Theearth’s extreme range of environments has already proven how frail the humanbody is. Without sophisticated gear,human beings cannot venture into the depths of the oceans, the expanses ofdeserts, and the high altitudes of mountains.This fact is doubly important for life in space, as the needs of humansmust be provided for, and to accomplish such a task plants with millennia-oldlineages will be combined with just out of the womb technology to create aviable environment in Æther.
Radiationin outer space can be differentiated into two kinds: nonionizing radiation andionizing radiation. Nonionizingradiation consists of long-wavelength electromagnetic radiation, which isdefined as electric and magnetic energy, or fields, traveling throughspace. The sun emits nearly all of theelectromagnetic radiation found in the solar system; the radiation intensity isapproximately 1390 W/m2 near the earth. However, an object in orbit around the earth also has to take intoaccount the radiation intensity emitted by the earth, 225 W/m2 [ref1].
Ionizingradiation is defined as high-energy particles and short wavelengthelectromagnetic-radiation that separate electrons from their atoms upon closepassage. It includes gamma radiation, Xradiation, alpha particles, beta particles, neutrons, protons, and heavynuclei. Two primary sources of ionizingradiation in space are Solar Cosmic Rays (SCR) and Galactic Cosmic Radiation(GCR). SCR are composed of protons,electrons, and other heavy nuclei with energies of 107 to 109eV. SCR coincide with very large solarflares that occur once or twice during the eleven-year solar cycle.
The amount of radiation that is absorbed can bequantified through the use of dosimetry.The SI unit for absorbed dose is the gray (Gy): 1 Gy = 1 J/kg.
Radiation | RBE |
X rays | 1 |
5 MeV γ rays | 0.5 |
1 MeV γ rays | 0.7 |
200 keV γ rays | 1 |
Electrons (β rays) | 1 |
Protons | 2-10 |
Neutrons | 2-10 |
α particles (He nucleus) | 10-20 |
Thus,the effective dose can be given as the product of RBE and Gy.
Whena high-energy particle enters the body, it can either undergo directinteraction with the atoms of the body, thus producing many ions, or it canundergo indirect interaction with the atoms and produce secondaryradiation. The secondary radiation thatis produced when high-energy particles interact with atoms or molecules in thehuman body is called Brehmsstrahlung radiation. Brehmsstrahlung radiation occurs when high-energy particles aredeflected and decelerated by charged particles. This secondary radiation also ionizes the surroundingtissue. In both cases, the ionizingeffects of the radiation are proportional to the energy absorbed by thesurrounding tissue. The ions producedcan produce free radicals, such as the highly reactive and unstable OHmolecule. A free radical can attackother compounds in the body to form even more free radicals and thus has far reachingconsequences. A dose of 0 to 0.5 Svwill result in no obvious effects, while doses from 0.5 to 1 will causeradiation sickness in 5-10% of exposed personnel. A dose of 10 Sv will most likely kill all who are exposed [ref1].
Somatic damageaffects the exposed organism during its lifetime and can be classified as acuteor long-term effects. Acute effects ofradiation are caused by exposure to high doses of radiation in a short timeframe, it is indicated by the symptoms of radiation sickness such as nausea,vomiting, discomfort, a decrease in the number of white blood cells, loss ofappetite, and fatigue. If exposed todoses higher than 2 Sv, one can also expect diarrhea, hemorrhaging, and hairloss. Effects of prolonged exposure tolow doses of radiation include cancers of the lung, breast, digestive system,and leukemia. One can expect anincrease in 2% to 5% chance of contracting cancer for every 0.5 Sv.
Radiation canalso inflict genetic damage; this type of damage harms the offspring of theexposed organism through damage of the genes and chromosomes.
Exposure toradiation of fetuses during 16 to 25 weeks of pregnancy results in adverseneuro-developmental effects such as mental retardation, reduced IQ, and seizuredisorders. Exposure during the gestationalperiod (8-15 weeks) results in even more damage, as it is the most sensitivetime for neurological developments. Theabove-mentioned three abnormalities, as well as microcephaly (the abnormalsmallness of the head) occurred in children born to the survivors of the atomicbomb detonations in Japan during the Second World War [ref 4].
