Kardashev scale

The Kardashev scale (Russian: шкала Кардашёва, romanized: shkala Kardashova) is a method of measuring a civilization's level of technological advancement based on the amount of energy it is capable of harnessing and using. As both a proposed method of tracking civilizational progress and a way to evaluate potential alien civilizations, it occupies an intersection between futures studies and xenology. The measure was proposed by Soviet astronomer Nikolai Kardashev in 1964, forming the basis for a series of papers proposing ways to detect super civilizations and direct the search for extraterrestrial intelligence.

Kardashev's initial model was developed starting from a functional definition of civilization, based on the immutability of physical laws, and using human civilization as a model for extrapolation. He proposed a classification of civilizations into three types, based on the axiom of exponential growth:

A Type I civilization (planetary) is able to access all the energy available on its planet and store it for consumption.

A Type II civilization (stellar) can directly consume a star's energy, such as through the use of a Dyson sphere.

A Type III civilization (galactic) is able to capture all the energy emitted by its galaxy, and every object within it, such as every star, black hole, etc.

Under this scale, the sum of human civilization does not yet reach Type I status, though it approaches it. Extensions of the scale have since been proposed, including a wider range of power levels (Types 0, IV, and V) and the use of metrics other than pure power, e.g., computational growth or food consumption.

Kardashev's publications

First publication (1964)

Kardashev first outlined his scale in a paper presented at the 1964 conference that communicated findings on BS-29-76, the Byurakan Conference in the Armenian SSR, which reviewed the Soviet radio astronomy space listening program.