Opentopia Directory Encyclopedia Tools

Kardashev scale

Encyclopedia : K : KA : KAR : Kardashev scale


Kardashev scale projections ranging from 1900 to 2100.
Enlarge
Kardashev scale projections ranging from 1900 to 2100.

The Kardashev scale is a general method of classifying how technologically advanced a civilization is, first proposed in 1964 by the Russian astronomer Nikolai Kardashev. It has three categories, based on the amount of usable energy a civilization has at its disposal and increasing logarithmically:

All such civilizations are purely hypothetical at this point. However, the Kardashev scale is of use to SETI researchers, science fiction authors, and futurists as a theoretical framework.

Usage and examples

Human civilization is currently somewhere far below Type I, as it is able to harness only a portion of the energy that is available on Earth. The current state of human civilization has thus been named Type 0. Although intermediate values were not discussed in Kardashev's original proposal, Carl Sagan argued that they could easily be defined by interpolating and extrapolating the values given above. He calculated humanity's current civilization to be 0.7. He used a power output of ~10TW and the formula:

[K = \frac-6} ]
where K is a civilization's Kardashev rating and W is its power output in watts. Note that Roman numerals are still used for the integer part of a civilization's rating, while the fractional part is written in decimal.

A possible method by which Earth can advance to a Type I civilization is to begin the heavy use of ocean thermal energy conversion, wind turbines and tidal power to obtain the energy received by Earth's oceans from the Sun. However there is no known way to successfully utilize the full potential of Earth's energy production without complete coating of the surface with man made structures. In the near and medium future, this is an impossibility given humans' current lifestyle. We are, however, already "harnessing" Earth's production through our dependence upon ecosystem services, which may prove more efficient and sustainable than our own technology well into the future. If we choose never to fully substitute synthetics for nature's services on this planet, we may still achieve a Type I civilization by assuring that Earth's ecosystem services are maximally functional.

A hypothetical Type II civilization might employ a Dyson sphere or other similar construct in order to utilize all of the energy output by a star, or perhaps more exotic means such as feeding stellar mass into a black hole to generate usable energy. Alternatively, it may occupy a large number of solar systems, absorbing a small but significant fraction of the output of each individual star. A Type III civilization might use the same techniques employed by a Type II civilization, applied to all of the stars of one or more galaxies individually, or perhaps might use other mechanisms not yet proposed.

A common and recognisable example of a fictional civilization capable of entering a Type III level is the Galactic Empire which features in many works of space opera. These civilizations utilise energy on a massive scale, generally being in between Type II and Type III.

Possible timeline

Humanity's current history indicates a timeline roughly shown here. These values are approximate, and include future predictions, from 0.8 onwards. They use Sagan's extrapolated version of the scale.
Type 0 Development of Civilization
0.25 (3 108 W) Roman Civilization 0.5 (1011 W) Industrial Revolution 0.6 (1012 W) 1891 to 1938 technological expansion 0.7 (1013 W) c. 2000: Nuclear Weapons and Fission power 0.8 (1014 W) c. 2100: Fusion power#redirect 0.9 (1015 W) c. 2200: Space elevators, the creation of an Ecumenopolis#redirect Type 0 to Type I transition: Civilization self-destructs or achieves a Technological singularity#redirect
Trends:
[\Longrightarrow] Increasing levels of technology, Up to 0.5, increasing levels of fragmentation, increasing energy usage, increasing area of habitation
[\Longleftarrow] After 0.5, Decreasing levels of fragmentation

Function as a teleology

When transformed from a scale of energy use measurement into a predictive, or normative, description of desirable future technology the Kardashev scale becomes teleological: it predicts an "end of history". As a description of past and future human history it should be compared with the Marxist theory of modes of production which makes similar assertions about combinations of technological and social structures, albeit across a shorter time span.[[Citing sources citation needed]]

Weakness by supposition?

