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Published August 2024 | Published
Journal Article Open

Radar for Europa Assessment and Sounding: Ocean to Near-Surface (REASON)

Blankenship, Donald D. ORCID icon
Moussessian, Alina
Chapin, Elaine
Young, Duncan A. ORCID icon
Wesley Patterson, G.
Plaut, Jeffrey J. ORCID icon
Freedman, Adam P.
Schroeder, Dustin M. ORCID icon
Grima, Cyril ORCID icon
Steinbrügge, Gregor ORCID icon
Soderlund, Krista M. ORCID icon
Ray, Trina
Richter, Thomas G.
Jones-Wilson, Laura ORCID icon
Wolfenbarger, Natalie S. ORCID icon
Scanlan, Kirk M. ORCID icon
Gerekos, Christopher ORCID icon
Chan, Kristian ORCID icon
Seker, Ilgin ORCID icon
Haynes, Mark S. ORCID icon
Barr Mlinar, Amy C. ORCID icon
Bruzzone, Lorenzo ORCID icon
Campbell, Bruce A.
Carter, Lynn M. ORCID icon
Elachi, Charles1 ORCID icon
Gim, Yonggyu
Hérique, Alain ORCID icon
Hussmann, Hauke ORCID icon
Kofman, Wlodek ORCID icon
Kurth, William S. ORCID icon
Mastrogiuseppe, Marco ORCID icon
McKinnon, William B. ORCID icon
Moore, Jeffrey M.
Nimmo, Francis ORCID icon
Paty, Carol ORCID icon
Plettemeier, Dirk ORCID icon
Schmidt, Britney E. ORCID icon
Zolotov, Mikhail Y. ORCID icon
Schenk, Paul M. ORCID icon
Collins, Simon
Figueroa, Harry
Fischman, Mark
Tardiff, Eric ORCID icon
Berkun, Andy
Paller, Mimi
Hoffman, James P.
Kurum, Andy
Sadowy, Gregory A.
Wheeler, Kevin B.
Decrossas, Emmanuel
Hussein, Yasser
Jin, Curtis ORCID icon
Boldissar, Frank
Chamberlain, Neil
Hernandez, Brenda
Maghsoudi, Elham
Mihaly, Jonathan
Worel, Shana
Singh, Vik
Pak, Kyung
Tanabe, Jordan
Johnson, Robert
Ashtijou, Mohammad
Alemu, Tafesse
Burke, Michael
Custodero, Brian
Tope, Michael C.
Hawkins, David ORCID icon
Aaron, Kim
Delory, Gregory T. ORCID icon
Turin, Paul S.
Kirchner, Donald L.
Srinivasan, Karthik
Xie, Julie
Ortloff, Brad
Tan, Ian
Noh, Tim
Clark, Duane ORCID icon
Duong, Vu
Joshi, Shivani ORCID icon
Lee, Jeng
Merida, Elvis
Akbar, Ruzbeh
Duan, Xueyang ORCID icon
Fenni, Ines ORCID icon
Sanchez-Barbetty, Mauricio
Parashare, Chaitali
Howard, Duane C.
Newman, Julie
Cruz, Marvin G.
Barabas, Neil J.
Amirahmadi, Ahmadreza
Palmer, Brendon ORCID icon
Gawande, Rohit S.
Milroy, Grace
Roberti, Rick
Leader, Frank E.
West, Richard D. ORCID icon
Martin, Jan
Venkatesh, Vijay
Adumitroaie, Virgil ORCID icon
Rains, Christine
Quach, Cuong
Turner, Jordi E.
O'Shea, Colleen M.
Kempf, Scott D. ORCID icon
Ng, Gregory ORCID icon
Buhl, Dillon P.
Urban, Timothy J.
  • 1. ROR icon California Institute of Technology

Abstract

AbstractThe Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) is a dual-frequency ice-penetrating radar (9 and 60 MHz) onboard the Europa Clipper mission. REASON is designed to probe Europa from exosphere to subsurface ocean, contributing the third dimension to observations of this enigmatic world. The hypotheses REASON will test are that (1) the ice shell of Europa hosts liquid water, (2) the ice shell overlies an ocean and is subject to tidal flexing, and (3) the exosphere, near-surface, ice shell, and ocean participate in material exchange essential to the habitability of this moon. REASON will investigate processes governing this material exchange by characterizing the distribution of putative non-ice material (e.g., brines, salts) in the subsurface, searching for an ice–ocean interface, characterizing the ice shell's global structure, and constraining the amplitude of Europa's radial tidal deformations. REASON will accomplish these science objectives using a combination of radar measurement techniques including altimetry, reflectometry, sounding, interferometry, plasma characterization, and ranging. Building on a rich heritage from Earth, the moon, and Mars, REASON will be the first ice-penetrating radar to explore the outer solar system. Because these radars are untested for the icy worlds in the outer solar system, a novel approach to measurement quality assessment was developed to represent uncertainties in key properties of Europa that affect REASON performance and ensure robustness across a range of plausible parameters suggested for the icy moon. REASON will shed light on a never-before-seen dimension of Europa and – in concert with other instruments on Europa Clipper – help to investigate whether Europa is a habitable world.

Copyright and License

© The Author(s) 2024. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

Acknowledgement

This work was supported by NASA through the Europa Clipper Project (80NM0018F0615). The REASON radar was designed, built, and tested at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). REASON science was supported by a contract with Marshall Space Flight Center (NNM16AA26C). This is UTIG contribution 3970. The contributions of Mauricio Sanchez-Barbetty, Duane C. Howard, and Julie Newman were made during their time as employees of the Jet Propulsion Laboratory. We acknowledge the support of the NASA Instrument Concepts for Europa Exploration (ICEE) program (13-ICEE13-18) for the development and field validation of techniques ultimately employed by the REASON investigation and thank the G. Unger Vetlesen foundation for their contribution to validation of terrestrial models for Europa’s ice shell. We would like to thank L3Harris Cincinnati Electronics Corporation and Wenzel Associates for their dedication in developing and building the DPUs and Synthesizers, respectively. Additionally, we would like to extend our gratitude to James Chinn, Wousik Kim, Allen Andersen, Dennis Thorbourn, and Eduardo Martin of JPL as well as Stephen Brown, Kenneth O’Connor, and Robert Meloy of GSFC for their invaluable help with IESD analysis and testing. We also want to thank the Space Simulator Laboratory at APL for their support during the cryogenics test campaign. Finally, we are grateful to Sean Peters, Anna Broome, and Thomas Teisberg for their feedback on this manuscript.

Conflict of Interest

The authors have no competing interests to declare that are relevant to the content of this article.

Additional Information

Europa Clipper: A Mission to Explore Ocean World Habitability

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Created:
July 2, 2024
Modified:
July 2, 2024