How the Radcliffe Wave moves through the backyard of our Sun
(yellow dot). Blue dots are clusters of baby stars. The white line is a
theoretical model by Ralf Konietzka and collaborators that explains the
current shape and motion of the Wave. The magenta and green lines at the
beginning show how and to what extent the Radcliffe Wave will move in
the future. Background is a cartoon model of the Milky Way. Credit: Ralf Konietzka, Alyssa Goodman & WorldWide Telescope
A few years ago, astronomers
at the Center for Astrophysics | Harvard & Smithsonian (CfA)
uncovered one of the Milky Way's greatest secrets: an enormous,
wave-shaped chain of gaseous clouds in our sun’s backyard, giving birth
to clusters of stars along the spiral arm of the galaxy we call home.
Naming this astonishing new structure the Radcliffe Wave, in honor of the Harvard Radcliffe Institute where the undulation was originally discovered, astronomers at CfA now report in Nature that the Radcliffe Wave not only looks like a wave, but also moves like one – oscillating through space much like "the wave" moving through a stadium full of fans.
"By using the motion of baby stars born in the gaseous clouds along the Radcliffe Wave," said Ralf Konietzka, the paper's lead author and a Ph.D. student at Harvard’s Kenneth C. Griffin Graduate School of Arts and Sciences and CfA, "we can trace the motion of their natal gas to show that the Radcliffe Wave is actually waving."
Naming this astonishing new structure the Radcliffe Wave, in honor of the Harvard Radcliffe Institute where the undulation was originally discovered, astronomers at CfA now report in Nature that the Radcliffe Wave not only looks like a wave, but also moves like one – oscillating through space much like "the wave" moving through a stadium full of fans.
"By using the motion of baby stars born in the gaseous clouds along the Radcliffe Wave," said Ralf Konietzka, the paper's lead author and a Ph.D. student at Harvard’s Kenneth C. Griffin Graduate School of Arts and Sciences and CfA, "we can trace the motion of their natal gas to show that the Radcliffe Wave is actually waving."
How the Radcliffe Wave moves through the backyard of our Sun (yellow dot). Blue dots are clusters of baby stars. The white line is a theoretical model by Ralf Konietzka and collaborators that explains the current shape and motion of the Wave. The magenta and green lines at the beginning show how and to what extent the Radcliffe Wave will move in the future. Background is a cartoon model of the Milky Way. Credit: Ralf Konietzka, Alyssa Goodman & WorldWide Telescope
In 2018 when University of Vienna professor João Alves was a fellow at Harvard Radcliffe Institute, he worked with Catherine Zucker – then a Ph.D. student at Harvard and now a Smithsonian Astrophysical Observatory (SAO) astrophysicist at CfA – and Alyssa Goodman,
Robert Wheeler Willson Professor of Applied Astronomy at CfA, to map
out the 3D positions of the stellar nurseries in the sun’s galactic
neighborhood. By combining brand-new data from the European Space
Agency's Gaia mission with the data-intensive "3D Dust Mapping"
technique – pioneered by Doug Finkbeiner, a Harvard professor at CfA and
his team – they noticed a pattern emerging, leading to the discovery of the Radcliffe Wave in 2020.
"It's the largest coherent structure that we know of, and it's really, really close to us," said Zucker. "It's been there the whole time. We just didn’t know about it, because we couldn’t build these high-resolution models of the distribution of gaseous clouds near the sun, in 3D."
The 2020 3D dust map, which was developed at the CfA, clearly showed that the Radcliffe Wave existed, but no measurements available then were good enough to see if the wave was moving. But in 2022, using a newer release of Gaia data, Alves' group assigned 3D motions to the young star clusters in the Radcliffe Wave. With the clusters' positions and motions in hand, Konietzka's team then determined that the entire Radcliffe Wave is indeed waving.
The star clusters along the Radcliffe Wave move up and down, like people in a sports stadium doing "the wave," creating a pattern that travels through our galactic backyard.
"Similar to how fans in a stadium are being pulled back to their seats by the Earth's gravity," said Konietzka, “the Radcliffe Wave oscillates due to the gravity of the Milky Way."
Understanding the behavior of this 9,000-light-year-long, gargantuan structure in our galactic backyard, just 500 light-years away from the sun at its closest point, allows researchers to now turn their attention to even more challenging questions. No one yet knows what caused the Radcliffe Wave or why it moves the way it does.
