The ultimate key to unlocking the heart of the Milky Way
At the centers of galaxies, supermassive black holes reside. This image of the central region of galaxy Messier 87 comes in the X-ray, via NASA’s Chandra X-ray observatory. The central, supermassive black hole is blasting out energetic particles at 99%+ the speed of light, which produces X-rays visible for up to 18,000 light-years from the galactic center. It is often easier to see these features in extragalactic objects than in our own galaxy, due to the large amount of obscuring material present within our own galaxy. Credit: NASA/CXC/SAO/B.Snios et al. But seeing into the Milky Way’s heart, especially from within it, presents challenges. Even the Milky Way, a relatively quiet galaxy with a relatively small central supermassive black hole, exhibits giant geysers of charged particles emanating from the galactic center. They can be revealed by radio telescopes, such as this image constructed with data from the Parkes radio telescope, a.k.a. The Dish. Credit: A. Mellinger (C. Michigan), E. Carretti (CSIRO), S-PASS Team, E. Bressert (CSIRO) Our galactic plane is rich in dust and gas: opaque …









