A new study published online Wednesday, May 3, in the journal Nature documents the first observation of an aging star swallowing a planet. After running out of fuel in its core, the star began to grow in size, shrinking the gap with its neighboring planet, eventually consuming it entirely. In about 5 billion years, our Sun will go through a similar aging process, possibly reaching 100 times its current diameter and becoming what’s known as a red giant. During that growth spurt, it will absorb Mercury, Venus, and possibly Earth.
Astronomers have identified many red giant stars and suspected that in some cases they consume nearby planets, but the phenomenon had never been directly observed before. “This type of event has been predicted for decades, but until now we have never actually observed how this process plays out,” said Kishalay De, an astronomer at the Massachusetts Institute of Technology in Cambridge and the study’s lead author.
Researchers discovered the event – formally called ZTF SLRN-2020 – using multiple ground-based observatories and NASA’s NEOWISE (Near-Earth Object Wide Field Infrared Survey Explorer) spacecraft, which is managed by the agency’s Jet Propulsion Laboratory. The planet was likely about the size of Jupiter, with an orbit even closer to its star than Mercury’s is to our Sun. The star is at the beginning of the final phase of its life – its red giant phase, which can last more than 100,000 years.
As the star expanded, its outer atmosphere eventually surrounded the planet. Drag from the atmosphere slowed the planet down, shrinking its orbit and eventually sending it below the star’s visible surface, like a meteor burning up in Earth’s atmosphere. The transfer of energy caused the star to temporarily increase in size and become a few hundred times brighter. Recent observations show the star has returned to the size and brightness it was before merging with the planet.
So he turned to the NEOWISE observatory, which scans the entire sky in infrared light (a range of wavelengths longer than visible light) every six months. Launched in 2009 and originally called WISE, the observatory produces all-sky maps that enable astronomers to see how objects change over time.
Looking at the NEOWISE data, De saw that the star brightened almost a year before ZTF spotted the flash. That brightening was evidence of dust (which emits infrared light) forming around the star. De and his colleagues think the dust indicates that the planet didn’t go down without a fight and that it pulled hot gas away from the puffy star’s surface as it spiraled toward its doom. As the gas drifted out into space, it would have cooled and become dust – like water vapor becoming snow. Even more gas was then flung into space during the collision of the star and the planet, producing more dust visible to both the ground-based infrared observatories and NEOWISE.
“Very few things in the universe brighten in infrared light and then brighten in optical light at different times,” said De. “So the fact that NEOWISE saw the star brighten a year before the optical eruption was critical to figuring out what this event was.”
Five billion years from now, when our Sun is expected to become a red giant, swallowing up Mercury, Venus, and possibly Earth, the light show should be much more subdued, according to De, since those planets are many times smaller than the Jupiter-size planet in the ZTF-captured event.
“If I were an observer looking at the solar system 5 billion years from now, I might see the Sun brighten a little, but nothing as dramatic as this, even though it will be the exact same physics at work,” he said.
Most mid-size stars will eventually become red giants, and theorists think that a handful of them consume nearby planets each year in our galaxy. The new observations provide astronomers with a template for what those events should look like, opening up the possibility of finding more.
“This discovery shows that it’s worthwhile to take observations of the entire sky and archive them, because we don’t yet know all of the interesting events we might be capturing,” said Joe Masiero, deputy principal investigator for NEOWISE at IPAC at Caltech. “With the NEOWISE archive, we can look back in time. We can find hidden treasures or learn something about an object that no other observatory can tell us.”
More About the Mission
Launched in 2009, the WISE mission scanned the entire sky twice in infrared light, snapping pictures of three-quarters of a billion objects, including remote galaxies, stars, and asteroids. The WISE mission concluded in 2011, but two years later NASA repurposed the spacecraft to track asteroids and other near-Earth objects, or NEOs. Both the mission and the spacecraft were renamed NEOWISE.
JPL managed and operated WISE for NASA’s Astrophysics Division within the Science Mission Directorate. Edward Wright at UCLA was the principal investigator. The mission was selected competitively under NASA’s Explorers Program managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland.
JPL manages and operates the NEOWISE mission for NASA’s Planetary Defense Coordination Office within the Science Mission Directorate in Washington. The principal investigator, Amy Mainzer, is at the University of Arizona. The Space Dynamics Laboratory in Logan, Utah, built the science instrument. Ball Aerospace & Technologies Corp. of Boulder, Colorado, built the spacecraft. Science data processing takes place at IPAC at Caltech in Pasadena. Caltech manages JPL for NASA.
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