User:BennettWise

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Planetary Engineering - General Definition[edit]

Projected temperature and precipitation changes relative to preindustrial; end-of-century response without (a) and with (b) geoengineering to avoid temperature rise above 1.5C. See https://dx.doi.org/10.1098/rsta.2016.0454.

Planetary engineering is the development and application of technology for the purpose of influencing the environment of a planet. Planetary engineering encompasses a variety of methods such as terraforming, seeding, and geoengineering.

Widely discussed in the scientific community, terraforming refers to the alteration of other planets to create a habitable environment for terrestrial life. Eeding refers to the introduction of life from Earth to habitable planets. Geoengineering refers to the engineering of a planet’s climate, and has already been applied on Earth. Each of these methods are composed of varying approaches and possess differing levels of feasibility and ethical concern.

Terraforming[edit]

This is a theoretical design for a power station on Mars. Terraforming designs are not yet planned. This was designed by D Mitriy, August 31st, 2009.

Terraforming is the process of modifying the atmosphere, temperature, surface topography or ecology of a planet, moon, or other body in order to replicate the environment of Earth.

Technologies[edit]

A common object of discussion on potential terraforming is the planet Mars. To terraform Mars, humans would need to create a new atmosphere, due to the planet’s high carbon dioxide concentration and low atmospheric pressure. This would be possible by introducing more greenhouse gases to below “freezing point from indigenous materials” [1]. To terraform Venus, carbon dioxide would need to be converted to graphite since Venus receives twice as much sunlight as Earth. This process is only possible if the greenhouse effect is removed with the use of 'high-altitude absorbing fine particles' or a sun shield, creating a more habitable Venus [1].

NASA has defined categories of habitability systems and technologies for terraforming to be feasible[2]. These topics include creating power-efficient systems for preserving and packaging  food for crews, preparing and cooking foods, dispensing water, and developing facilities for rest, trash and recycling, and areas for crew hygiene and rest[2].

Feasibility[edit]

A variety of planetary engineering challenges stand in the way of terraforming efforts. The atmospheric terraforming of Mars, for example, would require “significant quantities of gas” to be added to the Martian atmosphere[3]. This gas has been thought to be stored in solid and liquid form within Mars’ polar ice caps and underground reservoirs. It is unlikely, however, that enough CO2 for sufficient atmospheric change is present within Mars’ polar deposits, and liquid CO2 could only be present at warmer temperatures “deep within the crust”[3]. Furthermore, sublimating the entire volume of Mars’ polar caps would increase its current atmospheric pressure to 15 millibar, where an increase to around 1000 millibar would be required for habitability[3]. For reference, Earth’s average sea-level pressure is 1013.25 mbar.

First formally proposed by astrophysicist Carl Sagan, the terraforming of Venus has since been discussed through methods such as organic molecule-induced carbon conversion, sun reflection, increasing planetary spin, and various chemical means[4]. Due to the high presence of sulfuric acid and solar wind on Venus, which are harmful to organic environments, organic methods of carbon conversion have been found unfeasible[4]. Other methods, such as solar shading, hydrogen bombardment, and magnesium-calcium bombardment are theoretically sound but would require large-scale resources and space technologies not yet available to humans[4].

Ethical considerations[edit]

While successful terraforming would allow life to prosper on other planets, philosophers have debated whether this practice is morally sound. Certain ethics experts suggest that planets like Mars hold an intrinsic value independent of their utility to humanity and should therefore be free from human interference[5]. Through this ethical framework, terraforming attempts on these planets could be seen to threaten their intrinsically valuable environments, rendering these efforts unethical[5].

Seeding:[edit]

“Seeding is a term used for the process of introducing microbial or algae species on a planet or moon already offering habitable regions"[6] .From Planetary Engineering Page

True color image of Mars taken by the OSIRIS instrument on the ESA Rosetta spacecraft during its February 2007 flyby of the planet. The image was generated using the OSIRIS orange (red), green, and blue filters.
Environmental Considerations[edit]

Mars is the primary subject of discussion for seeding. Locations for seeding are chosen based on atmospheric temperature, air pressure, existence of harmful radiation, and availability of natural resources, such as water and other compounds essential to terrestrial life[7].

Developing microorganisms for seeding[edit]

Natural or engineered microorganisms must be created or discovered that can withstand the harsh environments of Mars. The first organisms used must be able to survive exposure to ionizing radiation and the high concentration of CO2 present in the Martian atmosphere[7]. Later organisms such as multicellular plants must be able to withstand the freezing temperatures, withstand high CO2 levels, and produce significant amounts of O2.

Microorganisms provide significant advantages over non-biological mechanisms. They are self-replicating, negating the needs to either transport or manufacture large machinery to the surface of Mars. They can also perform complicated chemical reactions with little maintenance to realize planet-scale terraforming[8].

Mars is the primary subject of discussion for seeding. Locations for seeding are chosen  based on  atmospheric temperature, air pressure, existence of harmful radiation, and availability of natural resources, such as water and other compounds essential to terrestrial life[9].

Necessary Technology:[edit]

Natural or engineered microorganisms must be created or discovered that can withstand the harsh environments of Mars. The first organisms used must be able to survive exposure to ionizing radiation and the high concentration of CO2 present in Mars's Atmosphere[10]. Later organisms such as multicellular plants must be able to withstand the freezing temperatures, withstand high CO2 levels, and produce significant amounts of O2.

Microorganisms provide significant advantages over non-biological mechanisms. They are self replicating, negating the needs to either transport or manufacture large machinery to the surface of mars. They can also perform complicated chemical reactions with little maintenance to realize planet-scale terraforming[11].

