A Simplified Gravitational Reference Sensor for NASA’s Mass Change Mission and Beyond
- 1University of Florida, United States of America (jwconklin@ufl.edu)
- *A full list of authors appears at the end of the abstract
The University of Florida, is leading a team that includes Caltech/JPL, Ball Aerospace, Fibertek, Inc, CrossTrac Engineering, Texas A&M University, and the University of Central Florida to develop a Simplified Gravitational Reference Sensor (S-GRS), an ultra-precise inertial sensor optimized for future Earth geodesy missions. Inertial sensors like the S-GRS are used to measure or compensate for all non-gravitational accelerations of the host spacecraft so that they can be removed in the data analysis to recover spacecraft motion due to Earth’s gravity field, the main science observable. Low-low satellite-to-satellite tracking missions like GRACE-FO that utilize laser ranging interferometers are technologically limited by the acceleration noise performance of their electrostatic accelerometers, as well as temporal aliasing associated with Earth’s dynamic gravity field. The S-GRS is estimated to be at least 40 times more sensitive than the GRACE accelerometers and more than 500 times more sensitive if operated on a drag-compensated platform. The S-GRS concept is a simplified version of the flight-proven LISA Pathfinder GRS. Our performance estimates are based on models vetted during the LISA Pathfinder flight and the expected Earth orbiting spacecraft environment based on flight data from GRACE-FO. The improved performance is enabled by removing the small grounding wire used in the GRACE accelerometers and replacing it with a UV photoemission-based charge management system, enabling more massive test masses and larger gaps between the test mass and its housing. We have shown that the increased S-GRS performance allows future missions to take full advantage of the improved sensitivity of the GRACE-FO Laser Ranging Interferometer (LRI) over microwave ranging systems in the gravity recovery analysis. A specific version of the S-GRS, optimized for NASA’s Mass Change Mission, is also under study as part of that mission’s Phase A development. This presentation will describe the S-GRS, its development timeline and performance estimates.
John W. Conklin1, Eric Bradley2, Joseph Controy1, Anthony Dávila Álvarez1, Stephen Bennett3, Riccardo Bevilacqua4, Neil Doughty3, Joseph Footdale3, Zane Forrester1, Paul Fulda1, John Hanson 5, Harold Hollis1, Moad Isteita3, Victoria Kennedy6, Ryan Kinzie4, Guido Mueller1, James Leitch3, Jennifer Lee3, Glenn McDaniel3, Cole Perkins1, Jose Sanjuan7, John Siu1, Robert Spero8, Mark Storm6, Brent Ware8, Peter Wass1, David Wiese8
How to cite: Conklin, J. and the Simplified Gravitational Reference Sensor team: A Simplified Gravitational Reference Sensor for NASA’s Mass Change Mission and Beyond, GRACE/GRACE-FO Science Team Meeting 2022, Potsdam, Germany, 18–20 Oct 2022, GSTM2022-80, https://doi.org/10.5194/gstm2022-80, 2022.