Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Kardashev scale
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
=== Sagan's finer classification === In 1973, [[Carl Sagan]] discovered Kardashev's work on the classification of civilizations.<ref name="Galantai-2006">{{Cite journal |last=Galantai |first=Zoltan |date=2006 |title=After Kardashev: Farewell to Super Civilizations |url=https://www.academia.edu/1018345 |journal=Contact in Contex |volume=2 |issue=2 |archive-date=2024-08-18 |access-date=2023-08-08 |archive-url=https://web.archive.org/web/20240818005401/https://www.academia.edu/1018345 |url-status=live }}</ref> He found that the differences between the types Kardashev identified were so great that they did not allow for the best possible modeling of the evolution of civilizations.<ref name="GalΓ‘ntai-2003" /> Consequently, Sagan proposes a more refined classification, still based on Kardashev's types, but integrating intermediate levels using the following [[Logarithmic scale|logarithmic]] [[interpolation]] formula:<ref name="Carrigan Jr.-20102">{{Cite journal |last=Carrigan Jr. |first=Richard A. |date=2010 |title=Starry Messages: Searching for Signatures of Interstellar Archaeology |journal=Journal of British Interplanetary Society |volume=63 |issue=90 |pages=121β126 |arxiv=1001.5455 |bibcode=2010JBIS...63...90C}}</ref> <math>K = \frac{\log_{10}{W}-6} {10}</math>, where ''K'' is the Kardashev type of a civilization and ''W'' is the amount of power it uses, in watts. Thus, a ''Type 1.1'' civilization would be defined by a power of 10<sup>17</sup> watts, while a ''Type 2.3'' civilization would be able to harness 10<sup>29</sup> watts. Moreover, the above formula could be used to extrapolate beyond Kardashev's original types. For example, a '''''Type 0''''' civilization, not defined by Kardashev, would control about 1 MW of power (equivalent to having around 100 campfires burning at any given time); on Earth, the emergence of Type 0 civilizations is roughly concurrent with the [[Cradle of civilization#Rise of civilization|rise of civilization]] in a general sense.<ref>{{Cite thesis |title=Environmental Change and Human Impact during the Mesolithic-Neolithic Transition in North-West Europe|url=https://research.manchester.ac.uk/files/84029587/FULL_TEXT.PDF |degree=PhD |publisher=[[University of Manchester]] |first=Sarah Elizabeth |last=Kneen |date=2014}}</ref> Sagan estimated that, according to this revised scale, 1970s humanity would be Type 0.7 (about 10 [[terawatts]]),<ref name="Sagan-19732">{{Cite journal |last=Sagan |first=Carl |date=1973-07-01 |title=On the detectivity of advanced galactic civilizations |url=https://dx.doi.org/10.1016/0019-1035%2873%2990112-7 |journal=Icarus |language=en |volume=19 |issue=3 |pages=350β352 |bibcode=1973Icar...19..350S |doi=10.1016/0019-1035(73)90112-7 |issn=0019-1035}}</ref> equivalent to 0.16% of the power available on Earth.<ref name="Wilson-20112">{{Cite book |last=Wilson |first=Richard |title=International Seminar on Nuclear War and Planetary Emergencies β 43rd Session |publisher=World Scientific Publishing Company |year=2011 |isbn=978-9814365925 |edition=1st |pages=51β61 |chapter=Energy and the Environment in the Next Millenium |doi=10.1142/8232}}</ref> This level is characterized, according to him, by the ability to self-destruct, which he calls "technological adolescence".<ref name="Lemarchand-20002"/> In 2021, the total [[World energy supply and consumption|world energy consumption]] was 595.15 [[Joule#Exajoule|exajoules]] (165,319 [[Kilowatt-hour#Watt-hour multiples|TWh]]),<ref>{{Cite web |title=The Statistical Review of World Energy 2022 |url=https://www.bp.com/content/dam/bp/business-sites/en/global/corporate/pdfs/energy-economics/statistical-review/bp-stats-review-2022-full-report.pdf |url-status=live |archive-url=https://web.archive.org/web/20230821195021/https://www.bp.com/content/dam/bp/business-sites/en/global/corporate/pdfs/energy-economics/statistical-review/bp-stats-review-2022-full-report.pdf |archive-date=2023-08-21 |access-date=2023-08-24 |website=bp}}</ref> equivalent to an average power consumption of 18.87 TW or a Kardashev rating of 0.73 (to 2 [[Significant figures|s.f.]]).<ref>{{Citation |last1=LePoire |first1=David J. |title=Energy Flow Trends in Big History |date=2020 |url=https://doi.org/10.1007/978-3-030-33730-8_9 |work=The 21st Century Singularity and Global Futures: A Big History Perspective |pages=185β200 |editor-last=Korotayev |editor-first=Andrey V. |access-date=2023-09-09 |series=World-Systems Evolution and Global Futures |place=Cham |publisher=Springer International Publishing |language=en |doi=10.1007/978-3-030-33730-8_9 |isbn=978-3-030-33730-8 |s2cid=213212248 |last2=Chandrankunnel |first2=Mathew |editor2-last=LePoire |editor2-first=David J.}}</ref> Sagan also suggests that, for completeness, an alphabetical scale should be added to indicate the level of [[Social change|social development]], expressed in the amount of information available to the civilization. Thus, a Class A civilization would be based on 10<sup>6</sup> [[bit]]s of information (less than any recorded human culture), a Class B on 10<sup>7</sup>, a Class C on 10<sup>8</sup>, and so on. Humanity in 1973 would belong to the "0.7 H" class.<ref name="books.google.com">{{cite book |last=Sagan |first=Carl |url=https://books.google.com/books?id=lL57o9YB0mAC&pg=PA156 |title=Cosmic Connection: An Extraterrestrial Perspective |year= 2000 |publisher=[[Cambridge University Press]] |others=[[Freeman Dyson]], David Morrison |isbn=978-0-521-78303-3 |editor-last=Agel |editor-first=Jerome |edition= |series= |location= |pages= |language= |chapter= |doi= |oclc= |id= |quote=I would suggest Type 1.0 as a civilization using 10<sup>16</sup> watts for interstellar communication; Type 1.1, 10<sup>17</sup> watts; Type 1.2, 10<sup>18</sup> watts, and so on. Our present civilization would be classed as something like Type 0.7. |author-link=Carl Sagan |access-date=2008-01-01 |orig-date=1973 |via=[[Google Books]]}}</ref> According to Sagan, the first civilization with which humanity would come into contact could be between "1.5 J" and "1.8 K"; a galactic supercivilization would be at the "3 Q" stage, while a federation of galaxies could be at the "4 Z" stage.<ref name="Lemarchand-20002"/> The information and energy axes are not strictly interdependent, so even a level Z civilization would not have to be Kardashev Type III.<ref name="books.google.com" /> Sagan believed that no civilization had yet reached level Z, speculating 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 large distances. In 2017, the total amount of information generated on the [[internet]] was [[Zettabyte Era|26 zettabytes]] (with an estimated 120 zettabytes in 2023),<ref>{{Cite web |title=Data growth worldwide 2010-2025 |url=https://www.statista.com/statistics/871513/worldwide-data-created/ |access-date=2023-11-19 |website=Statista |language=en |archive-date=2024-08-30 |archive-url=https://web.archive.org/web/20240830140921/https://www.statista.com/statistics/871513/worldwide-data-created/ |url-status=live }}</ref> equivalent to 0.73 R/S on Sagan's combined scale.
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Kardashev scale
(section)
Add topic