Sometimes, the best place to hide a secret is in broad daylight. Just ask the sun.

A new paper in Physical Review Letters details the discovery of the highest-energy light ever observed from the sun. The international team behind the discovery also found that this type of light, known as gamma rays, is surprisingly bright. That is, there’s more of it than scientists had previously anticipated.

Watching like a HAWCA figure that looks like a heat map shows a bright yellow spot at its center, ringed by “cooler” oranges and purples. This represents the excess of gamma rays observed by the HAWC Collaboration.What an excess of solar gamma rays looks like to the High-Altitude Water Cherenkov Observatory Collaboration, which includes researchers from the University of Maryland. Credit: Courtesy of the HAWC Collaboration

Although the high-energy light doesn’t reach the Earth’s surface (and thus is no threat to life), these gamma rays create cascades of particles that move at near the speed of light through the atmosphere. They were detected by an international group of scientists, including University of Maryland astrophysicists, using the High-Altitude Water Cherenkov Observatory, or HAWC.  

HAWC is an important part of the story. Unlike other observatories, it works around the clock observing more than 2/3 of the entire sky every day.

“HAWC has made numerous discoveries about very high energy gamma rays from exotic objects like supernova remnants, microquasars, and active galaxies, but this discovery comes from much closer to home – our own Sun,” says Jordan Goodman, UMD Distinguished University Professor and Principal Investigator for the HAWC project, which is funded by the National Science Foundation, the National Council of Humanities Science and Technology (CONACyT) of México, the U.S. Department of Energy, Los Alamos National Lab and the Max Planck Institute for Nuclear Physics in Heidelberg, 

“We now have observational techniques that weren’t possible a few years ago,” said Mehr Un Nisa, a postdoctoral research associate at Michigan State University and corresponding author of the new paper. 

“In this particular energy regime, other ground-based telescopes couldn’t look at the sun because they only work at night,” she said. “Ours operates 24/7.”

In addition to working differently from conventional telescopes, HAWC looks a lot different from the typical telescope.

Rather than a tube outfitted with glass lenses, HAWC uses a network of 300 large water tanks, each filled with about 200 metric tons of water. The network is nestled between two dormant volcano peaks in Mexico, more than 13,000 feet above sea level.

From this vantage point, it can observe the aftermath of gamma rays striking air in the atmosphere. Such collisions create what are called air showers, which are a bit like particle explosions that are imperceptible to the naked eye.

The energy of the original gamma ray is liberated and redistributed amongst new fragments consisting of lower energy particles and light. It’s these particles — and the new particles they create on their way down — that HAWC can “see.”

When the shower particles interact with water in HAWC’s tanks, they create what’s known as Cherenkov radiation that can be detected with the observatory’s instruments.

Nisa and her colleagues began collecting data in 2015. In 2021, the team had accrued enough data to start examining the sun’s gamma rays with sufficient scrutiny. The gamma rays lose energy in Earth’s atmosphere, meaning they don’t present a concern to life.

“After looking at six years’ worth of data, out popped this excess of gamma rays,” Nisa said. “When we first saw it, we were like, ‘We definitely messed this up. The sun cannot be this bright at these energies.’”

Making history

The sun gives off a lot of light spanning a range of energies, but some energies are more abundant than others.

For example, through its nuclear reactions, the sun provides a ton of visible light — that is, the light we see. This form of light carries an energy of about 1 electron volt, which is a handy unit of measure in physics.

The gamma rays that HAWC observed had about 1 trillion electron volts, or 1 tera electron volt, abbreviated 1 TeV. Not only was this energy level surprising, but so was the fact that they were seeing so much of it.

In the 1990s, scientists predicted that the sun could produce gamma rays when high-energy cosmic rays — particles accelerated by a cosmic powerhouse like a black hole or supernova — smash into protons in the sun. But, based on what was known about cosmic rays and the sun, the researchers also hypothesized it would be rare to see these gamma rays reach Earth.

At the time, though, there wasn’t an instrument capable of detecting such high-energy gamma rays and there wouldn’t be for a while. The first observation of gamma rays with energies of more than a billion electron volts came from NASA’s Fermi Gamma-ray Space Telescope in 2011.

Over the next several years, the Fermi mission showed that not only could these rays be very energetic, but also that there were about seven times more of them than scientists had originally expected. And it looked like there were gamma rays left to discover at even higher energies.

When a telescope launches into space, there’s a limit to how big and powerful its detectors can be. The Fermi telescope’s measurements of the sun’s gamma rays maxed out around 200 billion electron volts.

Theorists led by John Beacom and Annika Peter, both professors at Ohio State University, encouraged the HAWC Collaboration to take a look.

“They nudged us and said, ‘We’re not seeing a cutoff. You might be able to see something,” said Nisa.

The HAWC Collaboration includes more than 30 institutions across North America, Europe and Asia, and a sizeable portion of that is represented in the nearly 100 authors on the new paper. The University of Maryland team consists of Goodman, Research Scientist Andrew Smith, Project Engineer Michael Schneider and graduate students Kristi Engle, Elijah Wilox, Jason Fan, and Sohyoun Yun-Cárcamo.   

Now, for the first time, the team has shown that the energies of the sun’s rays extend into the TeV range, up to nearly 10 TeV, which does appear to be the maximum, Nisa said.

“This shows that HAWC is adding to our knowledge of our galaxy at the highest energies, and it’s opening up questions about our very own sun,” Nisa said. “It’s making us see things in a different light. Literally.”

 Original story courtesy of Michigan State University: