts
- Effect of spaceflight on the human body – Medical issues associated with spaceflight
- Extraterrestrial liquid water – Liquid water naturally occurring outside Earth
- Health threat from cosmic rays – Dangers posed to astronauts
- In situ resource utilization – Astronautical use of materials harvested in outer space
- Pantropy – Hypothetical process of space colonization
- Planetary engineering – Influencing a planet's global environments
- Planetary habitability – Known extent to which a planet is suitable for life
- Space colonization – Concept of permanent human habitation outside of Earth
- Terraforming of Mars – Hypothetical modification of Mars into a habitable planet
- Terraforming of Venus – Engineering the global environment of Venus to make it suitable for humans
Notes
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- ^ a b c Sagan 1997, pp. 276–7.
- ^ .
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- ^ Oberg, James Edward (1981). New Earths: Restructuring Earth and Other Planets. Stackpole Books, Harrisburg, Pennsylvania.
- .
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- ^ ποίησις in Liddell and Scott.
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- ^ a b Forget, Costard & Lognonné 2007, pp. 80–2.
- Cosmos. 25 November 2008. Archived from the originalon 2012-04-27. Retrieved 2009-06-18.
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- ^ Solar Wind, 2008
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- ^ Faure & Mensing 2007, p. 252.
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- ^ a b Benford, Greg (July 14, 2014). "How to Terraform the Moon". Slate. Retrieved 30 January 2017.
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- ^ Beech, Martin. Terraforming: The Creating of Habitable Worlds, pp. 217-219. Springer. Retrieved 29 Dec. 2023.
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- ^ Williams, Matt (2016-05-05). "How Do We Terraform Ceres?". Universe Today. Retrieved 2023-12-12.
- ^ Raymond, C.; Castillo-Rogez, J. C.; Park, R. S.; Ermakov, A.; et al. (September 2018). "Dawn Data Reveal Ceres' Complex Crustal Evolution" (PDF). European Planetary Science Congress. Vol. 12. Archived (PDF) from the original on 30 January 2020. Retrieved 19 July 2020.
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References
- Averner, M. M.; MacElroy, R. D., eds. (1976). On the Habitability of Mars: An Approach to Planetary Ecosynthesis. NASA. Retrieved April 4, 2023.
- Beech, Martin (21 April 2009). Terraforming: The Creating of Habitable Worlds. Springer Science & Business Media. ISBN 978-0-387-09796-1.
- Dalrymple, G. Brent (2004). Ancient Earth, ancient skies: the age of Earth and its cosmic surroundings. ISBN 0-8047-4933-7
- Faure, Gunter & Mensing, Teresa M. (2007). Introduction to planetary science: the geological perspective. Springer. ISBN 1-4020-5233-2.
- Fogg, Martyn J. (1995). Terraforming: Engineering Planetary Environments. SAE International, Warrendale, PA. ISBN 1-56091-609-5.
- Fogg, Martyn J. (1996). "A Planet Dweller's Dream". In Schmidt, Stanley; Zubrin, Robert (eds.). Islands in the Sky. New York: Wiley. pp. 143–67.
- .
- Fogg, Martyn J. (2000). The Ethical Dimensions of Space Settlement (PDF format). Space Policy, 16, 205–211. Also presented (1999) at the 50th International Astronautical Congress, Amsterdam (IAA-99-IAA.7.1.07).
- Forget, François; Costard, François & Lognonné, Philippe (2007). Planet Mars: Story of Another World. Springer. ISBN 0-387-48925-8.
- Kargel, Jeffrey Stuart (2004). Mars: a warmer, wetter planet. Springer. ISBN 1-85233-568-8.
- Knoll, Andrew H. (2008). "Cyanobacteria and earth history". In Herrero, Antonia; Flores, Enrique (eds.). The cyanobacteria: molecular biology, genomics, and evolution. Horizon Scientific Press. pp. 1–20. ISBN 978-1-904455-15-8.
- MacNiven, D. (1995). "Environmental Ethics and Planetary Engineering". Journal of the British Interplanetary Society. 48: 441–44.
- McKay Christopher P. & Haynes, Robert H. (1997). "Implanting Life on Mars as a Long Term Goal for Mars Exploration", in The Case for Mars IV: Considerations for Sending Humans, ed. Thomas R. Meyer (San Diego, California: American Astronautical Society/Univelt), Pp. 209–15.
- Read, Peter L.; Lewis, Stephen R. (2004). The Martian climate revisited: atmosphere and environment of a desert planet. Springer. ISBN 3-540-40743-X.
- ISBN 0-345-37659-5.
- Schubert, Gerald; Turcotte, Donald L.; Olson, Peter. (2001). Mantle convection in the Earth and planets. Cambridge University Press. ISBN 0-521-79836-1.
- Taylor, Richard L. S. (1992). "Paraterraforming – The world house concept". Bibcode:1992JBIS...45..341T.
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External links
- New Mars forum
- Terraformers Society of Canada
- Visualizing the steps of Solar System terraforming
- Research Paper: Technological Requirements for Terraforming Mars
- Terraformers Australia
- Terraformers UK
- The Terraformation of Worlds Archived 2019-06-09 at the Wayback Machine
- Terraformation de Mars
- Fogg, Martyn J. The Terraforming Information Pages
- BBC article on Charles Darwin's and Joseph Hooker's artificial ecosystem on Ascension Island that may be of interest to terraforming projects
- Choi, Charles Q. (November 1, 2010). "Bugs in Space: Microscopic miners could help humans thrive on other planets". Scientific American.
- Robotic Lunar Ecopoiesis Test Bed Principal Investigator: Paul Todd (2004)