The Milky Way is moving toward the region historically called the Great Attractor, but that motion is part of a larger flow of galaxies in our local cosmic neighbourhood rather than a simple falling into one object.
 
The Great Attractor is a gravitational concentration in the direction of the Hydra-Centaurus region, obscured by the Milky Way’s own dust and stars, so it was inferred from galaxy motions before it was directly mapped. It is now understood as part of the larger Laniakea Supercluster, which includes the Milky Way. Galaxies do not sit still in the expanding universe; they also have their own peculiar velocity due to local gravity. Observations show the Milky Way and nearby galaxies are streaming toward a mass concentration in that direction at roughly 600 km/s, though that motion is not caused by a single isolated thing but by multiple large-scale structures.
 
Current explanations suggest the Great Attractor accounts for only part of the motion, with the much more distant Shapley Supercluster likely contributing strongly as well. So, the phrase “pulled toward the Great Attractor” is a useful shorthand, but the real picture is a web of gravitational influences across the local universe. A good analogy is a river flowing downhill: the Milky Way is one boat in a broad current shaped by several valleys and slopes, not a single whirlpool. The Great Attractor names one especially influential part of that river current.
 
References
Hall, S. (2014, September 3). Meet Laniakea, Our Home Cluster. Universe Today.
 
News Staff. (2016, February 9). Hidden Galaxies Shed New Light on Great Attractor Gravitational Anomaly. Sci News.
 
Great Attractor. (2026, June 22). In Wikipedia, https://en.wikipedia.org/wiki/Great_Attractor

​Astronomers think the Milky Way absorbed a small dwarf galaxy dubbed Loki billions of years ago. The idea comes from a recent study of 20 metal-poor stars whose chemical patterns and orbits suggest they likely came from that ancient merger.
 
Loki is the name researchers gave to a suspected dwarf galaxy that merged with the Milky Way very early in our galaxy’s history. The stars linked to it appear to have been scattered when the merger happened, leaving behind a remnant population inside the Milky Way. The study looked at the stars’ chemical abundances and orbital behaviour. Their properties fit a short-lived dwarf galaxy that was chemically distinct from many other metal-poor stars in the Milky Way’s halo.
 
Astronomers identify stars from other galaxies by looking at their chemical fingerprints in starlight. Each element absorbs and emits light at very specific wavelengths, so a star’s spectrum reveals its elemental mix and lets scientists compare it with stars formed in the Milky Way. Stars that formed in a small dwarf galaxy often have a different enrichment history from Milky Way stars. They may show unusual ratios such as iron to magnesium, or a different spread in heavier elements, because their parent galaxy formed stars more slowly or experienced different gas inflow and merger history.
 
Researchers usually combine several clues. These include element ratios, especially iron, magnesium, and other alpha elements; how broad or narrow the abundance pattern is across many stars; and whether the stars cluster together in orbital space, which can indicate a shared origin. If a group of stars all share a distinctive chemical pattern that does not match typical Milky Way populations, that suggests they were born together in a separate system and later accreted by the Milky Way. In practice, astronomers use chemistry plus motion together, because chemistry alone is strong evidence but not always enough on its own.
 
This is still an interpretation based on a small sample, so the conclusion is promising but not final. Future larger surveys are expected to test whether those stars really trace back to one ancient galaxy.
 
References
Astronomy Staff. (2019, June). Ask Astro: How Do Scientists Determine the Chemical Compositions of the Planets and Stars? Astronomy.
 
Kasal, K. (2026, April 30). A Lost Galaxy Called Loki May Be Hiding Inside the Milky Way. Phys.Org.
 
Sutter, P. (2024, October 17). A Baby Milky Way May Have Swallowed a Dwarf Galaxy Named Loki. Astronomy. 
 
(2026, May 19). Star. In Wikipedia: https://en.wikipedia.org/wiki/Star
 
(2025, December 9). This Surprising Discovery Rewrites the Milky Way’s Origin Story. ScienceDaily. Royal Astronomical Society. https://www.sciencedaily.com/releases/2025/12/251209082301.htm
 
(2023, June 23). A Bird’s Eye View of the Milky Way. Max-Planck-Gesellschaft. https://www.mpg.de/20470314/reconstructing-alien-astronomers-view-of-our-home-galaxy-s-chemistry