Setting healthstandards for exposure to radiation is difficult, as the effect of heavy nucleion human tissue is not well known.Currently, some scientists advocate that any amount of radiation causessome damage, even down to low doses.Other scientists, however, believe that there a threshold exists belowwhich no radiation risks occur. Untilmore scientific evidence that can settle the matter with confidence is introduced,it would be safer to assume that even low doses of radiation pose danger tohuman life. The 1993 National Councilon Radiation Protection and Measurements (NCRP) recommendations were 1 mSvannual dose limit for continuous exposure and a 5 mSv annual dose limit forinfrequent exposure.
Thereare two main types of radiation protection: active shielding and passive bulkshielding. Active shielding includes amagnetic field that deflects charged particles from the crew area and amagnetic/electrostatic plasma shield that uses an electrostatic shield toprotect the interior from positively charged particles while a magnetic fieldconfines electrons from the space plasma to provide charge neutrality [ref 5].
Passive bulkshielding deflects or stops radiation before damage to sensitive electronics,living tissue, and structural components can be done. Aluminum is most commonly used in today’s spacecraft for passiveshielding, as it is both lightweight and high density [ref 1].
The residentialarea radiation shielding will consist of a lunar regolith/ice layer 4 metersthick. The lunar regolith/ice layerwill consist of a crushed lunar regolith matrix and ice supported by analuminum framework, the total density of the structure would be around 500-3000kg/m2. Lunar soil consistsmostly of SiO2, TiO2, Al2O3, MgO,CaO, and FeO [ref 1]. The lightelements, such as silicon, oxygen, and aluminum, will provide an excellentshield for both GCR and SCR. Theaddition of ice to the shielding will also aid in shielding against incomingparticles as well as diffusing the ions that are created from the interactionsof radiation and the passive shield, thereby preventing the ions amalgamatinginto and weakening the crystal structure of the aluminum framework [ref 9].
The windows thatpermit sunlight into the residential area of Æther will also have to filter outthe undesired wavelengths. This can beachieved through the use of selectively transparent glass, which absorb some wavelengthswhile allowing others to pass through.Selectively transparent glasses can be manufactured by depositing a thinlayer of metal onto the glass. Thickglass in itself is opaque to the long wavelengths of infrared radiation, whileleaded glass would also provide protection against X and gamma radiation. A“sandwich” would be made with leaded glass on the outsides and a layer of waterin between. This layer of water couldbe laced with aqueous solutes that decrease the amount of radiation thatreaches the colonists. The aluminummirrors that work in conjunction to reflect light into the habitable areas willalso be able to absorb some harmful radiation.During times of heightened solar flare activity, radiation shutters madeof CuW-Al panels could be drawn over the windows and residents would be advisedto stay inside radiation shelters.
As Æther is in afree falling orbit around earth, there will exist a microgravity environmentwithin it. This environment isundesirable for long-term habitation since humans cannot adapt toweightlessness. The human body reactsto the conditions associated with weightlessness in a series of interrelatedresponses that begin in the gravity receptor tissues, fluids, and weightbearing structures.
The gravityreceptors refer to the otolith organs in the inner ear; mechanical receptors inthe muscles, tendons, and joints; and pressure receptors in the skin.
Weightlessnessalso causes havoc in the body’s fluid systems, as the body is 60 percent waterby weight. On earth, fluids inside thebody have weight and are normally pulled towards the ground, creatinghydrostatic pressure [ref 27]. Thishydrostatic pressure primarily influences the distribution of fluids byaffecting how much blood leaks from arteries and into the interstitial space inbetween cells. Under weightlessnessconditions, this hydrostatic pressure is not present and redistribution ofbodily fluids occurs [ref 27]. Each legloses about one liter of fluid in the first day of micro gravity conditions,this fluid is redistributed to the upper body.Renal, hormonal, and mechanical mechanisms that regulate fluid andelectrolyte levels are affected by the shift in fluids.
Muscle and boneloss is also associated with long periods.Structural elements experience drastic changes in conditions ofweightlessness, as they no longer have to bear the weight associated withorgans on earth. Some skeletal musclesalso atrophy as different muscles are used for traversing through a weightlessenvironment. Muscles also switch overto fast-twitch muscle fibers, which are used for rapid movements, rather thanslow-twitch fibers, which are used for support against gravity’s pull.