Energy Consumption from 1989 to 1999
Enlarge
Energy Consumption from 1989 to 1999

It has been argued that, because we cannot understand advanced civilizations, we cannot predict their behavior; thus, Kardashev's visualization may not reflect what will actually occur for an advanced civilization. This central argument is found within the book .A more controversial discussion can be found at

It is also possible that the unique conditions on Earth allow for specific technologies to develop which would take many times longer for a civilization not having these conditions to achieve. The list of presumably unique conditions on Earth, and of related discoveries, is quite long. Some examples:

It is possible that the conditions for the creation of hydrocarbons, coal, or natural gas would not exist on other planets. These fuels were essential for us to move past dependence upon wood and animal based energy systems. Although waterwheel, wind, and solar energy technologies existed, they were not developed further until suitable industrial techniques were found to produce better materials. These techniques consume massive amounts of energy, and therefore could not be powered by the unimproved technologies. A similar argument could be made that without fossil fuel technologies, more powerful technologies, such as nuclear reactors, could not develop.

Counter-argument: abundance of alternative sources

Human perception has a natural bias towards the known energy development paths of Human civilization. It must also be noted that during both the 1973 energy crisis and the 1979 energy crisis highly industrialized societies continued to function; many moved towards developing alternative energy technologies on a massive scale under the assumption that these could provide the energy needed to continue industrial and commercial processes should fossil fuel supplies be compromised in some critical way.

Given this development, it is possible that a society could develop without a stage where fossil fuel based energy production occurs. This version of Buckminster Fuller's argument on current solar income conforms with Paul Hawken's idea of restorative economy, stating that fossil fuel based energy production is not essential nor desirable given the effects and alternatives. Also, it must be noted that the principles behind the fuel cell were discovered by Christian Friedrich Schönbein in 1838, and were applied by Sir William Grove in 1843, before there was widespread usage of fossil fuels other than coal. This raises the possibility that for alien civilizations fuel cells could be used in place of hydrocarbon fuels. It was only in the 1850s that the first industrial petroleum extraction was started by Edwin Drake.

Civilization implications

Possible Kardashev Scale Expansion of Human Civilization from [The Coming Dark Age]
Enlarge
Possible Kardashev Scale Expansion of Human Civilization from [The Coming Dark Age]

There are many historical examples of civilizations undergoing large-scale transitions, such as the Industrial Revolution and the Renaissance. The transition between Kardashev scale levels could potentially represent similarly dramatic periods of social upheaval, since they entail surpassing the hard limits of the resources available in a civilization's existing territory. A common speculation suggests that the transition from Type 0 to Type I might carry a strong risk of self-destruction since there would no longer be room for further expansion on the civilization's home planet. See Malthusian catastrophe for an example of such a speculation.

Some individuals have pointed to the faster upheaval of civilization periods as indicative of an upcoming change over to Type I civilization.

Contact constraints

For pre-Type I civilizations, it is costly to attempt contact with other more advanced civilizations because of the energy output needed. It has been predicted that in order to provide a reliable contact beacon of sufficient power to be noticeable to a Type II civilization, it must output such high energy levels that the cost would be between $1 trillion to $10 trillion in energy. The latter figure is the approximate annual gross domestic product of the United States at the end of the 1990s through the beginning of the 21st Century. As a result it has been suggested that civilization must advance high into Type I before the energy required for reliable contact with other civilizations becomes sufficiently low that it does not drain a civilization's economic resources.

Once civilizations have discovered each others' locations, however, the energy requirements for maintaining contact and exchanging information can be significantly reduced through the use of highly directional transmission technologies. In 1974, the Arecibo Observatory transmitted a message toward the M13 globular cluster about 25,000 light-years away, for example, and the use of larger antennae or shorter wavelengths would allow transmissions of the same energy to be focused on even more remote targets. See SETI for extensive discussion of these possibilities.