Impression of the hypothetical phrases of the terraforming of Mars. Copied from en:Image:MarsTransitionV.jpg

Geoengineering:[edit]

Geoengineering, or climate engineering, is a form of planetary engineering which involves the process of deliberate and large-scale alteration of the Earth’s climate system to combat climate change[12]. Examples of geoengineering are carbon dioxide removal (CDR), which removes carbon dioxide from the atmosphere, and the use of space mirrors to reflect solar energy to space[12][13]. Carbon dioxide removal (CDR) has multiple practices, the simplest being reforestation, to more complex processes such as direct air capture[12][14]. The latter is rather difficult to deploy on an industrial scale, for high costs and substantial energy usage would be some aspects to address[12].

Another geoengineering discipline is “solar radiation management” (SRM), which is the process of rapidly cooling down the Earth’s temperature[12]. Examples of this process include stimulating the cooling effect of volcanoes and enhancing the reflectivity of marine clouds[12]. When a volcano erupts, small particles known as aerosols proliferate throughout the atmosphere, reflecting the sun's energy back into space[12][15]. This results in a cooling effect, and humanity could conceivably inject these aerosols into the stratosphere, spurring large-scale cooling[12][15].

Visible ship tracks in the Nothern Pacific, on March 4th, 2009. On an overcast day, the clouds look uniform. However, NASA MODIS images' sesor reveals long skinny trails of brighter clouds hidden within. As ships travel across the ocean, pollution in the ships' exhaust create more cloud drops that are smaller in size, resulting in even brighter clouds.

Marine cloud brightening (MCB) is a solar radiation management theory that is designed to make marine clouds brighter, reflecting light back into deep space[16]. By reflecting light from the sun, this process could help offset anthropogenic global warming, which threatens the lives of all human beings and life on Earth[17]. One proposal involves spraying a vapor into low-laying sea clouds, creating more cloud condensation nuclei[18]. This would in theory result in the cloud becoming whiter, and reflecting light more efficiently[18].

  1. ^ a b Pollack, James B.; Sagan, Carl (1991-01-01). "Planetary engineering". Resources of Near-Earth Space: 38. Bibcode:1991rnes.nasa...38P.
  2. ^ a b "Habitats, Habitability, and Human Factors | NASA SBIR & STTR Program Homepage". sbir.nasa.gov. Retrieved 2021-11-05.
  3. ^ a b c Jakosky, Bruce M.; Edwards, Christopher S. (August 2018). "Inventory of CO2 available for terraforming Mars". Nature Astronomy. 2 (8): 634–639. doi:10.1038/s41550-018-0529-6. ISSN 2397-3366.
  4. ^ a b c Tawa, John; Shanmugham, Uma; Dao, Tam K.; Tsui, Venus; Nguyen, Phuong T.; Day, Stephanie (2011). "Vietnamese, Burmese, and Bhutanese Refugees: What Do We Know About Their Histories and How Do We Help Them". PsycEXTRA Dataset. doi:10.1037/e573292012-023. Retrieved 2021-11-05.
  5. ^ a b "The Ethics of Terraforming | Issue 38 | Philosophy Now". philosophynow.org. Retrieved 2021-11-05.
  6. ^ Lopez-Arreguin, A. J. R.; Montenegro, S. (2019-09-01). "Improving engineering models of terramechanics for planetary exploration". Results in Engineering. 3: 100027. doi:10.1016/j.rineng.2019.100027. ISSN 2590-1230.
  7. ^ a b Todd, Paul (2006-01-01). "PLANETARY BIOLOGY AND TERRAFORMING". Gravitational and Space Biology. 19.
  8. ^ Conde-Pueyo, Nuria; Vidiella, Blai; Sardanyés, Josep; Berdugo, Miguel; Maestre, Fernando T.; de Lorenzo, Victor; Solé, Ricard (2020-02-09). "Synthetic Biology for Terraformation Lessons from Mars, Earth, and the Microbiome". Life. 10 (2): 14. Bibcode:2020Life...10...14C. doi:10.3390/life10020014. ISSN 2075-1729. PMC 7175242. PMID 32050455.
  9. ^ Todd, Paul (2006-01-01). "PLANETARY BIOLOGY AND TERRAFORMING". Gravitational and Space Biology. 19.
  10. ^ "Planetary Engineering and Terraforming", Energy Demand and Climate Change, Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, pp. 209–218, 2009, doi:10.1002/9783527627035.ch20, ISBN 978-3-527-32446-0, retrieved 2021-11-03
  11. ^ Conde-Pueyo, Nuria; Vidiella, Blai; Sardanyés, Josep; Berdugo, Miguel; Maestre, Fernando T.; de Lorenzo, Victor; Solé, Ricard (2020-02-09). "Synthetic Biology for Terraformation Lessons from Mars, Earth, and the Microbiome". Life. 10 (2): 14. Bibcode:2020Life...10...14C. doi:10.3390/life10020014. ISSN 2075-1729. PMC 7175242. PMID 32050455.
  12. ^ a b c d e f g h "What is Climate Engineering? | Union of Concerned Scientists". www.ucsusa.org. Retrieved 2021-10-27.
  13. ^ "Explainer: Six ideas to limit global warming with solar geoengineering". Carbon Brief. 2018-05-09. Retrieved 2021-11-01.
  14. ^ "Effectively removing CO2 from the atmosphere". ScienceDaily. Retrieved 2021-10-27.
  15. ^ a b "Volcanoes Can Affect Climate". www.usgs.gov. Retrieved 2021-11-01.
  16. ^ "Marine cloud brightening", Wikipedia, 2021-08-11, retrieved 2021-11-03
  17. ^ Jackson, Randal. "The Effects of Climate Change". Climate Change: Vital Signs of the Planet. Retrieved 2021-11-03.
  18. ^ a b "Proposed Geoengineering Technologies". Geoengineering Monitor. Retrieved 2021-11-03.
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