Partialremedy of these symptoms can be achieved through exercise and the use of light-emittingdiode (LED) blankets, which prevents bone and muscle atrophy by submerging thebody in 680, 730, and 880 nm light [ref 29].However, the least discomfort can be achieved by rotating the colony toproduce a psuedo-gravity that mimics gravity on earth.
fig. 3.1
Rotational motion produces a“pull” radially outwards that many are tempted to call the centrifugal(“center-fleeing”) force, but in fact no such force exists.
fig. 3.2
If ac=v2/rand v= ωr, we can find an equation for ac in terms of ω,or the angular velocity. Since thedesired psuedo-gravity is 9.8 m/s2, the equation for revolutions perminute in terms of radius would be .
fig. 3.3
However,in a reference frame that rotates at a constant angular speed, there existsanother psuedoforce known as the Coriolis force. The Coriolis force affects any object that moves linearly withina rotating system. If the object movesfrom Ra radially towards Rb, where Ra is awith a smaller radius compared to Rb, the direction of the Coriolispseudoforce is counter to the direction of rotation. If the object moves radially from Rb to Ra,then the pseudoforce acts in the direction of rotation.
SinceÆther will have a major radius of 2000m, the angular velocity will be 0.07rad/s; and the rotation rate will be 0.6685 rpm, well within the allowablelimits. The rotation of Æther will beachieved by spinning it with thrusters positioned at the outermost edges of thetorus. To calculate the thrust needed,the equations τ =Ia and
τ = rFsinθ must beused, where τ equals the torque, I is the moment of inertia of Æther, ais the angular acceleration, r is the radius, and F is the force.
fig. 3.4
However, the thrusters will alsobe employed for maintaining the rotation of the colony, since variances inangular momentum will occur when objects move from the center to thetorus. Thus the thrusters should be ofa durable and reliable nature, preferably ion thrusters, since they are able togenerate low thrust at high efficiencies and are also very reliable.
Atmosphere management concerns the atmosphericrevitalization and contaminant control of the colony atmosphere.
III.C.1 CO2Concentration and Removal
CO2concentrations must remain at a low level in order for normal life tooccur. The adverse effects of highconcentrations of CO2 include headaches, mental depression, hearinglosses, dizziness, increased cardiovascular activity, nausea, and eventuallyunconsciousness. The partial pressureof CO2 on earth is 0.0318 kPa.Allowable levels of CO2 concentration are 1.01 kPa duringshort missions and 0.40 kPa for long missions such as an assignment to theInternational Space Station. In orderto prevent CO2 buildup due to human respiration (1 kg of CO2per day), methods of removing it from the atmosphere must be utilized [refDesigning for Human presence in space]..
Four ways toremove CO2 from the colony atmosphere are absorption (chemical orelectrochemical reaction with a sorbent material, adsorption (physicalattraction to a sorbent material), membrane separation, and biologicalconsumption. The main technology in use today that utilizes absorption for CO2removal is LiOH absorption, however, LiOH absorption is not acceptable forlong-term (over 2 weeks) use as it is not a regenerable process and thechemical reaction cannot be reversed.Molecular Sieves adsorb CO2 due to its microscopic pores,which allow O2 and N2 to pass through, but trap CO2.
4 bed molecularsystems (4BMS), which utilize 5A zeolite molecular sieves for trapping CO2,have already been flight proven on Skylab, and can be expected to perform for10 years without failure [refhttp://www.ae.utexas.edu/~campbell/fatmass/pdr2.htm]. 4BMS operates in a cycle, with equal amounts of time needed foradsorption and desorption of CO2.However, a vacuum environment is needed for the desorption of CO2.
Solid aminewater desorption utilizes heated solid amine to absorb/desorb CO2.
Electrochemicaldepolarization concentration (EDC) uses electrochemical reactions to remove CO2from the air, the net effect is the production of water from hydrogen and oxygen,the production of DC power and heat, and the concentration of carbondioxide. EDC has the advantages ofbeing able to operate in cyclic or continuous mode, easily alter the CO2removal rate, and produce DC power.However, the possibilities of H2 leakage must also beconsidered as well as the heat load and O2 demands.
TheO2 partial pressure at sea level is 21.4 kPa.
