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Mars’ Hidden Molten Layer: A New Peek Beneath the Martian Mantle

Artist’s view of Mars’ interior structure showing a molten layer at the base of the mantle and above the core. The purple line shows the path followed in Mars by the waves generated by the meteorite impact that occurred on September 2021 and diffracted along the CMB. The blue line represents the path followed by a seismic wave reflected at the top of the molten basal layer. Credit: IPGP / CNES / N. Starter

Recently, a team of scientists involved in NASAEstablished in 1958, the National Aeronautics and Space Administration (NASA) is an independent agency of the United States Federal Government that succeeded the National Advisory Committee for Aeronautics (NACA). It is responsible for the civilian space program, as well as aeronautics and aerospace research. Its vision is "To discover and expand knowledge for the benefit of humanity." Its core values are "safety, integrity, teamwork, excellence, and inclusion." NASA conducts research, develops technology and launches missions to explore and study Earth, the solar system, and the universe beyond. It also works to advance the state of knowledge in a wide range of scientific fields, including Earth and space science, planetary science, astrophysics, and heliophysics, and it collaborates with private companies and international partners to achieve its goals.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>NASA’s InSight mission completed an analysis of seismic data recorded on MarsMars is the second smallest planet in our solar system and the fourth planet from the sun. It is a dusty, cold, desert world with a very thin atmosphere. Iron oxide is prevalent in Mars' surface resulting in its reddish color and its nickname "The Red Planet." Mars' name comes from the Roman god of war.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>Mars after a meteorite impact that occurred in September 2021. Their findings drastically change our view of the internal structure and evolution of the Red Planet.

Based on these results and previous geophysical data, a study published in the journal Nature, in which researcher Attilio Rivoldini from the Royal Observatory of Belgium participated, proposes a new model for the interior of Mars, with a heterogeneous mantle containing a molten silicate layer above the liquid metal core.

Initial Findings and Assumptions

The first results based on data from the InSight mission significantly improved our knowledge of the interior structure of Mars. Assuming that the mantle is compositionally homogeneous and entirely solid, the results showed that the liquid metal core has a radius of about 1830±40 km and a relatively low density (6-6.2 g/cm3) with a large concentration of light elements. The size of the metal core was determined by the detection of seismic waves reflected at a solid-liquid interface ascribed to be the Core-Mantle Boundary (CMB).

Re-Evaluation After Recent Impact

However, since then, the analysis of new data generated by a powerful meteorite impact that occurred on September 18, 2021, questioned the first estimates of the internal structure of the Red Planet. An international team led by Henri Samuel, CNRS researcher at the Institute of Globe Physics in Paris, and involving Attilio Rivoldini from the Royal Observatory of Belgium, studied the propagation times of these waves and showed that a molten silicate layer at the base of the Martian mantle and above the metallic core can explain the new data.

Based on this finding, a new structure model has been deduced and published on October 26 in the journal Nature. That structure model is not only more consistent with all available geophysical data, but also explains better the evolution of Mars since its formation.

Seismic Anomalies Explained

A molten layer at the base of the mantle elucidates the abnormally slow propagation, hitherto unexplained, of seismic waves diffracted along the CMB in September 2021. Furthermore, for several earlier seismic events, the arrival times of seismic waves are compatible with reflections of seismic shear waves at the top of the molten layer (located several tens of kilometers above the metallic core) and not at the CMB, as previously assumed.

Implications for Core Size and Composition

The presence of this molten layer at the base of the mantle implies that the metallic core is 150 to 170 km smaller (i.e., a radius of 1650±20 km) than previous estimates.

“This smaller core is also 5 to 8% denser (i.e. 6.5 g/cm3). The fraction of light elements in the core is lower than previously thought and as such is more compatible with cosmochemical data deduced from the analysis of Martian meteorites and high-pressure experiments,” explains Attilio Rivoldini.

Mars’ Early Evolution

The authors of the study therefore propose that Mars experienced an early magma ocean stage whose crystallisation produced a stable layer at the base of the mantle, highly enriched in iron and radioactive elements. The heat released by radioactive decay generated a basal layer of molten silicates above the core.

