Technological level of a civilization that is "close to the level presently attained on Earth, with energy consumption at ≈4×1019erg/sec" (4×1012 watts). Currently, the civilization of Type I is usually defined as one that can harness all the energy that falls on a planet from its parent star (for Earth–Sun system, this value is close to 1.74×1017 watts), which is about four orders of magnitude higher than the amount presently attained on Earth, with energy consumption at ≈2×1013 watts. The astronomer Guillermo A. Lemarchand stated this as a level near contemporary terrestrial civilization with an energy capability equivalent to the solar insolation on Earth, between 1016 and 1017 watts.
A civilization capable of harnessing the energy radiated by its own star—for example, the stage of successful construction of a Dyson sphere or Matrioshka brain—with energy consumption at ≈4×1033 erg/sec. Lemarchand stated this as a civilization capable of using and channeling the entire radiation output of its star. The energy use would then be comparable to the luminosity of the Sun, about 4×1033 erg/sec (4×1026watts).
A civilization in possession of energy at the scale of its own galaxy, with energy consumption at ≈4×1044 erg/sec. Lemarchand stated this as a civilization with access to the power comparable to the luminosity of the entire Milky Way galaxy, about 4×1044 erg/sec (4×1037 watts).
Kardashev believed that a Type 4 civilization was impossible, so he did not go past Type 3. However, new types (0, IV, V, VI) have been proposed.
Current status of human civilization
Total World, Annual Primary Energy Consumption.
According to the astronomer Carl Sagan, humanity is currently going through a phase of technical adolescence, "typical of a civilization about to integrate the type I Kardashev scale."
At the current time, humanity has not yet reached Type I civilization status. Physicist and futurist Michio Kaku suggested that, if humans increase their energy consumption at an average rate of 3 percent each year, they may attain Type I status in 100–200 years, Type II status in a few thousand years, and Type III status in 100,000 to a million years.
Carl Sagan suggested defining intermediate values (not considered in Kardashev's original scale) by interpolating and extrapolating the values given above for types I (1016 W), II (1026 W) and III (1036 W), which would produce the formula
where value K is a civilization's Kardashev rating and P is the power it uses, in watts. Using this extrapolation, a "Type 0" civilization, not defined by Kardashev, would control about 1 MW of power, and humanity's civilization type as of 1973 was about 0.7 (apparently using 10 terawatt (TW) as the value for 1970s humanity).
In 2019, the total world energy consumption was 14864.9 Mtoe (175,249 TWh), equivalent to an average power consumption of 20.0 TW or 0.73 on Sagan's interpolated Kardashev scale.
In 2015, a study of galactic mid-infrared emissions came to the conclusion that "Kardashev Type-III civilizations are either very rare or do not exist in the local Universe".
In 2016, Paul Gilster, author of the Centauri Dreams website, described a signal apparently from the star HD 164595 as requiring the power of a Type I or Type II civilization, if produced by extraterrestrial lifeforms. However, in August 2016 it was discovered that the signal's origin was most likely a military satellite orbiting the Earth.
Type I civilization methods
Large-scale application of fusion power. According to mass–energy equivalence, Type I implies the conversion of about 2 kg of matter to energy per second. An equivalent energy release could theoretically be achieved by fusing approximately 280 kg of hydrogenintohelium per second, a rate roughly equivalent to 8.9×109 kg/year. A cubic km of water contains about 1011 kg of hydrogen, and the Earth's oceans contain about 1.3×109 cubic km of water, meaning that humans on Earth could sustain this rate of consumption over geological time-scales, in terms of available hydrogen.
Antimatter in large quantities would provide a mechanism to produce power on a scale several magnitudes above the current level of technology. In antimatter-matter collisions, the entire rest mass of the particles is converted to radiant energy. Their energy density (energy released per mass) is about four orders of magnitude greater than that from using nuclear fission, and about two orders of magnitude greater than the best possible yield from fusion. The reaction of 1 kg of anti-matter with 1 kg of matter would produce 1.8×1017J (180 petajoules) of energy. Although antimatter is sometimes proposed as a source of energy, this does not appear feasible. Artificially producing antimatter—according to current understanding of the laws of physics—involves first converting energy into mass, which yields no net energy. Artificially created antimatter is only usable as a medium of energy storage, not as an energy source, unless future technological developments (contrary to the conservation of the baryon number, such as a CP violation in favor of antimatter) allow the conversion of ordinary matter into anti-matter. Theoretically, humans may in the future have the capability to cultivate and harvest a number of naturally occurring sources of antimatter.
Another means to generate usable energy would be to feed a stellar mass into a black hole, and collect photons emitted by the accretion disc. Less exotic would be simply to capture photons already escaping from the accretion disc, reducing a black hole's angular momentum; this is known as the Penrose process. This, however, may only be possible for a Type III civilization to achieve.
Star lifting is a process where an advanced civilization could remove a substantial portion of a star's matter in a controlled manner for other uses.
Antimatter is likely to be produced as an industrial byproduct of a number of megascale engineering processes (such as the aforementioned star lifting) and, therefore, could be recycled.