Onthe space colony, O2 generation will be the task of the plantsonboard. The plants could also be usedfor CO2 removal from the colony atmosphere; however, since fasterplant growth rates can be achieved with a concentrated CO2atmospheric level, CO2 removal and concentration will be left to theEDC/APC systems onboard.
However,there is a loss of approximately 0.10 moles of CO2 if plants areintroduced into the colony CELSS, since humans exhale about 0.85 moles per moleof O2 consumed, and plants consume about 0.95 moles of O2for every mole of O2 produced.Variations in CO2 consumption and O2 productionrates also exist due to the fact that plants do not experience constant plantgrowth, but rather experience periods of accelerated growth when CO2consumption is at a higher level.Plants also stop producing CO2 and start consuming O2because of cellular respiration during periods when there is noillumination. High growth rates must beconsidered along with high yields as high temperatures 298 K (25º C) promoterapid growth but lead to low yields, while cooler temperatures 293 K (20 º C)promote higher yields but hinder rapid growth.Therefore, to ensure a stable means of oxygen generation while utilizingplants as the method of O2 generation, several methods arerecommended, such as providing multiple plant growth areas that are illuminatedat different times of the day, to ensure a steady source of oxygen night andday; altering illumination or temperature levels to control photosyntheticrates; and using a system of gas storage.
Tocompensate for times when plant O2 generation is below requiredlevels, artificial means of generating O2 must be considered.
Severalsystems considered for O2 generation onboard the colony are StaticFeed Water Electrolysis (SFWE), Solid Polymer Water Electrolysis (SPWE), andWater Vapor Electrolysis (WVE). SFWEwas rejected because of its use of asbestos, SPWE and WVE both are technologiesthat possess many desirable attributes.SPWE is a mature technology that is being used onboard the InternationalSpace Station for its Oxygen Generation Assembly. Integration of both SPWE and WVE would not be too difficult asSPWE could receive water from the CHX subsystem, and WVE could directlyelectrolyze atmospheric air. Thedrawback of SPWE are that it is sensitive to water contamination, while thedrawback of WVE is that it interferes with the humidity control of CHX.
Condensingheat exchangers (CHX) have been widely used to remove moisture and heat at thesame time from the atmosphere of space missions by using coolant-cooled fins tocondense humid air and then removing the condensation via “slurper holes” [ref1]. By using fins to maximize thesurface area, faster rates of heat exchange with a minimum of volume can beachieved. First, atmospheric air isdrawn into the system, and its humidity and temperature are recorded.
Tracegasses in the colony atmosphere will pose a threat since even the smallestamounts of harmful gas would create an unacceptably high concentration in therelatively small volume of the colony.Sources of trace gasses could include outgassing, CELSS processes, andevaporation of volatile substances, and special concern for those elementsshould be taken during the design stage.Trace contaminants which may be pose a threat in space missions includeacetone, C3 to C8 aliphatic saturated aldehydes, hydrogen chloride, isoprene,methylhydrazine, perfluoropropane and other aliphatic perfluoroalkanes,polydimethylcyclosiloxanes, dichlorofluoromethane (Freon 21),chlorodifluormethane (Freon 22), trichlorofluoromethane (Freon 11),dichlorodifluoromethane (Freon 12), 4-methyl-2-pentanone, chloroform, furan,hydrogen cyanide, carbon monoxide, benzene, acetaldehyde, methanol, indole, hydrogen,nitromethane, hydrazine, nitrogen dioxide, mercury, ammonia, and others [refs40, 41].
The technologiesavailable for active contamination monitoring include gas chromatography/massspectrometry (GC/MS), infrared dispersion/spectroscopy, and ultravioletspectroscopy [ref 40]. Thentechnologies such as particulate filters, activated charcoals, chemisorbantbeds, and catalytic burners are used to purge the atmosphere of undesiredcontaminants [ref 1].
The firstcomponent of GC/MS is a gas chromatograph, which uses gaseous diffusion toidentify different components of the airflow, while the second component ofGC/MS is a mass spectrometer, which utilizes the different deflections causedby a magnetic field to analyze molecular weights. GC/MS is a proven system both on space missions and duringearth-bound field use, and can identify virtually all chemicals encountered viaanalysis of the data obtained through both components.
