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

Last updated
Europa Clipper radar.jpg
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 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
Spacecraft Europa Clipper
Operator NASA
Launch dateOctober 10th, 2024 [1]
Rocket Falcon Heavy
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. [2]

Contents

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. [2] [3] [4] 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. [2]

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. [5]

The instrument was developed by the Jackson School of Geosciences, [5] and its Principal Investigator is Donald Blankenship. [5] REASON will be fabricated by engineers from NASA's Jet Propulsion Laboratory and the University of Iowa. [5]

Specifications table

REASONUnits/performance [6]
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 potential HF: 63 dB
VHF: 72 dB
Data rate5 - 80 Mbps
Data volume
per flyby
24 Gbits

Objectives

The scientific objectives of the REASON investigation are: [6]

Related Research Articles

<span class="mw-page-title-main">Europa (moon)</span> Smallest Galilean moon of Jupiter

Europa, or Jupiter II, is the smallest of the four Galilean moons orbiting Jupiter, and the sixth-closest to the planet of all the 95 known moons of Jupiter. It is also the sixth-largest moon in the Solar System. Europa was discovered independently by Simon Marius and Galileo Galilei and was named after Europa, the Phoenician mother of King Minos of Crete and lover of Zeus.

<span class="mw-page-title-main">Cryovolcano</span> Type of volcano that erupts volatiles such as water, ammonia or methane, instead of molten rock

A cryovolcano is a type of volcano that erupts gasses and volatile material such as liquid water, ammonia, and hydrocarbons, collectively referred to as cryolava, from a reservoir of subsurface cryomagma. These eruptions can take many forms, such as fissure and curtain eruptions, effusive cryolava flows, and large-scale resurfacing, and can vary greatly in output volumes. Immediately after an eruption, cryolava quickly freezes, constructing geological features and altering the surface.

<span class="mw-page-title-main">Ground-penetrating radar</span> Geophysical method that uses radar pulses to image the subsurface

Ground-penetrating radar (GPR) is a geophysical method that uses radar pulses to image the subsurface. It is a non-intrusive method of surveying the sub-surface to investigate underground utilities such as concrete, asphalt, metals, pipes, cables or masonry. This nondestructive method uses electromagnetic radiation in the microwave band of the radio spectrum, and detects the reflected signals from subsurface structures. GPR can have applications in a variety of media, including rock, soil, ice, fresh water, pavements and structures. In the right conditions, practitioners can use GPR to detect subsurface objects, changes in material properties, and voids and cracks.

<span class="mw-page-title-main">MARSIS</span>

MARSIS is a low frequency, pulse-limited radar sounder and altimeter developed by the University of Rome La Sapienza and Alenia Spazio. The Italian MARSIS instrument, which is operated by the European Space Agency, is operational and orbits Mars as an instrument for the ESA's Mars Express exploration mission.

<span class="mw-page-title-main">Chaos terrain</span> Distinctive area of broken or jumbled terrain

In astrogeology, chaos terrain, or chaotic terrain, is a planetary surface area where features such as ridges, cracks, and plains appear jumbled and enmeshed with one another. Chaos terrain is a notable feature of the planets Mars and Mercury, Jupiter's moon Europa, and the dwarf planet Pluto. In scientific nomenclature, "chaos" is used as a component of proper nouns.

Radioglaciology is the study of glaciers, ice sheets, ice caps and icy moons using ice penetrating radar. It employs a geophysical method similar to ground-penetrating radar and typically operates at frequencies in the MF, HF, VHF and UHF portions of the radio spectrum. This technique is also commonly referred to as "Ice Penetrating Radar (IPR)" or "Radio Echo Sounding (RES)".

<span class="mw-page-title-main">ALSE</span> Experiment undertaken on the Apollo 17 mission

The ALSE (Apollo Lunar Sounder Experiment) (also known as Scientific Experiment S-209, according to NASA designations) was a ground-penetrating radar (subsurface sounder) experiment that flew on the Apollo 17 mission.

<span class="mw-page-title-main">Regular moon</span> Satellites which formed around their parent planet

In astronomy, a regular moon or a regular satellite is a natural satellite following a relatively close, stable, and circular orbit which is generally aligned to its primary's equator. They form within discs of debris and gas that once surrounded their primary, usually the aftermath of a large collision or leftover material accumulated from the protoplanetary disc. Young regular moons then begin to accumulate material within the circumplanetary disc in a process similar to planetary accretion, as opposed to irregular moons, which formed independently before being captured into orbit around the primary.

<span class="mw-page-title-main">Jupiter Icy Moons Explorer</span> European Space Agency spacecraft

The Jupiter Icy Moons Explorer is an interplanetary spacecraft that was launched on 14 April 2023 from Guiana Space Centre in French Guiana by the European Space Agency (ESA) with Airbus Defence and Space as the main contractor. The mission is planned to study Ganymede, Callisto, and Europa, three of Jupiter's Galilean moons. They are thought to have significant bodies of liquid water beneath their icy surfaces which would make them potentially habitable environments.

