Revealing the secret life of Lithium in Sun-like stars

Our study shows that all low-mass, Sun-like stars don't just destroy lithium, but they also create it, later in their lives. This implies the Sun itself will manufacture lithium in the future, which is not predicted by models, indicating that there is some physical process missing in stellar theory.

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Lithium is becoming common in our everyday lives. It is the key ingredient in the batteries of our mobile phones and electric vehicles, but have you ever wondered where it comes from? 

A fragile element: Lithium is a special element -- it was the only metal produced in the Big Bang that created the universe 13.7 billion years ago. While other elements have been produced in copious amounts by stars since then, the amount of lithium has increased relatively little. The source of even this small amount of lithium is still a matter of scientific debate. About half is thought to come from high-energy cosmic rays hitting heavier elements like carbon and oxygen in interstellar space and breaking them up into lighter atoms.

Sketch of a lithium atom. Containing three protons in its nucleus, lithium is the third element in the periodic table. It was one of only three elements that formed in the Big Bang, along with hydrogen and helium. Wikipedia.

Astronomers regard lithium as fragile, easily destroyed in the hot interiors of stars. Observations of lithium on the surface of stars have confirmed that it is gradually destroyed as stars get older.

 The enigmatic lithium-rich giant stars: There is one group of stars that is a notable exception to this rule of lithium destruction: the so-called "lithium-rich giants". These stars, first discovered about 40 years ago, contain up to 1,000 times as much lithium as other giant stars. Although not very common - only 1% of giant stars are very lithium-rich - just how they create their lithium remains a mystery till this day.

One of the main problems astronomers has faced in identifying a way these stars could produce so much lithium was our lack of knowledge about exactly what type of red giant stars they were. All Sun-like stars eventually become red giant stars when they have burned through all the hydrogen in their cores, becoming brighter and redder in colour. They expand their size by hundreds of times, often engulfing the planets orbiting them (don't worry - the Sun won't do this for another 5 billion years).

When stars become giants they progress through three different giant phases (which all look quite similar in colour and brightness), so it is crucial to understand what phase lithium-rich stars are in when they produce lithium.

Of the many theories, one has now come to the fore. About ten years ago our group recognised that the lithium-rich giants were likely in the second giant phase (also known as the red clump stage). These giants burn helium in their cores for about 100 million years. This theory was later confirmed by studying the oscillations of these stars to determine their exact point in their life cycles. We now know for sure that the vast majority of very lithium-rich giants are red clump stars.

This Hubble Space Telescope image shows stars at various stages of their lives, from young blue-hot stars to cooler red giants. Our study focused on the lithium content of red giant stars. NASA, ESA, and T. Brown (STScI)

Investigating the red clump giants: In our new study, we combined large stellar surveys to investigate the lithium-rich giants. We used an Australian survey called Galah, a Chinese survey called LAMOST, and a European space telescope survey called Gaia. Our 200,000-strong sample of Sun-like stars (with mass and metallicity similar to the Sun) confirmed that lithium-rich stars are in the red clump phase. We also detected the expected destruction of lithium in the "red giant branch" phase, which comes just before the red clump.

Sun-like stars become lithium factories later in life: Something strange stood out - other stars in the red clump, although not extremely lithium-rich, contained much more lithium than stars in the late stage of the red giant branch. As the red clump phase comes directly after the red giant branch phase, we concluded the stars must be producing lithium when moving from one phase to the next. Importantly, it appeared that all of the red clump stars contained more lithium than those in the red giant branch phase. This implies the Sun itself will manufacture lithium in the future, as our study focused on Sun-like stars.

Image of the Sun taken by the SOHO space telescope. The Sun will also experience lithium production, as it evolves to the red clump phase in future. NASA/SOHO

In effect, by studying only the extremely lithium-rich stars, representing just 1% of giants, astronomers had been focusing on just the tip of the "lithium iceberg". It now appears all red clump stars have been enriched with lithium, and the extremely lithium-rich stars are only the tail end of the distribution. In our paper, we show that, on average, the stars increase their lithium content by a factor of 40. The amount of lithium produced in just one of these stars would be enough to make electric car batteries for 20,000 trillion cars.

Not predicted by theory: How this lithium enrichment comes about is unknown. It is not predicted by our best models of stars. Clearly there is some physical process missing in stellar theory. What we can say with our data is how often it occurs - it appears to happen to all Sun-like stars. We can also say when it occurs - sometime between the end of the red giant branch phase and the beginning of the red clump phase.

For our next study, we will attempt to constrain the timing of the lithium-production phase more precisely. This information will help stellar theorists, including those in our group, to determine what physical process is behind the lithium production.

Finally, since at least some of the newly created lithium will end up being blown off the star in stellar winds, it will also help us understand how much these stars enrich our galaxy with lithium, and, ultimately, planets like Earth.

Header image credit: NASA, ESA, and T. Brown (STScI).

Go to the profile of Yerra Bharat Kumar

Yerra Bharat Kumar

Postdoctoral Fellow, National Astronomical Observatories, Chinese Academy of Sciences

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