For decades, the standard model of early solar system dynamics included a period known as the Late Heavy Bombardment (LHB), a hypothesized epoch approximately 3.9 billion years ago during which the inner planets experienced a sudden, dramatic spike in asteroid and comet impacts. This consensus emerged primarily from radiometric dating of impact melt rocks returned by the Apollo missions; the samples, collected from diverse lunar equatorial regions, consistently yielded ages tightly clustered around the 3.9-billion-year mark. Because the Apollo landing sites were widely separated, planetary scientists inferred that the rocks recorded dozens of distinct basin-forming impacts occurring nearly simultaneously, implying a system-wide cataclysm.
However, recent re-evaluations of both lunar geology and the Apollo samples have cast significant doubt on the LHB hypothesis. The original consensus rested on the assumption that the impact melts collected at each Apollo site were produced by localized, independent cratering events. Yet, advanced geochemical fingerprinting and high-resolution computer modeling of ejecta trajectories suggest a different narrative. These studies indicate that the massive impact that formed the Imbrium basin—one of the youngest and largest craters on the Moon—was energetic enough to distribute its debris globally.
Consequently, researchers now argue that the widely separated Apollo sites were almost certainly contaminated by ejecta from the single Imbrium event. If the impact melts dated by scientists predominantly originate from this one colossal collision, the clustering of their ages ceases to be evidence for a sudden flurry of distinct impacts. Instead, the data more plausibly points to a single dominant event that obscured the broader cratering record. Thus, rather than experiencing a delayed, violent spike in impacts, the inner solar system likely underwent a gradual, continuous decline in bombardment following its initial formation.
Which one of the following most accurately expresses the main point of the passage?
- ARadiometric dating of impact melt rocks collected from widely separated lunar landing sites consistently yields ages clustered around 3.9 billion years ago.
- BThe geological history of the inner solar system is characterized by a gradual, continuous decline in asteroid collisions rather than by sudden, catastrophic spikes.
- CPlanetary scientists traditionally assumed that the formation of the Imbrium basin caused a sudden, dramatic spike in asteroid and comet impacts.
- The theory that the inner solar system underwent a sudden spike in meteor impacts is undermined by evidence that lunar sample ages reflect contamination from a single massive collision.Answer
- EAdvanced geochemical fingerprinting and computer modeling demonstrate that ejecta from the Imbrium impact was distributed globally across the Moon.