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Geophysical Observations of the 24 September 2023 OSIRIS-REx Sample Return Capsule Re-Entry

Authors :
Silber, Elizabeth A.
Bowman, Daniel C.
Carr, Chris G.
Eisenberg, David P.
Elbing, Brian R.
Fernando, Benjamin
Garcés, Milton A.
Haaser, Robert
Krishnamoorthy, Siddharth
Langston, Charles A.
Nishikawa, Yasuhiro
Webster, Jeremy
Anderson, Jacob F.
Arrowsmith, Stephen
Bazargan, Sonia
Beardslee, Luke
Beck, Brant
Bishop, Jordan W.
Blom, Philip
Bracht, Grant
Chichester, David L.
Christe, Anthony
Cummins, Kenneth
Cutts, James
Danielson, Lisa
Donahue, Carly
Eack, Kenneth
Fleigle, Michael
Fox, Douglas
Goel, Ashish
Green, David
Hasumi, Yuta
Hayward, Chris
Hicks, Dan
Hix, Jay
Horton, Stephen
Hough, Emalee
Huber, David P.
Hunt, Madeline A.
Inman, Jennifer
Islam, S. M. Ariful
Izraelevitz, Jacob
Jacob, Jamey D.
Clarke, Jacob
Johnson, James
KC, Real J.
Komjathy, Attila
Lam, Eric
LaPierre, Justin
Lewis, Kevin
Lewis, Richard D.
Liu, Patrick
Martire, Léo
McCleary, Meaghan
McGhee, Elisa A.
Mitra, Ipsita
Nag, Amitabh
Giraldo, Luis Ocampo
Pearson, Karen
Plaisir, Mathieu
Popenhagen, Sarah K.
Rassoul, Hamid
Giannone, Miro Ronac
Samnani, Mirza
Schmerr, Nicholas
Spillman, Kate
Srinivas, Girish
Takazawa, Samuel K.
Tempert, Alex
Turley, Reagan
Van Beek, Cory
Viens, Loïc
Walsh, Owen A.
Weinstein, Nathan
White, Robert
Williams, Brian
Wilson, Trevor C.
Wyckoff, Shirin
Yamamoto, Masa-yuki
Yap, Zachary
Yoshiyama, Tyler
Zeiler, Cleat
Publication Year :
2024

Abstract

Sample Return Capsules (SRCs) entering Earth's atmosphere at hypervelocity from interplanetary space are a valuable resource for studying meteor phenomena. The 24 September 2023 arrival of the OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) SRC provided an unprecedented chance for geophysical observations of a well-characterized source with known parameters, including timing and trajectory. A collaborative effort involving researchers from 16 institutions executed a carefully planned geophysical observational campaign at strategically chosen locations, deploying over 400 ground-based sensors encompassing infrasound, seismic, distributed acoustic sensing (DAS), and GPS technologies. Additionally, balloons equipped with infrasound sensors were launched to capture signals at higher altitudes. This campaign (the largest of its kind so far) yielded a wealth of invaluable data anticipated to fuel scientific inquiry for years to come. The success of the observational campaign is evidenced by the near-universal detection of signals across instruments, both proximal and distal. This paper presents a comprehensive overview of the collective scientific effort, field deployment, and preliminary findings. The early findings have the potential to inform future space missions and terrestrial campaigns, contributing to our understanding of meteoroid interactions with planetary atmospheres. Furthermore, the dataset collected during this campaign will improve entry and propagation models as well as augment the study of atmospheric dynamics and shock phenomena generated by meteoroids and similar sources.<br />Comment: 87 pages, 14 figures

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2407.02420
Document Type :
Working Paper
Full Text :
https://doi.org/10.3847/PSJ/ad5b5e