With a process known as spectroscopy, researchers from the Instituto de Astrofísica de Canarias and at the National Astronomical Observatories of Beijing studied the chemical composition of over 4,600 stars from two surveys, APOGEE and LAMOST, and mapped out which stars are part of the disk and which belong to the halo. The results , published May 7 in the journal Astronomy and Astrophysics, clearly show disk stars much farther from center of the galaxy than before.“Certainly, one would expect the existence of stars at very far distances from the galactic center, as part of the halo,” says Martín López Corredoira, lead author on the paper and researcher at Instituto de Astrofísica de Canaria. “But, as far as we know, nobody could previously say that stars [farther than 81,000 light-years] are confirmed spectroscopically to belong to the disk.”The researchers still believe the density of stars at the edge tapers off in an exponential manner — just farther away than previously thought. Although its diameter has been supersized, the Milky Way is still smaller than its neighbor Andromeda, which measures over 220,000 light-years across.While our galaxy is looking larger, it’s not putting on much weight. Because the outer reaches are much less dense than the center of the galaxy, the additional area is only sparsely populated with stars. These few extra stars are only a drop in the bucket compared to the rest of the galaxy, so overall the mass of the Milky Way remains largely unchanged.