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| PhD student Ji-In Jung, left, and Assistant Professor Sonia Tikoo examine a collection of lunar samples. Photo Credit: Harry Gregory |
By demonstrating that spaceflight doesn’t adversely affect the magnetism of moon rocks, Stanford researchers underscore the exciting potential of studying the magnetic histories stored in these samples.
For decades, scientists have pondered the mystery of the moon’s ancient magnetism. Based on analyses of lunar samples, its now-deceased magnetic field may have been active for more than 1.5 billion years – give or take a billion years. Scientists believe it was generated like the Earth’s via a dynamo process, whereby the spinning and churning of conductive liquid metal within a rocky planet’s core generates a magnetic field. However, researchers have grappled with how such a small planetary body could have sustained a long-lived magnetic field. Some have even questioned the legitimacy of return samples that point to the existence of an ancient dynamo, suggesting magnetism may have been acquired via exposure to strong magnetic fields onboard spacecraft during the return mission or from plasmas produced by massive impacts on the moon.
Stanford University scientists have now demonstrated that the magnetism in lunar samples is not adversely altered by the spacecraft journey back to Earth or certain laboratory procedures, disproving one of the two major oppositions to the ancient dynamo theory. The findings, published in Geophysical Research Letters Oct. 11, bode well for research stemming from other sample-return missions from space, since any magnetic contamination acquired during flight or on Earth can likely be easily removed.
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