A long-ago encounter between our galaxy and an orbiting dwarf might have ejected some of the Milky Way’s stars.

A deep look into the skies above the plane of the Milky Way reveals ethereal clouds and streams of stars. These stars aren’t in our galaxy’s disk — they’re part of the 1% of stars that comprise the stellar halo. They’re generally thought to be ghosts of dwarf galaxies past, long ago torn into shreds after encounters with our more massive galaxy.

Now, new research shows that some of these stars might not be dwarf remnants at all — they might have come from the Milky Way’s own disk. The question then becomes: How did they travel all the way from the disk out into the stellar halo?

Maria Bergemann (Max Planck Institute for Astronomy, Germany) and colleagues have explored stars in two stellar populations known as the Triangulum-Andromeda (TriAnd for short) and A13 using the Keck I telescope in Hawaii and Very Large Telescope in Chile. The results are published in Nature Astronomy.

Locations of TriAnd and A13 star "clouds"
This artist's conception shows the locations of the A13 and TriAnd groups of stars above and below the galactic plane. The Milky Way Galaxy is portrayed as seen in computer simulations, where a long-ago gravitational interaction with a dwarf galaxy has perturbed the shape of its disk.
© T.Mueller / NASA / JPL-Caltech

Both clouds are well outside the Sun’s galactic orbit, between 50,000 and 65,000 light-years from the galaxy’s center, and well into the stellar halo. A13 floats roughly 15,000 light-years above the galactic plane, while TriAnd is 16,000 light-years below the plane.

After collecting the spectra of 14 stars, the astronomers measured the abundances of elements heavier than hydrogen and helium. Stars in the stellar halo are usually poor in heavy elements. But the 14 halo stars the group studied were surprisingly rich in heavy elements, more akin to the galaxy’s disk than its halo.

Moreover, the heavy-element abundances of TriAnd and A13 stars were similar to each other. Even though they’re separated by about 30,000 light-years, the two groups appear to have a common origin.

So what’s their origin? Bergemann and colleagues think one possible scenario is that a large dwarf galaxy, known as Sagittarius, careened into the Milky Way somewhere between 5 billion and 9 billion years ago. This destroyed dwarf can still be seen as the most visible streams in the galactic halo. According to the team’s computer simulation, such an interaction would have disrupted the Milky Way’s disk, sending swirls of stars above and below the galactic plane.

“[These measurements] provide tantalizing evidence that there has been more activity in the Milky Way than previously thought,” says Ana Bonaca (Harvard-Smithsonian Center for Astrophysics).

Sagittarius Stream as seen on the sky
The destroyed Sagittarius dwarf galaxy was long ago torn into streams that wrap around the Milky Way. They're clearly visible in this partial map of the sky. The colors indicate the distances to the stars identified in the study - stars located in red areas are further away, while stars in the blue areas are closer. The dotted red lines trace out the Sagittarius streams, and the blue ellipses in the center show the current location of the Sagittarius Dwarf Galaxy.
S. Koposov / SDSS-III collaboration
Sagittarius Stream
This artist's impression shows the tidal tails of stars (white) streaming from the Sagittarius Dwarf Galaxy (orange) that orbits the Milky Way. The bright yellow circle to the right of the galaxy's center is our Sun (not to scale). Sagittarius is on the other side of the galaxy from us, but we can see its tidal tails of stars stretching across the sky as they wrap around our galaxy.
Amanda Smith / University of Cambridge

Further Reading

This isn't the first time a dwarf galaxy has been found to blame for galactic oddities. Find out how a collision with a dwarf might have sent ripples through the Milky Way, and how astronomers are trying to catch the culprit of the hit-and-run.


Image of janez.osojnik@guest.arnes.si

[email protected]

March 15, 2018 at 3:24 am

It is difficult to imagine the dwarf galaxy in Sagittarius and location of both clusters. What is the location (RA, D) of TriAnd and A13 on the starmap? Couldn't find it anywhere on the web. Thank you for the answer. Jani

You must be logged in to post a comment.

Image of Monica Young

Monica Young

March 15, 2018 at 9:42 am

I agree, the illustration provided offers perspective but makes it difficult to picture the A13 and TriAnd populations on either side of the plane. If you have access to Nature, Figure 1 of the paper (https://www.nature.com/articles/nature25490) shows the location of A13 and TriAnd in galactic coordinates relative to the Sun and the galactic plane. The Sagittarius dwarf stream is a different story - this stream of stars is quite elongated and wraps around the Milky Way at least twice. I've added a second illustration to show the Sagittarius not on the sky but in perspective, as it wraps around the galaxy.

You must be logged in to post a comment.

You must be logged in to post a comment.