WEBVTT FILE 1 00:00:00.000 --> 00:00:09.084 "What does Hubble’s infrared vision help  astronomers see?" 2 00:00:09.084 --> 00:00:12.985 Infrared is an important wavelength for astronomers because of several reasons. 3 00:00:12.985 --> 00:00:15.600 The expansion of the universe to see farther back, 4 00:00:15.600 --> 00:00:19.605 looking through dust clouds and  looking at cooler objects like planets. 5 00:00:19.605 --> 00:00:20.875 "Saturn - Visible" 6 00:00:20.875 --> 00:00:24.000 "Saturn - Infrared" 7 00:00:24.000 --> 00:00:26.152 "Jupiter - Visible" 8 00:00:26.152 --> 00:00:28.723 "Jupiter - Infrared" 9 00:00:28.723 --> 00:00:33.600 We can see into dust clouds the way that  infrared does it the longer wavelengths   10 00:00:33.600 --> 00:00:37.520 of light actually can go bending  around the obstacles like dust grains. 11 00:00:37.520 --> 00:00:41.440 So we see around the dust grains  and able to see inside those   12 00:00:41.440 --> 00:00:48.720 opaque clouds to see what's happening like  in the Orion Nebula and the Eagle Nebula. 13 00:00:48.720 --> 00:00:52.880 Infrared is important, also when we  want to see the most distant galaxies   14 00:00:52.880 --> 00:00:57.520 they appear to be running away from us at immense  speeds because of the expansion of the universe. 15 00:00:57.520 --> 00:01:01.200 The light that we receive from those  distant galaxies had been stretched 16 00:01:01.200 --> 00:01:06.320 along with the expansion of the universe so that  it is much longer wavelengths, which means it started   17 00:01:06.320 --> 00:01:10.800 off with visible light and it's now infrared. So if you want to see those first galaxies   18 00:01:10.800 --> 00:01:17.281 you need an infrared telescope to pick up the  light that started out as visible wavelengths. 19 00:01:17.281 --> 00:01:28.880 [ MUSIC ]