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Monday, July 2, 2018

Faulty Studies Mean Everything You Know About Nutrition Is Wrong


Pizza is healthy. At least that’s what I was told in kindergarten. After all, it has all the major food groups, which (at the time) included a big ol’ pyramid base of bread. I (and the other six-year-olds, I imagine) took that nutrition advice to heart well into adulthood. Being an adult means you can have pizza anytime you want.

Before you scoff at my poorly-informed nutritional choices, you should probably recognize that you have a fair amount of food misinformation swimming around your own head. Do you buy low-fat cheese and skim milk, count calories, go on juice cleanses — all because you think science says you should? 

Well, science has told you some lies over the years.

If the science surrounding nutrition and diet seems, well, confusing and awful, that’s because it usually is. Think about it. One day saturated fat is bad, then it’s fine? Fat was once the devil, but now it’s sugar? Wine both cures and prevents cancer?

In recent weeks, the science supporting many of our ideas of what makes up a healthy diet came under fire and fell apart. Nutrition research is rife with weak methodology, human error, and the biases of the scientists behind them. For instance, a major study that set out to see if alcohol consumption came with health benefits was cancelled after accepting tens of millions of dollars from the alcohol industry and hinting at favorable results.

Yes, articles about each incremental study are part of the problem. But the problem goes much deeper — the conclusions of the studies themselves are contradictory.

The U.S. Food and Drug Administration’s (FDA) most recent guidelines deem eggs too high in cholesterol and fat to be considered healthy, even though government agencies still list them as components of a healthy breakfast. There were a handful of studies intended to determine whether there was any distinction between “good” or “bad” Calories, but they became moot when the researchers failed to include a control group and allowed people who wanted certain results to weigh in, according to WIRED. Now we can’t even say for sure whether ten Calories of chocolate are inherently better or worse than ten Calories of broccoli.

And earlier this month, the cornerstone study that linked the Mediterranean diet to lower heart disease rates was retracted, according to The New York Times. Even though the study, titled “Primary Prevention of Cardiovascular Disease with a Mediterranean Diet” or PREDIMED, was amended with a correction after it was initially published, its authors argue that they can still make the same health claims that they did before. Some critics, however, remain unconvinced.

All this begs the question: why is it so hard to scientifically determine whether a certain diet or food is actually good for people? Are we doomed to endure the same, confusing mess of experiments that tell us that coffee is healthy one day but causes cancer the next?

All this begs the question: why is it so hard to scientifically determine whether a certain diet or food is actually good for people?
If we want to do better, we need to figure out a better way to control all of the tiny little extraneous details that can throw off nutrition studies.

“Nutrition research is a difficult task given all the extraneous variables that need to be controlled, therefore it’s important to take into account or control for as many of these variables as possible, i.e. anything that affects our diet, sleep, living situation, time of the year, activity levels, medical history,” Kelly Pritchett, a nutrition and exercise scientist at Central Washington University and spokesperson for the Academy of Nutrition and Dietetics, told Futurism. “I see this as a ‘control the controllables’ concept,” she added, arguing that researchers need to consider and remove variability from as many aspects of a study participant’s life as possible.

Taking better care of all these little unpredictable variables that can throw off a study’s conclusion, called confounding factors in academic literature, may have saved the Mediterranean diet study. Ideally, study participants would have been randomly assigned a diet; instead, as The New York Times reported, ten percent of all the study’s participants were not. Instead, all the members of a family and sometimes even entire villages were given the same diet. These inconsistent practices were never reported in the final writeup of the study.

But, you know, randomization is hard. Can you really expect scientists to stick to true randomization, ensuring that the only differences in health outcomes among participants are truly due to whether or not someone adhered to the Mediterranean diet? What happens when neighbors complain that they got less appetizing food than other people in their village? Can you expect the researchers to tell parents that they need to cook separate meals for their children, just for the sake of better science?

Yes. Yes you can. Because the person in charge of that portion of the study decided to take the easy way and let some people (who volunteered to participate in an experiment centered around a controlled diet) have the same food, the entire project had to be overhauled. All of its findings, on which many people worldwide based their eating habits, had to be called into question, perhaps thrown out altogether.

Just because the researchers claim that the Mediterranean diet is still linked to improved heart health after throwing out the compromised data, their research isn’t any less suspect, and it certainly doesn’t mean we can’t do better in the future.

“I think we do need to question the methodology and how the results are displayed, not just this article, but every article we read,” said Pritchett.

In an ideal world, diet studies would be conducted in a sterile lab, where everything from caloric intake to exercise and sleep of each participant is under the complete control of the scientists conducting the experiment. But, of course, this isn’t so simple — nutrition research like the Mediterranean diet study takes years to tease out any health benefits or risks of a certain food. And each time you impose a new control, you take away a little bit of real-world applicability.

After all, the people who might actually apply the conclusions of that research won’t live in a lab. They’ll be out in the world, trying to balance their diets as they work, study, exercise, sleep, and play.

Even providing food for participants instead of leaving them to plan out their meals could take away some of their stress, which has long been scientifically linked to a slower metabolism and increased fat retention.

In that sense, researchers will need to find ways to match their experiments to those lifestyles to find data that might be meaningful for peoples’ lives. But that doesn’t mean they can throw best scientific practices out the window, as some did while studying the Mediterranean diet.
Image credit: Emily Cho
Fortunately, there are new efforts to formalize how nutrition studies are done. The National Institutes of Health (NIH) recently funded research teams at Indiana and Tufts Universities to come up with clinical guidelines for randomized, controlled nutrition studies, Connie Weaver, a nutrition scientist at Purdue University who serves as director of the Women’s Global Health Institute, told Futurism.

“Currently, guidelines exist for drug and device trials but not for nutrition studies. Hopefully this effort will lead to guidelines and training that will improve scientific quality of diet studies,” Weaver added.

She also speculated that perhaps researchers could establish some guidelines to salvage some of the findings of tainted studies so that the next wave of scientists doesn’t need to start from zero.

It’s not yet clear what these guidelines will look like, but they will likely mirror the best practices of other scientific fields, emphasizing the randomization and blinds that the scientific community has come to expect and value — at least to whatever extent these techniques are possible out in the field.

But in the meantime, scientists may need to keep acting as public watchdogs, watching out for faulty science (and honest mistakes). Weaver told Futurism that she attended a recent talk about the PREDIMED study at which the speaker argued that public retractions and corrections will help keep scientists honest. As long as scientists are willing to point out mistakes in public, laypeople stand a chance of staying informed about what does and doesn’t count as a healthy meal.

Until these new guidelines go into effect, much of the onus for healthy eating may fall where it always has: on individuals and their choices.

“I do think that the general public tends to focus on the headlines or the abstract rather than reading the full article itself,” says Pritchett. “I would tell the general public the same as I tell my students: read the discussion first and work your way backwards to the introduction.”

“I do think that the general public tends to focus on the headlines or the abstract rather than reading the full article itself.”
Basically, make sure to look at the actual evidence before jumping on board with any glib claims. For instance, people scrolling through Facebook or Twitter right now would likely encounter headlines saying that pasta doesn’t cause weight gain. But what’s not as easy to see? Articles that take the time to mention that the study was funded by pasta companies. Probably a good caveat to take into account before changing

Alternatively, there’s the opposite approach. Since we know longer have science to say what’s healthy or unhealthy, this intrepid reporter will be skipping the entire skim-or-whole-milk conundrum and filling his cereal bowl with bourbon. Cheers, bubs.

Extraterrestrial liquid water

From Wikipedia, the free encyclopedia
 
Warm season flows in Palikir Crater (inside Newton crater) on Mars. While there is intriguing but inconclusive evidence suggestive of extraterrestrial liquid water, it has so far eluded direct confirmation.

