| advertise add site services publishers database health videos | ![]() | about toolbar stats live show health store more stuff JOIN/LOGIN |
Physicians Scales, Baby Scales, Chair Scales, Bed Scales, Dialysis... a1medicalsales.com | Detecto Physician Scales, Doctor Scales, Fitness Scales, Floor Scales,... ironcompany.com | Weighing Scales & Weights, Electronic Balances, Table Top Scales, Price... medicalsurgicals.com | Scales, Clinical Scales, Digital... a2zmed.com |
Kardashev scale projections for human civilization ranging from years 1900 to 2030, based on data from the International Energy Agency World Energy Outlook Various Kardashev scale projections covering 1900 to 2100. One results in a singularity. The Kardashev scale is a method of measuring a civilization's level of technological advancement. The scale is only theoretical and in terms of an actual civilization highly speculative; however, it puts energy consumption of an entire civilization in a cosmic perspective. It was first proposed in 1964 by the Soviet Russian astronomer Nikolai Kardashev. The scale has three designated categories called Type I, II, and III. These are based on the amount of usable energy a civilization has at its disposal, and the degree of space colonization. In general terms, a Type I civilization has achieved mastery of the resources of its home planet, Type II of its solar system, and Type III of its galaxy.[1] [edit] Energy useEnergy is a static quantity and is denoted in joules. Power is a measure of energy transfer over time, and is denoted in watts (joules per second). The three levels of the Kardashev Scale can be quantified in units of power (watts) and plotted on an increasing logarithmic scale.
Using nuclear explosion tests as a perspective, Tsar Bomba, the largest nuclear weapon ever detonated, released an estimated 57 megaton yield; even a Type I civilization makes use of roughly 25 megatons of TNT equivalent a second. A Type II civilization controls 4 × 109 times more energy (4 billion hydrogen bombs per second), and a type III 1011 times more yet. Current human civilization (2009) has a Kardashev value of about 0.718. However, the Kardashev scale was not developed to model a specific civilization. It's primarily used by SETI researchers, science fiction authors, and futurists as a theoretical framework.[citation needed] [edit] Current status of human civilizationHuman civilization is currently somewhere 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. In 1973, he calculated humanity's civilization type to be 0.7, in relationship to Kardashev's model for Types 0 and I.[4] Sagan used the arbitrary formula: Value K is a civilization's Kardashev rating and W is its power output in watts. Sagan used 10 TW as value W, which was considerably higher than present data suggests.[5] Sagan's overestimation makes little difference in regards to human civilization's K rating, effecting only a difference of 1% in the value of K (See Table Below). International Energy Agency World Energy Outlook (2005)[5] and section 7 of Key World Energy Statistics[6] project values for planetary power production yielding these corresponding Kardashev scale estimates:
As of 2007[update], the Fractional Kardashev equivalent is approximately 0.72, calculated using BP's primary energy consumption chart for 2007.[9] It is important to note that as Sagan's fractional Kardashev scale is base-10 logarithmic, a value of 0.72 means we are using approximately 0.16% of the total available planetary energy budget. Further information: World energy resources and consumption [edit] Energy developmentSee also: Energy development Methods by which a civilization could feasibly advance to Type I:
Type II civilizations might employ:
Type III civilizations might use the same techniques employed by a Type II civilization, but applied to all of the stars of one or more galaxies individually.[16] They may also be able to tap into the energy produced from a supermassive black hole which are believed to exist at the center of most galaxies. [edit] Civilization implicationsThere are many historical examples of civilizations undergoing large-scale transitions, such as the Industrial Revolution. 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[17] 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, similar to a Malthusian catastrophe. Excessive use of energy without adequate disposal of heat, for example, could make the planet of a civilization approaching Type I unsuitable to the biology of the dominant life-forms and their food sources. If Earth is an example, then sea temperatures in excess of 35 °C would jeopardize marine life and make the cooling of mammals to temperatures suitable for their metabolism difficult if not impossible. Of course, these theoretical speculations may not become problems in reality thanks to the application of future engineering and technology. [edit] Extensions to the original scaleThe sub-Type I state that human civilization currently occupies was not originally included in the Kardashev scale but is now referred to as "Type 0" or by its K value using Sagan's logarithmic formula (described above). Zoltan Galantai has defined a further extrapolation of the scale, a Type IV level which controls the energy output of the visible universe; this is within a few orders of magnitude of 1045 W. Such a civilization approaches or surpasses the limits of speculation based on current scientific understanding, and may not be possible. Frank J. Tipler's Omega point would presumably occupy this level, as would the Biocosm hypothesis. Galantai has argued that such a civilization could not be detected, as its activities would be indistinguishable from the workings of nature (there being nothing to compare them to).[18] However, Milan M. Ćirković has argued that "Type IV" should instead be used to refer to a civilization that has harnessed the power of its supercluster, or "the largest gravitationally bound structure it originated in (sic)".[19] For the Local Supercluster, this would be approximately 1042 W. Dr. Michio Kaku has discussed a type IV civilization, which could harness "extragalactic" energy sources such as dark energy, in his book Parallel Worlds.[20] In contrast to simply increasing the maximum power level covered by the scale, Carl Sagan suggested adding another dimension: the information available to the civilization. He assigned the letter A to represent 106 unique bits of information (less than any recorded human culture) and each successive letter to represent an order of magnitude increase, so that a level Z civilization would have 1031 bits. In this classification, 1973 Earth is a 0.7 H civilization, with access to 1013 bits of information. Sagan believed that no civilization has yet reached level Z, conjecturing that so much unique information would exceed that of all the intelligent species in a galactic supercluster and observing that the universe is not old enough to effectively exchange information over larger distances. The information and energy axes are independent, so that even a level Z civilization would not need to be Kardeshev Type III.[4] [edit] Extensions to the original scale in science-fiction
[edit] Connections with sociology and anthropologyKardashev'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 the 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 P measures the advancement of the culture, E is a measure of energy consumed, and T is the measure of efficiency of technical factors utilizing the energy. [edit] CriticismIt 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 Evolving the Alien: The Science of Extraterrestrial Life.[23] On a more direct level, since the Kardashev scale rates a civilization according to how much energy it is capable of harnessing, it "penalizes" a civilization that invents ways of making more efficient use of the energy already available to it, instead of simply harnessing yet more energy. If the population of North America, for example, were to switch from using incandescent lamps to fluorescent lighting, it would delay the construction of new power plants, and thus hamper the rate at which North American civilization's "Type" rating increased. [edit] See also
[edit] Further reading
[edit] References
[edit] External links
| ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| ↑ top of page ↑ | about thumbshots |