Strange Discovery: Venus Features a Lava Tube

There is compelling evidence that vast underground tunnels have been formed from lava on Venus. These formations are unusually wide and distinct from those found on other celestial bodies.

It is generally accepted that underground tunnels, carved through lava, exist as lava tubes on Earth, the Moon, and Mars. Smaller, low-gravity planets tend to develop more porous tubes as their rocky walls are less susceptible to collapse due to weaker gravity. For instance, the Moon has such large tubes that scientists have proposed utilizing them as habitats for astronauts, shielding them from intense solar winds.

Researchers have observed indications of these lava tubes on Venus, evident from surface holes that may have been formed by the underground features or by other geological activities associated with its active fault lines.

Recently, Barbara de Tofoli from the University of Padova in Italy along with her colleagues uncovered direct evidence of these lava tubes on Venus. Remarkably, despite Venus’s similarities to Earth regarding its mass and gravity, its lava tubes appear to be surprisingly wide, with a volume comparable to those found on the Moon.

“While Earth has a small number of lava tubes, Mars has a slightly larger count, and the Moon has even more. Venus disrupts this trend by featuring incredibly large tubes, indicating its potential significance,” she stated at the Europlanet Science Congress in Helsinki, Finland, earlier this month.

De Tofoli and her team used radar and mapping data from previous missions to examine the alignment of these pits near large volcanoes. They identified four distinct sites where alternative geological explanations, such as structural activities, were implausible. The pits were also found to align with the steepest sections of volcanic slopes, consistent with the movement of lava. Their depth-to-width ratio corresponded with known lava tubes.

The unexpectedly large size of these tubes, especially their width, implies that the extreme conditions on Venus, characterized by high temperatures and pressure, can influence the movement of molten rock beneath the surface. “Due to the extremely high pressure, the floor of these tubes is not eroded as intensely as it typically is on other planets; instead, it remains largely flat throughout the tube.”