extraterrestrial sample curation
{{Short description|Use and preservation of extraterrestrial samples}}
Image:Lunar Sample Processing Facility NASA JSC DSCN0202.JPG (ARES)]]
The curation of extraterrestrial samples (astromaterials) obtained by sample-return missions takes place at facilities specially designed to preserve both the sample integrity and protect the Earth. Astromaterials are classified as either non-restricted or restricted, depending on the nature of the Solar System body. Non-restricted samples include the Moon, asteroids, comets, solar particles and space dust. Restricted bodies include planets or moons suspected to have either past or present habitable environments to microscopic life, and therefore must be treated as extremely biohazardous.
Overview
Spacecraft instruments are subject to mass and power constraints, in addition to the limitations imposed by the extreme environment of outer space on the sensitive science instruments, so bringing extraterrestrial material to Earth is desired for extensive scientific analyses. For the purpose of planetary protection, astromaterial samples brought to Earth by sample-return missions must be received and curated in a specially-designed and equipped biocontainment facility that must also double as a cleanroom to preserve the science value of the samples.
Samples brought from non-restricted bodies such as the Moon, asteroids, comets, solar particles and space dust, are processed at specialized facilities rated Biosafety level-3 (BSL-3). Samples brought to Earth from a planet or moon suspected to have either past or present habitable environments to microscopic life would make it a Category V body, and must be curated at facilities rated Biosafety level-4 (BSL-4), as agreed in the Article IX of the Outer Space Treaty.s:Outer Space Treaty of 1967#Article IXFull text of the Outer Space Treaty [http://www.unoosa.org/oosa/en/SpaceLaw/gares/html/gares_21_2222.html Treaty on Principles Governing the Activities of States in the Exploration and Use of Outer Space, including the Moon and Other Celestial Bodies] {{webarchive|url=https://web.archive.org/web/20130708075800/http://www.unoosa.org/oosa/en/SpaceLaw/gares/html/gares_21_2222.html |date=2013-07-08 }} - See Article IX{{cite web | url = http://www.cnes.fr/web/CNES-en/5210-planetary-protection-treaties-and-recommendations.php | title = Planetary protection treaties and recommendations | access-date = 2012-09-11 | author = Centre National d’Etudes Spatiales (CNES) | date = 2008 | archive-date = 2014-08-20 | archive-url = https://web.archive.org/web/20140820211950/http://www.cnes.fr/web/CNES-en/5210-planetary-protection-treaties-and-recommendations.php | url-status = dead }} However, the existing BSL-4 facilities in the world do not have the complex requirements to ensure the preservation and protection of Earth and the sample simultaneously.{{Cite web |url=https://www.space.com/7625-protect-mars-samples-earth.html |title=How to Protect Mars Samples on Earth |first=Jeremy |last=Hsu |work=Space.com |date=3 December 2009}} While existing BSL-4 facilities deal primarily with fairly well-known organisms, a BSL-4 facility focused on extraterrestrial samples must pre-plan the systems carefully while being mindful that there will be unforeseen issues during sample evaluation and curation that will require independent thinking and solutions.[https://www.lpi.usra.edu/meetings/lifedetection2012/pdf/6013.pdf Planning for the Analytic Environment to Conduct Life Detection Experiments on Samples Returned from Mars: Observations and Issues (2012)] D. S. Bass, D. W. Beaty, C. C. Allen, A. C. Allwood, L. E. Borg, K. E. Buxbaum1, J. A. Hurowitz and M. D. Schulte. Lunar and Planetary Institute. 2012. Accessed: 19 August 2018. A challenge is that, while it is relatively easy to simply contain the samples once returned to Earth, researchers will want to take a portion and perform analyses. During all these handling procedures, the samples would need to be protected from Earthly contamination and from contact with the atmosphere.{{cite report |title=Mars Sample Return Receiving Facility - A Draft Test Protocol for Detecting Possible Biohazards in Martian Samples Returned to Earth |year=2002 |url=http://www.lpi.usra.edu/pss/presentations/200803/04-Atlas-PPSonMSR.pdf| quote=A Sample Return Facility will require combining technologies used for constructing maximum containment laboratories (e.g. Biosafety level 4 labs) with cleanroom technologies which will be needed to protect the Mars samples from Earth contamination.