Extraterrestrial liquid water (from the Latin words: extra ["outside of, beyond"] and terrestris ["of or belonging to Earth"]) is water in its liquid state that naturally occurs outside Earth. It is a subject of wide interest because it is recognised as one of the key prerequisites for life as we know it and thus surmised as essential for extraterrestrial life.[1]

With oceanic water covering 71% of its surface, Earth is the only planet known to have stable bodies of liquid water on its surface,[2] and liquid water is essential to all known life forms on Earth. The presence of water on the surface of Earth is a product of its atmospheric pressure and a stable orbit in the Sun's circumstellar habitable zone, though the origin of Earth's water remains unknown.

The main methods currently used for confirmation are absorption spectroscopy and geochemistry. These techniques have proven effective for atmospheric water vapour and ice. However, using current methods of astronomical spectroscopy it is substantially more difficult to detect liquid water on terrestrial planets, especially in the case of subsurface water. Due to this, astronomers, astrobiologists and planetary scientists use habitable zone, gravitational and tidal theory, models of planetary differentiation and radiometry to determine potential for liquid water. Water observed in volcanic activity can provide more compelling indirect evidence, as can fluvial features and the presence of antifreeze agents, such as salts or ammonia.

Using such methods, many scientists infer that liquid water once covered large areas of Mars and Venus.[3][4] Water is thought to exist as liquid beneath the surface of some planetary bodies, similar to groundwater on Earth. Water vapour is sometimes considered conclusive evidence for the presence of liquid water, although atmospheric water vapour may be found to exist in many places where liquid water does not. Similar indirect evidence, however, supports the existence of liquids below the surface of several moons and dwarf planets elsewhere in the Solar System.[1] Some are speculated to be large extraterrestrial "oceans".[1] Liquid water is thought to be common in other planetary systems, despite the lack of conclusive evidence, and there is a growing list of extrasolar candidates for liquid water.

Liquid water in the Solar System

As of December 2015, the confirmed liquid water in the Solar System outside Earth is 25-50 times the volume of Earth's water (1.3 billion cubic kilometers).[5]

Mars

A cross-section of Mars underground ice is exposed at the steep slope that appears bright blue in this enhanced-color view from the MRO.[6] The scene is about 500 meters wide. The scarp drops about 128 meters from the level ground in the upper third of the image

Water on Mars exists today almost exclusively as ice, with a small amount present in the atmosphere as vapour. Some liquid water may occur transiently on the Martian surface today but only under certain conditions.[7] No large standing bodies of liquid water exist because the atmospheric pressure at the surface averages just 600 pascals (0.087 psi)—about 0.6% of Earth's mean sea level pressure—and because the global average temperature is far too low (210 K (−63 °C)), leading to either rapid evaporation or freezing. Features called recurring slope lineae are thought to be caused by flows of brine — hydrated salts.[8][9][10]

Europa

Scientists' consensus is that a layer of liquid water exists beneath Europa's (moon of Jupiter) surface, and that heat from tidal flexing allows the subsurface ocean to remain liquid.[11] It is estimated that the outer crust of solid ice is approximately 10–30 km (6–19 mi) thick, including a ductile "warm ice" layer, which could mean that the liquid ocean underneath may be about 100 km (60 mi) deep.[12] This leads to a volume of Europa's oceans of 3 × 1018 m3, slightly more than two times the volume of Earth's oceans.

Enceladus

Enceladus, a moon of Saturn, has shown geysers of water, confirmed by the Cassini spacecraft in 2005 and analyzed more deeply in 2008. Gravimetric data in 2010-2011 confirmed a subsurface ocean. While previously believed to be localized, most likely in a portion of the southern hemisphere, evidence revealed in 2015 now suggests the subsurface ocean is global in nature.[13]

In addition to water, these geysers from vents near the south pole contained small amounts of salt, nitrogen, carbon dioxide, and volatile hydrocarbons. The melting of the ocean water and the geysers appear to be driven by tidal flux from Saturn.

Ganymede

A subsurface saline ocean is theorized to exist on Ganymede, a moon of Jupiter, following observation by the Hubble Space Telescope in 2015. Patterns in auroral belts and rocking of the magnetic field suggest the presence of an ocean. It is estimated to be 100 km deep with the surface lying below a crust of 150 km of ice.[14]

Ceres

Ceres appears to be differentiated into a rocky core and icy mantle, and may have a remnant internal ocean of liquid water under the layer of ice.[15][16][17][18] The surface is probably a mixture of water ice and various hydrated minerals such as carbonates and clay. In January 2014, emissions of water vapor were detected from several regions of Ceres.[19] This was unexpected, because large bodies in the asteroid belt do not typically emit vapor, a hallmark of comets. Ceres also features a mountain called Ahuna Mons that is thought to be a cryovolcanic dome that facilitates the movement of high viscosity cryovolcanic magma consisting of water ice softened by its content of salts.[20][21]

Ice giants

The "ice giant" (sometimes known as "water giant") planets Uranus and Neptune are thought to have a supercritical water ocean beneath their clouds, which accounts for about two-thirds of their total mass,[22][23] most likely surrounding small rocky cores. This kind of planet is thought to be common in extrasolar planetary systems.

Indicators, methods of detection and confirmation

Most known extrasolar planetary systems appear to have very different compositions to the Solar System, though there is probably sample bias arising from the detection methods.

Spectroscopy

Absorption spectrum of liquid water
 
Liquid water has not been detected in spectroscopic analysis of suspected seasonal Martian flows.
 
Liquid water has a distinct absorption spectroscopy signature compared to other states of water due to the state of its hydrogen bonds. Despite the confirmation of extraterrestrial water vapor and ice, however, the spectral signature of liquid water is yet to be confirmed outside of Earth. The signatures of surface water on terrestrial planets may be undetectable through thick atmospheres across the vast distances of space using current technology.

Seasonal flows on warm Martian slopes, though strongly suggestive of briny liquid water, have yet to indicate this in spectroscopic analysis.

Water vapor has been confirmed in numerous objects via spectroscopy, though it does not by itself confirm the presence of liquid water. However, when combined with other observations, the possibility might be inferred. For example, the density of GJ 1214 b would suggest that a large fraction of its mass is water and follow-up detection by the Hubble telescope of the presence if water vapor strongly suggests that exotic materials like 'hot ice' or 'superfluid water' may be present.[24][25]

Magnetic fields

For the Jovian moons Ganymede and Europa, the existence of a sub-ice ocean is inferred from the measurements of the magnetic field of Jupiter.[26][27] Since conductors moving through a magnetic field produce a counter-electromotive field, the presence of the water below the surface was deduced from the change in magnetic field as the moon passed from the northern to southern magnetic hemisphere of Jupiter.

