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.