A Search for Extraterrestrial Eukaryotes: Biological and Planetary Science Aspects

Abstract One pressing question in bioastronomy is to attempt to devise assays in the search for extraterrestrial eukaryotes (SETE). In the positive case of encountering a fossil of a certain microorganism, it is not yet clear how to identify it in an unequivocal manner, even if found arrested and pr...

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Published in:International Astronomical Union Colloquium
Main Author: Chela-Flores, Julian
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 1997
Subjects:
Ice
Online Access:http://dx.doi.org/10.1017/s0252921100015050
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spelling crcambridgeupr:10.1017/s0252921100015050 2024-03-03T08:45:18+00:00 A Search for Extraterrestrial Eukaryotes: Biological and Planetary Science Aspects Chela-Flores, Julian 1997 http://dx.doi.org/10.1017/s0252921100015050 en eng Cambridge University Press (CUP) International Astronomical Union Colloquium volume 161, page 525-532 ISSN 0252-9211 journal-article 1997 crcambridgeupr https://doi.org/10.1017/s0252921100015050 2024-02-08T08:30:59Z Abstract One pressing question in bioastronomy is to attempt to devise assays in the search for extraterrestrial eukaryotes (SETE). In the positive case of encountering a fossil of a certain microorganism, it is not yet clear how to identify it in an unequivocal manner, even if found arrested and preserved in the midst of biological activity, as in some known Archean sediments on Earth. On the other hand, for living microorganisms the present approach may have some advantages over the straightforward probe of the morphological features of the putative eukaryote, as we argue that we are not constrained to base identification on morphological properties, such as the presence of organelles, which are known to be missing in some higher taxa. We sketch a possible experimental set-up required for a robot to investigate whether eukaryogenesis has already taken place in Mars or Europa. Besides, we also discuss the biological and astronomical implications of a SETE program. Previous observation and theoretical work have suggested that underneath the ice crust of the Jovian satellite Europa there may be an ocean of liquid water. We therefore argue that as hot springs may be present at the bottom of that ocean, eukaryotes should be searched for, not only deep in the Martian permafrost, as discussed by others, but a SETE program should be extended to the aquatic environment of the Jovian satellite as well. Our current work emphasising gene silencing, may suggest how to decide on the degree evolution which microbiota may have reached in the Europa ocean, a topic which deserves our attention, as eukaryogenesis is the process which introduced the basic cellular plan of those Earth-bound organisms that have been raised to the level of intelligent beings. We make a specific suggestion for a robotic investigation of eukaryogenesis in solar system exploration. Article in Journal/Newspaper Ice permafrost Cambridge University Press International Astronomical Union Colloquium 161 525 532
institution Open Polar
collection Cambridge University Press
op_collection_id crcambridgeupr
language English
description Abstract One pressing question in bioastronomy is to attempt to devise assays in the search for extraterrestrial eukaryotes (SETE). In the positive case of encountering a fossil of a certain microorganism, it is not yet clear how to identify it in an unequivocal manner, even if found arrested and preserved in the midst of biological activity, as in some known Archean sediments on Earth. On the other hand, for living microorganisms the present approach may have some advantages over the straightforward probe of the morphological features of the putative eukaryote, as we argue that we are not constrained to base identification on morphological properties, such as the presence of organelles, which are known to be missing in some higher taxa. We sketch a possible experimental set-up required for a robot to investigate whether eukaryogenesis has already taken place in Mars or Europa. Besides, we also discuss the biological and astronomical implications of a SETE program. Previous observation and theoretical work have suggested that underneath the ice crust of the Jovian satellite Europa there may be an ocean of liquid water. We therefore argue that as hot springs may be present at the bottom of that ocean, eukaryotes should be searched for, not only deep in the Martian permafrost, as discussed by others, but a SETE program should be extended to the aquatic environment of the Jovian satellite as well. Our current work emphasising gene silencing, may suggest how to decide on the degree evolution which microbiota may have reached in the Europa ocean, a topic which deserves our attention, as eukaryogenesis is the process which introduced the basic cellular plan of those Earth-bound organisms that have been raised to the level of intelligent beings. We make a specific suggestion for a robotic investigation of eukaryogenesis in solar system exploration.
format Article in Journal/Newspaper
author Chela-Flores, Julian
spellingShingle Chela-Flores, Julian
A Search for Extraterrestrial Eukaryotes: Biological and Planetary Science Aspects
author_facet Chela-Flores, Julian
author_sort Chela-Flores, Julian
title A Search for Extraterrestrial Eukaryotes: Biological and Planetary Science Aspects
title_short A Search for Extraterrestrial Eukaryotes: Biological and Planetary Science Aspects
title_full A Search for Extraterrestrial Eukaryotes: Biological and Planetary Science Aspects
title_fullStr A Search for Extraterrestrial Eukaryotes: Biological and Planetary Science Aspects
title_full_unstemmed A Search for Extraterrestrial Eukaryotes: Biological and Planetary Science Aspects
title_sort search for extraterrestrial eukaryotes: biological and planetary science aspects
publisher Cambridge University Press (CUP)
publishDate 1997
url http://dx.doi.org/10.1017/s0252921100015050
genre Ice
permafrost
genre_facet Ice
permafrost
op_source International Astronomical Union Colloquium
volume 161, page 525-532
ISSN 0252-9211
op_doi https://doi.org/10.1017/s0252921100015050
container_title International Astronomical Union Colloquium
container_volume 161
container_start_page 525
op_container_end_page 532
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