Geological indicators

Thomas Gold has posited that many Solar System bodies could potentially hold groundwater below the surface.[28]
It is thought that liquid water may exist in the Martian subsurface. Research suggests that in the past there was liquid water flowing on the surface,[29] creating large areas similar to Earth's oceans. However, the question remains as to where the water has gone.[30] There are a number[31] of direct and indirect proofs of water's presence either on or under the surface, e.g. stream beds, polar caps, spectroscopic measurement, eroded craters or minerals directly connected to the existence of liquid water (such as Goethite). In an article in the Journal of Geophysical Research, scientists studied Lake Vostok in Antarctica and discovered that it may have implications for liquid water still being on Mars. Through their research, scientists came to the conclusion that if Lake Vostok existed before the perennial glaciation began, that it is likely that the lake did not freeze all the way to the bottom. Due to this hypothesis, scientists say that if water had existed before the polar ice caps on Mars, it is likely that there is still liquid water below the ice caps that may even contain evidence of life.[32]

"Chaos terrain", a common feature on Europa's surface, is interpreted by some[who?] as regions where the subsurface ocean has melted through the icy crust.[citation needed]

Volcanic observation

A possible mechanism for cryovolcanism on bodies like Enceladus

Geysers have been found on Enceladus, a moon of Saturn, and Europa, moon of Jupiter.[33] These contain water vapour and could be indicators of liquid water deeper down.[34] It could also be just ice.[35] In June 2009, evidence[clarification needed] was put forward for salty subterranean oceans on Enceladus.[36] On April 3, 2014, NASA reported that evidence[clarification needed] for a large underground ocean of liquid water on Enceladus, moon of planet Saturn, had been found by the Cassini spacecraft. According to the scientists, evidence of an underground ocean suggests that[how?] Enceladus is one of the most likely places in the solar system to "host microbial life".[37][38] Emissions of water vapor have been detected from several regions of the dwarf planet Ceres.[39] combined with evidence of ongoing cryovalcanic activity.[40]

Gravitational evidence

Scientists' consensus is that a layer of liquid water exists beneath Europa's surface, and that heat energy from tidal flexing allows the subsurface ocean to remain liquid.[41][42] The first hints of a subsurface ocean came from theoretical considerations of tidal heating (a consequence of Europa's slightly eccentric orbit and orbital resonance with the other Galilean moons).

Scientists used gravitational measurements from the Cassini spacecraft to confirm a water ocean under the crust of Enceladus. [37][38] Such tidal models have been used as theories for water layers in other Solar System moons. According to at least one gravitational study on Cassini data, Dione has an ocean 100 kilometers below the surface.[43]

Density calculation

Artists conception of the subsurface water ocean confirmed on Enceladus in 2014 as calculated using gravitational measurements and density estimations.[37][38]

Planetary scientists can use calculations of density to determine the composition of planets and their potential to possess liquid water, though the method is not highly accurate as the combination of many compounds and states can produce similar densities.

Scientists used low frequency radio signal from the Cassini probe to detect the existence of a layer of liquid water and ammonia beneath the surface of Saturn's moon Titan that are consistent with calculations of the moon's density.[44][45]

Initial analysis of 55 Cancri e's low density indicated that it consisted 30% supercritical fluid which Diana Valencia of the Massachusetts Institute of Technology proposed could be in the form of salty supercritical water,[46] though follow-up analysis of its transit failed to detect traces of either water or hydrogen.[47]

GJ 1214 b was the second exoplanet (after CoRoT-7b) to have an established mass and radius less than those of the giant Solar System planets. It is three times the size of Earth and about 6.5 times as massive. Its low density indicated that it is likely a mix of rock and water,[48] and follow-up observations using the Hubble telescope now seem to confirm that a large fraction of its mass is water, so it is a large waterworld. The high temperatures and pressures would form exotic materials like 'hot ice' or 'superfluid water'.[24][25]

Models of radioactive decay

Models of heat retention and heating via radioactive decay in smaller icy Solar System bodies suggest that Rhea, Titania, Oberon, Triton, Pluto, Eris, Sedna, and Orcus may have oceans underneath solid icy crusts approximately 100 km thick.[49] Of particular interest in these cases is the fact that the models indicate that the liquid layers are in direct contact with the rocky core, which allows efficient mixing of minerals and salts into the water. This is in contrast with the oceans that may be inside larger icy satellites like Ganymede, Callisto, or Titan, where layers of high-pressure phases of ice are thought to underlie the liquid water layer.[49]

Models of radioactive decay suggest that MOA-2007-BLG-192Lb, a small planet orbiting a small star could be as warm as the Earth and completely covered by a very deep ocean.[50]

Internal differentiation models

Diagram showing a possible internal structure of Ceres
 
Two models for the composition of Europa suggest a large subsurface ocean of liquid water. Similar models have been proposed for other celestial bodies in the Solar System

Models of Solar System objects indicate the presence of liquid water in their internal differentiation.
Some models of the dwarf planet Ceres, largest object in the asteroid belt indicate the possibility of a wet interior layer. Water vapor detected to be emitted by the dwarf planet[51][52] may be an indicator, through sublimation of surface ice.

A global layer of liquid water thick enough to decouple the crust from the mantle is thought to be present on Titan, Europa and, with less certainty, Callisto, Ganymede[49] and Triton.[53][54] Other icy moons may also have internal oceans, or have once had internal oceans that have now frozen.[49]

Habitable zone

Artist's impression of a class II planet with water vapor clouds, as seen from a hypothetical large moon with surface liquid water

A planet's orbit in the circumstellar habitable zone is a popular method used to predict its potential for surface water at its surface. Habitable zone theory has put forward several extrasolar candidates for liquid water, though they are highly speculative as a planet's orbit around a star alone does not guarantee that a planet it has liquid water. In addition to its orbit, a planetary mass object must have the potential for sufficient atmospheric pressure to support liquid water and a sufficient supply of hydrogen and oxygen at or near its surface.

The Gliese 581 planetary system contains multiple planets that may be candidates for surface water, including Gliese 581c,[55] Gliese 581d, might be warm enough for oceans if a greenhouse effect was operating,[56] and Gliese 581e.[57]

Gliese 667 C has three of them are in the habitable zone[58] including Gliese 667 Cc is estimated to have surface temperatures similar to Earth and a strong chance of liquid water.[59]

Kepler-22b one of the first 54 candidates found by the Kepler telescope and reported is 2.4 times the size of the Earth, with an estimated temperature of 22 °C. It is described as having the potential for surface water, though its composition is currently unknown.[60]

Among the 1,235 possible extrasolar planet candidates detected by NASA's planet-hunting Kepler space telescope during its first four months of operation, 54 are orbiting in the parent star's habitable 'Goldilocks' zone where liquid water could exist.[61] Five of these are near Earth-size.[62]

On 6 January 2015, NASA announced further observations conducted from May 2009 to April 2013 which included eight candidates between one and two times the size of Earth, orbiting in a habitable zone. Of these eight, six orbit stars that are similar to the Sun in size and temperature. Three of the newly confirmed exoplanets were found to orbit within habitable zones of stars similar to the Sun: two of the three, Kepler-438b and Kepler-442b, are near-Earth-size and likely rocky; the third, Kepler-440b, is a super-Earth.[63]

Water rich circumstellar disks

File:Artist impression of the protoplanetary disc surrounding the young star MWC 480.webmPlay media

Artist impression of the protoplanetary disc surrounding MWC 480 which contains large quantities of water and organic molecules - building blocks of life.

Long before the discovery of water on asteroids on comets and dwarf planets beyond Neptune, the Solar System's circumstellar disks, beyond the snow line, including the asteroid belt and the Kuiper Belt were thought to contain large amounts of water and these were believed to be the Origin of water on Earth.[citation needed] Given that many types of stars are thought to blow volatiles from the system through the photoevaporation effect, water content in circumstellar disks and rocky material in other planetary systems are very good indicators of a planetary system's potential for liquid water and a potential for organic chemistry, especially if detected within the planet forming regions or the habitable zone. Techniques such as interferometry can be used for this.

