Kardashev civilization(文明)Details |
![]() |
| log in |
Message boards : Science (non-SETI) : Kardashev civilization(文明)Details
| Author | Message |
|---|---|
|
The Kardashev scale is a general method of classifying how technologically advanced a civilization is. It was first proposed in 1964 by the Soviet 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 mastery of the resources of its home planet, Type II of its solar system, and Type III of its galaxy. | |
| ID: 801867 · | |
|
Thank you, Yon! | |
| ID: 802046 · | |
|
I'm a 'Type IV' trapped in a 'Type I' civilization... ;) | |
| ID: 802069 · | |
Thank you, Yon! That's all right,we are truly 'planetary community'. ____________ æ„›ï¹ä»ï¹å¿ï¹å–„ï¹å‹‡ Any people can sense their die just a couple of their live | |
| ID: 802195 · | |
I'm a 'Type IV' trapped in a 'Type I' civilization... ;) Because they claim to be 'Type V' civilization... ____________ æ„›ï¹ä»ï¹å¿ï¹å–„ï¹å‹‡ Any people can sense their die just a couple of their live | |
| ID: 802356 · | |
The Kardashev scale is a general method of classifying how technologically advanced a civilization is. It was first proposed in 1964 by the Soviet 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 mastery of the resources of its home planet, Type II of its solar system, and Type III of its galaxy....... Here is a similar view from renowned physicist Dr. Michio Kaku: <a href="http://video.google.ca/videosearch?q=kaku+seti&hl=en&emb=0#q=kaku%20civilization&hl=en&emb=0">michio kaku on civilization</a> <a href="http://www.youtube.com/watch?v=Cqt2CvYt9dQ&feature=related">more detail</a> He said physicists generally looks for three types of civilization in extraterrestrial intelligence. type 1: planetary. has ability to control anything planetary such as earthquakes, weather and so on. An example of such civilization is Buck Rogers. They harness energy from within the planet but i gather it would be anything except fossil fuel. type 2: stellar. harnesses energy directly from the sun like solar flare. Like star trek federation. type 3: galactic. harness energy from billions of stars within the galaxy. The borg or star wars empire are such example. he mentioned Q in another interview is of a type 4 which wasn't discussed (probably unknown or more sci-fi/imagination i think). In relation to where we are and how long before we get to the next civilization, we are currently at type 0. we harness our energy from dead plants (oil and coal). we are about 100 years away from reaching type 1. Type 2 is about 5000 years away. Type 3 is more like 100,000 to a million years in the distant future. one interesting note is he said 2001: space odyssey is the most authentic rendition of how type-3 ETs visit other civilizations. The aliens would create a robot that will exponentially replicate itself and position themselves in all the moons and wait for civilization in the galaxies to evolve. He said Kubrick deleted the 1st 5 mins of 2001 to make the movie more mystical. | |
| ID: 804037 · | |
|
Here is a similar view from renowned physicist Dr. Michio Kaku: | |
| ID: 804265 · | |
|
| |
| ID: 804290 · | |
Thanks too,i rather believed the classification that was made by these scientist,although its was based on our earth civilization modeling,but any outer advanced civilization can be seeing as the hominine. ____________ æ„›ï¹ä»ï¹å¿ï¹å–„ï¹å‹‡ Any people can sense their die just a couple of their live | |
| ID: 804506 · | |
|
The speed of the technology grown is different in different civilization,these is dual to the condition of one planet. | |
| ID: 809837 · | |
Message boards : Science (non-SETI) : Kardashev civilization(文明)Details
| Copyright © 2013 University of California |