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Mining in space could spur sustainable growth

Growth models with resources and environmental externalities typically assume that planet Earth is a closed economy. However, private firms like Blue Origin and SpaceX have reduced the cost of rocket launches by a factor of 20 over the last decade. What if these costs continue to decline, making min...

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Detalles Bibliográficos
Autores principales: Fleming, Maxwell, Lange, Ian, Shojaeinia, Sayeh, Stuermer, Martin
Formato: Online Artículo Texto
Lenguaje:English
Publicado: National Academy of Sciences 2023
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10614935/
https://www.ncbi.nlm.nih.gov/pubmed/37844231
http://dx.doi.org/10.1073/pnas.2221345120
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author Fleming, Maxwell
Lange, Ian
Shojaeinia, Sayeh
Stuermer, Martin
author_facet Fleming, Maxwell
Lange, Ian
Shojaeinia, Sayeh
Stuermer, Martin
author_sort Fleming, Maxwell
collection PubMed
description Growth models with resources and environmental externalities typically assume that planet Earth is a closed economy. However, private firms like Blue Origin and SpaceX have reduced the cost of rocket launches by a factor of 20 over the last decade. What if these costs continue to decline, making mining from asteroids or the moon feasible? What would be the implications for economic growth and the environment? This paper provides stylized facts about cost trends, geology, and the environmental impact of mining on Earth and potentially in Space. We extend a neoclassical growth model to investigate the transition from mining on Earth to Space. We find that such a transition could potentially allow for continued growth of metal use, while limiting environmental and social costs on Earth. Acknowledging the high uncertainty around the topic, our paper provides a starting point for research on how Space mining could contribute to sustainable growth on Earth.
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spelling pubmed-106149352023-10-31 Mining in space could spur sustainable growth Fleming, Maxwell Lange, Ian Shojaeinia, Sayeh Stuermer, Martin Proc Natl Acad Sci U S A Social Sciences Growth models with resources and environmental externalities typically assume that planet Earth is a closed economy. However, private firms like Blue Origin and SpaceX have reduced the cost of rocket launches by a factor of 20 over the last decade. What if these costs continue to decline, making mining from asteroids or the moon feasible? What would be the implications for economic growth and the environment? This paper provides stylized facts about cost trends, geology, and the environmental impact of mining on Earth and potentially in Space. We extend a neoclassical growth model to investigate the transition from mining on Earth to Space. We find that such a transition could potentially allow for continued growth of metal use, while limiting environmental and social costs on Earth. Acknowledging the high uncertainty around the topic, our paper provides a starting point for research on how Space mining could contribute to sustainable growth on Earth. National Academy of Sciences 2023-10-16 2023-10-24 /pmc/articles/PMC10614935/ /pubmed/37844231 http://dx.doi.org/10.1073/pnas.2221345120 Text en Copyright © 2023 the Author(s). Published by PNAS. https://creativecommons.org/licenses/by-nc-nd/4.0/This open access article is distributed under Creative Commons Attribution-NonCommercial-NoDerivatives License 4.0 (CC BY-NC-ND) (https://creativecommons.org/licenses/by-nc-nd/4.0/) .
spellingShingle Social Sciences
Fleming, Maxwell
Lange, Ian
Shojaeinia, Sayeh
Stuermer, Martin
Mining in space could spur sustainable growth
title Mining in space could spur sustainable growth
title_full Mining in space could spur sustainable growth
title_fullStr Mining in space could spur sustainable growth
title_full_unstemmed Mining in space could spur sustainable growth
title_short Mining in space could spur sustainable growth
title_sort mining in space could spur sustainable growth
topic Social Sciences
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10614935/
https://www.ncbi.nlm.nih.gov/pubmed/37844231
http://dx.doi.org/10.1073/pnas.2221345120
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