Hubble Space Telescope reveals richest view of Andromeda galaxy to date (image)

Astronomers announced last week that they had completed a decade-long, meticulous effort to assemble a full portrait of our neighboring galaxy, Andromeda. The result is a stunning panoramic view that provides the most detailed image yet of the entire galaxy; its science-packed features could revolutionize our understanding of how spiral galaxies across the universe form and evolve.

Around 2015, astronomers took on the painstaking task of stitching together Hubble Space Telescope images of this galaxy, but that effort had focused on the galaxy’s northern half. Still, however, the resulting image showcased a sweeping view of 100 million stars packed into about 1.5 billion pixels.

Speaking during the 245th American Astronomical Society (AAS) press conference in Maryland, Zhuo Chen of the University of Washington told reporters she and her colleagues had just finished a similar effort for the galaxy’s southern half, adding almost 100 million stars to the previous mosaic.

Together, the two halves capture the glow of nearly 200 million stars across the Andromeda galaxy, marking the largest ever portrait assembled from Hubble telescope observations.

“It’s like photographing a beach and resolving individual grains of sand,” said Chen. “This is the first time that we can see such detailed structures for an external galaxy.”

Due to its proximity to the Milky Way, the Andromeda galaxy appears six times the diameter of the full moon in the sky (as seen from Earth) which was a lot of “celestial real estate” for Hubble’s pinpoint view. So, the panoramic mosaic required hundreds of snapshots taken across 1,000 orbits by the telescope, according to a NASA statement.

Beyond the awe-inspiring beauty of the image, this portrait will be an invaluable tool for astronomers to piece together Andromeda’s tumultuous history, chiefly its mergers with smaller satellite galaxies. Hubble observations of the galaxy’s age, mass of stars and heavy-element abundance would help researchers test competing models of galaxy evolution that predict distinct signatures across the two halves of the disk.

For instance, one theory posits the southern half may have been recently disturbed, likely by a single major merger around 2 billion to 4 billion years ago, leading to a pocket of star formation and unusually coherent streams of stars. By contrast, the northern half appears to be relatively calm with a less complex morphology. “That’s the big signature we can compare using our latest southern half observations,” said Chen.