A Submersible, Off-Axis Holographic Microscope for Detection of Microbial Motility and Morphology in Aqueous and Icy Environments
Abstract
Sea ice is an analog environment for several of astrobiology's near-term targets: Mars, Europa, Enceladus, and perhaps other Jovian or Saturnian moons. Microorganisms, both eukaryotic and prokaryotic, remain active within brine channels inside the ice, making it unnecessary to penetrate through to liquid water below in order to detect life. We have developed a submersible digital holographic microscope (DHM) that is capable of resolving individual bacterial cells, and demonstrated its utility for immediately imaging samples taken directly from sea ice at several locations near Nuuk, Greenland. In all samples, the appearance and motility of eukaryotes were conclusive signs of life. The appearance of prokaryotic cells alone was not sufficient to confirm life, but when prokaryotic motility occurred, it was rapid and conclusive. Warming the samples to above-freezing temperatures or supplementing with serine increased the number of motile cells and the speed of motility; supplementing with serine also stimulated chemotaxis. These results show that DHM is a useful technique for detection of active organisms in extreme environments, and that motility may be used as a biosignature in the liquid brines that persist in ice. These findings have important implications for the design of missions to icy environments and suggest ways in which DHM imaging may be integrated with chemical life-detection suites in order to create more conclusive life detection packages.
Additional Information
© 2016 Lindensmith et al. This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. Received: November 17, 2015. Accepted: January 7, 2016. Published: January 26, 2016. This work was supported by the Gordon and Betty Moore Foundation (GBMF) grant numbers 4037 (McGill University, JN, subcontract to University of Washington, JWD, GMS) and 4038 (California Institute of Technology, CAL, SR, MB, JKW, ES). The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript. We thank Ivali Lennert, Carl Isaksen and Malene Simon of the Greenland Climate Research Center in Nuuk, and Shelly Carpenter, Kelsey Ammondson, and Stanley Ammondson for assistance in the field. We thank Morteza Gharib for providing laboratory space and facilities on the Caltech campus to support this work. We thank Shelly Carpenter for generating Fig 1, and the reviewer who assisted in identifying the organisms in Fig 10. Author Contributions: Conceived and designed the experiments: JWD GMS JLN CAL. Performed the experiments: CAL SR GMS JWD JLN. Analyzed the data: GMS JLN. Contributed reagents/materials/analysis tools: MB ES JKW. Wrote the paper: JLN JWD. Data Availability: All raw hologram files and metadata for their reconstruction are available from the Dryad database (doi:10.5061/dryad.rc63v). Additional files, including some reconstructions, are available on our public Motility Database found at motility.caltech.edu. The authors have declared that no competing interests exist.Attached Files
Published - journal.pone.0147700.pdf
Supplemental Material - journal.pone.0147700.s001.MOV
Supplemental Material - journal.pone.0147700.s002.AVI
Supplemental Material - journal.pone.0147700.s003.AVI
Supplemental Material - journal.pone.0147700.s004.AVI
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Supplemental Material - journal.pone.0147700.s007.AVI
Supplemental Material - journal.pone.0147700.s008.AVI
Supplemental Material - journal.pone.0147700.s009.AVI
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Additional details
- PMCID
- PMC4422661
- Eprint ID
- 64158
- Resolver ID
- CaltechAUTHORS:20160202-092152387
- 4037
- Gordon and Betty Moore Foundation
- 4038
- Gordon and Betty Moore Foundation
- Created
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2016-02-03Created from EPrint's datestamp field
- Updated
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2023-06-01Created from EPrint's last_modified field