In 2007, such a disk was found in the habitable zone of MWC 480.[64] In 2008, such a disk was found around the star AA Tauri.[65] In 2009, a similar disk was discovered around the young star HD 142527.[66]

In 2013, a water-rich debris disk around GD 61 accompanied by a confirmed rocky object consisting of magnesium, silicon, iron, and oxygen.[67][68] The same year, another water rich disk was spotted around HD 100546 has ices close to the star.[69]

There is, of course, no guarantee that the other conditions will be found that allow liquid water to be present on a planetary surface. Should planetary mass objects be present, a single, gas giant planet, with or without planetary mass moons, orbiting close to the circumstellar habitable zone, could prevent the necessary conditions from occurring in the system. However, it would mean that planetary mass objects, such as the icy bodies of the solar system, could have abundant quantities of liquid within them.

History

Lunar maria are vast basaltic plains on the Moon that were thought to be bodies of water by early astronomers, who referred to them as "seas". Galileo expressed some doubt about the lunar 'seas' in his Dialogue Concerning the Two Chief World Systems.[a]

Before space probes were landed, the idea of oceans on Venus was credible science, but the planet was discovered to be much too hot.

Telescopic observations from the time of Galileo onward have shown that Mars has no features resembling watery oceans.[citation needed] Mars' dryness was long recognized, and gave credibility to the spurious Martian canals.

Ancient water on Venus

NASA's Goddard Institute for Space Studies and others have postulated that Venus may have had a shallow ocean in the past for up to 2 billion years,[70][71][72][73][74] with as much water as Earth.[75] Depending on the parameters used in their theoretical model, the last liquid water could have evaporated as recently as 715 million years ago.[72] Currently, the only known water on Venus is in the form of a tiny amount of atmospheric vapor (20 ppm).[76][77] Hydrogen, a component of water, is still being lost to space nowadays as detected by ESA's Venus Express spacecraft.[75]

Evidence of past surface water

An artist's impression of ancient Mars and its hypothesized oceans based on geological data

Assuming that the Giant impact hypothesis is correct, there were never real seas or oceans on the Moon, only perhaps a little moisture (liquid or ice) in some places, when the Moon had a thin atmosphere created by degassing of volcanoes or impacts of icy bodies.

The Dawn space probe found possible evidence of past water flow on the asteroid Vesta,[78] leading to speculation of underground reservoirs of water-ice.[79]

Astronomers speculate that Venus had liquid water and perhaps oceans in its very early history.[80] Given that Venus has been completely resurfaced by its own active geology, the idea of a primeval ocean is hard to test. Rock samples may one day give the answer.[81]

It was once thought that Mars might have dried up from something more Earth-like. The initial discovery of a cratered surface made this seem unlikely, but further evidence has changed this view. Liquid water may have existed on the surface of Mars in the distant past, and several basins on Mars have been proposed as dry sea beds.[3] The largest is Vastitas Borealis; others include Hellas Planitia and Argyre Planitia.

There is currently much debate over whether Mars once had an ocean of water in its northern hemisphere, and over what happened to it if it did. Recent findings by the Mars Exploration Rover mission indicate it had some long-term standing water in at least one location, but its extent is not known. The Opportunity Mars rover photographed bright veins of a mineral leading to conclusive confirmation of deposition by liquid water.[82]

On December 9, 2013, NASA reported that the planet Mars had a large freshwater lake (which could have been a hospitable environment for microbial life) based on evidence from the Curiosity rover studying Aeolis Palus near Mount Sharp in Gale Crater.[83][84]

Liquid water on comets and asteroids

Comets contain large proportions of water ice, but are generally thought to be completely frozen due to their small size and large distance from the Sun. However, studies on dust collected from comet Wild-2 show evidence for liquid water inside the comet at some point in the past.[85] It is yet unclear what source of heat may have caused melting of some of the comet's water ice.

Nevertheless, on 10 December 2014, scientists reported that the composition of water vapor from comet Churyumov–Gerasimenko, as determined by the Rosetta spacecraft, is substantially different from that found on Earth. That is, the ratio of deuterium to hydrogen in the water from the comet was determined to be three times that found for terrestrial water. This makes it very unlikely that water found on Earth came from comets such as comet Churyumov–Gerasimenko according to the scientists.[86][87]

The asteroid 24 Themis was the first found to have water, including liquid pressurised by non-atmospheric means, dissolved into mineral through ionising radiation. Water has also been found to flow on the large asteroid 4 Vesta heated through periodic impacts.[88]

Extrasolar habitable zone candidates for water

Most known extrasolar planetary systems appear to have very different compositions to the Solar System, though there is probably sample bias arising from the detection methods.
The goal of current searches is to find Earth-sized planets in the habitable zone of their planetary systems (also sometimes called the Goldilocks zone).[89] Planets with oceans could include Earth-sized moons of giant planets, though it remains speculative whether such 'moons' really exist. The Kepler telescope might be sensitive enough to detect them.[90] There is speculation that rocky planets hosting water may be commonplace throughout the Milky Way.[91]

Space colonization

From Wikipedia, the free encyclopedia

Artist's conception of a colony on the Moon

Artist's conception of the interior of a Bernal sphere
Space colonization (also called space settlement, or extraterrestrial colonization) is permanent human habitation off the planet Earth.

This article is mainly about colonies on bodies apart from Earth. For free space colonies in micro-g see space habitat.

Many arguments have been made for and against space colonization.[1] The two most common in favor of colonization are survival of human civilization and the biosphere in the event of a planetary-scale disaster (natural or man-made), and the availability of additional resources in space that could enable expansion of human society. The most common objections to colonization include concerns that the commodification of the cosmos may be likely to enhance the interests of the already powerful, including major economic and military institutions, and to exacerbate pre-existing detrimental processes such as wars, economic inequality, and environmental degradation.[2][3][4]

No space colonies have been built so far. Currently, the building of a space colony would present a set of huge technological and economic challenges. Space settlements would have to provide for nearly all (or all) the material needs of hundreds or thousands of humans, in an environment out in space that is very hostile to human life. They would involve technologies, such as controlled ecological life support systems, that have yet to be developed in any meaningful way. They would also have to deal with the as-yet unknown issue of how humans would behave and thrive in such places long-term. Because of the present cost of sending anything from the surface of the Earth into orbit (around $2,500 per-pound to orbit, expected to further decrease),[5] a space colony would currently be a massively expensive project.

There are yet no plans for building space colonies by any large-scale organization, either government or private. However, many proposals, speculations, and designs for space settlements have been made through the years, and a considerable number of space colonization advocates and groups are active. Several famous scientists, such as Freeman Dyson, have come out in favor of space settlement.[6]

On the technological front, there is ongoing progress in making access to space cheaper (reusable launch systems could reach $10 per-pound to orbit),[7] and in creating automated manufacturing and construction techniques.[8]

Reasons

Survival of human civilization

The primary argument calling for space colonization is the long-term survival of human civilization. By developing alternative locations off Earth, the planet's species, including humans, could live on in the event of natural or man-made disasters on our own planet.

