Marte está vivo.

La vista topográfica codificada por colores muestra la elevación relativa de las características de Cerberus Fossae; los rojos y blancos son relativamente más altos que los azules y violetas. La imagen se basa en un modelo de terreno digital de la región a partir del cual se puede derivar la topografía del paisaje. Crédito: ESA/DLR/FU Berlín, CC BY-SA 3.0 IGO

Hasta ahora,[{» attribute=»»>Mars has generally been considered a geologically dead planet. An international team of scientists now reports that seismic signals indicate vulcanism still plays an active role in shaping the Martian surface.

Ever since the NASA InSight Mission deployed the SEIS seismometer on the surface of Mars in 2018, seismologists and geophysicists at ETH Zurich have been listening to the seismic pings of more than 1,300 marsquakes. Again and again, the researchers registered smaller and larger Mars quakes. A detailed analysis of the quakes’ location and spectral character eventually brought a surprise. With epicenters originating in the vicinity of the Cerberus Fossae — a region consisting of a series of rifts or graben — these quakes tell a new story. A story that suggests an active role is still played by vulcanism in shaping the Martian surface.

Mars shows signs of geological life

Led by ETH Zurich, an international team of researchers analyzed a cluster of more than 20 recent marsquakes that originated in the Cerberus Fossae graben system. From the seismic data, scientists concluded that the low-frequency quakes indicate a potentially warm source that could be explained by present-day molten lava, i.e., magma at that depth, and volcanic activity on Mars. Specifically, they found that the quakes are located mostly in the innermost part of Cerberus Fossae.

This image, taken on January 27, 2018, during orbit 17813 by the High Resolution Stereo Camera (HRSC) on ESA’s Mars Express, shows a portion of the Cerberus Fossae system in Elysium Planitia near the Martian equator. Credit: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO

When they scanned observational orbital images of the same area, they noticed that the epicenters were located very close to a structure that has previously been described as a “young volcanic fissure.” Darker deposits of dust around this fissure are present not only in the dominant direction of the wind, but in all directions surrounding the Cerberus Fossae Mantling Unit.

“The darker shade of the dust signifies geological evidence of more recent volcanic activity – perhaps within the past 50,000 years — relatively young, in geological terms,” explains Simon Stähler, the lead author of the paper, which has was published on October 27 in the journal Nature. Stähler is a Senior Scientist working in the Seismology and Geodynamics group led by Professor Domenico Giardini at the Institute of Geophysics, ETH Zurich.

Why study the terrestrial neighbor?

Exploring Earth’s planetary neighbors is no easy task. Mars is the only planet, other than Earth, on which scientists have ground-based rovers, landers, and now even drones that transmit data. So far, all other planetary exploration has relied on orbital imagery.

“InSight’s SEIS is the most sensitive seismometer ever installed on another planet,” says Domenico Giardini. “It affords geophysicists and seismologists an opportunity to work with current data showing what is happening on Mars today — both at the surface and in its interior.” The seismic data, along with orbital images, ensures a greater degree of confidence for scientific inferences.

One of the fractures (graben) that make up the Cerberus Fossae system. The fractures cut through hills and craters, indicating their relative youth. SA/DLR/FU Berlin, CC BY-SA 3.0 IGO

One of our nearest terrestrial neighbors, Mars is important for understanding similar geological processes on Earth. The red planet is the only one we know of, so far, that has a core composition of iron, nickel, and sulfur that might have once supported a magnetic field. Topographical evidence also indicates that Mars once held vast expanses of water and possibly a denser atmosphere. Even today, scientists have learned that frozen water, although possibly mostly dry ice, still exists on its polar caps.

“While there is much more to learn, the evidence of potential magma on Mars is intriguing,” Anna Mittelholz, Postdoctoral Fellow at ETH Zurich and Harvard University.

Last remnants of geophysical life

Looking at images of the vast dry, dusty Martian landscape it is difficult to imagine that about 3.6 billion years ago Mars was very much alive, at least in a geophysical sense. It spewed volcanic debris for a long enough time to give rise to Tharsis Montes region, the largest volcanic system in our solar system and the Olympus Mons – a volcano nearly three times the elevation of Mount Everest.

Cerberus Fossae in context of its surrounds in the Elysium Planitia region of Mars near the equator. Credit: NASA MGS MOLA Science Team

The quakes coming from the nearby Cerberus Fossae — named for a creature from Greek mythology known as the “hell-hound of Hades” that guards the underworld – suggest that Mars is not quite dead yet. Here the weight of the volcanic region is sinking and forming parallel graben (or rifts) that pull the crust of Mars apart, much like the cracks that appear on the top of a cake while its baking. According to Stähler, it is possible that what we are seeing are the last remnants of this once-active volcanic region or that the magma is right now moving eastward to the next location of eruption.

Reference: “Tectonics of Cerberus Fossae unveiled by marsquakes” by Simon C. Stähler, Anna Mittelholz, Cleément Perrin, Taichi Kawamura, Doyeon Kim, Martin Knapmeyer, Géraldine Zenhäusern, John Clinton, Domenico Giardini, Philippe Lognonné and W. Bruce Banerdt, 27 October 2022, Nature Astronomy.
DOI: 10.1038/s41550-022-01803-y

This study involved scientists from ETH Zurich, Harvard University, Nantes Université, CNRS Paris, the German Aerospace Center (DLR) in Berlin, and Caltech.

NASA InSight mission

InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) is an unmanned external NASA Mars mission. In November 2018, the stationary lander, which is equipped with a seismometer and a heat probe, safely landed on the Martian surface. The geophysical instruments on the red planet permit exploration of its interior. A number of European partners, including France’s Centre National d’Études Spatiales (CNES) and the German Aerospace Center (DLR), are supporting the InSight mission. CNES provided the Seismic Experiment for Interior Structure (SEIS) instrument to NASA, with the principal investigator at IPGP (Institut de Physique du Globe de Paris). Significant contributions for SEIS came from IPGP; the Max Planck Institute for Solar System Research (MPS) in Germany; Imperial College London and Oxford University in the United Kingdom; and Jet Propulsion Laboratory (USA).