<span class="mw-page-title-main">Europa Clipper</span> Planned NASA space mission to Jupiter

Europa Clipper is a space probe in development by NASA. Planned for launch in October 2024, the spacecraft is being developed to study the Galilean moon Europa through a series of flybys while in orbit around Jupiter.

Planetary oceanography, also called astro-oceanography or exo-oceanography, is the study of oceans on planets and moons other than Earth. Unlike other planetary sciences like astrobiology, astrochemistry, and planetary geology, it only began after the discovery of underground oceans in Saturn's moon Titan and Jupiter's moon Europa. This field remains speculative until further missions reach the oceans beneath the rock or ice layer of the moons. There are many theories about oceans or even ocean worlds of celestial bodies in the Solar System, from oceans made of diamond in Neptune to a gigantic ocean of liquid hydrogen that may exist underneath Jupiter's surface.

Journey to Enceladus and Titan (JET) is an astrobiology mission concept to assess the habitability potential of Enceladus and Titan, moons of Saturn.

<span class="mw-page-title-main">Europa Lander</span> Proposed NASA lander for Europa

The Europa Lander is a proposed astrobiology mission concept by NASA to send a lander to Europa, an icy moon of Jupiter. If funded and developed as a large strategic science mission, it would be launched in 2027 to complement the studies by the Europa Clipper orbiter mission and perform analyses on site.

<span class="mw-page-title-main">Surface Dust Analyser</span>

The SUrface Dust Analyser (SUDA) is a time-of-flight mass spectrometer of reflectron-type that employs impact ionization and is optimised for a high mass resolution. The instrument was selected in May 2015 to fly on board the Europa Clipper mission, that is planned for 2025 to Jupiter's moon Europa.

The Europa Imaging System (EIS) is a visible spectrum wide and narrow angle camera on board the planned Europa Clipper mission that will map most of Europa at 50 m (160 ft) resolution, and will provide images of selected surface areas at up to 0.5 m resolution.

The Interior Characterization of Europa using Magnetometry (ICEMAG) is a multi-frequency magnetometer that was proposed to be flown on board the Europa Clipper mission to Jupiter's moon Europa, but its inclusion was cancelled in March 2019. Magnetic induction is a powerful tool for probing the subsurface and determine Europa's ocean depth, salinity, and ice shell thickness, as well as detecting erupting plume activity.

<span class="mw-page-title-main">Plasma Instrument for Magnetic Sounding</span> Faraday cup instrument for Europa Clipper

The Plasma Instrument for Magnetic Sounding (PIMS) is a Faraday cup based instrument that will fly on board the Europa Clipper orbiter to explore Jupiter's moon Europa. PIMS will measure the plasma that populates Jupiter's magnetosphere and Europa's ionosphere.

<span class="mw-page-title-main">Subglacial lakes on Mars</span>

Salty subglacial lakes are controversially inferred from radar measurements to exist below the South Polar Layered Deposits (SPLD) in Ultimi Scopuli of Mars' southern ice cap. The idea of subglacial lakes due to basal melting at the polar ice caps on Mars was first hypothesized in the 1980s. For liquid water to persist below the SPLD, researchers propose that perchlorate is dissolved in the water, which lowers the freezing temperature, but other explanations such as saline ice or hydrous minerals have been offered. Challenges for explaining sufficiently warm conditions for liquid water to exist below the southern ice cap include low amounts of geothermal heating from the subsurface and overlying pressure from the ice. As a result, it is disputed whether radar detections of bright reflectors were instead caused by other materials such as saline ice or deposits of minerals such as clays. While lakes with salt concentrations 20 times that of the ocean pose challenges for life, potential subglacial lakes on Mars are of high interest for astrobiology because microbial ecosystems have been found in deep subglacial lakes on Earth, such as in Lake Whillans in Antarctica below 800 m of ice.

<span class="mw-page-title-main">Europa Clipper Magnetometer</span> Europa Clippers magnetometer instrument

The Europa Clipper Magnetometer (ECM) is a spacecraft magnetometer aboard the planned Europa Clipper mission. It will be used to precisely measure Europa's magnetic field during consecutive fly-bys, allowing scientists to potentially confirm the existence of Europa's hypothesised subsurface ocean. If this ocean exists, the instrument will be able to determine its depth and salinity, as well as the thickness of the moon's icy shell.

References

  1. Foust, Jeff (11 February 2021). "NASA to use commercial launch vehicle for Europa Clipper". SpaceNews. Retrieved 26 March 2024.
  2. 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.
  3. 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.
  4. 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.
  5. 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.
  6. 1 2 Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) (PDF). D. Blankenship. 2015