On two occasions, theoretical physicist and cosmologist Stephen Hawking has argued for space colonization as a means of saving humanity. In 2001, Hawking predicted that the human race would become extinct within the next thousand years, unless colonies could be established in space.[9] In 2006, he stated that humanity faces two options: either we colonize space within the next two hundred years and build residential units on other planets, or we will face the prospect of long-term extinction.[10]

In 2005, then NASA Administrator Michael Griffin identified space colonization as the ultimate goal of current spaceflight programs, saying:
... the goal isn't just scientific exploration ... it's also about extending the range of human habitat out from Earth into the solar system as we go forward in time ... In the long run a single-planet species will not survive ... If we humans want to survive for hundreds of thousands or millions of years, we must ultimately populate other planets. Now, today the technology is such that this is barely conceivable. We're in the infancy of it. ... I'm talking about that one day, I don't know when that day is, but there will be more human beings who live off the Earth than on it. We may well have people living on the Moon. We may have people living on the moons of Jupiter and other planets. We may have people making habitats on asteroids ... I know that humans will colonize the solar system and one day go beyond.[11]
Louis J. Halle, formerly of the United States Department of State, wrote in Foreign Affairs (Summer 1980) that the colonization of space will protect humanity in the event of global nuclear warfare.[12] The physicist Paul Davies also supports the view that if a planetary catastrophe threatens the survival of the human species on Earth, a self-sufficient colony could "reverse-colonize" Earth and restore human civilization. The author and journalist William E. Burrows and the biochemist Robert Shapiro proposed a private project, the Alliance to Rescue Civilization, with the goal of establishing an off-Earth "backup" of human civilization.[13]

Based on his Copernican principle, J. Richard Gott has estimated that the human race could survive for another 7.8 million years, but it is not likely to ever colonize other planets. However, he expressed a hope to be proven wrong, because "colonizing other worlds is our best chance to hedge our bets and improve the survival prospects of our species".[14]

Vast resources in space

Resources in space, both in materials and energy, are enormous. The Solar System alone has, according to different estimates, enough material and energy to support anywhere from several thousand to over a billion times that of the current Earth-based human population.[15][16][17] Outside the Solar System, several hundred billion other stars in the observable universe provide opportunities for both colonization and resource collection, though travel to any of them is impossible on any practical time-scale without interstellar travel by use of generation ships or revolutionary new methods of travel, such as faster-than-light (FTL).

Asteroid mining will also be a key player in space colonization. Water and materials to make structures and shielding can be easily found in asteroids. Instead of resupplying on Earth, mining and fuel stations need to be established on asteroids to facilitate better space travel.[18] Optical mining is the term NASA uses to describe extracting materials from asteroids. NASA believes by using propellant derived from asteroids for exploration to the moon, Mars, and beyond will save $100 billion. If funding and technology come sooner than estimated, asteroid mining might be possible within a decade.[19]

All these planets and other bodies offer a virtually endless supply of resources providing limitless growth potential. Harnessing these resources can lead to much economic development.[20]

Expansion with fewer negative consequences

Expansion of humans and technological progress has usually resulted in some form of environmental devastation, and destruction of ecosystems and their accompanying wildlife. In the past, expansion has often come at the expense of displacing many indigenous peoples, the resulting treatment of these peoples ranging anywhere from encroachment to genocide. Because space has no known life, this need not be a consequence, as some space settlement advocates have pointed out.[21][22]

Alleviating overpopulation and resource demand

Another argument for space colonization is to mitigate the negative effects of overpopulation.[clarification needed] If the resources of space were opened to use and viable life-supporting habitats were built, Earth would no longer define the limitations of growth. Although many of Earth's resources are non-renewable, off-planet colonies could satisfy the majority of the planet's resource requirements. With the availability of extraterrestrial resources, demand on terrestrial ones would decline.[23]

Other arguments

Additional goals cite the innate human drive to explore and discover, a quality recognized at the core of progress and thriving civilizations.[24][25]

Nick Bostrom has argued that from a utilitarian perspective, space colonization should be a chief goal as it would enable a very large population to live for a very long period of time (possibly billions of years), which would produce an enormous amount of utility (or happiness).[26] He claims that it is more important to reduce existential risks to increase the probability of eventual colonization than to accelerate technological development so that space colonization could happen sooner. In his paper, he assumes that the created lives will have positive ethical value despite the problem of suffering.
In a 2001 interview with Freeman Dyson, J. Richard Gott and Sid Goldstein, they were asked for reasons why some humans should live in space.[6] Their answers were:

Goals

Although some items of the infrastructure requirements above can already be easily produced on Earth and would therefore not be very valuable as trade items (oxygen, water, base metal ores, silicates, etc.), other high value items are more abundant, more easily produced, of higher quality, or can only be produced in space. These would provide (over the long-term) a very high return on the initial investment in space infrastructure.[27]

Some of these high-value trade goods include precious metals,[28][29] gemstones,[30] power,[31] solar cells,[32] ball bearings,[32] semi-conductors,[32] and pharmaceuticals.[32]

The mining and extraction of metals from a small asteroid the size of 3554 Amun or (6178) 1986 DA, both small near-Earth asteroids, would be 30 times as much metal as humans have mined throughout history. A metal asteroid this size would be worth approximately US$20 trillion at 2001 market prices.

Space colonization is seen as a long-term goal of some national space programs. Since the advent of the 21st-century commercialization of space, which saw greater cooperation between NASA and the private sector, several private companies have announced plans toward the colonization of Mars. Among entrepreneurs leading the call for space colonization are Elon Musk, Dennis Tito and Bas Lansdorp.[33][34][35]

The main impediments to commercial exploitation of these resources are the very high cost of initial investment,[36] the very long period required for the expected return on those investments (The Eros Project plans a 50-year development),[37] and the fact that the venture has never been carried out before — the high-risk nature of the investment.

Major governments and well-funded corporations have announced plans for new categories of activities: space tourism and hotels, prototype space-based solar-power satellites, heavy-lift boosters and asteroid mining—that create needs and capabilities for humans to be present in space.[38][39][40]

Method

Building colonies in space would require access to water, food, space, people, construction materials, energy, transportation, communications, life support, simulated gravity, radiation protection and capital investment. It is likely the colonies would be located near the necessary physical resources. The practice of space architecture seeks to transform spaceflight from a heroic test of human endurance to a normality within the bounds of comfortable experience. As is true of other frontier-opening endeavors, the capital investment necessary for space colonization would probably come from governments,[41] an argument made by John Hickman[42] and Neil deGrasse Tyson.[43]

Materials

Colonies on the Moon, Mars, or asteroids could extract local materials. The Moon is deficient in volatiles such as argon, helium and compounds of carbon, hydrogen and nitrogen. The LCROSS impacter was targeted at the Cabeus crater which was chosen as having a high concentration of water for the Moon. A plume of material erupted in which some water was detected. Mission chief scientist Anthony Colaprete estimated that the Cabeus crater contains material with 1% water or possibly more.[44] Water ice should also be in other permanently shadowed craters near the lunar poles. Although helium is present only in low concentrations on the Moon, where it is deposited into regolith by the solar wind, an estimated million tons of He-3 exists over all.[45] It also has industrially significant oxygen, silicon, and metals such as iron, aluminum, and titanium.

Launching materials from Earth is expensive, so bulk materials for colonies could come from the Moon, a near-Earth object (NEO), Phobos, or Deimos. The benefits of using such sources include: a lower gravitational force, no atmospheric drag on cargo vessels, and no biosphere to damage. Many NEOs contain substantial amounts of metals. Underneath a drier outer crust (much like oil shale), some other NEOs are inactive comets which include billions of tons of water ice and kerogen hydrocarbons, as well as some nitrogen compounds.[46]

Farther out, Jupiter's Trojan asteroids are thought to be rich in water ice and other volatiles.[47]

Recycling of some raw materials would almost certainly be necessary.

Energy

Solar energy in orbit is abundant, reliable, and is commonly used to power satellites today. There is no night in free space, and no clouds or atmosphere to block sunlight. Light intensity obeys an inverse-square law. So the solar energy available at distance d from the Sun is E = 1367/d2 W/m2, where d is measured in astronomical units (AU) and 1367 watts/m2 is the energy available at the distance of Earth's orbit from the Sun, 1 AU.[48]

In the weightlessness and vacuum of space, high temperatures for industrial processes can easily be achieved in solar ovens with huge parabolic reflectors made of metallic foil with very lightweight support structures. Flat mirrors to reflect sunlight around radiation shields into living areas (to avoid line-of-sight access for cosmic rays, or to make the Sun's image appear to move across their "sky") or onto crops are even lighter and easier to build.

