If there’s one rule that’s practically universal in astronomy, it’s this: you can only observe the parts of the Universe that your instruments are sensitive to. As a result, when most of us think about the objects that are out there in the cosmos, we think about the components that are easiest to see: things that are bright, close by, and that emit radiation in the form of visible light. When we think of galaxies, we think of the stars within them; when we think of stars, we think primarily of the ones that appear brightest to our eyes and in our telescopes. But there’s a whole Universe out there to explore, and much of it doesn’t emit any visible light at all.
This is true even for large spiral galaxies like the Milky Way. We aren’t just a collection of stars, with the occasional “dust lane” of neutral matter that blocks the starlight from behind it, but rather a rich network of gas and dust, dotted with stars and with cavities blown in them by violent stellar cataclysms. By looking at 19 nearby, face-on spiral galaxies with JWST’s remarkable, unprecedentedly sharp and powerful eyes, the PHANGS (Physics at High Angular resolution in Nearby GalaxieS) collaboration has at last uncovered the life cycles of stars within them. From breathtaking sights to breakthrough science, here’s what was revealed when we took our greatest look of all at these nearby Milky Way analogues.