“Something’s Messing With the Milky Way” –ESA’s Gaia Spacecraft Reveals What & Why

Milky Way Galaxy Warped Shape

 

Something is warping our home galaxy. Astronomers suspect that Sagittarius, a dwarf galaxy orbiting the Milky Way might be causing the ripple, and may have burst through the Milky Way’s galactic disc several times in the distant past. Astronomers think that Sagittarius will be gradually absorbed by the Milky Way, a process which is already underway. The Gaia Spacecraft, with its unique survey of more than one billion stars in our galaxy, might hold the key to unraveling the mystery.

In a cosmological setting the disc of a galaxy continuously experiences gravitational torques and perturbations, which can cause the disc to wobble, flare and warp. The study of these warps and their dynamic nature can reveal key information on the formation history of galaxies and the mass distribution of their halos.

Our Milky Way presents a unique case study. With Gaia, for the first time, we have a large amount of data on a vast amount stars, the motion of which is measured so precisely that we can try to understand the large scale motions of the Milky Way and model its formation history, says ESA’s Gaia deputy project scientist Jos de Bruijne. “This is something unique. This really is the Gaia revolution.”

Gaia Confirms Ancient Hints

A team of scientists using data from the second Gaia data release has now confirmed previous hints that this warp is not static but changes its orientation over time, a phenomenon called precession and it could be compared to the wobble of a spinning top as its axis rotate Data from the ESA’s star-mapping satellite suggests the distortion might be caused by the ongoing collision with the smaller, galaxy, which sends ripples through the galactic disc like a rock thrown into water.

“Milky Way’s Hidden Past” –Gaia Unveils Dark-Matter Object 1-100 Million Times Mass of the Sun

Astronomers have known since the late 1950s that the Milky Way’s disc—where most of its hundreds of billions of stars reside—is not flat but somewhat curved upwards on one side and downwards on the other. For years, they debated what is causing this warp. They proposed various theories including the influence of the intergalactic magnetic field or the effects of a dark matter halo, a large amount of unseen matter that is expected to surround galaxies. If such a halo had an irregular shape, its gravitational force could bend the galactic disc.

The image above shows that the galactic disc of the Milky Way is not flat but warped upwards on one side and downwards on the other. Data from ESA’s galaxy-mapping spacecraft Gaia provides new insights into the behavior of the warp and its possible origins. The two smaller galaxies in the lower right corner are the Large and Small Magellanic Clouds, two satellite galaxies of the Milky Way. ( Stefan Payne-Wardenaar; Magellanic Clouds: Robert Gendler/ESO)

 

 

The speed at which the warp precesses is much faster than expected—faster than the intergalactic magnetic field or the dark matter halo would allow. That suggests the warp must be caused by something else. Something more powerful—like a collision with another galaxy.

“We measured the speed of the warp by comparing the data with our models. Based on the obtained velocity, the warp would complete one rotation around the center of the Milky Way in 600 to 700 million years,” says Eloisa Poggio of the Turin Astrophysical Observatory, Italy, who is the lead author of the study, published in Nature Astronomy. “That’s much faster than what we expected based on predictions from other models, such as those looking at the effects of the non-spherical halo.”

Mapping the Milky Way in 3D

The warp’s speed is, however, slower than the speed at which the stars themselves orbit the galactic center. The sun, for example, completes one rotation in about 220 million years.

Such insights were only possible thanks to the unprecedented ability of the Gaia mission to map our galaxy, the Milky Way, in 3-D, by accurately determining positions of more than one billion stars in the sky and estimating their distance from us. The flying saucer-like telescope also measures the velocities at which individual stars move in the sky, allowing astronomers to ‘play’ the movie of the Milky Way’s history back- and forward in time over millions of years.

Dark Matter Storm is Speeding Toward Our Sun–“A Remnant of a Dwarf Galaxy Swallowed by the Milky Way”

“It’s like having a car and trying to measure the velocity and direction of travel of this car over a very short period of time and then, based on those values, trying to model the past and future trajectory of the car,” says Ronald Drimmel, a research astronomer at the Turin Astrophysical Observatory and co-author of the paper. “If we make such measurements for many cars, we could model the flow of traffic. Similarly, by measuring the apparent motions of millions of stars across the sky we can model large scale processes such as the motion of the warp.”

As impressive as the warp and its precession appear on the galactic scale, the scientists reassure us that it has no noticeable effects on life on our planet.

Our Solar System at Outer Range

“The sun is at the distance of 26 000 light years from the galactic center where the amplitude of the warp is very small,” Eloisa says. “Our measurements were mostly dedicated to the outer parts of the galactic disc, out to 52, 000 light years from the galactic center and beyond.”

 

Milky Way Disk

The structure of our galaxy, the Milky Way, with its warped galactic disc, where the majority of its hundreds of billions of stars reside. Data from ESA’s star-observer Gaia recently proved that the disc’s warp is precessing, essentially moving around similarly to a wobbling spinning top. The speed of the warp’s rotation is so high that it must have been caused by a rather powerful event, astronomers believe, perhaps an ongoing collision with another, smaller, galaxy which sends ripples through the disc like a rock thrown into water. (Stefan Payne-Wardenaar; Inset: NASA/JPL-Caltech; Layout: ESA)

Gaia previously uncovered evidence of collisions between the Milky Way and other galaxies in the recent and distant past, which can still be observed in the motion patterns of large groups of stars billions of years after the events occurred.

Meanwhile, the satellite, currently in the sixth year of its mission, keeps scanning the sky and a Europe-wide consortium is busy processing and analyzing the data that keeps flowing towards Earth. Astronomers across the world are looking forward to the next two Gaia data releases, planned for later in 2020 and in the second half of 2021, respectively, to tackle further mysteries of the galaxy we call home.

Source:: E. Poggio et al. Evidence of a dynamically evolving Galactic warp, Nature Astronomy (2020). DOI: 10.1038/s41550-020-1017-3

The Daily Galaxy, Sam Cabot, via the European Space Agency