Technosignatures: Waste Heat And Habitability: Constraints From Technological Energy Consumption
Waste heat production represents an inevitable consequence of energy conversion as per the laws of thermodynamics.
Based on this fact, by using simple theoretical models, we analyze constraints on the habitability of Earth-like terrestrial planets hosting putative technological species and technospheres characterized by persistent exponential growth of energy consumption and waste heat generation: in particular, we quantify the deleterious effects of rising surface temperature on biospheric processes and the eventual loss of liquid water.
Irrespective of whether these sources of energy are ultimately stellar or planetary (e.g., nuclear, fossil fuels) in nature, we demonstrate that the loss of habitable conditions on such terrestrial planets may be expected to occur on timescales of ≲1000 years, as measured from the start of the exponential phase, provided that the annual growth rate of energy consumption is of order 1%.
We conclude by discussing the types of evolutionary trajectories that might be feasible for industrialized technological species, and sketch the ensuing implications for technosignature searches.
Amedeo Balbi, Manasvi Lingam
Comments: 76 pages, 4 figure. Submitted, under revision
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR); Applied Physics (physics.app-ph); Physics and Society (physics.soc-ph); Space Physics (physics.space-ph)
Cite as: arXiv:2409.06737 [astro-ph.EP] (or arXiv:2409.06737v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2409.06737
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Submission history
From: Amedeo Balbi
[v1] Mon, 9 Sep 2024 18:31:50 UTC (129 KB)
https://arxiv.org/abs/2409.06737
Astrobiology, SETI,