Infrareddispersion/spectroscopy would be used in conjunction with GC/MS during analysisof organic contaminants to verify its conclusions and provide furtherdata. Infrared dispersion/spectroscopyoperates on the principle that different molecules absorb different wavelengthsof an infrared beam that is shone through it.By analyzing the resultant complex spectrum with Fourier transforms, thecomponents of the air sample can be determined. The infrared dispersion/spectroscopy technique pairs nicely withGC/MS since it can determine the nature of a contaminant that does not possessa unique molecular weight [ref 40].
Removal techniqueswould utilize all of the purging technologies.First the air would be passed through several HEPA filters to trap dustparticles and microorganisms, these would preferably be placed in an easily accessibleplace, so that they can be exchanged for fresh ones once they have reached theend of their lifespan. Then thecontaminated air is passed over activated charcoal beds, which adsorb ammoniaand water-soluble contaminants [ref 1].These beds can be “recharged” via desorption during exposure to vacuumand heat. A catalytic oxidizer based onpalladium oxidizes hydrocarbons not adsorbed by the charcoal beds, while LiOHpost- and presorbant beds adsorb acids [ref 1, 40]. The CHX can also remove soluble contaminants as the watercondenses and drops to the bottom of the exchanger [ref 40].
Toensure proper mixture of oxygen into the atmosphere, removal of heat, and theremoval of carbon dioxide and trace contaminants, a minimum air velocity insidethe colony is needed. Maintaining aproper ventilation system is also crucial to supplying the atmosphericmanagement subsystems with air from the colony atmosphere.
fig. 3.5
The air velocity created by thevents should not be so excessive as to cause drafts (>0.2 m/s) but should beabove the recommended 0.08 m/s required for adequate removal of carbon dioxideand other substances toxic in various amount [refs 1, 40].
Solidand liquid organic waste onboard the colony will have to be treated andconverted into useful substances so that an accumulation of unwanted mass isavoided. Waste onboard the colony willmostly consist of feces, urine, food preparation byproducts, packaging, etc.
Wateris essential for human life, as humans use water for nutrition andcleansing. Additionally, manymanufacturing and research processes will require the use of water.
Alot of organic waste will occur during harvesting and food processing, when theinedible parts of a plant are discarded.Waste also occurs when in the house in the form of bodily excretions anddiscarded materials or food. Thus,collection facilities should be in place to properly dispose of thiswaste. Collection of feces and urinewill be through earth-like toilets that would utilize “gravity” action and willuse a flow of water to carry away the waste.Colonists will be encouraged to presort their organic and inorganictrash. The organic trash could then gointo paper or biodegradable plastic bags, while the inorganic trash could gointo a communal collection bin. Theorganic trash would then be fed into the waste processing system while inorganicmatter would be sent to the recycling facilities.
Mostorganic wastes onboard the colony would be inedible plant mass such as roots,stems, and leaves. Processing of thismaterial can either be bioregenerative recovery of the plant nutrients or totaloxidation of the plant matter.Bioregenerative recovery of the plant matter was selected in order tomaximize the nutrients gained from the growing of plants.
Cellulose,the primary structural component of cell walls in plants, is a polysaccharideof glucose. Many methods exist tohydrolyze cellulose into glucose, which could then be added to the human diet,but most of them involve chemicals or high temperatures that also decompose theresultant glucose. Cellulase is a groupof enzymes, which hydrolyze cellulose, cellulases are most common in fungi andmicrobial sources. Pretreatment of theplant matter is necessary before efficient hydrolysis of cellulose can occur,since cellulose in plants is “sealed” with lignin and commonly found in thepresence of hemicellulose [ref 1].These additional substances inhibit enzyme contact with cellulose andonly after they have been removed can cellulose conversion rates of over 50% beachieved [ref 1]. The ideal method forremoval of lignin and hemicellulose is thought to be hot water treatment.
Humanwastes primarily consist of urine and feces.The first step in processing this waste is collection andsegregation. Urine would probably becollected along with feces via the colony sewage system.
SCWO oxidizesorganic compounds using water in its supercritical state.
Wet oxidation issimilar to SCWO in that it also heats and pressurizes aqueous waste in thepresence of oxygen. However, thepressures and temperatures involved are not as drastic (14 MPa, 473-573K). The disadvantages of this systemare that the organic compounds are not totally converted into CO2and other simple compounds, so there is a small amount of ash residue [ref 1].
