A new survey from the Hubble Space Telescope offers an exciting look at the dwarf galaxies that orbit the Andromeda galaxy. This marks the first time we’ve seen a broad view of these smaller galaxies surrounding Andromeda.
The findings indicate that Andromeda’s dwarf galaxies have had a much wilder history than those of the Milky Way. While the Milky Way’s smaller galaxies have evolved in a calm manner, Andromeda’s galaxies have collided and interacted chaotically over billions of years.
These insights were shared in a study published in The Astrophysical Journal. The authors suggest that what we know about the Milky Way may not apply to other galaxies, which is a significant revelation for astronomers. Daniel Weisz, a co-author of the study from UC Berkeley, emphasizes, “Low-mass galaxies in different ecosystems have taken different paths than those in our Milky Way.”
Andromeda, located about 2.5 million light-years from Earth, is the closest major galaxy to us and is on a collision course with the Milky Way, expected to merge in about 5 billion years. While it appears faintly as a spindle shape in the night sky, there’s a hidden world of dwarf galaxies around it that requires powerful telescopes to study.
Starting in late 2019, Hubble spent two years capturing images and data about 36 dwarf galaxies orbiting Andromeda up to 1.63 million light-years away. This work has given scientists a detailed 3D view of Andromeda’s galaxy ecosystem, allowing them to track how these smaller galaxies have evolved over nearly 14 billion years.
“Everything in the Andromeda system is very scattered and disturbed,” Weisz noted. “It seems something significant happened not too long ago.” Researchers believe that a collision between Andromeda and a larger galaxy a few billion years ago might be responsible. The satellite galaxy Messier 32, visible on Andromeda’s lower left, could be a remnant of this cosmic smashup.
Interestingly, the study also uncovered a rare group of galaxies around Andromeda that are not found near the Milky Way. These galaxies formed stars early and kept doing so at a much slower rate than expected. Given Andromeda’s strong gravity, they should have lost their star-forming gas long ago, similar to what’s seen with the Milky Way’s satellites.
“This doesn’t show up in our computer simulations,” said Alessandro Savino, the lead author of the study. “No one knows what to make of that so far.”
Another surprising discovery is that about half of Andromeda’s dwarf galaxies orbit in a flat plane, all moving in unison. This arrangement is unlike what we see with other galaxies, including our own.
Weisz described this finding as “weird” and expressed the ongoing mystery behind their formation. The galaxies in this “Great Plane of Andromeda” don’t show any clear patterns in star formation, suggesting that this arrangement may be a chance occurrence rather than a distinct structure.
Weisz concludes, “There’s a lot of diversity in the Andromeda satellite system that needs to be understood. The way these galaxies come together is key to unraveling the history of Andromeda.” This ongoing research continues to shed light on the complex dynamics of our cosmic neighbors.