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The Milky Way’s shape — a peculiar disk

Popular media is abuzz today with news regarding research by NAOC (National Astronomical Observatories of Chinese Academy of Sciences) on the shape of our galaxy, the Milky Way, published in Nature Astronomy today. A peculiar disk. A new 3D model.

Original article on Nature Astronomy: “An intuitive 3D map of the Galactic warp’s precession traced by classical Cepheids” (February 4, 2019).

Here’re two examples about that article: ABC Science News and Phys.org. The Phys.org article contains visualizations.

Milky Way is ‘S-shaped’, 3D map reveals, in a new way of looking at our celestial home

Key points:

  • We have long thought the Milky Way was warped, but it is also twisted, according to a new study of pulsating stars.
  • The new map is the most accurate representation of the Milky Way so far, say astronomers.
  • The Gaia telescope will give us a much better picture in the future.

The map provides an “unprecedented view of the Milky Way”, said study co-author Richard de Grijs of Macquarie University.

To create the map, Professor de Grijs and colleagues from the Chinese Academy of Sciences focused on 1,339 pulsating beacons known as Cepheid stars.

To cut through the dust, Professor de Grijs and colleagues based their calculations on observations of Cepheid stars made using the Wide-Field Infrared Survey Explorer, which detects longer wavelengths than visible light.

Joss Bland-Hawthorn of the University of Sydney agreed the new study was a first step, which will be followed up in more detail by observatories such as the Gaia space telescope.

“This is probably the cleanest demonstration of the warp in stars and it looks different from the warp in gas,” said Professor Bland-Hawthorn, who was also not involved in the new study.

But we don’t really know what causes these warps, he added.

The Milky Way is warped

The Milky Way galaxy’s disk of stars is anything but stable and flat. Instead, it becomes increasingly warped and twisted far away from the Milky Way’s center, according to astronomers from National Astronomical Observatories of Chinese Academy of Sciences (NAOC).

“Somewhat to our surprise, we found that in 3-D, our collection of 1339 Cepheid stars and the Milky Way’s gas disk follow each other closely. This offers new insights into the formation of our home galaxy,” says Prof. Richard de Grijs from Macquarie University in Sydney, Australia, and senior co-author of the paper. “Perhaps more importantly, in the Milky Way’s outer regions, we found that the S-like stellar disk is warped in a progressively twisted spiral pattern.”

“This new morphology provides a crucial updated map for studies of our galaxy’s stellar motions and the origins of the Milky Way’s disk,” says Dr. DENG Licai, senior researcher at NAOC and co-author of the paper.

We’ve come a long way from “perfect” celestial spheres, eh.


5 thoughts on “The Milky Way’s shape — a peculiar disk

  1. Milky Way Collided with Dark-Matter Dominated Galaxy Less Than Billion Years Ago (June 18, 2019)

    According to new research led by Rochester Institute of Technology (RIT), the collision of the recently-discovered dwarf galaxy Antlia 2 with our Milky Way Galaxy hundreds of millions of years ago is responsible for ripples in the Milky Way’s outer gas disk.

    Dr. Chakrabarti and her colleagues also explored other potential causes for the ripples in the Milky Way’s outer disk, but ruled out the other candidates.

    The team’s paper will be published in the Astrophysical Journal Letters.

  2. This Space.com article “This 3D Map of the Milky Way Is the Best View Yet of Our Galaxy’s Warped, Twisted Shape” (August 1, 2019) by Charles Q. Choi discusses recent research on the Milky Way’s shape using Cepheid variable stars.

    These new findings shed light on the warped, twisted shape of the galaxy’s disk, researchers added.

    Using the Optical Gravitational Lensing Experiment, which monitors the brightness of nearly 2 billion stars, the scientists charted the distance between the sun and more than 2,400 Cepheids throughout the Milky Way. “This took six years but it was worth it,” study lead author Dorota Skowron, an astrophysicist at the University of Warsaw in Poland, told Space.com.

    Better 3D maps of the Milky Way can help scientists better understand its shape. For instance, “the number of the main spiral arms is still debated; also, the severity of the spiraling of the arms,” Skowron said.

  3. Lots of media coverage recently about research on “bubbles” of gamma and X-ray emissions about 25 thousand light-years distant above and below the Milky Way’s galactic center – Fermi bubbles. This Space.com artcle by Paul Sutter on September 4, 2019 is an example: “Something Strange Is Happening in the Fermi Bubbles.”

    [One possibility is that] millions of years ago, Sag A* (the more common name for our giant black hole, because who wants to keep typing or saying “Sagittarius” all the time?) ate a giant meal and got a bad case of indigestion, with the infalling material heating up, twisting around in a complicated dance of electric and magnetic forces, and managing to escape the clutches of the event horizon before falling in. That material, energized beyond belief, raced away from the center of the galaxy, riding on jets of particles accelerated to nearly the speed of light. As they fled to safety, these particles spread and thinned out, but maintained their energetic state to the present day.

  4. There’s a well done animation is this article about galactic evolution.

    ESA > “Galactic crash may have triggered Solar System formation” (May 25, 2020).

    Astronomers have known that Sagittarius [a galaxy discovered in the 1990s to be orbiting the Milky Way] repeatedly smashes through the Milky Way’s disc, as its orbit around the galaxy’s core tightens as a result of gravitational forces. Previous studies suggested that Sagittarius, a so called dwarf galaxy, had had a profound effect on how stars move in the Milky Way. Some even claim that the 10,000 times more massive Milky Way’s trademark spiral structure might be a result of the at least three known crashes with Sagittarius over the past six billion years.

    A new study, based on data gathered by ESA’s galaxy mapping powerhouse Gaia, revealed for the first time that the influence of Sagittarius on the Milky Way may be even more substantial. The ripples caused by the collisions seem to have triggered major star formation episodes, one of which roughly coincided with the time of the formation of the Sun some 4.7 billion years ago.

  5. Beyond visible light, the ultraviolet eyes of NASA’s Hubble Space Telescope continue to provide insights into the history of our very own Milky Way.

    Space.com > “Ancient explosion in Milky Way’s core lit up gas outside the galaxy” by Elizabeth Howell (June 4, 2020).

    Embedded in the center of our galaxy, the Milky Way, a supermassive black hole known as Sagittarius A* (Sgr A*) had unleashed a massive amount of energy. New research shows that the energy was so pervasive that it illuminated gas associated with two satellite galaxies of our own: the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC).

    This shows us that different regions of the galaxy are linked — what happens in the galactic center makes a difference to what happens out in the Magellanic Stream,” Fox added [1], referring to the massive, ribbon-like gas structure that trails the Magellanic Clouds. “We’re learning about how the black hole impacts the galaxy and its environment.”

    [1] Andrew Fox, the principal investigator of the study and an astronomer at the Space Telescope Science Institute (STScI) in Baltimore.

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