Combustioninvolves the rapid exothermic oxidation of organic matter.
Electrochemicalincineration has the potential to degrade organic substances into carbondioxide, nitrogen, and hydrogen gas through an electrolysis process.
Another wastemanagement technology is Waste Management-Water Systems (WM-WS).
WM-MS,electrochemical incineration, and SCWO are all promising systems indevelopment. At this time, insufficientdata is available in determining which system would be the most suitable toprocess organic waste, but SCWO seems to be the technology farthest along indevelopment, as it is already being developed for the destruction of chemicalwastes on earth. After being processedthrough SCWO, the waste feed is then routed to the agricultural sections, whereit will be analyzed, adjusted, and used as a nutrient source.
Recycling ofinorganic materials would utilize processes similar to those on earth.
After collection from the CHX and SCWO systems, therecycled water would then be tested for purity and then stored inside theWBS. During the period of emergency,all unnecessary water consumption would be prohibited.
Inorder to ensure the safety of machines and humans, the water supply must abideby water quality guidelines.
(units are mL/g, unless otherwise stated) | |
Total Solids | 100 |
pH | 6.0-8.5 |
Ammonia | 0.5 |
Arsenic | 0.01 |
Barium | 1.0 |
Cadmium | 0.005 |
Calcium | 30 |
Chlorine | 200 |
Chromium | 0.05 |
Copper | 1.0 |
Iodine | 15 |
Iron | 0.3 |
Lead | 0.05 |
Magnesium | 50 |
Manganese | 0.05 |
Mercury | 0.002 |
Nickel | 0.05 |
Nitrate | 10 |
Potassium | 340 |
Selenium | 0.01 |
Silver | 0.05 |
Sulfate | 250 |
Sulfide | 0.05 |
Zinc | 5.0 |
Cations | 30 |
Anions | 30 |
Carbon dioxide | 15 |
Bacteria (Colony Forming Units/100mL) | 1 |
Total Acids (µg/L) | 500 |
Cyanide (µg/L) | 200 |
Halogenated Hydrocarbons (µg/L) | 10 |
Total Phenols (µg/L) | 1 |
Total Alcohols (µg/L) | 500 |
Total Organic Carbon (µg/L) | 500 |
[ref 40]
Thesepollutants should be monitored by an automatic system that would divert theunacceptable water to processing systems.There exists chemical, thermal, light, and mechanical methods todisinfect water [ref 40]. Mechanicalfiltration would be useful for separating nonsoluble and large particlecontaminants and thus would come at the very beginning of the disinfectionsystem. Since thermal and light meansof disinfecting water mostly affect biological contaminants, the tainted waterwould first be subjected to heat and UV irradiation treatment before being subjectedto chemical treatment. Chemical meansto disinfect water include iodine, ozone, and silver. Since silver and iodine are both contaminants, ozone was chosento disinfect water. Mechanicalfiltration, thermal processing, UV irradiation, and ozone treatment are alltechnologies proven on earth and should not pose significant problems duringimplementation.
Photosynthesiscan fulfill the need for food production, atmospheric regeneration, wastemanagement, as well as water management, since it produces edible biomass; oxygenfrom atmospheric carbon dioxide; simple compounds such as nitrogen and carbondioxide from biodegradable substances; and potable water from transpiration inplant leaves.
Two kingdoms of organismsthat carry on photosynthesis are Protista and Plantae.
Higher plantshave the advantages of transpiring water, which makes water purification muchsimpler; of being the basis for much food normally eaten by humans andproviding most of the nutrients needed by humans; of being capable of removingsome volatile and liquid contaminants produced by humans or machinery; and ofproviding an aesthetically pleasing environment to the colonists.
Sincethe process of photosynthesis relies on the light energy, providing properillumination in the agriculture areas is of vital importance.
However, in thelower level of the habitat section, either indirect solar lighting orartificial lighting will have to be used, since the lower level does notdirectly receive solar light. Indirectsolar lighting involves the collection and transportation of light with the useof mirrors, lenses, and optical fibers.The primary goal in designing a solar light collection system is tofilter out the unnecessary wavelengths and supply light at the requiredintensities. Selectively transparentcoatings or lenses can be used to filter out undesirable frequencies such as infraredand ultraviolet. Artificial lightingseems to be the better method, since indirect solar lighting would requirelarge structures to collect and transport light [ref 1].
