1 00:00:00,090 --> 00:00:04,160 One of the key things of the James Webb Space Telescope is designed to do is 2 00:00:04,180 --> 00:00:08,280 detect the very first stars and galaxies that were born in the very early universe. 3 00:00:08,300 --> 00:00:12,480 So this is a part of the universe that we haven't seen at all yet. 4 00:00:12,500 --> 00:00:16,550 We don't know what's out there. The more distant in space we look, the further back 5 00:00:16,570 --> 00:00:20,610 we're looking in time. With Hubble we're about to push back and see pretty far 6 00:00:20,630 --> 00:00:24,680 into the distant universe, but we do reach a limit. And so we're designing 7 00:00:24,700 --> 00:00:28,750 the James Webb Space Telescope to see past the point of Hubble and to see 8 00:00:28,770 --> 00:00:32,940 the very first stars and galaxies light up after the Big Bang. 9 00:00:32,960 --> 00:00:36,990 We know that there is a time in the universe's past 10 00:00:37,010 --> 00:00:41,100 where the galaxies were the first to light up. Basically the 11 00:00:41,120 --> 00:00:45,250 stars and galaxies send out ionizing radiation, which 12 00:00:45,270 --> 00:00:49,450 clears out the fog of the hydrogen in the universe. So once that 13 00:00:49,470 --> 00:00:53,540 hydrogen fog is cleared out, the stars and galaxies can shine through. 14 00:00:53,560 --> 00:00:57,660 And so getting to that point just beyond what we call the dark ages is one 15 00:00:57,680 --> 00:01:00,007 of the major goals of the telescope.