}}[http://www.marsinstitute.info/epo/docs/draft_protocol.pdf A Draft Test Protocol for Detecting Possible Biohazards in Martian Samples Returned to Earth] {{webarchive|url=https://web.archive.org/web/20060222131531/http://www.marsinstitute.info/epo/docs/draft_protocol.pdf |date=2006-02-22 }}[http://www.lpi.usra.edu/meetings/lpsc2005/pdf/1395.pdf Cleanroom Robotics -Appropriate Technology for a Sample Receiving Facility]. 2005.{{Cite web |url=http://www.nap.edu/reports/13117/App%20G%2008_Mars-Sample-Return-Orbiter.pdf |title=2010 Mars Sample Return Orbiter decadal survey |access-date=2018-09-26 |archive-date=2017-05-08 |archive-url=https://web.archive.org/web/20170508063742/https://www.nap.edu/reports/13117/App%20G%2008_Mars-Sample-Return-Orbiter.pdf |url-status=dead }}
Non-restricted materials
File:OSIRIS-REx Sample Return (NHQ202309240002).jpg's Sample Return Capsule in Utah after reentry to Earth{{cite news |last=Kuthunur |first=Sharmila |title='What is that material?': Potentially hazardous asteroid Bennu stumps scientists with its odd makeup - Scientists found signs of organic molecules in the first samples of potentially hazardous asteroid Bennu, as well as a 'head scratching' material that has yet to be identified. |url=https://www.livescience.com/space/space-exploration/what-is-that-material-potentially-hazardous-asteroid-bennu-stumps-scientists-with-its-odd-makeup |date=13 December 2023 |work=LiveScience |url-status=live |archiveurl=https://archive.today/20231214014121/https://www.livescience.com/space/space-exploration/what-is-that-material-potentially-hazardous-asteroid-bennu-stumps-scientists-with-its-odd-makeup |archivedate=14 December 2023 |accessdate=13 December 2023 }}{{cite news |last=Rabie |first=Passant |title=It's Been 2 Months. Why Can't NASA Open the Asteroid Sample Container? - The space agency is having to develop new tools to crack open the canister containing bits from asteroid Bennu |url=https://gizmodo.com/nasa-osiris-rex-asteroid-samples-bennu-stuck-container-1851102598 |date=15 December 2023 |work=Gizmodo |url-status=live |archiveurl=https://archive.today/20231215230642/https://gizmodo.com/nasa-osiris-rex-asteroid-samples-bennu-stuck-container-1851102598 |archivedate=15 December 2023 |accessdate=16 December 2023 }}]]
As of 2019, only the Japanese space agency JAXA and the United States space agency NASA operate BSL-3 laboratories in the world exclusively dedicated to the curation of samples from non-restricted bodies.{{Cite web |url=http://www.planetary.org/blogs/jason-davis/why-sample-return.html |title=What's the benefit of sample-return? |first=Jason |last=Davis |work=The Planetary Society |date=5 July 2018}}{{cite journal|doi=10.1016/j.chemer.2010.12.003|title=Curating NASA's extraterrestrial samples—Past, present, and future|journal=Geochemistry|volume=71|issue=1|pages=1–20|year=2011|last1=Allen|first1=Carlton|last2=Allton|first2=Judith|last3=Lofgren|first3=Gary|last4=Righter|first4=Kevin|last5=Zolensky|first5=Michael|bibcode=2011ChEG...71....1A|hdl=2060/20100042395|hdl-access=free}}[https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/20160006349.pdf Curating NASA's Future Extraterrestrial Samplke COllections: How do we achieve maximum proficiency?] (PDF). Francis McCubbin, etal. 41st COSPAR Scientific Assembly 2016. The key feature of JAXA's curation facility, the Extraterrestrial Sample Curation Center, is the ability to observe, take out a portion and preserve a precious return-sample without being exposed to the atmosphere and other contaminants.[https://www.nipr.ac.jp/symposium2014/program/abstract/OA_Abe_00323_01.pdf Current status of JAXA's Extraterrestrial Sample Curation Center]. (PDF). M. Abe, T. Yada, M. Uesugi, Y. Karouji, A. Nakato, K. Kumagai, and T. Okada1. 2014.
The Luna Soviet missions samples are studied and stored at the Vernadsky Institute of Geochemistry and Analytical Chemistry at the Russian Academy of Sciences.[http://www.euro-cares.eu/files/Submitted%20Deliverables/D6.3%20Transport.pdf Transport to Curation Facility]. Euro-CARES. Andrea Longobardo, Fabrizio Dirri, Ernesto Palomba. 31 October 2016.
Restricted materials
File:NIAID Integrated Research Facility - Positive Pressure Personnel Suit.jpg
Return-samples obtained from a Category V body, must be curated at facilities rated Biosafety level-4 (BSL-4). Because the existing BSL-4 facilities in the world do not have the complex requirements to ensure the preservation and protection of Earth and the sample simultaneously, there are currently at least two proposals to build a BSL-4 facility dedicated to curation of restricted (potentially biohazard) extraterrestrial materials.