Hypothetical extensions

The exponential structure of the scale allows ready extrapolation to higher types. For example:

Fictional extensions

These extensions are mainly used in science fiction. They are not "official" and may differ from source to source. For example, some authors would class a "Type V" civilization as Type IV instead. Further examples of extensions of the scale follow:

Hypothetical futures

Science fiction, having extended these values has also provided guides for possible future changes associated with the fractionalized version of the Kardashev scale. One possible future is presented here. The majority of the assumptions presented here are derived from scientific literature. Nikolai Kardashev's article On the Inevitability and the Possible Structures of Supercivilizations, (connection timed out as of last access date) where he explains that with increasing energy levels come increasing technology, decreasing cohesiveness, and varying likelihood of survival and contact, largely is a guide to this section. These civilizations and the changes within them are also referenced in Kardashev's papers Cosmology and Civilization (connection timed out as of last access date) and Transmission of Information by Extraterrestrial Civilizations. (connection timed out as of last access date) The last framework for these explanations can be found at ENERGY AND CULTURE. (connection timed out as of last access date) This article provides a much more detailed explanation than that which exists here. It presents a theoretical way to describe trends within more advanced civilizations, along with a specific description of different civilization types. This section takes the article as a guide work, but not as a source, for any such derivation would be plagiarization of the specific descriptions of the different types of civilizations.

Type I

Kaku quotes Dyson as calculating that Earth will achieve a Type I civilization around the year 2200. This estimate is based on a simple extrapolation of the current development rate of Earth's energy budget.

Type I Single Planetary Civilization
Early (1016 W to 1019 W) Middle (1020 W to 1023 W) Late (1024 W to 1026 W) (debatable)
near space colonization, near space industry, Asteroid mining, Planet Mining for fuels and energy First Interstellar travel Stress caused by size of civilization, at this point it can fragment into multiple planetary civilizations—reversion from single civilization early in type 1. Construction begins on a Dyson Sphere, Alderson disk, or Ringworld.
Trends:
[\Longrightarrow] Increasing levels of technology, Increasing levels of space exploration, space based energy sources increase, offworld civilization centers increase, increasing energy usage, increasing area of habitation
[\Longleftarrow] Decreasing levels of centrality, societies and civilizations increasingly are not the same, due to time differences breaking single social bonds [1]

Type II

According to Kaku, Kardaschev has estimated the development of such a civilization at the year 5200.
Type II Civilization has extended to the entire Solar System
Early (1026 W to 1029 W) Middle (1030 W to 1033 W) (debatable) Late (1034 W to 1036 W) (debatable)
Dyson Sphere completion, Exploration and colonization of nearby star systems. star lifting and Shkadov thrusters, Stress caused by size of civilization, at this point it can fragment into multiple solar system based civilizations—reversion to single star based civilization early, Automated galactic or intergalactic colonization effort may begin
Trends:
[\Longrightarrow] Increasing levels of technology, Exponential growth in stars that are colonized, centralized systems increasingly draw resources from further systems which have not had their resources harvested–– driving increased expansion
[\Longleftarrow] Decreasing levels of centrality, increasing likelihood of fragmentation into single star systems if resources cannot be adequately transferred from central sources, resource based wars may reemerge after disappearance during Type I

Type III

According to Kaku, Kardaschev has estimated the development of such a civilization at the year 7800.
Type III Colonization of the Milky Way Galaxy has completed
Early (1036 W to 1039 W) (debatable) Middle (1040 W to 1043 W) (debatable) Late (1044 W to 1046 W) (debatable)
(Continued) colonization of nearby galaxies. Highly hypothetical at this point, there are no proposals for this or higher levels.
Trends:
[\Longrightarrow] Increasing levels of technology, centralized systems increasingly draw resources from further systems which have not had their resources harvested–– driving increased expansion
[\Longleftarrow] Slow growth in galaxies that are colonized due to speed limitations, making centrality impossible

Type IV & V

Type IV Colonization of the Local Supercluster (1046 W to 1056 W) Can escape the universe via creating a black hole.
Type V Colonization of the Visible universe (1056 W to 1066 W)

Current values

Given past and projected values for planetary power production from the International Energy Agency, it can be shown that:

