Gravity Study Gives Insights into Hidden Features Beneath Lost Ocean of Mars and Rising Olympus Mons
Studies of gravity variations at Mars have revealed dense, large-scale structures hidden beneath the sediment layers of a lost ocean. The analysis, which combines models and data from multiple missions, also shows that active processes in the martian mantle may be giving a boost to the largest volcano in the Solar System, Olympus Mons. The findings have been presented this week at the Europlanet Science Congress (EPSC) in Berlin by Bart Root of Delft University of Technology (TU Delft).
Mars has many hidden structures, such as ice deposits, but the features discovered in the northern polar plains are a mystery because they are covered with a thick and smooth sediment layer believed to deposited on ancient seabed.
“These dense structures could be volcanic in origin or could be compacted material due to ancient impacts. There are around 20 features of varying sizes that we have identified dotted around the area surrounding the north polar cap – one of which resembles the shape of a dog,” said Dr Root. “There seems to be no trace of them at the surface. However, through gravity data, we have a tantalising glimpse into the older history of the northern hemisphere of Mars.”
Dr Root and colleagues from TU Delft and Utrecht University used tiny deviations in the orbits of satellites to investigate the gravity field of Mars and find clues about the planet’s internal mass distribution. This data was fed into models that use new observations from NASA’s Insight mission on the thickness and flexibility of the martian crust, as well as the dynamics of the planet’s mantle and deep interior, to create a global density map of Mars.
Map highlighting the dense gravitational structures in the northern hemisphere. The regions denoted by the black lines are high mass anomalies that do not show any correlation with geology and topography. These hidden subsurface structures are covered by sediments from an old ocean. Their origin is still a mystery and a dedicated gravity mission, like MaQuIs, is needed to reveal their nature. Credit: Root et al.
The density map shows that the northern polar features are approximately 300-400 kg/m3 denser than their surroundings. However, the study has also revealed new insights into the structures underlying the huge volcanic region of Tharsis Rise, which includes the colossal volcano, Olympus Mons.
Although volcanoes are very dense, the Tharsis area is much higher than the average surface of Mars, and is ringed by a region of comparatively weak gravity. This gravity anomaly is hard to explain by looking at differences in the martian crust and upper mantle alone. The study by Dr Root and his team suggests that a light mass around 1750 kilometres across and at a depth of 1100 kilometres is giving the entire Tharsis region a boost upwards. This could be explained by huge plume of lava, deep within the martian interior, travelling up towards the surface.
“The NASA InSight mission has given us vital new information about the hard outer layer of Mars. This means we need to rethink how we understand the support for the Olympus Mons volcano and its surroundings,” said Dr Root. “It shows that Mars might still have active movements happening inside it, affecting and possibly making new volcanic features on the surface.”
Dr Root is part of the team proposing the Martian Quantum Gravity (MaQuls) mission, which aims to use technology developed for missions like GRAIL and GRACE on the Moon and Earth respectively to map in detail the gravity field of Mars.
“Observations with MaQuIs would enable us to better explore the subsurface of Mars. This would help us to find out more about these mysterious hidden features and study ongoing mantle convection, as well as understand dynamic surface processes like atmospheric seasonal changes and the detection of ground water reservoirs,” said Dr Lisa Wörner of DLR, who presented on the MaQuIs mission at EPSC2024 this week.
Further information
Root, B., Alkahal, R., Qin, W., and Thieulot, C.: Exploration of high mass subsurface structures in the northern hemisphere with joint flexure and mantle convection modelling of the Martian gravity field , Europlanet Science Congress 2024, Berlin, Germany, 8–13 Sep 2024, EPSC2024-730, https://doi.org/10.5194/epsc2024-730.
Woerner, L.: Quantum Technologies for Planetary Geodesy, Europlanet Science Congress 2024, Berlin, Germany, 8–13 Sep 2024, EPSC2024-632, https://doi.org/10.5194/epsc2024-632.
About the Europlanet Science Congress (EPSC)
The Europlanet Science Congress (https://www.epsc2024.eu/), established in 2006 as the European Planetary Science Congress, is the largest planetary science meeting in Europe and regularly attracts around 1200 participants. It covers the entire range of planetary sciences with an extensive mix of talks, workshops and poster sessions, as well as providing a unique space for networking and exchanges of experiences.
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About Europlanet
Europlanet (www.europlanet-society.org) is a not-for-profit association that provides the planetary science community with access to research infrastructure and services. The Europlanet Association Sans But Lucratif (AISBL), established in 2023, builds on the heritage of a series of projects funded by the European Commission between 2005 and 2024 to support the planetary science community in Europe and around the world. Today, Europlanet is an independent membership organisation that provides mobility programmes, community services and training.
Europlanet received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement numbers 871149 (Europlanet 2024 Research Infrastructure) and 654208 (Europlanet 2020 RI), FP7 under grant agreement number 228319 (Europlanet RI) and FP6 under grant agreement number RICA-CT-2004-001637 (European Planetology Network).
Astrobiology
