The mystery of the Milky Way's central

We Finally Know What These Mysterious Objects Near SgrA* Are! · 14:35 · Video: Anton Petrov · Watch at the source

In short: At the heart of our galaxy lies Sagittarius A*, a supermassive black hole surrounded by objects that defy easy classification. Some behave like stars, while others resemble gas clouds. For years, these 'G-objects' have puzzled astronomers, but new research is beginning to untangle their origins and the gravitational forces shaping them.

The G-object population, specifically objects like G1 and G2, presents a significant astronomical puzzle. G2, for instance, contains several Earth masses of material and appears as a compact mix of gas and dust. However, it moves with the trajectory of a star, despite showing no visible signs of starlight from its interior. This hybrid nature led to predictions that SgrA* would shred G2 in 2014; instead, the object survived the close encounter with only slight deformation.

Recent observations have identified a specific member of this population, a dusty source known as D9. Analysis suggests D9 is likely a binary system composed of a Herbig Ae/Be star and a lower-mass T-Tauri star. This discovery is significant because it provides a concrete example of a G-object's composition. The system is approximately 2.7 million years old and is currently undergoing a three-body interaction with SgrA*, which may eventually lead to a merging event.

Beyond individual objects, the broader stellar environment near SgrA* is defined by the 'paradox of youth.' While old stars are expected to descend toward the center, the region is dominated by young, massive stars less than 15 million years old. A new unified model proposes that these diverse populations—the chaotic S-stars, the clockwise disk, and the scattered outer stars—all formed simultaneously from a single gas disk. This model suggests that an intermediate-mass companion, such as a black hole or dense cluster about 10,000 times the mass of the sun, sculpted these orbits over millions of years through long-range gravitational influence.

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