Accounting for approximately 1% of the total stellar mass, the stellar halo — the diffuse cloud of stars surrounding the Galactic disk — plays an outsized role in our understanding of the Milky Way. For decades, the general assumption has been that the halo is more or less spherical and isotropic, or the same in every direction. Now new research led by the Harvard & Smithsonian’s Center for Astrophysics shows the halo is oblong and...
