Saturday, November 27, 2021

Late Heavy Bombardment of the Moon Revealed

The Moon’s surface is covered by numerous craters that date back to the impacts of asteroids. Age determinations on lunar rocks formed during these impacts show a surprising clustering at ages of about 3.9 billion years before present, or about 500 million years after the Moon was formed. These observations have led to the theory of a Late Heavy Bombardment of the Moon (or LHB).

Apollo sample 60335 with visible metal globules: These metal globules come from asteroids that have hit the Moon.
Apollo sample 60335 with visible metal globules: These metal globules come from asteroids that have hit the Moon. (Image: via AG Kleine)

But what was the origin of this late bombardment and where did the asteroids that hit the Moon come from? Scientists discuss two possibilities. One is that these bodies could represent the leftover material from the main phase of Earth’s formation that hit the Moon with continuously decreasing frequency. Another hypothesis is that about 3.9 billion years ago, instabilities in the orbits of the gas giant planets led to a sudden sharp increase in impacts from asteroids and comets from the outer solar system.

It is known from theoretical calculations that the orbits of the gas giants changed at some point in the early history of the solar system, scattering a large number of bodies from the outer solar system inwards, which collided with the Earth and the Moon, among others. (Image: via NASA)

Planetologists at the University of Münster have tested these hypotheses with very precise isotope measurements of lunar rocks formed during the bombardment 3.9 billion years ago. Their result and conclusion: There was no sudden increase in the impact rate, and the bombardment of the Moon goes back to continuous impacts of asteroids left over from the main phase of the Earth’s formation. The results are published in the current issue of the journal Science Advances.

About the Moon study

The scientists from Münster examined lunar rocks that were formed during the bombardment 3.9 billion years ago. These rocks contain tiny metal globules consisting of material from the impactor asteroids. By studying the isotopic composition of these metal globules, researchers can determine where in the solar system these bodies originated. They focused on the elements ruthenium and molybdenum because these elements show systematic changes in their isotopic composition depending on where they were formed in the solar system. Dr. Emily Worsham, planetologist and lead author of the study said:

“Our research shows that the bombardment of the Moon was by the same bodies that formed the Earth and Moon.”

The impact craters on the Moon, therefore, are due to a continuous bombardment of leftover asteroids from the main phase of the Earth’s formation. This also allows scientists to rule out a sudden increase in the impact rate due to bombardment with bodies from the outer solar system. But then where did the clustering of ages of 3.9 billion years come from? Worsham explained:

“It has previously been suggested that the lunar rocks studied so far are mostly made up of material from a single impact basin – the Mare Imbrium in the north-central Earth-facing side of the Moon.”

It is known from theoretical calculations that the orbits of the gas giants changed at some point in the early history of the solar system, scattering a large number of bodies from the outer solar system inwards, which collided with the Earth and the Moon, among others, Prof. Dr. Thorsten Kleine said:

“This event must have taken place earlier than previously thought, because we find no evidence of impacts by asteroids or comets from the outer reaches of the solar system in the lunar rocks.”

The change in the orbits of the gas giant planets therefore probably took place during the main formation phase of the Earth-like planets – that is, in the first roughly 100 million years of the solar system – which in turn agrees well with recent dynamical models, Kleine added:

“Our study, therefore, also shows that the Earth-like planets incorporated water-rich bodies from the outer solar system relatively early, during their formation, thus creating the conditions for the emergence of life.”

Provided by: Westfälische Wilhelms-Universität Münster [Note: Materials may be edited for content and length.]

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Troy Oakes
Troy was born and raised in Australia and has always wanted to know why and how things work, which led him to his love for science. He is a professional photographer and enjoys taking pictures of Australia's beautiful landscapes. He is also a professional storm chaser where he currently lives in Hervey Bay, Australia.
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