"Now we can go and test all these different theories for why the wave formed in the first place," Zucker said.
"Those theories range from explosions of massive stars, called supernovae, to out-of-galaxy disturbances, like a dwarf satellite galaxy colliding with our Milky Way," Konietzka added.
The Nature article also includes a calculation on how much dark matter might be contributing to the gravity responsible for the Wave's motion.
"It turns out that no significant dark matter is needed to explain the motion we observe," Konietzka said. “The gravity of ordinary matter alone is enough to drive the waving of the Wave."
In addition, the discovery of the oscillation raises new questions about the preponderance of these waves both across the Milky Way and other galaxies. Since the Radcliffe Wave appears to form the backbone of the nearest spiral arm in the Milky Way, the waving of the Wave could imply that spiral arms of galaxies oscillate in general, making galaxies even more dynamic than previously thought.
"The question is, what caused the displacement giving rise to the waving we see?," Goodman said. “And does it happen all over the galaxy? In all galaxies? Does it happen occasionally? Does it happen all the time?"
The authors of the Nature paper are Ralf Konietzka, Alyssa A. Goodman and Catherine Zucker, all from CfA, Andreas Burkert (Max Planck Institute for Extraterrestrial Physics in Garching, Germany), João Alves (University of Vienna), Michael Foley (Harvard graduate student at CfA), and Cameren Swiggum, Maria Koller, Núria Miret-Roig, all from the University of Vienna.
The National Science Foundation, NASA, ESA, and the European Research Council (ERC) Advanced Grant ISM-FLOW supported this work.
"It's the largest coherent structure that we know of, and it's really, really close to us," said Zucker. "It's been there the whole time. We just didn’t know about it, because we couldn’t build these high-resolution models of the distribution of gaseous clouds near the sun, in 3D."
The 2020 3D dust map, which was developed at the CfA, clearly showed that the Radcliffe Wave existed, but no measurements available then were good enough to see if the wave was moving. But in 2022, using a newer release of Gaia data, Alves' group assigned 3D motions to the young star clusters in the Radcliffe Wave. With the clusters' positions and motions in hand, Konietzka's team then determined that the entire Radcliffe Wave is indeed waving.
The star clusters along the Radcliffe Wave move up and down, like people in a sports stadium doing "the wave," creating a pattern that travels through our galactic backyard.
"Similar to how fans in a stadium are being pulled back to their seats by the Earth's gravity," said Konietzka, “the Radcliffe Wave oscillates due to the gravity of the Milky Way."
Understanding the behavior of this 9,000-light-year-long, gargantuan structure in our galactic backyard, just 500 light-years away from the sun at its closest point, allows researchers to now turn their attention to even more challenging questions. No one yet knows what caused the Radcliffe Wave or why it moves the way it does.
"Now we can go and test all these different theories for why the wave formed in the first place," Zucker said.
"Those theories range from explosions of massive stars, called supernovae, to out-of-galaxy disturbances, like a dwarf satellite galaxy colliding with our Milky Way," Konietzka added.
The Nature article also includes a calculation on how much dark matter might be contributing to the gravity responsible for the Wave's motion.
"It turns out that no significant dark matter is needed to explain the motion we observe," Konietzka said. “The gravity of ordinary matter alone is enough to drive the waving of the Wave."
In addition, the discovery of the oscillation raises new questions about the preponderance of these waves both across the Milky Way and other galaxies. Since the Radcliffe Wave appears to form the backbone of the nearest spiral arm in the Milky Way, the waving of the Wave could imply that spiral arms of galaxies oscillate in general, making galaxies even more dynamic than previously thought.
"The question is, what caused the displacement giving rise to the waving we see?," Goodman said. “And does it happen all over the galaxy? In all galaxies? Does it happen occasionally? Does it happen all the time?"
The authors of the Nature paper are Ralf Konietzka, Alyssa A. Goodman and Catherine Zucker, all from CfA, Andreas Burkert (Max Planck Institute for Extraterrestrial Physics in Garching, Germany), João Alves (University of Vienna), Michael Foley (Harvard graduate student at CfA), and Cameren Swiggum, Maria Koller, Núria Miret-Roig, all from the University of Vienna.
The National Science Foundation, NASA, ESA, and the European Research Council (ERC) Advanced Grant ISM-FLOW supported this work.
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