Reeneath
Mars' northern polar ice cap, dense elements
have drawn attention. Their origin remains
unknown, and hypotheses are multiplying.
These buried structures, detected through
gravimetric analyses, are thought to be
remnants from a time when Mars harbored vast
oceans. Bart Root's team at Delft University
has highlighted these anomalies under
sediments that would have once covered an
ancient seabed.
Map highlighting the dense structures
in the northern hemisphere. The regions
marked by black lines are high mass
anomalies that do not show correlation
with the geology and topography. These
hidden subsurface structures are covered
by sediments from an ancient ocean.
Their origin remains a mystery, and a
dedicated gravitational mission, like
MaQuIs, is needed to uncover their
nature.
Credit: Root et al.
The elements are significantly denser than
their immediate surroundings, with an
estimated density between 300 and 400
kilograms per cubic meter higher than the
surrounding area. According to the
researchers, several hypotheses are being
considered to explain their origin. They could
be the result of ancient volcanic activity,
having left massive deposits beneath the
surface.
Another possible explanation is that these
structures formed following meteorite impacts,
which could have compacted the Martian soil.
However, no visible traces on the surface can
confirm these hypotheses, making their origin
and nature even more puzzling.
Among the most fascinating discoveries, some
of these formations are found around the
volcanic region of Tharsis, where the famous
Olympus Mons rises. Yet, contrary to
predictions, this area is not sinking under
its own weight. In fact, observations reveal
surprising terrain elevation. This could be
explained by the upward movement of a magma
plume beneath the lithosphere, suggesting that
volcanic activity might still be possible in
the near future.
These new data suggest that Mars still retains
an active internal dynamic. Researchers
mention the possibility that these internal
movements could generate new geological
features at the surface of the red planet.
Thus, these discoveries could challenge our
understanding of Mars, hinting at still
unknown phenomena beneath its surface.
What is a magma plume?
A magma plume is a rising column of molten
rock from the deep interior of a planet. This
column of magma ascends through the mantle,
driven by internal heat. When it reaches the
lithosphere, it can cause volcanoes or other
geological formations.
On Mars, evidence suggests that a magma plume
might be rising beneath the Tharsis region,
where Olympus Mons is located (the tallest
known feature in the Solar System). This
phenomenon could explain the unexpected
elevation of the terrain, counteracting the
pressure exerted by the volcanoes' weight and
hinting at potential future volcanic activity.
How does gravimetry work to explore Mars?
Gravimetry is an analysis method that measures
variations in a planet's gravitational field.
On Mars, it helps detect density differences
beneath the surface, revealing hidden
structures. These variations affect the
movements of satellites in orbit.
Researchers use these tiny deviations to map
the distribution of Mars' internal masses.
Using this data, they can identify anomalies,
such as magma pockets, buried craters, or
ancient sediments, without needing to drill
into the surface.