Radar view of pits on Venus volcano flank suggesting lava tube entrancesPhoto by Tomáš Malík on Pexels

Scientists have uncovered clear signs of huge underground lava tubes on Venus, our nearest planetary neighbor. These tunnels, some wide enough to swallow a city block, sit beneath the planet's scorching surface and hint at ongoing volcanic forces. The findings come from detailed analysis of old radar maps and new computer models, pointing to structures formed by flowing lava.

Background

Venus sits just inside Earth's orbit, closer to the Sun, with a surface hot enough to melt lead at over 460 degrees Celsius. A thick blanket of clouds hides the ground from view, so spacecraft like NASA's Magellan from the 1990s used radar to map it. Those maps showed odd pits and channels near volcanoes, but until now, no one could say for sure what caused them.

For years, experts guessed these might be entrances to lava tubes—empty tunnels left when the top of a lava flow hardens while liquid rock drains away below. On Earth, we see them in places like Hawaii. The Moon and Mars have bigger ones because lower gravity lets roofs hold up better. Venus, with gravity close to Earth's at 91 percent, should not support such large versions. Yet recent work challenges that idea.

Researchers started piecing this together by looking at pits on volcano slopes. These openings line up with the downhill flow of lava, just as you would expect. They modeled how lava behaves there, factoring in the planet's heat, pressure, and rock strength. The result: tubes that dwarf anything on our world.

Key Details

The new evidence comes from a team that spotted four key pits on Venus volcano flanks, all in areas blanketed by lava flows. These pits point downhill, matching the path lava would take. One study used data from Magellan to confirm this setup fits the classic lava tube formation: a solid roof over an empty space where molten rock once flowed.

Size and Stability

Computer models pushed the limits. Using a method called Finite Element Limit Analysis, researchers tested how big these tubes could get before collapsing. They found widths up to one kilometer possible in strong rock, with stable sizes around a few hundred meters. Roof thickness, tube height, and rock type all play a part. These match channels seen in orbital images, plus surface hints like pit chains.

Venus conditions help. The intense heat softens rock just enough, while high pressure keeps things intact. Volumes could make these the biggest subsurface voids in the solar system. They cluster near big volcanoes like Idunn Mons and Maat Mons, where fresh lava signs appear in radar scans.

Other data backs active geology. Circular features called coronae, some hundreds of miles wide, show hot plumes rising from deep inside. Gravity maps from Magellan reveal less dense material under 52 of 75 studied coronae, driving surface changes without Earth's plate tectonics.

"The characteristics of the observed Venusian lava tubes, particularly their large scale, suggest that Venus may host some of the most extensive subsurface cavities in the solar system." – Research team in Icarus paper

What This Means

These tubes offer a glimpse into Venus's hidden geology. They track how heat moves inside the planet and how its crust shifts without plate tectonics. Understanding them could explain why Venus turned into a runaway greenhouse hellscape while Earth stayed livable.

The discovery raises questions about current activity. Surface changes at key spots suggest lava flows or ash today. Sulfur in the air and wind patterns point to volcanoes stirring the atmosphere. If tubes link to this, Venus might reshape its face right now.

Future missions will check. NASA's DAVINCI will drop a probe through the clouds to sample air and snap descent pictures. VERITAS will map the surface in detail. Europe's EnVision, due in 2031, carries a radar sounder to peer underground, perfect for spotting tubes and voids.

Stable, vast tunnels could shield explorers from surface heat. Humans might one day enter them for samples or bases, though the air inside would still be deadly. This work ties past eruptions to present forces, filling gaps in Venus's story.

Experts now hunt for more signs: gravity quirks, skylights, or empty spaces in new scans. Each find sharpens models of volcanic spread, wind effects on ash plumes, and chemical cycles. Venus, long a mystery, starts to reveal its inner workings through these buried paths.

The research appears in journals like Icarus and builds on decades of data. Teams stress the need for better tools to confirm tubes and measure activity. As missions launch, answers about our twin planet's fire will come into focus.

Author

  • Vincent K

    Vincent Keller is a senior investigative reporter at The News Gallery, specializing in accountability journalism and in depth reporting. With a focus on facts, context, and clarity, his work aims to cut through noise and deliver stories that matter. Keller is known for his measured approach and commitment to responsible, evidence based reporting.

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