The Late Heavy Bombardment is a hypothesized period roughly 4.1 to 3.8 billion years ago during which the inner Solar System, including Earth, the Moon and Mars, experienced a markedly elevated rate of asteroid and comet impacts compared to both earlier and later periods. The main evidence comes from the ages of impact melt rocks collected from the Moon during the Apollo missions, which cluster suspiciously close together in time rather than declining smoothly from the era of planet formation. The reality, timing and even the existence of a distinct spike remain debated among planetary scientists, with some proposing instead a more gradual decline that only appears spike-like because of sampling bias in the lunar samples available.
Facts
Concept Domain Formulated Year Proposed ByFouad Tera, Dimitri A. Papanastassiou, and Gerald J. Wasserburg, in their 1974 paper on isotopic evidence for a terminal lunar cataclysm. 1 Connections
Sources
1. Wikipedia (space and spaceflight articles)
Wikimedia FoundationWikipedia, Late Heavy Bombardment, Evidence for a cataclysm sectionQuote, Wikipedia, Late Heavy Bombardment, Evidence for a cataclysm section
They named it the 'lunar cataclysm' and proposed that it represented a dramatic increase in the rate of bombardment of the Moon around 3.9 Ga.
View the Source Late Heavy Bombardment (Wikipedia)
Wikipedia, Late Heavy Bombardment, lead section
The Late Heavy Bombardment (LHB), or lunar cataclysm, is a hypothesized astronomical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, at a time corresponding to the Neohadean and Eoarchean eras on Earth.
In Group: Origin and Evolution of the Solar System, Lead sentence
The Late Heavy Bombardment (LHB), or lunar cataclysm, is a hypothesized astronomical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, at a time corresponding to the Neohadean and Eoarchean eras on Earth.
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