Kardashev scale

Kardashev scale

Imagine a civilization so advanced it harnesses the energy of entire galaxies. The Kardashev scale, a method of measuring a civilization's level of technological advancement, offers a fascinating lens through which to view potential futures. Let's delve into its intriguing depths.

The Kardashev scale is a hypothetical method of measuring a civilization’s level of technological advancement based on the amount of energy it is able to use.

The measure was proposed by Soviet astronomer Nikolai Kurashev in 1964

Stellar engines can be used to move stars

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

Other proposed changes to the scale include:

Planet mastery (Robert Zubrin): Metrics other than pure power usage have also been proposed.

Microdimensional mastery (John Barrow)

Humans have found it more cost-effective to extend their abilities to manipulate their environment over increasingly small scales rather than increasingly large ones.

Large-scale application of fusion power

Antimatter in large quantities would provide a mechanism to produce power on a scale several magnitudes above the current level of technology

Kardashev believed that a Type 4 civilization was impossible[citation needed], so he did not go past Type 3

However, new types (0, IV, V, VI) have been proposed.

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.

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.

The transition between Kardashev scale levels could potentially represent 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[26] 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.

Carl Sagan suggested defining intermediate values 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:

K is a civilization’s Kardashev rating, and P is the power it uses, in watts.

Kardashev civilizations are either very rare or do not exist in the local Universe.

In 2015, a study of galactic mid-infrared emissions came to the conclusion that “Kardsahev Type-III civilizations are probably very rare”

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