Radar for Europa Assessment and Sounding: Ocean to Near-surface
|Manufacturer||Jackson School of Geosciences |
|Instrument type||Ice penetrating radar|
|Function||Characterize ice shell structure|
|Mission duration||Cruise: 3-6 years|
Science phase: ≥ 3 years
|Dimensions||Antenna: 16 m (52 ft)|
|Power consumption||55 W|
|Data rate||5 - 80 Mbps|
|Launch date||≈ 2025 |
|Launch site||Kennedy Space Center|
The Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) is a multi-frequency, multi-channel ice penetrating radar system that will be flown on board the Europa Clipper mission to Jupiter's moon Europa. REASON investigation will provide the first direct measurements of Europa's ice shell surface character and subsurface structure.
The REASON instrument makes innovative use of radar sounding, altimetry, reflectometry, plasma and particles analyses. These investigations will use a dual-frequency radar emitting HF (9 MHz) and VHF (60 MHz) with concurrent shallow and deep sounding. Both VHF and HF radiating elements are mounted on a single boom, reducing antenna mass. The mission plan also includes using REASON as a nadir altimeter capable of measuring tides to test ice shell and ocean hypotheses as well as characterizing roughness across the surface to identify potential landing sites for a future Europa Lander.
The REASON instrument will also be able to spot pockets of water within the ice shell that could serve as a passageway for chemicals on the moon's surface to the ocean below — an environment where life could potentially develop.
The instrument was developed by the Jackson School of Geosciences, and its Principal Investigator is Donald Blankenship. REASON will be fabricated by engineers from NASA's Jet Propulsion Laboratory and the University of Iowa.
|Electronics mass||17.5 kg|
|Antenna mass||14.7 kg|
|Total mass||32.2 kg|
|Operating power||55 W|
|Antenna length||16 m (52 ft)|
|300 m to 4.5 km|
|1 km to 30 km|
|Pulse length||30 - 100 μs|
|Operational altitude||10 - 1000 km|
|Radar potential||HF: 63 dB|
VHF: 72 dB
|Data rate||5 - 80 Mbps|
The scientific objectives of the REASON investigation are: 
- Characterize the distribution of any shallow subsurface water
- Search for an ice-ocean interface and characterize the ice shell's global structure
- Investigate the processes governing material exchange among the ocean, ice shell, surface, and atmosphere
- Constrain the amplitude and phase of gravitational tides
- Characterize scientifically compelling sites, and hazards, for a potential future Europa Lander mission
- Europa Clipper passes key review. Jeff Foust, Space News. 22 August 2019.
- REASON for Europa. Moussessian, A.; Blankenship, D. D.; Plaut, J. J.; Patterson, G. W.; Gim, Y.; Schroeder, D. M.; Soderlund, K. M.; Grima, C.; Young, D. A.; Chapin, E. American Geophysical Union, Fall Meeting 2015, abstract #P13E-05. December 2015.
- Grima, Cyril; Blankenship, Donald; Schroeder, Dustin M. (November 2015). "Radar signal propagation through the ionosphere of Europa". Planetary and Space Science. 117: 421–428. Bibcode:2015P&SS..117..421G. doi:10.1016/j.pss.2015.08.017.
- Aglyamov, Yury; Schroeder, Dustin M.; Vance, Steven D. (1 January 2017). "Bright prospects for radar detection of Europa's ocean". Icarus. 281: 334–337. Bibcode:2017Icar..281..334A. doi:10.1016/j.icarus.2016.08.014.
- Caputo, Anton (1 June 2015). "Radar Techniques Used in Antarctica Will Scour Europa for Life-Supporting Environments". UT News. Retrieved 2017-11-04.
- Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) (PDF). D. Blankenship. 2015