- 1NASA Goddard Space Flight Center, Greenbelt, Maryland, United States of America (erwan.m.mazarico@nasa.gov)
- 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, United States of America
- 3University of Illinois, Chicago, Illinois, United States of America
- 4University of Rome La Sapienza, Rome, Italy
- 5German Aerospace Center (DLR), Berlin, Germany
- 6Lunar and Planetary Institute, Universities Space Research Association, Houston, Texas, United States of America
- 7Washington University in St. Louis, St. Louis, Missouri, United States of America
- 8University of California, Santa Cruz, California, United States of America
- 9Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, United States of America
- 10University of Bologna, Bologna, Italy
- 11Boston University, Boston, Massachusetts, United States of America
- *A full list of authors appears at the end of the abstract
NASA’s Europa Clipper flagship mission launched on October 14, 2024 and will arrive at Jupiter in April 2030. There, it will investigate the habitability of Jupiter’s moon Europa. Gravity and Radio Science (G/RS) is one of ten complementary investigations devoted to understanding Europa through studies of its ice shell and ocean, its composition, and its geology. G/RS makes use of the Europa Clipper telecommunications system to obtain radiometric tracking data during the Europa flybys.
Unlike past missions, the primary raw data for the G/RS investigation are obtained from Open-Loop Receivers (OLR) at the Deep Space Network (DSN) ground stations. Indeed, the flyby geometry, spacecraft attitude, and spacecraft antenna configuration are such that the signal-to-noise ratio of the return radio signals will be small (<10 dB-Hz) and insufficient for the typical closed-loop tracking. Processing of the OLR with special retracking algorithms will be necessary to obtain range-rate (Doppler) observations. Given the lack of a stable oscillator onboard Europa Clipper, two-way tracking will be used to achieve high frequency stability, leveraging the accurate DSN clocks. Radio tracking during the flybys will be performed at a single frequency (X-band), so careful modeling of media perturbations is important to maximize the G/RS results. We will discuss recent work to assess the impact of media perturbations from the Io Plasma Torus on orbit reconstruction and geophysical parameter recovery.
G/RS will obtain measurements of Europa’s static and time-variable gravity field. The tidal Love number k2 will verify the presence of a subsurface ocean and help constrain the ice shell. The moment of inertia, derived from degree-2 gravity coefficients, will help determine the interior structure. The radio tracking data will also be sensitive to Europa’s ionosphere when geometry allows.
We will present the G/RS investigation and observation plans, its expected performance, and provide a first look at the tracking data during cruise.
Erwan Mazarico, Dustin Buccino, Julie Castillo-Rogez, Andrew Dombard, Antonio Genova, Hauke Hussmann, Walter Kiefer, Jonathan Lunine, William McKinnon, Francis Nimmo, Ryan Park, James Roberts, Paolo Tortora, Paul Withers, Gael Cascioli, Martina Caussi, Martina Ciambellini, Benjamin Idini, Andrea Magnanini, Alyssa Mills, Flavio Petricca, and Marco Zannoni
How to cite: Mazarico, E., Buccino, D., Castillo-Rogez, J., Dombard, A., Genova, A., Hussmann, H., Kiefer, W., Lunine, J., McKinnon, W., Nimmo, F., Park, R., Roberts, J., Tortora, P., and Withers, P. and the Europa Clipper G/RS Team: The Europa Clipper Gravity and Radio Science (G/RS) Investigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2924, https://doi.org/10.5194/egusphere-egu25-2924, 2025.
