Radar for Europa Assessment and Sounding: Ocean to Near-surface

Artist's impression of the Europa Clipper's REASON instrument in action, using dual-frequency radar to map Europa's ice layer
Operator NASA
Manufacturer Jackson School of Geosciences
and JPL
Instrument type Ice penetrating radar
Function Characterize ice shell structure
Mission duration Cruise: 3-6 years
Science phase: ≥ 3 years
Properties
Mass 32.2 kg
Dimensions Antenna: 16 m (52 ft)
Power consumption 55 W
Data rate 5 - 80 Mbps
Host Spacecraft
Spacecraft Europa Clipper
Operator NASA
Launch date ≈ 2025
Rocket SLS
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.[1]

Overview

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.[1][2][3] 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.[1]

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.[4]

The instrument was developed by the Jackson School of Geosciences,[4] and its Principal Investigator is Donald Blankenship.[4] REASON will be fabricated by engineers from NASA's Jet Propulsion Laboratory and the University of Iowa.[4]

REASONUnits/performance[5]
Electronics mass17.5 kg
Antenna mass14.7 kg
Total mass32.2 kg
Operating power55 W
Antenna length16 m (52 ft)
VHF
(shallow sounding)		300 m to 4.5 km
HF
(deep sounding)		1 km to 30 km
Pulse length30 - 100 μs
Operational altitude10 - 1000 km
Radar potentialHF: 63 dB
VHF: 72 dB
Data rate5 - 80 Mbps
Data volume
per flyby		24 Gbits

Objectives

The scientific objectives of the REASON investigation are: [5]

  • 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

References

  1. 1 2 3 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.
  2. ↑ Grima, Cyril; Blankenship, Donald; Shroeder, 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. Retrieved 2017-11-04.
  3. ↑ Aglyamov, Yury; Shroeder, 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. Retrieved 2017-11-04.
  4. 1 2 3 4 Caputo, Anton (1 June 2015). "Radar Techniques Used in Antarctica Will Scour Europa for Life-Supporting Environments". UT News. Retrieved 2017-11-04.
  5. 1 2 Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) (PDF). D. Blankenship. 2015
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