MARSIS

Last updated
Illustration of Mars Express with MARSIS antenna deployed Mars Express illustration highlighting MARSIS antenna.jpg
Illustration of Mars Express with MARSIS antenna deployed

MARSIS (Mars Advanced Radar for Subsurface and Ionosphere Sounding) is a low frequency, pulse-limited radar sounder and altimeter developed by the University of Rome La Sapienza and Alenia Spazio (today Thales Alenia Space Italy). [1] 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.

Contents

The MARSIS Principal Investigator is Giovanni Picardi from the University of Rome "La Sapienza", Italy. [2] It features ground-penetrating radar capabilities, which uses synthetic aperture technique and a secondary receiving antenna to isolate subsurface reflections. [3] MARSIS identified buried basins on Mars. [4] MARSIS was funded by ASI (Italy) and NASA (USA). [5] The processor runs the real-time operating system EONIC Virtuoso. [6]

Deployment

Mars SouthPole
Site of Subglacial Water
(25 July 2018) Mars-SubglacialWater-SouthPoleRegion-20180725.jpg

On May 4, 2005, Mars Express deployed the first of its two 20-metre-long radar booms for the MARSIS experiment. At first the boom didn't lock fully into place; [7] however, exposing it to sunlight for a few minutes on May 10 fixed the glitch. [8] The second 20 m boom was successfully deployed on June 14. Both 20 m booms were needed to create a 40 m dipole antenna for MARSIS to work; a less crucial 7-meter-long monopole antenna was deployed on June 17. The radar booms were originally scheduled to be deployed in April 2004, but this was delayed out of fear that the deployment could damage the spacecraft through a whiplash effect. Due to the delay it was decided to split the four-week commissioning phase in two parts, with two weeks running up to July 4 and another two weeks in December 2005.

The deployment of the booms was a critical and highly complex task, requiring effective inter-agency cooperation between ESA, NASA, industry partners, and public Universities.

Science

MARSIS transmits a series of modulated chirps at frequencies between 1.8 and 5.0 MHz in subsurface sounding mode, with a 1 MHz bandwidth. It also emits chirps sweeping between 0.1 and 5.4 MHz when ionosphere sounding. Depending on the mode, the pulsewidth is 30, 91 or 250 μs, and the nominal Pulse repetition frequency is 130 Hz. Transmitted power is either 1.5 or 5 W. [3]

Nominal science observations began during July 2005. [9]

A 2012 paper by the MARSIS team measured a difference between the dielectric constant of the northern and southern high-latitude regions. [10] This is evidence that the material that fills the northern basin is a lower-density material, which could be interpreted as evidence of an ancient northern ocean. [11]

Using MARSIS data, 22 Italian scientists reported in July 2018 the discovery of a subglacial lake on Mars, 1.5 km (0.93 mi) below the southern polar ice cap, and extending horizontally about 20 km (12 mi), the first known stable body of water on Mars. [12] [13] [14] [15]

Size of the MARSIS antenna (horizontal line) compared to the spacecraft and a human silhouette MARSIS antenna.svg
Size of the MARSIS antenna (horizontal line) compared to the spacecraft and a human silhouette

See also

Related Research Articles

<i>Mars Express</i> European Mars orbiter

Mars Express is a space exploration mission being conducted by the European Space Agency (ESA). The Mars Express mission is exploring the planet Mars, and is the first planetary mission attempted by the agency. "Express" originally referred to the speed and efficiency with which the spacecraft was designed and built. However, "Express" also describes the spacecraft's relatively short interplanetary voyage, a result of being launched when the orbits of Earth and Mars brought them closer than they had been in about 60,000 years.

<span class="mw-page-title-main">Deep Space 2</span> NASA space probe part of the New Millennium Program

Deep Space 2 was a NASA space probe, part of the New Millennium Program. It included two highly advanced miniature space probes that were sent to Mars aboard the Mars Polar Lander in January 1999. The probes were named "Scott" and "Amundsen", in honor of Robert Falcon Scott and Roald Amundsen, the first explorers to reach the Earth's South Pole. Intended to be the first spacecraft to penetrate below the surface of another planet, after entering the Mars atmosphere DS2 was to detach from the Mars Polar Lander mother ship and plummet to the surface using only an aeroshell impactor, with no parachute. The mission was declared a failure on March 13, 2000, after all attempts to reestablish communications following the descent went unanswered.

