University of Manchester’s Joshua Snape, Katherine Joy and Romain Tartese dig into what we’ve learned from the Chang’e-5 moon samples and how it could enhance our understanding of the solar system.
Lava was still flowing on the surface of the moon 1.97bn years ago – and now we have the rocks to prove it. This is the result of new work from an international collaboration of planetary scientists, of which we’re a part, published in the journal Science.
Together with researchers from China, Australia, Sweden and the US, we’ve been studying samples collected from the moon by the China National Space Administration during the Chang’e-5 mission.
Chang’e-5 was an uncrewed mission including a robotic lander, which landed on the near side of the moon (the Earth-facing side) in December 2020. The mission returned 1.7kg of lunar rocks to Earth — the first samples collected from the moon since 1976 with the Soviet Union’s Luna 24 mission.
A goal of the Chang’e-5 mission was to find evidence of some of the youngest volcanic eruptions on the Moon. Although scientists have previously been able to predict volcanic rocks of this age on the moon by studying the number of impact craters on the lunar surface, it is impossible to confirm this without having samples to examine.
Analysis of the samples took place using the sensitive high-resolution ion microprobe (Shrimp) instrument at the Shrimp centre in Beijing, China.
First, the material was sorted. Our colleagues in China manually picked out several tiny fragments of basalt (a volcanic rock), roughly 2mm in size, for investigation. This was followed by laboratory analyses, building on techniques developed in the 1970s for the analysis of the first Apollo samples. The process of determining the age of the rocks was complex but, in essence, we used a focused beam of charged particles to eject material from various mineral phases in the rocks and analysed the ejected material.
Our efforts were rewarded when we were able to determine an eruption age for these lavas of 1.97bn years, a whole billion years younger than any previously dated basaltic lava from the Moon.
A new scientific mystery
Many volcanic eruptions occurred on the moon’s surface over its geological history, forming large sheets of basaltic rock, referred to as the lunar mare. These can be seen as dark patches looking up at the moon.
But most of the volcanic activity occurred between 3bn and 4bn years ago. Planetary scientists have confirmed this by dating basalts from the Apollo and Luna rock collections, as well as meteorites that originated from the moon. Until now though, younger volcanic rocks predicted by crater-counting studies had remained elusive.
In order for volcanic eruptions to occur, heat is required on the inside of a planet to generate the molten material involved in the process. For a planet the size of the moon, it is thought that this heat would have been lost long before these eruptions 2bn years ago.
This work has therefore opened up a new scientific mystery of how a small rocky planetary body like the moon could have retained enough interior heat to continue producing volcanic eruptions 2.5bn years after it first formed 4.5bn years ago.
So what’s going on? While scientists have previously suggested that high concentrations of radioactive elements in the lunar interior could have melted rocky material inside the moon, the compositions of these samples indicate this was not the driving force in this case.
It remains to be seen whether so-called tidal heating could have played a role, where heat was generated in the moon’s interior by the stretching and squeezing (think of an elastic band warming up through friction as you stretch it) due to gravity between the moon, Earth and sun.
Alternatively, it may be that a unique aspect of the moon’s mantle composition could have resulted in a lower melting temperature, therefore explaining how the molten material was formed. Work is now continuing on the samples to try to shed light on this question.
Analysing samples from the Apollo missions in the early 1970s revolutionised our understanding of how dynamic our solar system is, and how planets form and evolve. Now, once more, this new study proves the incredible scientific value of returning samples from other planetary bodies to decode their secrets in laboratories on Earth.
Importantly, validating the crater-counting approach with lunar samples also has key implications for dating the surfaces of other planets from which we haven’t yet collected samples (such as Mars, Venus and Mercury). It will enhance our understanding of the solar system more broadly.
Joshua Snape is a research fellow at the University of Manchester, studying how the moon and other planetary bodies evolved. Katherine Joy is a professor and research fellow at the university, studying the geological history of the moon, and Romain Tartese is a senior research fellow focused on the history of planetary bodies in the solar system.