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

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Artist's impression of the Europa Clipper's REASON instrument in action, using dual-frequency radar to map Europa's ice layer
OperatorNASA
ManufacturerJackson School of Geosciences
and JPL
Instrument typeIce penetrating radar
FunctionCharacterize ice shell structure
Mission durationCruise: 5.5 years
Science phase: 4 years
Properties
Mass32.2 kg
DimensionsAntenna: 16 m (52 ft)
Power consumption55 W
Data rate5 - 80 Mbps
Host spacecraft
SpacecraftEuropa Clipper
OperatorNASA
Launch dateOctober 14, 2024, 16:06:00 (2024-10-14UTC16:06Z) UTC (12:06 p.m. EDT)
RocketFalcon Heavy
Launch siteKennedy 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

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REASON deployment

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 was fabricated by engineers from NASA's Jet Propulsion Laboratory and the University of Iowa.[4]

Specifications table

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REASON Units/performance[5]
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)
VHF
(shallow sounding)		 300 m to 4.5 km
HF
(deep sounding)		 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
Data volume
per flyby		 24 Gbits

Objectives

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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

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  1. ^ a b c 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; 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.
  3. ^ 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.
  4. ^ a b c d Caputo, Anton (1 June 2015). "Radar Techniques Used in Antarctica Will Scour Europa for Life-Supporting Environments". UT News. Retrieved 2017-11-04.
  5. ^ a b Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) (PDF). D. Blankenship. 2015
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