Grooves and gashes associated with the Imbrium Basin on the moon have long been puzzling. New research shows how some of these features were formed and uses them to estimate the size of the Imbrium impactor. The study suggests it was big enough to be considered a protoplanet. Credit: NASA/Northeast Planetary Data Center/Brown University
The asteroid that slammed into the moon 3.8 billion years ago creating the Imbrium Basin may have had a diameter of at least 150 miles, according to a new estimate. The work helps explain puzzling geological features on the moon’s near side, and has implications for understanding the evolution of the early solar system. This new size estimate suggests the impactor was 2X larger in diameter and 10X more massive than previous estimates.
Previous estimates, Schultz said, were based solely on computer models and yielded a size estimate of only about 50 miles in diameter. These new findings help to explain some of the puzzling geological features that surround the Imbrium Basin. The work also suggests – based on the sizes of other impact basins in the Moon, Mars and Mercury – that the early solar system was likely well stocked with protoplanet-sized asteroids.
The Imbrium Basin – seen from Earth as a dark patch in the NW quadrant of the Moon’s face – measures ~750 miles across. The basin is surrounded by grooves and gashes, large enough to be seen with even small telescopes from Earth, created by rocks blasted out of the crater when it was formed. These features, known as the Imbrium Sculpture, radiate out from the center of the basin but are concentrated on the basin’s southeast side. That suggests that the impactor traveled from the northwest, impacting at an oblique angle rather than straight on.
But in addition to features radiating from the basin’s center, there is a second set of grooves with a different alignment. These appear to come from a region to the northwest, along the trajectory from which the impactor came. “This second set of grooves was a real mystery,” Schultz said. “No one was quite sure where they came from.” Through hypervelocity impact experiments performed using the Vertical Gun Range at the NASA Ames Research Center, Schultz was able to show that those grooves were likely formed by chunks of the impactor that sheared off on initial contact with the surface. The grooves created by those chunks enabled Schultz to estimate the size of the impactor.
The Vertical Gun Range employs a 14-ft cannon that fires small projectiles at up to 16,000 miles/hr, while impact plates and high-speed cameras record the ballistic dynamics. During his experiments with low-angle impacts, Schultz noticed impactors tend to start breaking apart when they first make contact with the surface. That point of initial contact is actually behind or “up-range” of the final crater, where the bulk of the impactor digs into the surface. The chunks that break off up-range of the final crater continue to travel at a high rate of speed, scouring and grooving the surface.
With an understanding of how those grooves were created, Schultz could use them to find the Imbrium impact point. And because the fragments would have broken off from the either side of the impactor, the groove trajectories could be used to estimate the impactor’s size. Those calculations yielded an estimated diameter of 250 km or 150 miles across, large enough for the object to be classified as a protoplanet.
Schultz et al used similar methods to estimate the sizes of impactors related to several other basins on the Moon created by oblique impacts. Those estimates – for the Moscoviense and Orientale basins on the Moon’s far side – yielded impactor sizes of 100 and 110 kilometers across respectively, larger than some previous estimates. Combining these new estimates with the fact that there are even larger impact basins on the Moon and other planets, Schultz concludes that protoplanet-sized asteroids may have been common in the early solar system.
The surviving fragments from these impactors would have littered the ancient surface of the Moon, slowly becoming mixed with native soil and rock. That could help explain why samples returned from the Apollo missions had such a high meteoritic content. That is particularly true of Apollo 16, which landed downrange from the Imbrium impact. Furthermore, Schultz’s work suggests fragments from these giants could account for a many of the impacts that occurred during a period called the Late Heavy Bombardment, which occurred from about 3.8 billion years ago to around 4 billion years, when scientists think most of the craters we see on the Moon and Mercury were formed.
The impact models Schultz and Crawford developed suggest that thousands of the chunks that crumbled off of the Imbrium impactor and others would have broken and kept going, escaping the Moon’s gravity and flying off into space. On subsequent orbits around the sun, those chunks would have crossed the Earth and Moon orbits again and again, creating a strong possibility of subsequent impacts. Some of those objects would have been a kilometer or two across, large enough to create 20-kilometer craters. “These chips off the old blocks could have contributed significantly to the impact record we see on the Moon and other terrestrial planets,” Schultz said. https://news.brown.edu/articles/2016/07/imbrium
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