1 00:00:00,100 --> 00:00:04,150 The more distant in space we look, the farther back we're looking in time. 2 00:00:04,170 --> 00:00:08,200 And so we're designing the James Webb Space Telescope to see past the point where 3 00:00:08,220 --> 00:00:12,380 Hubble could see and to see the very first stars and galaxies to light 4 00:00:12,400 --> 00:00:16,570 up after the Big Bang. The James Webb Space Telescope is designed as an 5 00:00:16,590 --> 00:00:20,630 infrared telescope because infrared is really where the key science questions 6 00:00:20,650 --> 00:00:24,760 will be answered. To see those very very distant galaxies 7 00:00:24,780 --> 00:00:28,800 the light from those galaxies has been red shifted. The expansion of the universe 8 00:00:28,820 --> 00:00:32,830 stretches space-time, the light from the galaxies gets stretched 9 00:00:32,850 --> 00:00:36,870 as well. And so longer wavelengths of light are redder. 10 00:00:36,890 --> 00:00:41,010 So at some point in the distant past the light from those galaxies 11 00:00:41,030 --> 00:00:45,090 has been shifted - red shifted – all the way out of the visible spectrum 12 00:00:45,110 --> 00:00:49,210 into the infrared part of the spectrum. So having an infrared telescope 13 00:00:49,230 --> 00:00:53,360 in space is one of the things that will allow us to see those very first galaxies. 14 00:00:53,380 --> 00:00:55,469 music