Scientists have trained an artificial intelligence (AI) to help understand the evolution of young stars and their planets – a new benchmark in the use of AI in astronomy.
Isabelle Dubach
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Young stars – just like young humans – are prone to temper flares. But star flares can incinerate everything around them, including the atmospheres of nearby planets starting to form.
Finding out how often young stars erupt can help scientists understand where to look for habitable planets. But until now, searching for these flares involved poring over thousands of measurements of star brightness variations, called ‘light curves’, by eye.
Now, an international team of scientists including UNSW Sydney’s Dr have used machine learning to make the search faster and more effective.
The scientists taught a neural network – a type of artificial intelligence – to detect the telltale light patterns of a stellar flare.
“With the help of the neural network, we were able to find more than 23,000 flares across thousands of young stars,” said Dr Montet, Scientia Lecturer at and co-author of the study.
“Finding stellar flares – which can be lethal for the developing atmospheres of nearby planets – can help us work out where to look for habitable planets.”
The findings, published over the weekend in the and the , offer a new benchmark in the use of AI in astronomy, as well as a better understanding of the evolution of young stars and their planets.
“When we say young, we mean only a million to 800 million years old,” said Ms Adina Feinstein, a University of Chicago graduate student and first author on the paper.
“Any planets near a star are still forming at this point. This is a particularly fragile time, and a flare from a star can easily evaporate any water or atmosphere that’s been collected.”
A protective planetary blanket: Earth's atmosphere helps regulate the planet's temperature, absorbs harmful solar rays, and contains life-sustaining ingredients like oxygen and carbon dioxide. Photo: Unsplash.
NASA’s TESS telescope, aboard a satellite that has been orbiting Earth since 2018, is specifically designed to search for exoplanets. Flares from faraway stars show up on TESS’s images, but traditional algorithms have a hard time picking out the shape from the background noise of star activity.
But neural networks are particularly good at looking for patterns – like Google’s AI picking cats out of internet images – and to look to them to classify astronomical data.
Ms Feinstein and Dr Montet worked with a team of scientists from NASA, the Flatiron Institute, Fermi National Accelerator Laboratory, the Massachusetts Institute of Technology and the University of Texas at Austin to pull together a set of identified flares and not-flares to train the neural net.
“The neural net turned out to be really good at finding small flares,” said Dr Montet, who was the principal investigator on the study.
“Those are actually really hard to find with other methods.”
Once the researchers were satisfied with the neural net’s performance, they applied it to the full set of data: more than 3200 stars.
They found that stars like our sun only have a few flares, and those flares seem to drop off after about 50 million years.
“This is good for fostering planetary atmospheres – a calmer stellar environment means the atmospheres have a better chance of surviving,” Ms Feinstein said.
In contrast, cooler stars called red dwarfs tended to flare much more frequently.
“Red dwarfs have been seen to host small rocky planets; if those planets are being bombarded when they’re young, this could prove detrimental for retaining any atmosphere,” she said.
The research team found over 23,000 flares across thousands of young stars with the help of the neural net. Image: Shutterstock.
The results help scientists understand the odds of habitable planets surviving around different types of stars, and how atmospheres form. This can help them pinpoint the most likely places to look for habitable planets elsewhere in the universe.
The scientists also investigated the connection between stellar flares and star spots, like the kind we see on our own sun’s surface.
“The spottiest our sun ever gets is maybe 0.3% of the surface,” said Dr Montet.
“For some of these stars we’re seeing, the surface is basically all spots. This reinforces the idea that spots and flares are connected, as magnetic events.”
The scientists next want to adapt the neural net to look for planets lurking around young stars.
“Currently we only know of about a dozen younger than 50 million years, but they’re so valuable for learning how planetary atmospheres evolve,” Ms Feinstein said.
Dr Montet will also be extending this neural net framework at UNSW.
“We will apply these same methods in a search for young planets in the same data set,” he said.
“This will hopefully lead to a 'rise of the machines' where we can apply machine learning algorithms to find a bunch of exciting new planets using the same methods.”