There are manytypes of artificial lighting, from fluorescent tubes and high-pressure sodiumlamps to light-emitting diodes (LEDs).Interest in the latter is particularly high due to their low heatgeneration, high electrical efficiency, low mass, and low volume.
Solar lightingaugmented with artificial lighting will be utilized in the agricultural areason the primary floor, while the agricultural areas on the lower level will beentirely lit by LEDs.
Plants can derive their nutrients from either soilsubstrates or from water-based solutions.Soils can be either earth-like or synthetic. The advantages of using earth-like soils are not readilyapparent; among other things, they require a large amount of mass, do not offera readily adjustable nutrient concentration, and could possibly lead tomicrobiological contamination.Synthetic soils consist primarily of zeolites, which enable it to storeand slowly release the desired nutrients over a long period of time.
Substrate-lessnutrient delivery systems include hydroponics and aeroponics.
Theatmosphere should be carefully designed to maximize growth, and attentionshould be given to atmosphere composition, temperature, humidity, ventilation,and toxicant levels [ref 1].
Whilethe goal of the CELSS is to provide an environment that is as Earth-like aspossible, the opposite may be true when determining the atmosphere compositionin the plant growth chambers. Plantsgenerally do well when the O2 partial pressures are reduced, andwhen CO2 partial pressures are increased. C4 pathway plants have an optimal CO2concentration of about 350 ppm, while C3 plants have a higheroptimal concentration of approximately 1000 ppm [ref 1].
Preservinga stable temperature is important for plant growth as they contain enzymes thatoperate at an optimal temperature. Mostplants prefer a temperature range of 285-301K, but specific temperatures varywith species, carbon dioxide concentration, irradiance intensity, and photoperiod.
Transpirationis a major process that impacts photosynthesis, and is impacted by the humidityof the atmosphere. High humidity levelsare preferable since they reduce transpiration rates; therefore the water needsof the plants are reduced. Yet plantsalso need an adequate transpiration rate that can sufficiently cool off theleaves. Thus humidity controls shouldbe linked to temperature monitoring of plants.
Takingthe varied requirements of plants into account, plants will be grown inself-contained modules that can be easily reprogrammed for differentspecies. These modules would also allowthe repair and cleaning of different sections of the plant growth area withouthaving to disrupt a large number of plants.
Humandiets must contain certain amounts of carbohydrates, certain amino acids, fats,calcium, iron, iodine, fluorine, potassium, zinc, vitamin A, vitamin B1,vitamin B2, vitamin B12, niacin, folic acid, vitamin C,vitamin D, vitamin E, vitamin K, as well as trace amounts of other minerals.
Whileplants are a more efficient method of obtaining protein, the culinary benefitsof the inclusion of animals into the diet cannot be overlooked.
Unfortunately,some conflicts will arise between the colonists’ innate tastes and the abilityto cater to those tastes using foods grown on Æther. The European and North American reliance on dairy products [ref 48],for example, will conflict with the scarcity and high price of such desiredgoods. Fortunately, some othercultures, such as Hinduistic Indian, do not rely heavily on animal products andtheir dietary needs should not pose a problem. It is hoped that the colonists will be able tomaintain their traditional diets while at the same time being able to sampledifferent foods from all over the world.
Thedevelopment of acceptable substitute will be of great concern to colonynutritionist who will strive to create the most appealing of diets whilerestricted by the number of raw materials.Substitutes are already used on earth, including many products made outof soy and peanuts. However, recentadvances in biochemistry that have lead to the identification of organiccompounds responsible for the taste for wine give hope to the possibility thatauthentic-tasting steaks or burgers can be synthesized from the crops grown in Æther.
Theneed for preparation of different foods falls into three general categories,little to no processing, primary processing, and secondary processing [ref1]. Foods that require little to noprocessing are either fruits or vegetables that may be eaten raw, and thus onlyrequire washing, peeling, or cutting before being served.
III.F.3 Food Storage
If raw materials or processed foods are not to beconsumed immediately, refrigeration is necessary to prevent spoilage.
Biodegradablepackaging based on either cellulose or bioplastics should be used to lower theamount of unrecyclable waste. Ediblerice (or wafer) has been used for quite some time on earth, and may prove to beuseful in Æther. Plastic and metalcontainers should be reused and not thrown away after the first use.