Year Energy production Fractional Kardashev
scale equivalent
exajoules/year terawatts QuadsQuads: 1 quadrillion BTU mtoesmtoes: million tonnes (metric tons) of oil equivalents
1900 21 .67 20 500 0.58
1970 190 6.0 180 4500 0.68
1973 260 8.2 240 6200 0.69
1985 290 9.2 270 6900 0.70
1989 320 10 300 7600 0.70
1993 340 11 320 8100 0.70
1995 360 12 340 8700 0.71
2000 420 13 400 10000 0.71
2001 420 13 400 10000 0.71
2002 430 14 410 10400 0.71
2004 440 14 420 10600 0.72
2010 510 16 480 12100 0.72
2030 680 22 650 16300 0.73

Literature describing different Kardashev Types

These categorizations are not firm, and are neither complete nor absolute. Most science fiction space opera writers do not specifically write their works with Kardashev classification in mind.

Connections with sociology and anthropology

Kardashev's theory can be viewed as the expansion of some social theories, especially from social evolutionism. It is close to the theory of Leslie White, author of The Evolution of Culture: The Development of Civilization to the Fall of Rome (1959). White attempted to create a theory explaining the entire history of humanity. The most important factor in his theory is technology: Social systems are determined by technological systems, wrote White in his book, echoing the earlier theory of Lewis Henry Morgan. As measure of society advancement he proposed the measure energy consumption of a given society (thus his theory is known as energy theory of cultural evolution). He differentiates between five stages of human development. In the first stage, people use energy of their own muscles. In the second stage, they use energy of domesticated animals. In the third stage, they use the energy of plants (which White refers to as agricultural revolution). In the fourth stage, they learn to use the energy of natural resources - such as coal, oil and gas. Finally, in the fifth stage, they harness nuclear energy. White introduced a formula P=E×T, where E is a measure of energy consumed, and T is the measure of efficiency of technical factors utilising the energy.

Notes

See also

References

External links

Sustainability and energy development   [Edit]
Energy production Active solar | Anaerobic digestion | Biomass | Blue energy | Deep lake water cooling | Distributed generation | Electricity generation | Energy tower | Fuel cell | Fusion power | Geothermal power | Hydroelectricity | Mechanical biological treatment | Ocean thermal energy conversion | Passive solar | Seasonal thermal store | Solar cell | Solar panel | Solar pond | Solar power | Solar power tower | Solar thermal energy | Solar tracker | Solar updraft tower | Tidal power | Trombe wall | Water turbine | Wave power | Wind farm | Wind power | Wind turbine
Energy development and use Energy development > Environmental concerns with electricity generation | Future energy development | Inertial fusion power plant | Hydrogen economy | Hubbert peak | Renewable energy | Hypermodernity | Technological singularity
Energy and
sustainability status
Ecosystem services > Kardashev scale | TPE | UN Human Development Index | Value of Earth | Appropriate technology | Infrastructural capital
Sustainability Autonomous building > Ecoforestry | Ecological economics | Earth sheltering | Development economics | Environmental design | Exploitation of natural resources | Green building | Green chemistry | Green gross domestic product | Natural building | Permaculture | Self-sufficiency | Straw-bale construction | Sustainability | Sustainable agriculture | Sustainable design | Sustainable development | Sustainable industries | Sustainable living | The Natural Step | Windcatcher
Sustainability management Commission on Sustainable Development > Human development theory | Maldevelopment | Rio Declaration on Environment and Development | Rocky Mountain Institute | Sim Van der Ryn | Underdevelopment | World Business Council for Sustainable Development | World Summit on Sustainable Development | Precautionary principle | Intermediate Technology Development Group
Energy and
conservation
Energy conservation > Energy-efficient landscaping | Passive house | Superinsulation | Voluntary simplicity | Ecological footprint | Ecovillage | Waste | Zero energy building
Transportation Battery electric vehicle > Electric vehicle | Hydrogen car | Trolleybus
Communication Wireless Mesh

 


From Wikipedia, the Free Encyclopedia. Original article here. Support Wikipedia by contributing or donating.
All text is available under the terms of the GNU Free Documentation License See Wikipedia Copyrights for details.

Search Titles
0123456789
ABCDEFGHIJ
KLMNOPQRST
UVWXYZ?

E-mail this article to:

Personal Message: