
Moon’s South Pole to Reveal Clues About Lunar Birth and Early History in Upcoming NASA Artemis Missions
NASA’s Artemis program is set to uncover the moon’s secrets, including its birth and early history, with new research suggesting that the moon’s south pole holds a treasure trove of clues. A recent study published in Nature provides new insights into the moon’s violent early history, shedding light on the mystery of why the far side of the moon is heavily cratered while the near side is relatively smooth. As astronauts prepare to touch down near the moon’s south pole in the coming years, they may discover a remarkable archive of clues about the moon’s formation and evolution.
The upcoming NASA Artemis missions are expected to uncover the moon’s secrets, including its birth and early history. When astronauts land near the moon’s south pole, they may discover a remarkable archive of clues about how the moon was born. This possibility comes from new research led by Jeffrey Andrews-Hanna, a planetary scientist at the University of Arizona. The study, published on October 8 in Nature, paints a vivid picture of the moon’s violent early history and could shed light on one of lunar science’s enduring mysteries: why the far side of the moon is heavily cratered while the near side, which hosted the Apollo landings of the 1960s and 1970s, is comparatively smooth.
The Moon’s Violent Early History
Around 4.3 billion years ago, when the solar system was still young, a massive asteroid struck the far side of the moon. The colossal impact carved out the South Pole-Aitken basin (SPA), an immense crater measuring roughly 1,200 miles from north to south and 1,000 miles from east to west. Its elongated, oval shape suggests the asteroid hit at an angle rather than head-on. By comparing SPA with other giant impact sites across the solar system, Andrews-Hanna’s team found a consistent pattern: these enormous craters narrow in the direction the impactor was traveling, forming a shape similar to a teardrop or avocado. Contrary to earlier assumptions that the asteroid came from the south, their analysis shows the SPA basin tapers toward the south, meaning the asteroid likely arrived from the north.
Key Highlights of the Study
* The asteroid that formed the SPA basin likely came from the north, not the south, as previously assumed.
* The SPA basin is an immense crater measuring roughly 1,200 miles from north to south and 1,000 miles from east to west.
* The asteroid’s impact created a massive ejecta blanket, with the southern, or down-range, rim buried under thick layers of debris blasted from deep within the moon.
* The northern, up-range end of the SPA basin contains less debris, making it a less desirable location for studying the moon’s early history.
* The Artemis missions will be landing on the down-range rim of the basin, the best place to study the largest and oldest impact basin on the moon.
According to Andrews-Hanna, “This means that the Artemis missions will be landing on the down-range rim of the basin — the best place to study the largest and oldest impact basin on the moon, where most of the ejecta, material from deep within the moon’s interior, should be piled up.” Further evidence for a north-to-south impact came from studying the moon’s topography, crustal thickness, and surface chemistry. Together, these clues not only strengthen the case for the asteroid’s northern origin but also reveal new details about the moon’s inner structure and how it evolved over time.
The Moon’s Inner Structure and Evolution
Scientists have long believed that the early moon was once completely molten, forming a global “magma ocean.” As it cooled, denser minerals sank to create the mantle, while lighter ones floated upward to form the crust. Some elements, however, failed to fit neatly into these solid layers and accumulated in the last remnants of molten material. Those residual ingredients included potassium, rare earth elements, and phosphorus — collectively known as “KREEP,” with the “K” representing potassium’s chemical symbol. Andrews-Hanna noted that these elements are unusually concentrated on the moon’s near side.
The Magma Ocean and KREEP-Rich Material
* The early moon was once completely molten, forming a global “magma ocean.”
* As the magma ocean cooled, denser minerals sank to create the mantle, while lighter ones floated upward to form the crust.
* KREEP-rich material, including potassium, rare earth elements, and phosphorus, accumulated in the last remnants of molten material.
* The KREEP-rich material is unusually concentrated on the moon’s near side, causing it to heat up and leading to intense volcanism that formed the dark volcanic plains.
According to Andrews-Hanna, “If you’ve ever left a can of soda in the freezer, you may have noticed that as the water becomes solid, the high fructose corn syrup resists freezing until the very end and instead becomes concentrated in the last bits of liquid. We think something similar happened on the moon with KREEP.” As the magma ocean gradually solidified into crust and mantle, the KREEP-rich material became concentrated on the moon’s near side, causing it to heat up and leading to intense volcanism that formed the dark volcanic plains.
Implications for the Artemis Missions
The new study of the SPA impact crater revealed a striking and unexpected asymmetry around the basin that supports the theory that the KREEP-rich material ended up on the near side. The ejecta blanket on the western side of the SPA basin is rich in radioactive thorium, but not on its eastern flank. This suggests that the gash left by the impact created a window through the moon’s skin right at the boundary separating the crust underlain by the last remnants of the KREEP-enriched magma ocean from the “regular” crust. Once astronauts bring samples back to Earth, researchers hope to find more pieces to the puzzle and gain a better understanding of the moon’s early history and evolution.
What to Expect from the Artemis Missions
* The Artemis missions will provide a unique opportunity to study the moon’s early history and evolution.
* Astronauts will land on the down-range rim of the SPA basin, the best place to study the largest and oldest impact basin on the moon.
* The samples brought back to Earth will be analyzed by scientists around the world, providing new insights into the moon’s composition and evolution.
* The study of the moon’s early history and evolution will help us better understand the formation and evolution of the solar system.
In conclusion, the upcoming NASA Artemis missions are set to uncover the moon’s secrets, including its birth and early history. The new research led by Jeffrey Andrews-Hanna provides new insights into the moon’s violent early history and sheds light on the mystery of why the far side of the moon is heavily cratered while the near side is relatively smooth. As astronauts prepare to touch down near the moon’s south pole, they may discover a remarkable archive of clues about the moon’s formation and evolution.
Keywords:
* Moon’s south pole
* NASA Artemis program
* Lunar birth and early history
* South Pole-Aitken basin (SPA)
* Magma ocean
* KREEP-rich material
* Moon’s inner structure and evolution
* Solar system formation and evolution
Hashtags:
* #MoonExploration
* #ArtemisProgram
* #LunarScience
* #SpaceResearch
* #SolarSystemFormation
* #NASA
* #SpaceMissions
* #MoonHistory
* #LunarGeology
* #PlanetaryScience
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