1 00:00:02,420 --> 00:00:09,110 [Music] 2 00:00:13,270 --> 00:00:10,950 infrared is an important wavelength for 3 00:00:14,950 --> 00:00:13,280 astronomers because several reasons the 4 00:00:16,870 --> 00:00:14,960 expansion of the universe to see farther 5 00:00:19,430 --> 00:00:16,880 back looking through dust clouds and 6 00:00:29,269 --> 00:00:19,440 looking at cooler objects like planets 7 00:00:33,590 --> 00:00:31,830 we can see into dust clouds the way that 8 00:00:35,270 --> 00:00:33,600 infrared does it the longer wavelengths 9 00:00:37,510 --> 00:00:35,280 of light actually can go bending around 10 00:00:39,910 --> 00:00:37,520 the obstacles like dust grains 11 00:00:42,310 --> 00:00:39,920 so we see around the dust grains and 12 00:00:44,069 --> 00:00:42,320 able to see inside those opaque clouds 13 00:00:48,630 --> 00:00:44,079 to see what's happening like in the 14 00:00:52,869 --> 00:00:50,630 infrared is important also when we want 15 00:00:54,389 --> 00:00:52,879 to see the most distant galaxies 16 00:00:56,229 --> 00:00:54,399 they appear to be running away from us 17 00:00:58,150 --> 00:00:56,239 at immense speeds because of the 18 00:00:59,990 --> 00:00:58,160 expansion of the universe the light that 19 00:01:01,750 --> 00:01:00,000 we received from those distant galaxies 20 00:01:03,510 --> 00:01:01,760 had been stretched along with the 21 00:01:05,830 --> 00:01:03,520 expansion of the universe so that it is 22 00:01:07,270 --> 00:01:05,840 much longer wavelengths which means 23 00:01:08,870 --> 00:01:07,280 started off with visible light and 24 00:01:10,230 --> 00:01:08,880 that's now infrared 25 00:01:12,070 --> 00:01:10,240 so if you want to see those first 26 00:01:13,910 --> 00:01:12,080 galaxies you need an infrared telescope 27 00:01:21,000 --> 00:01:13,920 to pick up the light that started out as