Large solar power photovoltaic cell arrays or thermal power plants would be needed to meet the electrical power needs of the settlers' use. In developed parts of Earth, electrical consumption can average 1 kilowatt/person (or roughly 10 megawatt-hours per person per year.)[49] These power plants could be at a short distance from the main structures if wires are used to transmit the power, or much farther away with wireless power transmission.

A major export of the initial space settlement designs was anticipated to be large solar power satellites that would use wireless power transmission (phase-locked microwave beams or lasers emitting wavelengths that special solar cells convert with high efficiency) to send power to locations on Earth, or to colonies on the Moon or other locations in space. For locations on Earth, this method of getting power is extremely benign, with zero emissions and far less ground area required per watt than for conventional solar panels. Once these satellites are primarily built from lunar or asteroid-derived materials, the price of SPS electricity could be lower than energy from fossil fuel or nuclear energy; replacing these would have significant benefits such as the elimination of greenhouse gases and nuclear waste from electricity generation.

Transmitting solar energy wirelessly from the Earth to the Moon and back is also an idea proposed for the benefit of space colonization and energy resources. Physicist Dr. David Criswell, who worked for NASA during the Apollo missions, came up with the idea of using power beams to transfer energy from space. These beams, microwaves with a wavelength of about 12 cm, will be almost untouched as they travel through the atmosphere. They can also be aimed at more industrial areas to keep away from humans or animal activities.[50] This will allow for safer and more reliable methods of transferring solar energy.

In 2008, scientists were able to send a 20 watt microwave signal from a mountain in Maui to the island of Hawaii. Since then JAXA and Mitsubishi has teamed up on a $21 billion project in order to place satellites in orbit which could generate up to 1 gigawatt of energy.[51] These are the next advancements being done today in order to make energy be transmitted wirelessly for space-based solar energy.

However, the value of SPS power delivered wirelessly to other locations in space will typically be far higher than to Earth. Otherwise, the means of generating the power would need to be included with these projects and pay the heavy penalty of Earth launch costs. Therefore, other than proposed demonstration projects for power delivered to Earth,[39] the first priority for SPS electricity is likely to be locations in space, such as communications satellites, fuel depots or "orbital tugboat" boosters transferring cargo and passengers between low-Earth orbit (LEO) and other orbits such as geosynchronous orbit (GEO), lunar orbit or highly-eccentric Earth orbit (HEEO).[52]:132 The system will also rely on satellites and receiving stations on Earth to convert the energy into electricity. Because of this energy can be transmitted easily from dayside to nightside meaning power is reliable 24/7.[53]

Nuclear power is sometimes proposed for colonies located on the Moon or on Mars, as the supply of solar energy is too discontinuous in these locations; the Moon has nights of two Earth weeks in duration. Mars has nights, relatively high gravity, and an atmosphere featuring large dust storms to cover and degrade solar panels. Also, Mars' greater distance from the Sun (1.5 astronomical units, AU) translates into E/(1.52 = 2.25) only ½-⅔ the solar energy of Earth orbit.[54] Another method would be transmitting energy wirelessly to the lunar or Martian colonies from solar power satellites (SPSs) as described above; the difficulties of generating power in these locations make the relative advantages of SPSs much greater there than for power beamed to locations on Earth. In order to also be able to fulfill the requirements of a moon base and energy to supply life support, maintenance, communications, and research, a combination of both nuclear and solar energy will be used in the first colonies.[50]

For both solar thermal and nuclear power generation in airless environments, such as the Moon and space, and to a lesser extent the very thin Martian atmosphere, one of the main difficulties is dispersing the inevitable heat generated. This requires fairly large radiator areas.

Life support

In space settlements, a life support system must recycle or import all the nutrients without "crashing." The closest terrestrial analogue to space life support is possibly that of a nuclear submarine. Nuclear submarines use mechanical life support systems to support humans for months without surfacing, and this same basic technology could presumably be employed for space use. However, nuclear submarines run "open loop"—extracting oxygen from seawater, and typically dumping carbon dioxide overboard, although they recycle existing oxygen.[citation needed] Recycling of the carbon dioxide has been approached in the literature using the Sabatier process or the Bosch reaction.

Although a fully mechanistic life support system is conceivable, a closed ecological system is generally proposed for life support. The Biosphere 2 project in Arizona has shown that a complex, small, enclosed, man-made biosphere can support eight people for at least a year, although there were many problems. A year or so into the two-year mission oxygen had to be replenished, which strongly suggests that they achieved atmospheric closure.

The relationship between organisms, their habitat and the non-Earth environment can be:
A combination of the above technologies is also possible.

Radiation protection

Cosmic rays and solar flares create a lethal radiation environment in space. In Earth orbit, the Van Allen belts make living above the Earth's atmosphere difficult. To protect life, settlements must be surrounded by sufficient mass to absorb most incoming radiation, unless magnetic or plasma radiation shields were developed.[55]

Passive mass shielding of four metric tons per square meter of surface area will reduce radiation dosage to several mSv or less annually, well below the rate of some populated high natural background areas on Earth.[56] This can be leftover material (slag) from processing lunar soil and asteroids into oxygen, metals, and other useful materials. However, it represents a significant obstacle to maneuvering vessels with such massive bulk (mobile spacecraft being particularly likely to use less massive active shielding).[55] Inertia would necessitate powerful thrusters to start or stop rotation, or electric motors to spin two massive portions of a vessel in opposite senses. Shielding material can be stationary around a rotating interior.

Self-replication

Space manufacturing could enable self-replication. Some think it's the ultimate goal because it allows an exponential increase in colonies, while eliminating costs to and dependence on Earth.[57] It could be argued that the establishment of such a colony would be Earth's first act of self-replication.[58] Intermediate goals include colonies that expect only information from Earth (science, engineering, entertainment) and colonies that just require periodic supply of light weight objects, such as integrated circuits, medicines, genetic material and tools.

Psychological adjustment

The monotony and loneliness that comes from a prolonged space mission can leave astronauts susceptible to cabin fever or having a psychotic break. Moreover, lack of sleep, fatigue, and work overload can affect an astronaut's ability to perform well in an environment such as space where every action is critical.[59]

Population size

In 2002, the anthropologist John H. Moore estimated that a population of 150–180 would permit a stable society to exist for 60 to 80 generations — equivalent to 2000 years.

A much smaller initial population of as little as two women should be viable as long as human embryos are available from Earth. Use of a sperm bank from Earth also allows a smaller starting base with negligible inbreeding.

Researchers in conservation biology have tended to adopt the "50/500" rule of thumb initially advanced by Franklin and Soule. This rule says a short-term effective population size (Ne) of 50 is needed to prevent an unacceptable rate of inbreeding, whereas a long‐term Ne of 500 is required to maintain overall genetic variability. The Ne = 50 prescription corresponds to an inbreeding rate of 1% per generation, approximately half the maximum rate tolerated by domestic animal breeders. The Ne = 500 value attempts to balance the rate of gain in genetic variation due to mutation with the rate of loss due to genetic drift.

Assuming a journey of 6,300 years, the astrophysicist Frédéric Marin and the particle physicist Camille Beluffi calculated that the minimum viable population for a generation ship to reach Proxima Centauri would be 98 settlers.[60][61]

Location


Artist Les Bossinas' 1989 concept of Mars mission

Location is a frequent point of contention between space colonization advocates. The location of colonization can be on a physical body planet, dwarf planet, natural satellite, or asteroid or orbiting one. For colonies not on a body see also space habitat.