The first is the European Sample Curation Facility (ESCF),[https://ttu-ir.tdl.org/ttu-ir/bitstream/handle/2346/73091/ICES_2017_323.pdf EURO EURO-CARES Extraterrestrial Sample Curation Facility: Architecture as an enabler of science] {{Webarchive|url=https://web.archive.org/web/20180925220131/https://ttu-ir.tdl.org/ttu-ir/bitstream/handle/2346/73091/ICES_2017_323.pdf |date=2018-09-25 }}. (PDF) Aurore Hutzler, Emre Kilic, Allan Bennett, Ludovic Ferrière. 47th International Conference on Environmental Systems, 16–20 July 2017, Charleston, South Carolina. Document ICES-2017-323.[http://www.euro-cares.eu/ EURO-CARES.] European Curation of Astromaterials Returned from Exploration of Space. Accessed: 25 September 2018. proposed to be built in Vienna, would curate non-restricted samples as well as BSL-4 biocontainment of restricted material obtained from Category V bodies such as Mars, Europa, Enceladus, etc.
The other proposal is by NASA and is tentatively known as the Mars Sample-Return Receiving Facility (MSRRF).{{cite web|url=http://www.lpi.usra.edu/pss/presentations/200803/04-Atlas-PPSonMSR.pdf|title=Mars Sample Return Receiving Facility|publisher=NASA |author= Ronald Atlas|date=2002 }}{{cite web|url=https://www.lpi.usra.edu/pss/presentations/200803/04-Atlas-PPSonMSR.pdf| title=Mars Sample Return Receiving Facility |publisher=NASA |author= Ronald Atlas| date=2008}} At least three different designs were submitted in 2009. If funded, this American facility would be expected to take 7 to 10 years from design to completion,{{cite report |title=Assessment of Planetary Protection Requirements for Mars Sample Return Missions |publisher=National Research Council |year=2009 |chapter=7: "Sample-Receiving Facility and Program Oversight" |page=59 |chapter-url=http://www.nap.edu/openbook.php?record_id=12576&page=59}}[http://planetaryprotection.nasa.gov/summary/msr Mars Sample Return: Issues and Recommendations (Planetary Protection Office Summary)] Task Group on Issues in Sample Return. National Academies Press, Washington, DC (1997) and an additional two years is recommended for the staff to become proficient and accustomed to the facilities. NASA is also assessing a 2017 proposal to build a mobile and modular BSL-4 facility to secure a sample return capsule at the landing site to conduct preliminary biohazard analyses.[https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/20170001664.pdf Mobile/Modular BSL-4 Facilities for Meeting Restricted Earth Return Containment Requirements]. M. J. Calaway, F. M. McCubbin, J. H. Allton, R. A. Zeigler, and L. F. Pace. (PDF) NASA. 2017. After completion of biohazard testing, decisions could be made to sterilize the sample or transport all or portions to a permanent quarantine storage facility anywhere in the world.
The systems of such facilities must be able to contain unknown biohazards, as the sizes of any putative alien microorganisms or infectious agents are unknown. Ideally it should filter particles of 0.01 μm or larger, and release of a particle 0.05 μm or larger is unacceptable under any circumstance.[https://science.nasa.gov/media/medialibrary/2013/01/17/ESF_Mars_Sample_Return_backward_contamination_study.pdf European Science Foundation - Mars Sample Return backward contamination - Strategic advice and requirements] {{webarchive|url=https://web.archive.org/web/20160602150139/http://science.nasa.gov/media/medialibrary/2013/01/17/ESF_Mars_Sample_Return_backward_contamination_study.pdf |date=2016-06-02 }} The reason for this extremely small size limit of 0.01 μm is for consideration of gene transfer agents (GTAs) which are virus-like particles that are produced by some microorganisms that package random segments of DNA capable of horizontal gene transfer. These randomly incorporate segments of the host genome and can transfer them to other evolutionarily distant hosts, and do that without killing the new host. In this way many archaea and bacteria can swap DNA with each other. This raises the possibility that Martian life, if it has a common origin with Earth life in the distant past, could swap DNA with Earth microorganisms in the same way. Another reason for the 0.01 μm limit is because of the discovery of ultramicrobacteria as small as 0.2 μm across.
Robotic advocates consider that humans represent a significant source of contamination for the samples, and that a BSL-4 facility with robotic systems is the best way forward.
See also
{{Portal|Astronomy|Biology}}
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- {{annotated link|Astrobiology}}
- {{annotated link|Biocontainment}}
- {{annotated link|Biological hazard}}
- {{annotated link|Mars sample-return mission}}
- {{annotated link|Planetary geology}}
- {{annotated link|Safety engineering}}
- {{annotated link|Select agent}}
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References
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{{Astrobiology}}
{{Exoplanet}}
{{U.S. biological defense}}
{{Molecules detected in outer space}}