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Article Dans Une Revue Astrobiology Année : 2022

COSPAR Sample Safety Assessment Framework (SSAF)

Gerhard Kminek
  • Fonction : Auteur
James N. Benardini
  • Fonction : Auteur
Frank E. Brenker
  • Fonction : Auteur
Timothy Brooks
  • Fonction : Auteur
Aaron S. Burton
  • Fonction : Auteur
Suresh Dhaniyala
  • Fonction : Auteur
Jason P. Dworkin
  • Fonction : Auteur
Jeffrey L. Fortman
  • Fonction : Auteur
Mihaela Glamoclija
  • Fonction : Auteur
Monica M. Grady
  • Fonction : Auteur
Heather V. Graham
  • Fonction : Auteur
Junichi Haruyama
  • Fonction : Auteur
Thomas L. Kieft
  • Fonction : Auteur
Marion Koopmans
  • Fonction : Auteur
Francis M. Mccubbin
  • Fonction : Auteur
Michael A. Meyer
  • Fonction : Auteur
Tullis C. Onstott
  • Fonction : Auteur
Neil Pearce
  • Fonction : Auteur
Lisa M. Pratt
  • Fonction : Auteur
Mark A. Sephton
  • Fonction : Auteur
Sandra Siljeström
  • Fonction : Auteur
Haruna Sugahara
  • Fonction : Auteur
Shino Suzuki
  • Fonction : Auteur
Yohey Suzuki
  • Fonction : Auteur
Michel Viso
  • Fonction : Auteur

Résumé

The Committee on Space Research (COSPAR) Sample Safety Assessment Framework (SSAF) has been developed by a COSPAR appointed Working Group. The objective of the sample safety assessment would be to evaluate whether samples returned from Mars could be harmful for Earth's systems (e.g., environment, biosphere, geochemical cycles). During the Working Group's deliberations, it became clear that a comprehensive assessment to predict the effects of introducing life in new environments or ecologies is difficult and practically impossible, even for terrestrial life and certainly more so for unknown extraterrestrial life. To manage expectations, the scope of the SSAF was adjusted to evaluate only whether the presence of martian life can be excluded in samples returned from Mars. If the presence of martian life cannot be excluded, a Hold & Critical Review must be established to evaluate the risk management measures and decide on the next steps. The SSAF starts from a positive hypothesis (there is martian life in the samples), which is complementary to the null-hypothesis (there is no martian life in the samples) typically used for science. Testing the positive hypothesis includes four elements: (1) Bayesian statistics, (2) subsampling strategy, (3) test sequence, and (4) decision criteria. The test sequence capability covers self-replicating and non-self-replicating biology and biologically active molecules. Most of the investigations associated with the SSAF would need to be carried out within biological containment. The SSAF is described in sufficient detail to support planning activities for a Sample Receiving Facility (SRF) and for preparing science announcements, while at the same time acknowledging that further work is required before a detailed Sample Safety Assessment Protocol (SSAP) can be developed. The three major open issues to be addressed to optimize and implement the SSAF are (1) setting a value for the level of assurance to effectively exclude the presence of martian life in the samples, (2) carrying out an analogue test program, and (3) acquiring relevant contamination knowledge from all Mars Sample Return (MSR) flight and ground elements. Although the SSAF was developed specifically for assessing samples from Mars in the context of the currently planned NASA-ESA MSR Campaign, this framework and the basic safety approach are applicable to any other Mars sample return mission concept, with minor adjustments in the execution part related to the specific nature of the samples to be returned. The SSAF is also considered a sound basis for other COSPAR Planetary Protection Category V, restricted Earth return missions beyond Mars. It is anticipated that the SSAF will be subject to future review by the various MSR stakeholders.
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insu-03748530 , version 1 (10-08-2022)

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Gerhard Kminek, James N. Benardini, Frank E. Brenker, Timothy Brooks, Aaron S. Burton, et al.. COSPAR Sample Safety Assessment Framework (SSAF). Astrobiology, 2022, 22, pp.S-186. ⟨10.1089/ast.2022.0017⟩. ⟨insu-03748530⟩
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