Near-Earth space

The Moon

Due to its proximity and familiarity, Earth's Moon is discussed as a target for colonization. It has the benefits of proximity to Earth and lower escape velocity, allowing for easier exchange of goods and services. A drawback of the Moon is its low abundance of volatiles necessary for life such as hydrogen, nitrogen, and carbon. Water-ice deposits that exist in some polar craters could serve as a source for these elements. An alternative solution is to bring hydrogen from near-Earth asteroids and combine it with oxygen extracted from lunar rock.

The Moon's low surface gravity is also a concern, as it is unknown whether 1/6g is enough to maintain human health for long periods.[citation needed]

The Moon's lack of atmosphere provides no protection from space radiation or meteoroids. The early Moon colonies may shelter in ancient Lunar lava tubes to gain protection. The two-week day/night cycle makes use of solar power more difficult.

Lagrange points


A contour plot of the gravitational potential of the Sun and Earth, showing the five Earth–Sun Lagrange points

Another near-Earth possibility are the five Earth–Moon Lagrange points. Although they would generally also take a few days to reach with current technology, many of these points would have near-continuous solar power because their distance from Earth would result in only brief and infrequent eclipses of light from the Sun. However, the fact that the Earth–Moon Lagrange points L4 and L5 tend to collect dust and debris, whereas L1-L3 require active station-keeping measures to maintain a stable position, make them somewhat less suitable places for habitation than was originally believed. Additionally, the orbit of L2L5 takes them out of the protection of the Earth's magnetosphere for approximately two-thirds of the time, exposing them to the health threat from cosmic rays.

The five Earth–Sun Lagrange points would totally eliminate eclipses, but only L1 and L2 would be reachable in a few days' time. The other three Earth–Sun points would require months to reach.

The inner planets

Mercury

Colonizing Mercury would involve similar challenges as the Moon as there are few volatile elements, no atmosphere and the surface gravity is lower than Earth's. However, the planet also receives almost seven times the solar flux as the Earth/Moon system. Geologist Stephen Gillett has suggested this will make Mercury an ideal place to build solar sails, which could launch as folded up "chunks" by mass driver from Mercury's surface. Once in space the solar sails would deploy. Since Mercury's solar constant is 6.5 times higher than Earth's, energy for the mass driver should be easy to come by, and solar sails near Mercury would have 6.5 times the thrust they do near Earth. This could make Mercury an ideal place to acquire materials useful in building hardware to send to (and terraform) Venus. Vast solar collectors could also be built on or near Mercury to produce power for large scale engineering activities such as laser-pushed lightsails to nearby star systems.[62]

Asteroid belt

Colonization of asteroids would require space habitats. The asteroid belt has significant overall material available, the largest object being Ceres, although it is thinly distributed as it covers a vast region of space. Unmanned supply craft should be practical with little technological advance, even crossing 500 million kilometers of space. The colonists would have a strong interest in assuring their asteroid did not hit Earth or any other body of significant mass, but would have extreme difficulty in moving an asteroid[citation needed] of any size. The orbits of the Earth and most asteroids are very distant from each other in terms of delta-v and the asteroidal bodies have enormous momentum. Rockets or mass drivers can perhaps be installed on asteroids to direct their path into a safe course.

Moons of outer planets

Jovian moons – Europa, Callisto and Ganymede

The Artemis Project designed a plan to colonize Europa, one of Jupiter's moons. Scientists were to inhabit igloos and drill down into the Europan ice crust, exploring any sub-surface ocean. This plan discusses possible use of "air pockets" for human habitation. Europa is considered one of the more habitable bodies in the Solar System and so merits investigation as a possible abode for life.
NASA performed a study called HOPE (Revolutionary Concepts for Human Outer Planet Exploration) regarding the future exploration of the Solar System.[63] The target chosen was Callisto due to its distance from Jupiter, and thus the planet's harmful radiation. It could be possible to build a surface base that would produce fuel for further exploration of the Solar System.

Three of the Galilean moons (Europa, Ganymede, Callisto) have an abundance of volatiles that may support colonization efforts.

Moons of Saturn – Titan, Enceladus, and others

Titan is suggested as a target for colonization,[64] because it is the only moon in the Solar System to have a dense atmosphere and is rich in carbon-bearing compounds. Titan has ice water and large methane oceans.[65] Robert Zubrin identified Titan as possessing an abundance of all the elements necessary to support life[where?], making Titan perhaps the most advantageous locale in the outer Solar System for colonization, and saying "In certain ways, Titan is the most hospitable extraterrestrial world within our solar system for human colonization".

Enceladus is a small, icy moon orbiting close to Saturn, notable for its extremely bright surface and the geyser-like plumes of ice and water vapor that erupt from its southern polar region. If Enceladus has liquid water, it joins Mars and Jupiter's moon Europa as one of the prime places in the Solar System to look for extraterrestrial life and possible future settlements.

Other large satellites: Rhea, Iapetus, Dione, Tethys, and Mimas, all have large quantities of volatiles, which can be used to support settlements.

Trans-Neptunian region

The Kuiper belt is estimated to have 70,000 bodies of 100 km or larger.

Freeman Dyson has suggested that within a few centuries human civilization will have relocated to the Kuiper belt.[66]

The Oort cloud is estimated to have up to a trillion comets.

Outside the Solar System


A star forming region in the Large Magellanic Cloud

Looking beyond the Solar System, there are up to several hundred billion potential stars with possible colonization targets. The main difficulty is the vast distances to other stars: roughly a hundred thousand times further away than the planets in the Solar System. This means that some combination of very high speed (some percentage of the speed of light), or travel times lasting centuries or millennia, would be required. These speeds are far beyond what current spacecraft propulsion systems can provide.

Many scientific papers have been published about interstellar travel. Given sufficient travel time and engineering work, both unmanned and generational voyages seem possible, though representing a very considerable technological and economic challenge unlikely to be met for some time, particularly for manned probes.[citation needed]

Space colonization technology could in principle allow human expansion at high, but sub-relativistic speeds, substantially less than the speed of light, c.  An interstellar colony ship would be similar to a space habitat, with the addition of major propulsion capabilities and independent energy generation.

Hypothetical starship concepts proposed both by scientists and in hard science fiction include:
  • A generation ship would travel much slower than light, with consequent interstellar trip times of many decades or centuries. The crew would go through generations before the journey is complete, so that none of the initial crew would be expected to survive to arrive at the destination, assuming current human lifespans.
  • A sleeper ship, in which most or all of the crew spend the journey in some form of hibernation or suspended animation, allowing some or all who undertake the journey to survive to the end.
  • An embryo-carrying interstellar starship (EIS), much smaller than a generation ship or sleeper ship, transporting human embryos or DNA in a frozen or dormant state to the destination. (Obvious biological and psychological problems in birthing, raising, and educating such voyagers, neglected here, may not be fundamental.)
  • A nuclear fusion or fission powered ship (e.g. ion drive) of some kind, achieving velocities of up to perhaps 10% c  permitting one-way trips to nearby stars with durations comparable to a human lifetime.
  • A Project Orion-ship, a nuclear-powered concept proposed by Freeman Dyson which would use nuclear explosions to propel a starship. A special case of the preceding nuclear rocket concepts, with similar potential velocity capability, but possibly easier technology.
  • Laser propulsion concepts, using some form of beaming of power from the Solar System might allow a light-sail or other ship to reach high speeds, comparable to those theoretically attainable by the fusion-powered electric rocket, above. These methods would need some means, such as supplementary nuclear propulsion, to stop at the destination, but a hybrid (light-sail for acceleration, fusion-electric for deceleration) system might be possible.
The above concepts all appear limited to high, but still sub-relativistic speeds, due to fundamental energy and reaction mass considerations, and all would entail trip times which might be enabled by space colonization technology, permitting self-contained habitats with lifetimes of decades to centuries. Yet human interstellar expansion at average speeds of even 0.1% of c  would permit settlement of the entire Galaxy in less than one half of a galactic rotation period of ~250,000,000 years, which is comparable to the timescale of other galactic processes. Thus, even if interstellar travel at near relativistic speeds is never feasible (which cannot be clearly determined at this time), the development of space colonization could allow human expansion beyond the Solar System without requiring technological advances that cannot yet be reasonably foreseen. This could greatly improve the chances for the survival of intelligent life over cosmic timescales, given the many natural and human-related hazards that have been widely noted.

