WEBVTT FILE 1 00:00:00.200 --> 00:00:01.200 X-rays. 2 00:00:01.200 --> 00:00:03.833 When you think of X-rays,you might think of broken bones. 3 00:00:03.833 --> 00:00:06.733 But here at NASA, X-rays let us see so much more. 4 00:00:06.733 --> 00:00:10.100 Unlike taking an X-ray of our skeleton, which involves projecting X-rays 5 00:00:10.100 --> 00:00:11.100 through our body, 6 00:00:11.100 --> 00:00:14.633 we look at X-rays naturally emitted by things like stellar explosions. 7 00:00:14.700 --> 00:00:16.866 X-rays are part of the electromagnetic spectrum, 8 00:00:16.866 --> 00:00:20.133 the full spectrum of energy waves that runs from radio to gamma rays. 9 00:00:20.200 --> 00:00:22.166 In the middle of the spectrum is visible light, 10 00:00:22.166 --> 00:00:25.866 the rainbow of color that human eyes can see. X-rays, emitted by hot gases 11 00:00:25.866 --> 00:00:29.100 throughout the universe, are considerably more energetic than visible light waves. 12 00:00:29.266 --> 00:00:30.733 This means the wavelengths are quite small, 13 00:00:30.733 --> 00:00:33.266 so they slip right between the atoms of most objects, 14 00:00:33.266 --> 00:00:36.700 including the mirrors we use in telescopes to focus other kinds of light. 15 00:00:36.800 --> 00:00:39.800 X-ray telescopes, like those on Chandra and JAXA's XRISM spacecraft, 16 00:00:39.800 --> 00:00:40.933 use specially- designed mirrors 17 00:00:40.933 --> 00:00:44.666 set at a shallow angle to minimize spaces between the mirrors atoms. 18 00:00:44.733 --> 00:00:47.000 This allows X-rays to bounce off the surface of the mirror, 19 00:00:47.000 --> 00:00:49.466 like a rock skipping off the surface of a pond. 20 00:00:49.466 --> 00:00:52.266 Studying X-rays will help us unravel mysteries of our universe, 21 00:00:52.266 --> 00:00:54.733 like the internal structure of neutron stars 22 00:00:54.733 --> 00:00:57.100 or near-light-speed jets from black holes. 23 00:00:57.100 --> 00:00:59.466 It's all about seeing things in a different wavelength of light.