Tait, Kimberly TMcCubbin, Francis M.Smith, Caroline LAgee, Carl B.Busemann, HennerCavalazzi, BarbaraDebaille, VincianeHutzler, AuroreUsui, TomohiroKminek, GerhardMeyer, Michael ABeaty, David WCarrier, Brandi LeeHaltigin, TimothyHays, Lindsay ECockell, Charles S.Glavin, Daniel P.Grady, Monica M.Hauber, ErnstMarty, BernardPratt, Lisa MRegberg, Aaron B.Smith, Alvin LSummons, Roger E.Swindle, Timothy DTosca, Nicholas J.Udry, AryaVelbel, Michael A.Wadhwa, MeenakshiWestall, FrancesZorzano, Maria-Paz2023-07-102023-07-102022-06-02Tait, K T, McCubbin, F M, Smith, C L, Agee, C B, Busemann, H, Cavalazzi, B, Debaille, V, Hutzler, A, Usui, T, Kminek, G, Meyer, M A, Beaty, D W, Carrier, B L, Haltigin, T, Hays, L E, Cockell, C S, Glavin, D P, Grady, M M, Hauber, E, Marty, B, Pratt, L M, Regberg, A B, Smith, A L, Summons, R E, Swindle, T D, Tosca, N J, Udry, A, Velbel, M A, Wadhwa, M, Westall, F & Zorzano, M-P 2022, 'Preliminary Planning for Mars Sample Return (MSR) Curation Activities in a Sample Receiving Facility', Astrobiology, vol. 22, no. S1, pp. s57-s80. https://doi.org/10.1089/AST.2021.01051531-1074RIS: urn:4EA444C4AE5CBBF8793675B64B125926https://hdl.handle.net/2164/21167Acknowledgments We would like to thank the entire MSPG-2 committee for their input and discussions during our bi-weekly meetings, and especially Gerhard Kminek, Tim Haltigin, Nicholas Tosca, and Michael Velbel for their input on this document. We especially acknowledge the subject matter experts Professor Ben Weiss (MIT) and Dr. Rohit Bhartia (Photon Systems Inc) for their important input on magnetometers and Deep UV Fluorescence, respectively. We also thank Dr. Paul Northrup and Dr. Mark Rivers for their input on synchrotron radiation techniques and Dr. Juliane Gross (Rutgers University/NASA Johnson Space Center) and Dr. Paul Lucey (University of Hawaii, Manoa) for their discussions on Multispectral Imaging and Hyperspectral Scanning and as well Dr. Ryan Ziegler and Scott Eckley (NASA, Johnson Space Center) for discussions and input on X-ray Computed Tomography. We also appreciate comments from an SRF implementation team coordinated by Richard Mattingly. The decision to implement Mars Sample Return will not be finalized until NASA’s completion of the National Environmental Policy Act (NEPA) process. This document is being made available for planning and information purposes only. Disclosure Statement No competing interests. Funding Information A portion of this work was funded by the National Aeronautics and Space Administration (NASA) and the European Space Agency (ESA). Acknowledgments We would like to thank the entire MSPG-2 committee for their input and discussions during our bi-weekly meetings, and especially Gerhard Kminek, Tim Haltigin, Nicholas Tosca, and Michael Velbel for their input on this document. We especially acknowledge the subject matter experts Professor Ben Weiss (MIT) and Dr. Rohit Bhartia (Photon Systems Inc) for their important input on magnetometers and Deep UV Fluorescence, respectively. We also thank Dr. Paul Northrup and Dr. Mark Rivers for their input on synchrotron radiation techniques and Dr. Juliane Gross (Rutgers University/NASA Johnson Space Center) and Dr. Paul Lucey (University of Hawaii, Manoa) for their discussions on Multispectral Imaging and Hyperspectral Scanning and as well Dr. Ryan Ziegler and Scott Eckley (NASA, Johnson Space Center) for discussions and input on X-ray Computed Tomography. We also appreciate comments from an SRF implementation team coordinated by Richard Mattingly. The decision to implement Mars Sample Return will not be finalized until NASA’s completion of the National Environmental Policy Act (NEPA) process. This document is being made available for planning and information purposes only. Disclosure Statement No competing interests. Funding Information A portion of this work was funded by the National Aeronautics and Space Administration (NASA) and the European Space Agency (ESA).241195780engQB AstronomyQBJournal article10.1089/AST.2021.010522