If humanity does gain access to a large amount of energy, on the order of the mass-energy of entire planets, it may eventually become feasible to construct Alcubierre drives. These are one of the few methods of superluminal travel which may be possible under current physics. However it is probable that such a device could never exist, due to the fundamental challenges posed. For more on this see Difficulties of making and using an Alcubierre Drive.

Intergalactic travel

Looking beyond the Milky Way, there are at least 2 trillion other galaxies in the observable universe. The distances between galaxies are on the order of a million times farther than those between the stars. Because of the speed of light limit on how fast any material objects can travel in space, intergalactic travel would either have to involve voyages lasting millions of years,[67] or a possible faster than light propulsion method based on speculative physics, such as the Alcubierre drive. There are, however, no scientific reasons for stating that intergalactic travel is impossible in principle.

Funding

Space colonization 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 space colonization to be available given traditional launch costs,[68][full citation needed] there is some prospect of a radical reduction to launch costs in the 2010s, which would consequently lessen the cost of any efforts in that direction. With a published price of US$56.5 million per launch of up to 13,150 kg (28,990 lb) payload[69] to low Earth orbit, SpaceX Falcon 9 rockets are already the "cheapest in the industry".[70] Advancements currently being developed as part of the SpaceX reusable launch system development program to enable reusable Falcon 9s "could drop the price by an order of magnitude, sparking more space-based enterprise, which in turn would drop the cost of access to space still further through economies of scale."[70] 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.[71]

The President's Commission on Implementation of United States Space Exploration Policy suggested that an inducement prize should be established, perhaps by government, for the achievement of space colonization, for example by offering the prize to the first organization to place humans on the Moon and sustain them for a fixed period before they return to Earth.[72]

Terrestrial analogues to space colonies

The most famous attempt to build an analogue to a self-sufficient colony is Biosphere 2, which attempted to duplicate Earth's biosphere. BIOS-3 is another closed ecosystem, completed in 1972 in Krasnoyarsk, Siberia.

Many space agencies build testbeds for advanced life support systems, but these are designed for long duration human spaceflight, not permanent colonization.

Remote research stations in inhospitable climates, such as the Amundsen–Scott South Pole Station or Devon Island Mars Arctic Research Station, can also provide some practice for off-world outpost construction and operation. The Mars Desert Research Station has a habitat for similar reasons, but the surrounding climate is not strictly inhospitable.

History

The first known work on space colonization was The Brick Moon, a work of fiction published in 1869 by Edward Everett Hale, about an inhabited artificial satellite.[73]

The Russian schoolmaster and physicist Konstantin Tsiolkovsky foresaw elements of the space community in his book Beyond Planet Earth written about 1900. Tsiolkovsky had his space travelers building greenhouses and raising crops in space.[74] Tsiolkovsky believed that going into space would help perfect human beings, leading to immortality and peace.[75]

Others have also written about space colonies as Lasswitz in 1897 and Bernal, Oberth, Von Pirquet and Noordung in the 1920s. Wernher von Braun contributed his ideas in a 1952 Colliers article. In the 1950s and 1960s, Dandridge M. Cole[76] published his ideas.

Another seminal book on the subject was the book The High Frontier: Human Colonies in Space by Gerard K. O'Neill[77] in 1977 which was followed the same year by Colonies in Space by T. A. Heppenheimer.[78]

M. Dyson wrote Home on the Moon; Living on a Space Frontier in 2003;[79] Peter Eckart wrote Lunar Base Handbook in 2006[80] and then Harrison Schmitt's Return to the Moon written in 2007.[81]

As of 2013, Bigelow Aerospace is the only private commercial spaceflight company that has launched two experimental space station modules, Genesis I (2006) and Genesis II (2007),[82] into Earth-orbit, and has indicated that their first production model of the space habitat, the BA 330, could be launched by 2017.[83]

Planetary protection

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,[84][85] 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).[86] There have been several planetary workshops on this issue, but with no final guidelines for a way forward yet.[87] Human explorers would also be vulnerable to back contamination to Earth if they become carriers of microorganisms.[88]

Objections

A corollary to the Fermi paradox—"nobody else is doing it"—is the argument that, because no evidence of alien colonization technology exists, it is statistically unlikely to even be possible to use that same level of technology ourselves.

Colonizing space would require massive amounts of financial, physical, and human capital devoted to research, development, production, and deployment. Earth's natural resources do not increase to a noteworthy extent (which is in keeping with the "only one Earth" position of environmentalists). Thus, considerable efforts in colonizing places outside Earth would appear as a hazardous waste of the Earth's limited resources for an aim without a clear end.

The fundamental problem of public things, needed for survival, such as space programs, is the free rider problem. Convincing the public to fund such programs would require additional self-interest arguments: If the objective of space colonization is to provide a "backup" in case everyone on Earth is killed, then why should someone on Earth pay for something that is only useful after they are dead? This assumes that space colonization is not widely acknowledged as a sufficiently valuable social goal.

Seen as a relief to the problem of overpopulation even as early as 1758,[89] and listed as one of Stephen Hawking's reasons for pursuing space exploration,[90] it has become apparent that space colonisation in response to overpopulation is unwarranted. Indeed, the birth rates of many developed countries, specifically spacefaring ones, are at or below replacement rates, thus negating the need to use colonisation as a means of population control.[89]

Other objections include concerns that the forthcoming colonization and commodification of the cosmos may be likely to enhance the interests of the already powerful, including major economic and military institutions e.g. the large financial institutions, the major aerospace companies and the military–industrial complex, to lead to new wars, and to exacerbate pre-existing exploitation of workers and resources, economic inequality, poverty, social division and marginalization, environmental degradation, and other detrimental processes or institutions.[2][3][4]

Additional concerns include creating a culture in which humans are no longer seen as human, but rather as material assets. The issues of human dignity, morality, philosophy, culture, bioethics, and the threat of megalomaniac leaders in these new "societies" would all have to be addressed in order for space colonization to meet the psychological and social needs of people living in isolated colonies.[91]

As an alternative or addendum for the future of the human race, many science fiction writers have focused on the realm of the 'inner-space', that is the computer-aided exploration of the human mind and human consciousness—possibly en route developmentally to a Matrioshka Brain.

Robotic exploration is proposed as an alternative to gain many of the same scientific advantages without the limited mission duration and high cost of life support and return transportation involved in manned missions.

Another concern is the potential to cause interplanetary contamination on planets that may harbor hypothetical extraterrestrial life.

Physical, mental and emotional health risks to colonizers

An additional concern is the health of the humans who may participate in a colonization venture, including a range of physical, mental and emotional health risks.

Involved organizations

Organizations that contribute to space colonization include:

In fiction

Although established space colonies are a stock element in science fiction stories, fictional works that explore the themes, social or practical, of the settlement and occupation of a habitable world are much rarer.

Lie group

From Wikipedia, the free encyclopedia https://en.wikipedia.org/wiki/Lie_group In mathematics , a Lie gro...