Type 2 Civilization
Part one · The Goal

Catch the whole star.

A Type II civilization uses all the energy its star gives off. We use a tiny fraction of what reaches one planet. This site is about the distance between those two, and how it gets closed.

STAR OUTPUT · 400 TRILLION TRILLION WATTS COLLECTOR SWARM · NOT TO SCALE
The Kardashev scale

Three rungs, each ten billion times the last

In 1964 the astronomer Nikolai Kardashev proposed ranking civilizations by one number: how much power they use. Carl Sagan later turned the three types into a smooth scale.

Type I · A planet
1016 watts

Uses power on the scale of everything a planet has available. Weather, tides and sunlight are all within its reach.

Type II · A star
1026 watts

Captures the full output of its star, most likely with a vast swarm of collectors in orbit. This is the goal the site is named for.

Type III · A galaxy
1036 watts

Commands the energy of a whole galaxy of stars. Nobody has a serious plan for this one yet.

Where we are

Humanity is about a Type 0.73

We run on roughly twenty trillion watts. On Sagan's scale that puts us most of the way to Type I, but each tenth of a type is ten times more power, so the remaining climb is still large.

Drag the slider to see what a given amount of power is worth.

Kardashev type0.73
Power used1013.3 watts

Reading

Three books that started this

One pick each, with the reason and the catch. These are ordinary links. We do not earn a commission from them. If that changes, we will say so next to the link and on our affiliate disclosure page.

Carl Sagan · 1973

The Cosmic Connection

Why this one: the book where Sagan turns Kardashev's three types into the decimal scale used on this page.

The catch: it is fifty years old, and the space science shows its age.

Find it at Open Library
Michio Kaku · 2011

Physics of the Future

Why this one: a readable tour of how a society might climb from Type 0 to Type I this century.

The catch: it is optimistic, and some of its near-term forecasts have already slipped.

Find it at Open Library
Vaclav Smil · 2017

Energy and Civilization: A History

Why this one: a careful history of how societies grow by capturing more power, from muscle and fire to fuels and electricity.

The catch: it is dense, and it stays on Earth. It will not walk you through a star-scale collector.

Find it at Open Library
Guides

Longer reads

Plain-language pages that go further than the sketches on this home page.

The bigger story

Five things it takes to get there

Each part of the climb has its own site. Start with whichever you care about most.

01 · You are hereThe GoalEnergy and the Kardashev scale
02 · Robot MotionThe HandsRobots that do the building 03 · Sentient CloudThe MindArtificial intelligence that runs it
04 · ComingThe PlaceLaunch, the Moon and beyond
05 · ComingThe PeopleLiving long enough to see it
Kardashev IIThe ScoreLive numbers and milestones
A couple of shops

Places to start, if you want them

These are ordinary links, not a storefront. We do not earn a commission from them. If that changes, we will say so next to the link and on our affiliate disclosure page. These are shops, not reviews, and not a claim that we bought or tested the goods.