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Science
16 November 2024

Volcanoes Once Roamed The Moon's Far Side

Chang'e-6 mission reveals ancient eruptions changed the lunar surface for over a billion years

Recent lunar exploration has unveiled astonishing revelations about the Moon's far side, shedding light on its volcanic history. Specifically, findings from China’s Chang’e-6 mission have confirmed the presence of volcanic activity on this little-explored region, with evidence dating back as far as 4.2 billion years. This groundbreaking discovery stems from the analysis of lunar soil samples collected during Chang’e-6's mission, which marked the first time material from the far side of the Moon was returned to Earth.

The Chang’e-6 mission, which lasted 53 days, utilized a robotic lander to scoop and drill the lunar surface, gathering significant samples for analysis. Among these samples were fragments of basalt, the type of volcanic rock formed from cooled lava, which scientists identified as solid evidence of volcanoes being active approximately 2.8 billion years ago. Importantly, one outlier rock sample pushed the timeline of volcanic activity back even earlier, indicating persistent activity through geological time.

At around 4.5 billion years old, Earth is younger than its celestial companion, the Moon, which formed shortly after. The earlier volcanic activity on the Moon parallels early geological activities on Earth, where the earliest known life forms appeared around 3.7 billion years ago, offering unique insights across these planetary evolutions. The Moon’s surface was initially molten and scorching, eventually forming the grey, cratered surface we observe today.

Volcanic activity on the Moon’s far side had been theorized based on various missions, yet direct evidence had remained elusive until now. Before the Chang’e-6 findings, researchers had noted geological disparities between the Moon's near and far sides, where the near side exhibits large basalt plains created from ancient volcanic eruptions. This new research confirms similar history on the far side, allowing for greater analysis and comparison.

Christopher Hamilton, a planetary volcanology expert at the University of Arizona, emphasized the significance of obtaining these samples, noting, “To obtain a sample from this area is really important because it’s an area we have no data for.” Analyzing the basalt fragments has now provided the first real data confirming the far side's geological past.

The technical process of the analysis included utilizing lead isotopes to date the 108 basalt fragments collected during the mission. Previous assumptions based on remote sensing had suggested the far side could have been volcanically active, but these assumptions were primarily theoretical. The results validate those earlier hypotheses and confirm over 1 billion years of volcanic eruptions, extending the Moon’s active geological phase.

Another fascinating aspect of this research is the disparity between the Moon's two hemispheres. The far side typically shows fewer lava plains and is characterized more by its craters. According to Qiu-Li Li, one of the study's co-authors from the Chinese Academy of Sciences, the contrasting geological characteristics pose questions about why the two parts of the Moon differ so significantly.

Published findings appeared both in Science and Nature, highlighting how these insights may assist scientists in constructing more accurate timelines for lunar activity. The high-precision Pb-Pb dating of zircon minerals and Rb-Sr dating of other volcanic materials yielded isochron ages consistent with the 2.83 billion-year timeframe reported.

This research paves the way for future missions aimed at extracting more samples and analyzing different regions of the Moon to broaden our comparative knowledge of both the Earth and its lunar companion. The existence of volcanic activity for such extended periods also implies significant internal heating, possibly from the Moon's mantle’s composition. Understanding these processes could offer insights applicable to other rocky bodies across the solar system, including Mars and Mercury, opening exciting new possibilities for lunar and planetary research.

While the Moon has long been viewed as our celestial sidekick, the intensified research uncovers aspects about its dynamic past, prompting scientists to rethink the geological narrative of our nearest neighbor. The work from China’s Chang’e missions exemplifies the advancements made possible through modern technology and international space collaborations, enhancing our comprehension of lunar geology.

These developments herald the importance of continued lunar exploration and research. The Chang’e-6 mission serves not only as proof of volcanic activity on the Moon’s far side but as inspiration for upcoming exploratory missions by various space agencies. Future investigations aim to resolve remaining questions about the Moon’s surface evolution, its internal structure, and the potential for sustaining extraterrestrial life.

With mounting evidence and newfound interest, the Moon's role as both a geological subject of study and a target for colonization will likely expand, providing new chapters for lunar exploration and our quest for knowledge beyond Earth.

Looking forward, the findings surrounding the far side of the Moon could lead to collaborative missions between countries focused on unraveling the enigmas of solar system bodies. This research showcases the Moon’s ancient fiery past, enhancing our broader appreciation of celestial dynamics and the forces shaping our cosmic neighborhood.

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