For more on this study:

Reference: “Geophysical evidence for an enriched molten silicate layer above Mars’s core” by Henri Samuel, Mélanie Drilleau, Attilio Rivoldini, Zongbo Xu, Quancheng Huang, Raphaël F. Garcia, Vedran Lekić, Jessica C. E. Irving, James Badro, Philippe H. Lognonné, James A. D. Connolly, Taichi Kawamura, Tamara Gudkova and William B. Banerdt, 25 October 2023, Nature.
DOI: 10.1038/s41586-023-06601-8

About InSight and SEIS:

NASA’s InSight mission officially ended in December 2022 after more than four years of collecting unique science data on Mars.

JPLThe Jet Propulsion Laboratory (JPL) is a federally funded research and development center that was established in 1936. It is owned by NASA and managed by the California Institute of Technology (Caltech). The laboratory's primary function is the construction and operation of planetary robotic spacecraft, though it also conducts Earth-orbit and astronomy missions. It is also responsible for operating NASA's Deep Space Network. JPL implements programs in planetary exploration, Earth science, space-based astronomy and technology development, while applying its capabilities to technical and scientific problems of national significance.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>JPL managed the InSight mission on behalf of NASA’s Science Mission Directorate. InSight is part of NASA’s Discovery program, managed by the Marshall Space Flight Center (MSFC), NASA’s Huntsville, Alabama facility. Lockheed Martin Space in Denver built the InSight probe, including its cruise stage and lander, and supported operation of the spacecraft for the mission. CNES was the prime contractor for SEIS and the Paris Institute of Globe Physics (Université Paris Cité/IPGP/CNRS) assumed scientific responsibility. CNES finances the French contributions, coordinates the international consortium (*) and was responsible for the integration, testing and supply of the complete instrument to NASA. IPGP designed the VBB (Very Broad Band) sensors, tested them before their delivery to CNES and contributes to the operation of VBBs on Mars.

The SEIS and APSS operations were carried out by CNES within FOCSE-SISMOC, with the support of the Centro de Astrobiologia (Spain). SEIS data are formatted and distributed by the Mars SEIS Data Service of IPG Paris, as part of the National Observation Service InSight to which LPG also contributes and, for Seismo activities at the School, GéoAzur. Daily identification of earthquakes was carried out by InSight’s Mars Quake Service, a collaborative operational service led by ETH Zurich to which seismologists from IPG Paris, the University of BristolThe University of Bristol, a red brick research university in Bristol, England, received its royal charter in 1909. However, it can trace its history back to 1876 (as University College, Bristol) and 1595 (as Merchant Venturers School). It is organized into six academic faculties composed of multiple schools and departments running over 200 undergraduate courses.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>University of Bristol (UK) and Imperial College LondonEstablished on July 8, 1907, by Royal Charter, Imperial College London is a public research university in London with a focus on science, engineering, medicine, and business. Its main campus is located in South Kensington, and it has an innovation campus in White City, a research field station at Silwood Park, and teaching hospitals throughout London. Its full legal name is the Imperial College of Science, Technology and Medicine.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>Imperial College London ( UK).

Several other CNRS laboratories including LMD (CNRS/ENS Paris/École polytechnique/Sorbonne University), LPG (CNRS/Nantes University/Le Mans University/University of Angers), IRAP (CNRS/University of Toulouse/CNES ), the LGL-TPE (CNRS/École Normale Supérieure de Lyon/Claude Bernard University Lyon 1), the IMPMC (Sorbonne University/National Museum of Natural History/CNRS) and LAGRANGE (CNRS/Université Côte d’Azur/Observatoire of the Côte d’Azur) are participating with the IPGP and ISAE-SUPAERO in the analysis of data from the InSight mission. These analyse are supported by CNES and the National Research Agency as part of the ANR MArs Geophysical InSight (MAGIS) project.

(*) in collaboration with SODERN for the production of the VBB, the JPL, the Swiss Federal Institute of Technology in Zurich (ETH, Zurich Switzerland), the Max Planck Institute for Solar System Research (MPS, Göttingen, Germany), the Imperial College London and the University of OxfordThe University of Oxford is a collegiate research university in Oxford, England that is made up of 39 constituent colleges, and a range of academic departments, which are organized into four divisions. It was established circa 1096, making it the oldest university in the English-speaking world and the world's second-oldest university in continuous operation after the University of Bologna.” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]” tabindex=”0″ role=”link”>University of Oxford provided the SEIS subsystems and are involved in the scientific exploitation of SEIS.

Source: SciTechDaily