GSTM2022-27, updated on 30 Aug 2024
https://doi.org/10.5194/gstm2022-27
GRACE/GRACE-FO Science Team Meeting 2022
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Mass Change as a core element of NASA’s Earth System Observatory: update and progress on pre-formulation activities

David Wiese1, Charley Dunn1, Michael Gross1, Frank Webb1, Neil Dahya1, Andre Girerd1, Srinivas Bettadpur2, Bernard Bienstock1, Brent Ware1, Carmen Boening1, Jonathan Chrone3, Bryant Loomis4, Scott Luthcke4, Matthew Rodell4, Jeanne Sauber4, Nicole Herrmann5, and Lucia Tsaoussi5
David Wiese et al.
  • 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, United States of America
  • 2Center for Space Research, The University of Texas at Austin, Austin, Texas, United States of America
  • 3NASA Langley Research Center, Hampton, Virginia, United States of America
  • 4NASA Goddard Space Flight Center, Greenbelt, Maryland, United States of America
  • 5NASA Headquarters, Washington DC, United States of America

The 2017-2027 US National Academy of Sciences Decadal Survey (DS) for Earth Science and Applications from Space classified mass change as one of five Designated Observables having the highest priority in terms of Earth observations required to better understand the Earth system over the next decade.  In response to this designation, NASA initiated multi-center studies with an overarching goal of defining observing system architectures for each Designated Observable.  The Mass Change Designated Observable study concluded in 2021, after identifying a small subset of high value observing system architectures for further study during Pre-Phase A formulation.  Mass Change is in the process of concluding Pre-Phase A activities and transitioning to Phase A, after successfully passing a Mission Concept Review in June 2022.  The baseline architecture is a partnership between NASA and DLR with an architecture design similar in nature to GRACE-FO.  This concept meets the primary goal of maintaining continuity in the mass change data record.  In parallel, ESA is continuing their Phase A studies focused on launching an inclined pair of satellites to complement this baseline architecture which would result in a demonstration of the Bender constellation and thus enhance the overall science and applications value of the observing system.  In this talk, an overview of Mass Change pre-formulation activities will be provided, as well as a status update on next steps and associated milestones.

How to cite: Wiese, D., Dunn, C., Gross, M., Webb, F., Dahya, N., Girerd, A., Bettadpur, S., Bienstock, B., Ware, B., Boening, C., Chrone, J., Loomis, B., Luthcke, S., Rodell, M., Sauber, J., Herrmann, N., and Tsaoussi, L.: Mass Change as a core element of NASA’s Earth System Observatory: update and progress on pre-formulation activities, GRACE/GRACE-FO Science Team Meeting 2022, Potsdam, Germany, 18–20 Oct 2022, GSTM2022-27, https://doi.org/10.5194/gstm2022-27, 2022.

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