Characterizing biofilms and their associated biosignatures in an Arctic hypersaline cold spring Mars analog

The last surface-level aqueous environments on Mars were likely sulfurous brines that formed as the climate cooled and large bodies of water receded during the transition from the wet Noachian to the dry Hesperian (4.1 – 3.0 Gya). To understand the diversity of microorganisms that could have inhabit...

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Published in:ARPHA Conference Abstracts
Main Authors: Blenner-Hassett, Olivia, Altshuler, Ianina, Magnuson, Elisse, Whyte, Lyle
Format: Article in Journal/Newspaper
Language:unknown
Published: Pensoft Publishers 2023
Subjects:
Online Access:https://doi.org/10.3897/aca.6.e111363
id ftzenodo:oai:zenodo.org:10411948
record_format openpolar
spelling ftzenodo:oai:zenodo.org:10411948 2024-09-09T19:24:07+00:00 Characterizing biofilms and their associated biosignatures in an Arctic hypersaline cold spring Mars analog Blenner-Hassett, Olivia Altshuler, Ianina Magnuson, Elisse Whyte, Lyle 2023-10-18 https://doi.org/10.3897/aca.6.e111363 unknown Pensoft Publishers https://doi.org/10.3897/aca.6.e111363 oai:zenodo.org:10411948 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode ARPHA Conference Abstracts, 6, e111363, (2023-10-18) Astrobiology Mars Analogue Microbial Diversity Polar Microbiology info:eu-repo/semantics/article 2023 ftzenodo https://doi.org/10.3897/aca.6.e111363 2024-07-26T06:19:57Z The last surface-level aqueous environments on Mars were likely sulfurous brines that formed as the climate cooled and large bodies of water receded during the transition from the wet Noachian to the dry Hesperian (4.1 – 3.0 Gya). To understand the diversity of microorganisms that could have inhabited such environments and their associated biosignatures, we turn to analogous environments on Earth. Here we investigated biofilm communities and their associated biosignatures at Gypsum Hill, (GH), a perennial cold spring system located at nearly 80°N on Axel Heiberg Island in the Canadian high Arctic. The biofilms develop during the summer months alongside the oligotrophic and sulphur rich GH brines and spread out along the flood plains formed by meltwater and spring run-off. Our objective was to link the microbial community structure of the biofilms to geochemical changes across the GH site as an analog to the micro-niches that could have formed during the recession of an ancient Martian Ocean. We collected 14 morphologically distinct biofilms over two field season and found that minor variations in chemistry between proximal sites impacted community structure. 16S amplicon sequencing revealed that biofilms closest to outflow channels were dominated by sulfur oxidizing bacteria, suggesting that primary production may be driven by chemolithoautotrophy. The community structure shifted towards more heterotrophic and phototrophic populations the further the biofilms appeared from a spring source. Microbial eukaryotes at the GH site were investigated for the first time through 18S sequencing with diatoms and photoautotrophic algae dominating all biofilms. Lastly, we linked the biofilm communities to potential biosignatures by examining lipid profiles to help guide the search and identification of potential remnants of hypothetical ancient Martian life. Article in Journal/Newspaper Arctic Axel Heiberg Island Zenodo Arctic Heiberg ENVELOPE(13.964,13.964,66.424,66.424) Axel Heiberg Island ENVELOPE(-91.001,-91.001,79.752,79.752) Gypsum Hill ENVELOPE(-90.751,-90.751,79.402,79.402) ARPHA Conference Abstracts 6
institution Open Polar
collection Zenodo
op_collection_id ftzenodo
language unknown
topic Astrobiology
Mars Analogue
Microbial Diversity
Polar Microbiology
spellingShingle Astrobiology
Mars Analogue
Microbial Diversity
Polar Microbiology
Blenner-Hassett, Olivia
Altshuler, Ianina
Magnuson, Elisse
Whyte, Lyle
Characterizing biofilms and their associated biosignatures in an Arctic hypersaline cold spring Mars analog
topic_facet Astrobiology
Mars Analogue
Microbial Diversity
Polar Microbiology
description The last surface-level aqueous environments on Mars were likely sulfurous brines that formed as the climate cooled and large bodies of water receded during the transition from the wet Noachian to the dry Hesperian (4.1 – 3.0 Gya). To understand the diversity of microorganisms that could have inhabited such environments and their associated biosignatures, we turn to analogous environments on Earth. Here we investigated biofilm communities and their associated biosignatures at Gypsum Hill, (GH), a perennial cold spring system located at nearly 80°N on Axel Heiberg Island in the Canadian high Arctic. The biofilms develop during the summer months alongside the oligotrophic and sulphur rich GH brines and spread out along the flood plains formed by meltwater and spring run-off. Our objective was to link the microbial community structure of the biofilms to geochemical changes across the GH site as an analog to the micro-niches that could have formed during the recession of an ancient Martian Ocean. We collected 14 morphologically distinct biofilms over two field season and found that minor variations in chemistry between proximal sites impacted community structure. 16S amplicon sequencing revealed that biofilms closest to outflow channels were dominated by sulfur oxidizing bacteria, suggesting that primary production may be driven by chemolithoautotrophy. The community structure shifted towards more heterotrophic and phototrophic populations the further the biofilms appeared from a spring source. Microbial eukaryotes at the GH site were investigated for the first time through 18S sequencing with diatoms and photoautotrophic algae dominating all biofilms. Lastly, we linked the biofilm communities to potential biosignatures by examining lipid profiles to help guide the search and identification of potential remnants of hypothetical ancient Martian life.
format Article in Journal/Newspaper
author Blenner-Hassett, Olivia
Altshuler, Ianina
Magnuson, Elisse
Whyte, Lyle
author_facet Blenner-Hassett, Olivia
Altshuler, Ianina
Magnuson, Elisse
Whyte, Lyle
author_sort Blenner-Hassett, Olivia
title Characterizing biofilms and their associated biosignatures in an Arctic hypersaline cold spring Mars analog
title_short Characterizing biofilms and their associated biosignatures in an Arctic hypersaline cold spring Mars analog
title_full Characterizing biofilms and their associated biosignatures in an Arctic hypersaline cold spring Mars analog
title_fullStr Characterizing biofilms and their associated biosignatures in an Arctic hypersaline cold spring Mars analog
title_full_unstemmed Characterizing biofilms and their associated biosignatures in an Arctic hypersaline cold spring Mars analog
title_sort characterizing biofilms and their associated biosignatures in an arctic hypersaline cold spring mars analog
publisher Pensoft Publishers
publishDate 2023
url https://doi.org/10.3897/aca.6.e111363
long_lat ENVELOPE(13.964,13.964,66.424,66.424)
ENVELOPE(-91.001,-91.001,79.752,79.752)
ENVELOPE(-90.751,-90.751,79.402,79.402)
geographic Arctic
Heiberg
Axel Heiberg Island
Gypsum Hill
geographic_facet Arctic
Heiberg
Axel Heiberg Island
Gypsum Hill
genre Arctic
Axel Heiberg Island
genre_facet Arctic
Axel Heiberg Island
op_source ARPHA Conference Abstracts, 6, e111363, (2023-10-18)
op_relation https://doi.org/10.3897/aca.6.e111363
oai:zenodo.org:10411948
op_rights info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
op_doi https://doi.org/10.3897/aca.6.e111363
container_title ARPHA Conference Abstracts
container_volume 6
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