<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">Space-based radar</span> Use of radar systems mounted on satellites

Space-based radar or spaceborne radar is a radar operating in outer space; orbiting radar is a radar in orbit and Earth orbiting radar is a radar in geocentric orbit. A number of Earth-observing satellites, such as RADARSAT, have employed synthetic aperture radar (SAR) to obtain terrain and land-cover information about the Earth.

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">Planum Australe</span> Planum on Mars

Planum Australe is the southern polar plain on Mars. It extends southward of roughly 75°S and is centered at 83.9°S 160.0°E. The geology of this region was to be explored by the failed NASA mission Mars Polar Lander, which lost contact on entry into the Martian atmosphere.

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

SHARAD is a subsurface sounding radar embarked on the Mars Reconnaissance Orbiter (MRO) probe. It complements the MARSIS radar on Mars Express orbiter, providing lower penetration capabilities but much finer resolution.

<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">Northern Light (spacecraft)</span> Cancelled Canadian Mars lander and rover mission

Northern Light was a concept mission for a robotic mission to Mars that would consist of a lander and a rover, being studied by a consortium of Canadian universities, companies and organisations. The primary contractor for the spacecraft was Thoth Technology Inc.

Scalloped topography is common in the mid-latitudes of Mars, between 45° and 60° north and south. It is particularly prominent in the region of Utopia Planitia, in the northern hemisphere, and in the region of Peneus and Amphitrites Paterae in the southern hemisphere. Such topography consists of shallow, rimless depressions with scalloped edges, commonly referred to as "scalloped depressions" or simply "scallops". Scalloped depressions can be isolated or clustered and sometimes seem to coalesce. A typical scalloped depression displays a gentle equator-facing slope and a steeper pole-facing scarp. This topographic asymmetry is probably due to differences in insolation. Scalloped depressions are believed to form from the removal of subsurface material, possibly interstitial ice, by sublimation. This process may still be happening at present. This topography may be of great importance for future colonization of Mars because it may point to deposits of pure ice.

<span class="mw-page-title-main">Martian polar ice caps</span> Polar water ice deposits on Mars

The planet Mars has two permanent polar ice caps. During a pole's winter, it lies in continuous darkness, chilling the surface and causing the deposition of 25–30% of the atmosphere into slabs of CO2 ice (dry ice). When the poles are again exposed to sunlight, the frozen CO2 sublimes. These seasonal actions transport large amounts of dust and water vapor, giving rise to Earth-like frost and large cirrus clouds.

<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 the 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">Tianwen-1</span> Interplanetary mission by China to place an orbiter, lander, and rover on Mars

Tianwen-1 Chinese: 天问一号 is an interplanetary mission by the China National Space Administration (CNSA) which sent a robotic spacecraft to Mars, consisting of 6 spacecraft: an orbiter, two deployable cameras, lander, remote camera, and the Zhurong rover. The spacecraft, with a total mass of nearly five tons, is one of the heaviest probes launched to Mars and carries 14 scientific instruments. It is the first in a series of planned missions undertaken by CNSA as part of its Planetary Exploration of China program.

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

The Radar Imager for Mars' subsurface experiment (RIMFAX) is a ground-penetrating radar on NASA's Perseverance rover, part of the Mars 2020 mission. It uses radar waves to see geologic features under the surface.

<span class="mw-page-title-main">Radar for Europa Assessment and Sounding: Ocean to Near-surface</span> Ice-penetrating radar for Europa Clipper

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.

<span class="mw-page-title-main">EnVision</span> Proposed mission to Venus

EnVision is an orbital mission to Venus being developed by the European Space Agency (ESA) that is planned to perform high-resolution radar mapping and atmospheric studies. EnVision is designed to help scientists understand the relationships between its geological activity and the atmosphere, and it would investigate why Venus and Earth took such different evolutionary paths. The probe was selected as the fifth medium mission (M5) of ESA's Cosmic Vision programme in June 2021, with launch planned for 2031. The mission will be conducted in collaboration with NASA, with the potential sharing of responsibilities currently under assessment.

WISDOM is a ground-penetrating radar that is part of the science payload on board the European Space Agency'sRosalind Franklin rover, tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched in August–October 2022 and land on Mars in spring 2023.

