A Plethora of the Earth-like Planet: Ramifications of a Fuzzy World

Fuente: arXiv
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Main Author: von Hegner, Ian
Format: Preprint
Published: 2023
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author von Hegner, Ian
author_facet von Hegner, Ian
contents One primary reason for the formulation of the term Earth-like planet and the search for such planets in the galaxy is because life has arisen in such a world. Thus, this search seems justifiable as it is known here what one is looking for. However, the Earth-like concept represents an attempt to set up sharp boundaries for an inhabited planet, even though nature often comes as continua. The analyses in this work show that the term does not represent a clear-cut entity as a general Earth-likeness cannot be abstracted. Thus, the complex variation of environment and life means that the singular term Earth-like planet is more appropriately treated as a fuzzy world. Such a fuzzification has the consequence of the term being not only more limited than assumed but may even be deceptive, as an Earth-like planet on one hand can be in a segment in which it does not seem particularly Earth-like, but still possesses life, but on the other hand can appear very Earth-like but not possess life anyway. An atmosphere can provide a biosignature by being displaced from thermodynamic equilibrium, derived from antagonistic adaptation, in which life as a double-edged sword, on one hand, continuously makes the external environment less favourable for itself, while on the other, increasing its capacity to do so. Yet, there is an issue with using this as a search criterion for potentially inhabited worlds, as such planets can give impressions that do not reflect what has gone on; they can even give a ghost biosignature. These novel analyses do not represent a limitation in the search for Earth-like planets, as the plethora of Earth-like planets shows the possibility that the number of inhabited worlds can be large, but do represent a limitation in the search for life on such worlds.
format Preprint
id arxiv_https___arxiv_org_abs_2403_12441
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle A Plethora of the Earth-like Planet: Ramifications of a Fuzzy World
von Hegner, Ian
Popular Physics
One primary reason for the formulation of the term Earth-like planet and the search for such planets in the galaxy is because life has arisen in such a world. Thus, this search seems justifiable as it is known here what one is looking for. However, the Earth-like concept represents an attempt to set up sharp boundaries for an inhabited planet, even though nature often comes as continua. The analyses in this work show that the term does not represent a clear-cut entity as a general Earth-likeness cannot be abstracted. Thus, the complex variation of environment and life means that the singular term Earth-like planet is more appropriately treated as a fuzzy world. Such a fuzzification has the consequence of the term being not only more limited than assumed but may even be deceptive, as an Earth-like planet on one hand can be in a segment in which it does not seem particularly Earth-like, but still possesses life, but on the other hand can appear very Earth-like but not possess life anyway. An atmosphere can provide a biosignature by being displaced from thermodynamic equilibrium, derived from antagonistic adaptation, in which life as a double-edged sword, on one hand, continuously makes the external environment less favourable for itself, while on the other, increasing its capacity to do so. Yet, there is an issue with using this as a search criterion for potentially inhabited worlds, as such planets can give impressions that do not reflect what has gone on; they can even give a ghost biosignature. These novel analyses do not represent a limitation in the search for Earth-like planets, as the plethora of Earth-like planets shows the possibility that the number of inhabited worlds can be large, but do represent a limitation in the search for life on such worlds.
title A Plethora of the Earth-like Planet: Ramifications of a Fuzzy World
topic Popular Physics
url https://arxiv.org/abs/2403.12441