Where has the moon’s lost magnetism gone? This enigma has intrigued scientists for decades, particularly after evidence collected by orbiting spacecraft indicated an unexpectedly strong magnetic field encoded in lunar rocks. In stark contrast, today’s moon lacks an intrinsic magnetic field. A study conducted by scientists at the Massachusetts Institute of Technology (MIT) proposes a possible resolution to this mystery. They hypothesize that a combination of ancient, feeble lunar magnetism and a massive impact could have temporarily generated potent magnetic fields, especially concentrated on the moon’s far side.
As detailed in findings published in the journal Science Advances, researchers used intricate simulations to demonstrate how an impact event, such as that from a colossal asteroid, could create a cloud of ionized particles enveloping the moon. This plasma would circulate around the lunar surface, concentrating on the hemisphere opposite the impact. At that location, the plasma could briefly augment the moon’s weak magnetic field. Geological samples within that region could potentially hold records of the magnetic spike before it dissipated swiftly.
This hypothesis offers a plausible explanation for the clusters of highly magnetized rocks identified in the lunar far side, particularly near the south pole. Strikingly, one of the largest recognized impact basins, the Imbrium basin, is situated on the near side, aligning perfectly with these magnetic anomalies. The researchers are inclined to believe that this impact might have unleashed the plasma cloud central to their simulations.
Isaac Narrett, the study’s lead author and a graduate student in MIT’s Department of Earth, Atmospheric and Planetary Sciences, remarked on the perplexity surrounding the moon’s magnetic phenomena. "There are large parts of lunar magnetism that are still unexplained," he noted, further asserting that the majority of the strong magnetic fields detected by orbiting spacecraft can be rationalized via this process, particularly on the moon’s far side.
Historical data from lunar surface samples collected by NASA’s Apollo missions during the 1960s and 70s, along with global magnetic measurements conducted by orbiting spacecraft, have long indicated remnant magnetism in surface rocks, primarily on the moon’s far side. The prevailing theory ties this magnetism to a global magnetic field produced by an internal "dynamo," similar to Earth’s, where molten materials churn within its core. While this process is believed to have existed in the moon’s past, its significantly smaller core suggests a much weaker magnetic field, raising concerns as to whether it can account for the highly magnetized rocks observed, particularly on the far side.
An alternative theory proposed by scientists previously considered the possibility of a gigantic impact that might have generated plasma to enhance the moon’s feeble magnetic field. In 2020, researchers, including Narrett’s co-authors Rona Oran and Benjamin Weiss, simulated a titanic impact on the moon, coupling it with the limited solar-generated magnetic field. Ultimately, these simulations indicated that the impact would not sufficiently amplify the solar magnetic field to elucidate the strong magnetic measurements discovered in lunar rocks, effectively dismissing the potential role of plasma-induced impacts in addressing the moon’s magnetic deficiencies.
In their current study, the research team adopted a fresh perspective. They initially presumed that the moon once possessed a dynamo capable of generating its own magnetic field, albeit a weak one. By estimating the size of its core, they predicted the moon’s magnetic field could have reached approximately 1 microtesla, about 50 times weaker than the Earth’s present-day magnetic field.
Armed with this foundational assumption, the scientists simulated a massive impact on the moon’s surface—akin to what is believed to have created the Imbrium basin. Utilizing simulations detailed by collaborator Katarina Miljkovic, the team recreated the plasma cloud birthed from the forceful impact that vaporized surface materials. They also employed computational methodologies developed by partners at the University of Michigan to simulate the behavior of the resulting plasma as it interacted with the moon’s inherent weak magnetic field.
The simulations revealed that as the plasma cloud emerged from the impact, portions of it would escape into space, while the remainder would envelop the moon and concentrate on the opposing sid. There, the plasma could briefly compress and amplify the moon’s already weak magnetic field. Narrett noted that this entire sequence—from the onset of amplified magnetism to its rapid decline back to baseline—was remarkably swift, likely occurring within a span of around 40 minutes.
A key question arises: would this ephemeral magnetic spike be sufficient for surrounding rocks to record the changed magnetic state? The researchers affirmatively answer this with the assistance of an additional effect linked to the impact. They concluded that an impact of the scale seen in Imbrium would generate a pressure wave traversing through the moon, akin to seismic shocks. These waves would converge on the far side, creating conditions that would momentarily “jitter” the surrounding rocks.
This jarring would briefly disrupt the arrangement of electrons in these rocks—subatomic particles that ordinarily align with external magnetic fields. The researchers propose that the rocks were jolted just as the impact’s plasma amplified the moon’s magnetic field. Once settled, the electrons would align in accordance with the transient high magnetic field.
As Benjamin Weiss illustrated metaphorically, “It’s as if you throw a 52-card deck in the air, in a magnetic field, and each card has a compass needle. When the cards settle back to the ground, they do so in a new orientation,” corresponding to their new magnetization process. This innovative combination of a lunar dynamo, paired with a massive impact and the resultant shockwave, could satisfactorily account for the moon’s highly magnetic surface rocks, particularly in regions where sunlight seldom reaches.
An intriguing avenue for future research to substantiate this hypothesis lies in the possibility of directly sampling lunar rocks. Investigating the lunar far side’s geological formations, notably near the south pole, could offer scientists definitive insights into signs of shock and heightened magnetism. NASA’s Artemis program aims to explore these undisturbed regions, providing a valuable opportunity for researchers.
The allure of the moon’s mysterious magnetic history continues to fascinate the scientific community. Researchers have navigated a complex web of hypotheses, proposing various explanations for the moon’s magnetic features. Narrett and his team’s conclusion suggests a dual influence—a blend of historical dynamism within the moon’s core and the dramatic forces unleashed by cosmic impacts. This audacious proposition stands as a testable hypothesis, offering an exciting new chapter in lunar studies.
In conclusion, the moon has long served as a celestial body of scientific intrigue, harboring intricate mysteries that continue to stimulate the passions of researchers. With the continued advancements in exploration missions like Artemis and the analytical capabilities provided by modern technology, scientists remain poised to unravel the remaining secrets of the moon’s magnetism and its complex geological history, cementing an ever-deepening understanding of our nearest celestial neighbor.
Subject of Research: Lunar Magnetism and Impact Events
Article Title: Impact plasma amplification of the ancient lunar dynamo
News Publication Date: 23-May-2025
Web References: DOI Link
References: Science Advances
Image Credits: MIT News Office
Keywords
Lunar magnetism, plasma amplification, lunar dynamo, impact events, geological history.
