Vast Hidden Magma Systems Discovered on Mars
Researchers from the University of Oxford have discovered evidence of ancient, Earth-like magmatic systems beneath the surface of Mars. The study suggests that Mars may have experienced complex internal geological recycling despite lacking plate tectonics.
Why it matters
This discovery challenges existing models of Martian geology and provides new insights into the potential habitability of rocky planets.
Researchers from the University of Oxford have uncovered evidence that Mars once hosted enormous, Earth-like magmatic systems deep beneath its surface - despite the planet lacking the plate tectonics long thought necessary for this kind of geological complexity. The findings, published today (26 June) in Nature Astronomy , reveal fascinating new possibilities for how rocky planets become habitable.
The article is a scientific report based on peer-reviewed findings published in Nature Astronomy.
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