Researchers have confirmed the existence of a large underground cave on the Moon using radar data from NASA’s Lunar Reconnaissance Orbiter. Located in the Mare Tranquillitatis, the cave is a former lava tube that could provide a stable, shielded environment for future human lunar bases.
TLDR: Scientists have identified the first confirmed lunar cave, a massive underground lava tube in the Mare Tranquillitatis. Discovered via radar analysis, the cavern offers natural protection from radiation and extreme temperatures, making it a prime candidate for future astronaut shelters and long-term lunar habitation.
Researchers have officially confirmed the existence of a massive underground cave on the Moon, accessible through a deep, vertical pit in the Mare Tranquillitatis. This landmark discovery, published in the journal Nature Astronomy, represents a major breakthrough in lunar science and human exploration. By re-analyzing radar data collected over a decade ago by NASA’s Lunar Reconnaissance Orbiter (LRO), scientists have provided the first definitive evidence of an accessible lava tube beneath the lunar surface—a geological feature that has been hypothesized for decades but never before confirmed with such precision.
The cave is located at the base of the Tranquillitatis pit, which is the deepest known pit on the Moon, originally identified in 2009. This pit is essentially a “skylight,” created when a portion of a lava tube’s roof collapsed. The new analysis of radar reflections suggests that the cavern extending from the bottom of this pit is at least 40 meters wide and tens of meters long, though researchers believe it could extend for kilometers. These structures formed billions of years ago during the Moon’s active volcanic period. As molten lava flowed across the surface, the outer layers cooled and hardened into a crust, while the liquid interior continued to flow. Once the volcanic activity ceased and the lava drained away, it left behind hollow, tube-like conduits.
This subterranean discovery offers a transformative environment for future lunar exploration and long-term human habitation. The lunar surface is an incredibly hostile environment, characterized by extreme temperature fluctuations—swinging from a scorching 127 degrees Celsius during the day to a frigid minus 173 degrees Celsius at night. Furthermore, the lack of a substantial atmosphere leaves the surface exposed to a constant bombardment of solar radiation, cosmic rays, and micrometeorites. The interior of a lava tube, however, provides a naturally shielded environment where temperatures remain relatively stable and the thick basaltic ceiling acts as a robust barrier against external hazards.
The study was spearheaded by Lorenzo Bruzzone and Leonardo Carrer from the University of Trento in Italy. Their team utilized advanced signal processing techniques to re-examine data from the LRO’s Miniature Radio Frequency (Mini-RF) instrument. To validate their findings, the researchers compared the lunar radar signatures with data from terrestrial lava tubes found in Lanzarote, Spain, and Hawaii. This comparative analysis allowed them to distinguish between simple debris piles at the bottom of the pit and a genuine void extending into the lunar crust. The radar waves effectively “bounced” off the floor of the cave, confirming the presence of an open gallery.
Despite the promise of these caves, accessing them presents a formidable engineering challenge. The Tranquillitatis pit features sheer vertical walls that drop more than 100 meters to the cave floor. Future missions will likely require specialized robotic systems, such as rappelling rovers or autonomous drones, to navigate the descent and explore the interior. These missions will be crucial for assessing the structural integrity of the cave ceilings and the chemical composition of the walls. This would be a necessary precursor to any permanent human settlement.
Beyond their utility as shelters, these caves are of immense scientific value. Because the interiors have been shielded from space weathering for billions of years, they likely contain a pristine record of the Moon’s volcanic history and mineralogical evolution. Furthermore, the confirmation of this cave suggests that similar structures may exist at the lunar poles. In these permanently shadowed regions, lava tubes could potentially harbor water ice, a critical resource for sustainable human presence. This discovery marks a fundamental shift in lunar strategy, moving from surface-based habitats to utilizing the Moon’s natural geological architecture for the next phase of space exploration.

