volume 23 publication number e16

How we can mine asteroids for space food

Publication typeJournal Article
Publication date2024-10-03
scimago Q3
wos Q3
SJR0.309
CiteScore3.7
Impact factor1.0
ISSN14735504, 15743006, 14753006
Abstract

To deeply explore the solar system, it will be necessary to become less reliant on the resupply tether to Earth. An approach explored in this study is to convert hydrocarbons in asteroids to human edible food. After comparing the experimental pyrolysis breakdown products, which were able to be converted to biomass using a consortia, it was hypothesized that equivalent chemicals found on asteroids could also be converted to biomass with the same nutritional content as the pyrolyzed products. This study is a mathematical exercise that explores the potential food yield that could be produced from these methodologies. This study uses the abundance of aliphatic hydrocarbons in the Murchison meteorite (>35 ppm) as a baseline for the calculations, representing the minimum amount of organic matter that could theoretically be attributed to biomass production. Calculations for the total carbon in solvent-insoluble organic matter (IOM) represent the maximum amount of organic matter that could theoretically be attributed to food production. These two values will provide a range of realistic yields to determine how much food could theoretically be extractable from an asteroid. The results of this study found that if only the aliphatic hydrocarbons can be converted into biomass (minimum scenario) the resulting mass of edible biomass extractable from asteroid Bennu ranges from 5.070 × 107 g to 2.390 × 108 g. If the biomass extraction process, however, is more efficient, and all IOM is converted into edible biomass (maximum scenario), then the mass of edible biomass extractable from asteroid Bennu ranges from 1.391 × 109 g to 6.556 × 109 g. This would provide between 5.762 × 108 and 1.581 × 1010 calories that is enough to support between 600 and 17 000 astronaut life years. The asteroid mass needed to support one astronaut for one year is between 160 000 metric tons and 5000 metric tons. Based on these results, this approach of using carbon in asteroids to provide a distributed food source for humans appears promising, but there are substantial areas of future work.

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Pilles E. et al. How we can mine asteroids for space food // International Journal of Astrobiology. 2024. Vol. 23. e16
GOST all authors (up to 50) Copy
Pilles E., Nicklin R. I., Pearce J. How we can mine asteroids for space food // International Journal of Astrobiology. 2024. Vol. 23. e16
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TY - JOUR
DO - 10.1017/s1473550424000119
UR - https://www.cambridge.org/core/product/identifier/S1473550424000119/type/journal_article
TI - How we can mine asteroids for space food
T2 - International Journal of Astrobiology
AU - Pilles, Eric
AU - Nicklin, Richard I.
AU - Pearce, Joshua
PY - 2024
DA - 2024/10/03
PB - Cambridge University Press
VL - 23
SN - 1473-5504
SN - 1574-3006
SN - 1475-3006
ER -
BibTex
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@article{2024_Pilles,
author = {Eric Pilles and Richard I. Nicklin and Joshua Pearce},
title = {How we can mine asteroids for space food},
journal = {International Journal of Astrobiology},
year = {2024},
volume = {23},
publisher = {Cambridge University Press},
month = {oct},
url = {https://www.cambridge.org/core/product/identifier/S1473550424000119/type/journal_article},
pages = {e16},
doi = {10.1017/s1473550424000119}
}