The European Space Agency’s XMM-Newton and NASA’s Chandra X-ray space telescopes have spotted the aftermath of three bright explosions echoing through the outer spiral arms of our galaxy, the Milky Way. By measuring the distance to these echoes, they found the outer arms to be up to 10% farther away than previously thought.
Perhaps surprisingly, we don’t know much about the structure of our galaxy’s outer regions. It’s difficult to observe our galaxy from the inside: The solar system is well embedded in its disk, preventing a bird’s-eye view, and many regions are obscured by thick clouds of cosmic dust.
But this is changing: We have learned a huge amount since the launch of ESA’s star-surveying Gaia space telescope. Using data collected by Gaia, scientists are mapping the Milky Way galaxy in more detail than ever before by measuring precise distances to its stars. Before Gaia, we weren’t even sure whether our galaxy had two or four spiral arms (we now know the answer to be four).








