Qualitative classification of extraterrestrial civilizations
arXiv:2005.13221 · doi:10.1051/0004-6361/202037597
Abstract
Abridged: The interest towards searches for extraterrestrial civilizations (ETCs) was boosted by the discovery of thousands of exoplanets. We turn to the classification of ETCs for new considerations that may help to design better strategies for ETCs searches. We take a basic taxonomic approach to ETCs and investigate the implications of the new classification on ETCs observational patterns. We use as a counter-example to our qualitative classification the quantitative scheme of Kardashev. We propose a classification based on the abilities of ETCs to modify their environment and to integrate with it: Class 0 uses the environment as it is, Class 1 modifies the it to fit its needs, Class 2 modifies itself to fit the environment and Class 3 ETC is fully integrated with the environment. Combined with the classical Kardashev's scale our scheme forms a 2d scheme for interpreting ETC properties. The new framework makes it obvious that the available energy is not an unique measure of ETCs, it may not even correlate with how well that energy is used. The possibility for progress without increased energy consumption implies lower detectability, so the existence of a Kardashev Type III ETC in the Milky Way cannot be ruled out. This reasoning weakens the Fermi paradox, allowing the existence of advanced, yet not energy hungry, low detectability ETCs. The integration of ETCs with environment makes it impossible to tell apart technosignatures from natural phenomena. Thus, the most likely opportunity for SETI searches is to look for beacons, specifically set up by them for young civilizations like us (if they want to do that is a matter of speculation). The other SETI window is to search for ETCs at technological level close to ours. To rephrase the saying of A. Clarke, sufficiently advanced civilizations are indistinguishable from nature.
arXiv commentaccepted in A&A; 7 pages, 1 figure; the acknowledgements were updated in the new version
References in corpus (24)
- Planck 2015 results. XIII. Cosmological parameters
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- The Gaia mission
- Biosignatures from Earth-Like Planets Around M Dwarfs
- The Radial Velocity Experiment (RAVE): Fifth Data Release
- Vegetation's Red Edge: A Possible Spectroscopic Biosignature of Extraterrestrial Plants
- A Dying Universe: The Long Term Fate and Evolution of Astrophysical Objects
- The Ĝ Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. III. The Reddest Extended Sources in WISE
- The Ĝ Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. I. Background and Justification
- The Ĝ Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. II. Framework, Strategy, and First Result
- The Ĝ Search for Extraterrestrial Civilizations with Large Energy Supplies. IV. The Signatures and Information Content of Transiting Megastructures
- How Much SETI Has Been Done? Finding Needles in the n-Dimensional Cosmic Haystack
- IRAS-based whole-sky upper limit on Dyson Spheres
- Extragalactic SETI: The Tully-Fisher relation as a probe of Dysonian astroengineering in disk galaxies
- Relative Likelihood of Success in the Searches for Primitive versus Intelligent Extraterrestrial Life
- Kardashev's Classification at 50+: A Fine Vehicle with Room for Improvement
- SETI with Gaia: The observational signatures of nearly complete Dyson spheres
- On the search for artificial Dyson-like structures around pulsars
- The application of the Mid-IR radio correlation to the sample and the search for advanced extraterrestrial civilisations
- On the possibility of the Dyson spheres observable beyond the infrared spectrum
- Biotechnology and the lifetime of technical civilizations
- Estimates for the number of visible galaxy-spanning civilizations and the cosmological expansion of life
- Sunscreen: Photometric Signatures of Galaxies Partially Cloaked in Dyson Spheres
- Intelligent Life in Cosmology