<span class="mw-page-title-main">Mars Exploration Ice Mapper</span>

The International-Mars Ice Mapper (I-MIM) mission is a proposed Mars orbiter being developed by NASA in collaboration with the Japan Aerospace Exploration Agency (JAXA), the Canadian Space Agency (CSA), and the Italian Space Agency (ASI). As the mission concept evolves, there may be opportunities for other space agency and commercial partners to join the mission. The goal of the orbiter is the quantification of extent and volume of water ice in non-polar regions of Mars. The results are intended to support future Mars missions, especially with respect to the search for habitable environments and accessible In situ resource utilization (ISRU) resources. The International-Mars Ice Mapper is an "exploration precursor mission", comparing it to the Lunar Reconnaissance Orbiter (LRO) mission. The mission was envisioned to be launched as early as 2026. However, in March 2022, it was revealed in its fiscal year 2023 budget proposal that the US government would terminate NASA financial support for the Mars Ice Mapper, casting the project's future into uncertainty.

<i>Zhurong</i> (rover) Chinese rover on Mars

Zhurong is a Chinese rover on Mars, the country's first to land on another planet after it previously landed two rovers on the Moon. The rover is part of the Tianwen-1 mission to Mars conducted by the China National Space Administration (CNSA).

<span class="mw-page-title-main">Planetary Exploration of China</span> Chinese Solar System exploration program

The Planetary Exploration of China, also known as Tianwen, is the robotic interplanetary spaceflight program conducted by the China National Space Administration (CNSA). The program aims to explore planets of the Solar System, starting from Mars, and will be expanded to Jupiter and more in the future.

References

  1. Flamini, E.; Fois, F.; Calabrese, D.; Bombaci, O.; Catallo, C.; Croce, A.; Croci, R.; Guelfi, M.; Zampolini, E.; Picardi, G.; Seu, R.; Mecozzi, R.; Biccari, D.; Cartacci, M.; Cicchetti, A.; Masdea, A.; Alberti, G.; Maffei, S.; Papa, C. (2007). "Sounding Mars with SHARAD & MARSIS". 2007 4th International Workshop on, Advanced Ground Penetrating Radar. pp. 246–251. doi:10.1109/AGPR.2007.386561. ISBN   978-1-4244-0886-3. S2CID   25906305.
  2. "MARSIS: Subsurface Sounding Radar/Altimeter". www.esa.int. ESA. 25 October 2017.
  3. 1 2 "MARSIS instrument home page". Due to severe limitations on the available mass, the antennas are of a novel design, each consisting of a folding composite tube that supports a pair of wires constituting the conductive element of the antenna. The antennas are deployed by pyrotechnic release mechanisms.
  4. MARSIS FINDS BURIED BASINS IN CHRYSE PLANITIA Dec 2006
  5. Buried Basins Discovered by Radar Undated
  6. Calabrese, D. (2003-12-16). "MARSIS Flight User Manual" (PDF). esac.esa.int. Retrieved 2022-06-25.
  7. Glitch strikes Mars Express's radar boom - space, New Scientist, May 9, 2005
  8. Mars Express's kinky radar straightened out - space, New Scientist, May 12, 2005
  9. ESA Portal, Mars Express radar ready to work
  10. Jérémie Mouginot, Antoine Pommerol, Pierre Beck, Wlodek Kofman and Stephen M. Clifford, "Dielectric map of the Martian northern hemisphere and the nature of plain filling materials," Geophysical Research Letters, 39, No. 2, 19 Jan 2012 (abstract)(article at UCI) accessed Nov. 17 2014
  11. Emily Lakdawalla, "Has Mars Express MARSIS data proved that Mars once had a northern ocean?" Planetary Society, February 7, 2012 (accessed Nov. 17 2014)
  12. Orosei, R.; et al. (25 July 2018). "Radar evidence of subglacial liquid water on Mars" (PDF). Science . 361 (6401): 490–493. arXiv: 2004.04587 . Bibcode:2018Sci...361..490O. doi: 10.1126/science.aar7268 . hdl:11573/1148029. PMID   30045881.
  13. Chang, Kenneth; Overbye, Dennis (25 July 2018). "A Watery Lake Is Detected on Mars, Raising the Potential for Alien Life - The discovery suggests that watery conditions beneath the icy southern polar cap may have provided one of the critical building blocks for life on the red planet". The New York Times . Retrieved 25 July 2018.
  14. "Huge reservoir of liquid water detected under the surface of Mars". EurekAlert . 25 July 2018. Retrieved 25 July 2018.
  15. Halton, Mary (25 July 2018). "Liquid water 'lake' revealed on Mars". BBC News . Retrieved 25 July 2018.
  16. R. Orosei et al., "Science results from the MARSIS and SHARAD subsurface sounding radars on Mars and their relevance to radar sounding of icy moons in the Jovian system", EPSC2010-726, European Planetary Science Congress 2010, Vol. 5 (accessed Nov. 17 2014)