In multiple-star systems of a sufficiently large number of stars, absorbing a small but significant fraction of the output of each individual star.
Type III civilization methods
Type III civilizations might use the same techniques employed by a Type II civilization, but applied to all possible stars of one or more galaxies individually.
They may also be able to tap into the energy released from the supermassive black holes believed to exist at the center of most galaxies.
White holes could theoretically provide large amounts of energy from collecting the matter propelling outwards.
Capturing the energy of gamma-ray bursts is another theoretically possible power source for a highly advanced civilization.
The emissions from quasars are comparable to small active galaxies and could provide a massive power source if collectible.
There are many historical examples of human civilization 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 suggests that the transition from Type 0 to Type I might carry a strong risk of self-destruction since, in some scenarios, there would no longer be room for further expansion on the civilization's home planet, as in a Malthusian catastrophe. Excessive use of energy without adequate heat disposal, for example, could plausibly 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 (95 °F) 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, possibly through the applications of future engineering and technology. Also, by the time a civilization reaches Type I it may have colonized other planets or created O'Neill-type colonies, so that waste heat could be distributed throughout the planetary system.
Many extensions and modifications to the Kardashev scale have been proposed.
Types 0, IV, and V Kardashev rating: The most straightforward extension of the scale to even more hypothetical Type IV beings who can control or use the entire universe or Type V who control collections of universes. This would also include Type 0 civilizations, who do not rank on the Kardashev scale. The power output of the visible universe 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.
Zoltán Galántai 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).
Other proposed changes to the scale use different metrics such as 'mastery' of systems, amount of information used, or progress in control of the very small as opposed to the very large:
Planet mastery (Robert Zubrin): Metrics other than pure power usage have also been proposed. One is 'mastery' of a planet, system or galaxy rather than considering energy alone.
Information mastery (Carl Sagan): Alternatively, Carl Sagan suggested adding another dimension in addition to pure energy usage: 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, in 2018, Earth was a 0.73 J civilization.
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 exchange information effectively over larger distances.
The information and energy axes are not strictly interdependent so that even a level Z civilization would not need to be Kardashev Type III.
Microdimensional mastery (John Barrow):John D. Barrow observed that humans have found it more cost-effective to extend their abilities to manipulate their environment over increasingly small scales rather than increasingly large ones. He, therefore, proposes a reverse classification downward from Type I-minus to Type Omega-minus:
Type I-minus is capable of manipulating objects over the scale of themselves: building structures, mining, joining and breaking solids;
Type II-minus is capable of manipulating genes and altering the development of living things, transplanting or replacing parts of themselves, reading and engineering their genetic code;
Type III-minus is capable of manipulating molecules and molecular bonds, creating new materials;
Type IV-minus is capable of manipulating individual atoms, creating nanotechnologies on the atomic scale, and creating complex forms of artificial life;
Type V-minus is capable of manipulating the atomic nucleus and engineering the nucleons that compose it;
Type VI-minus is capable of manipulating the most elementary particles of matter (quarks and leptons) to create organized complexity among populations of elementary particles; culminating in:
Type Omega-minus is capable of manipulating the basic structure of space and time.
The human civilization is somewhere between type III-minus and types IV-minus according to this classification.
Civilizational range (Robert Zubrin):Robert Zubrin adapts the Kardashev scale to refer to how widespread a civilization is in space, rather than to its energy use.
In his definition, a Type I civilization has spread across its planet.
A Type II has extensive colonies in its respective stellar system, and
It has been argued that we cannot predict their behavior because we cannot understand advanced civilizations. Thus, the Kardashev scale may not be relevant or useful for classifying extraterrestrial civilizations. This central argument is found in the 2002 book Evolving the Alien: The Science of Extraterrestrial Life.
The Kardashev scale ranks the advancement of civilizations along the lines of empires and their colonies; however, based on human history, empires are notably ephemeral political structures that inevitably fall. We might consider that intelligent beings would rather aspire to live in greater balance with their environments, prolonging not only their own lives but those of other beings they can cooperate with and grow in societies of mutual aid.
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Supercivilizations as Possible Products of the Progressive Evolution of Matter: also by Kardashev
Search for Artificial Stellar Sources of Infrared Radiation, by Freeman J. Dyson
The Radio Search For Intelligent Extraterrestral Life, by Frank Drake
Freitas Jr., Robert A. Energy and Culture (chapter 15).
Griffin, John (February 2010). Operation TOGA: Type One Go Ahead. ISBN 978-1-4502-0702-7.
Library resources about Kardashev scale
Resources in your library
Resources in other libraries
Astrobiology: The Living Universe
Detectability of Extraterrestrial Technological Activities
Flash Animation on Civilizations
After Kardashev: Farewell to Super Civilizations
Exotic Civilizations: Beyond Kardashev
Description of civilization types from Dr. Michio Kaku
Search for Type III civilizations
What Do Alien Civilizations Look Like? The Kardashev Scale, a short YouTube video by Kurzgesagt, explaining and visualizing the topic
Kardashev Scale, the big picture on space civilizations, an audio podcast by SciFi Thoughts