Fire is the mostundesirable mishap to happen in a spacecraft.The confined interiors of any space habitat have the effect of greatlyincreasing the lethality of a fire.Methods of reducing losses due to fires include prevention, detection,and suppression. Fire prevention isimplemented during the design phase and minimizes the probability that a firewill occur onboard by using nonflammable materials in construction.
III.G.1 Fire Prevention
The use offlammable materials in everyday objects should be avoided so as to prevent theaccumulation of such substances.Prevention of fires can be done by not utilizing napped (fuzzy) finisheson clothing; designing garments so that a minimum of loose clothing is used;manufacturing carpets and other textile items out of flame resistant or flameretardant material; reducing the number of ignition sources; separatingflammable material with non-flammable material; isolating flammable materialfrom ignition sources; creating flame barriers through the use of non-flammablematerials such as metals and ceramics; using metallic coatings on substrates;and coating flammable surfaces with Fluorel® [ref 10].
Traditionally,space habitats have utilized the inherent human sense of as smell to detect thepresence of fire. However, in avoluminous space settlement, fires may break out where humans are not nearby todetect its presence, thus automatic fire detectors must be present in all partsof the colony [ref 13]. Current methodsof fire detection sense the presence of smoke or flame.
Smoke detectorsare usually employed in ventilation ducts while flame detectors are installedin open areas. Two types of smokedetectors are photoelectric detectors and ionization detectors.
Flame detectorsare triggered by the ultraviolet, visible, and infrared radiation that firesproduce. Monitoring of all wavelengths(UV, visible, and IR) is desirable so that false alarms are kept to aminimum. Integrated UV, IR, and visiblesensors have already been fabricated using CMOS technology, and willundoubtedly be available for use in the future.
Once a fire hasbeen detected, it should be expediently extinguished. However, the methods used to extinguish the fire should not harmthe surrounding equipment and the environment of Æther.
CO2is an effective fire suppressant and is normally stored as a liquid at roomtemperature with high pressures. Whenliquid carbon dioxide is released from an extinguisher, the liquid immediatelychanges to a gas because of the pressure difference. This process is highly endothermic and helps in cooling thefire. Additionally, carbon dioxide isdenser than normal air, and will suffocate the fire by depriving it of oxygen.
Water based firesuppression systems fall into two categories, sprinklers and fine water mistsystems, with the two differing only in the droplet size.
Water will beused in most locations, but carbon dioxide suppression systems will beimplemented in vital places where humans are not normally present, such as theareas which house CELSS machinery.
The Æther space colony will require a vast amount ofelectrical power to function seamlessly.The issues needed to be discussed are power distribution, generation,and storage.
Copper wires will be used to distribute powerthroughout Æther, and wire diameters would have to be large enough to preventfires from breaking out due to excess heat caused by resistance of thewire. High voltages will be used todistribute power, so that the current can be minimized, thus reducing energyloss due to resistance. Power from thephotovoltaic cells or from the flywheel storage units will first be convertedinto AC then sent through primary transmission lines at high voltages.
Ætherwill have a centrally located hexagonal solar panel with sides of 900 metersthat has a hexagonal shaped hole with sides of 380 meters in the center plustwo rectangular panels with length of 600 meters and width of 300 meters belowthe hexagon. The total combined surfacearea of all the panels is 3.45 million m2, thus enabling the spacecolony to soak up 5.3 million kilowatts, but due to solar cell efficiencies ofapproximately 13%, that only means 689 thousand kilowatts that the colony canactually use.
There are manycutting-edge technologies available for power storage on Aether.
III.H.3.a
A flywheel is anelectromechanical system that stores energy by spinning a disk at highspeeds. When power is needed therotational energy of the disk is used to turn a dynamo.
III.H.3.b
A capacitor
Currently,the most widely used fuel cell is the hydrogen-oxygen fuel cell.
Allof the above mentioned systems would be implemented on Æther since differentones have the most advantages in certain situations. However, the main power storage method used will be the flywheelfor its high efficiency levels, emergency power could be distributed from areliable source based on batteries or fuel cells during times of duress.
Curator: Al Globus If you find any errors on this page contact Al Globus. |
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