EGU24-12983, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-12983
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Juno Microwave Radiometer Observations of Europa’s Subsurface Ice Shell

Steve Levin1, Zhimeng Zhang2, Scott Bolton3, Shannon Brown1, Anton Ermakov4, Ryunosuke Akiba4, Sidharth Misra1, Paul Hartogh5, and David Stevenson2
Steve Levin et al.
  • 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States of America (steven.levin@jpl.nasa.gov)
  • 2California Institute of Technology, Pasadena, United States of America
  • 3Southwest Research Institute
  • 4Stanford University/UC Berkeley
  • 5Max Plank Institute for Solar System Research

Juno flew less than 360 km from the surface of Jupiter’s moon Europa on 29 September, 2022, and mapped part of the ice shell with the Microwave Radiometer (MWR) at frequencies of 0.6, 1.2, 2.5, 4.8, 9.6, and 22 GHz.  The partial map covers a latitude range from ~20oS to ~50oN and a longitude range from 70oW to 50oE.  At these frequencies, the emission originates well beneath the nearly-transparent surface, probing from as deep as 28 km (at 0.6 GHz) and less than 20 m (at 22 GHz), depending on the purity of the ice.  Microwave reflection plays an important role, and MWR data suggest the presence of small (radius a few cm) scatterers at depths of many meters.  Spatial variation is dominated by reflection, especially for the higher-frequency channels, and correlates with terrain type.  We present analysis of the data and discuss the implications. 

How to cite: Levin, S., Zhang, Z., Bolton, S., Brown, S., Ermakov, A., Akiba, R., Misra, S., Hartogh, P., and Stevenson, D.: Juno Microwave Radiometer Observations of Europa’s Subsurface Ice Shell, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-12983, https://doi.org/10.5194/egusphere-egu24-12983, 2024.