1 00:00:10,070 --> 00:00:02,450 [Music] 2 00:00:13,570 --> 00:00:12,049 we know that the universe is expanding 3 00:00:16,369 --> 00:00:13,580 we've known that for almost 100 years 4 00:00:18,410 --> 00:00:16,379 the rate at which the universe expands 5 00:00:19,490 --> 00:00:18,420 is a number we refer to as the Hubble 6 00:00:21,230 --> 00:00:19,500 constant 7 00:00:23,269 --> 00:00:21,240 when Hubble was launched one of its main 8 00:00:24,710 --> 00:00:23,279 objectives was to measure the Hubble 9 00:00:27,769 --> 00:00:24,720 constant the expansion rate of the 10 00:00:30,349 --> 00:00:27,779 universe by resolving individual stars 11 00:00:32,150 --> 00:00:30,359 in distant galaxies Hubble was really 12 00:00:35,090 --> 00:00:32,160 the first telescope that allowed us to 13 00:00:38,030 --> 00:00:35,100 easily resolve the individual components 14 00:00:40,549 --> 00:00:38,040 the stars in a distant Galaxy to gauge 15 00:00:42,110 --> 00:00:40,559 its distance and that's part of the 16 00:00:44,569 --> 00:00:42,120 ingredients you need to measure the 17 00:00:46,670 --> 00:00:44,579 expansion rate of the universe over time 18 00:00:48,709 --> 00:00:46,680 Hubble also was improved by a series of 19 00:00:51,110 --> 00:00:48,719 servicing missions that increased the 20 00:00:52,970 --> 00:00:51,120 sensitivity resolution and also 21 00:00:55,610 --> 00:00:52,980 ultimately allowed us to make 22 00:00:58,369 --> 00:00:55,620 observations in the near infrared which 23 00:00:59,930 --> 00:00:58,379 reduces the effects of dust dust is 24 00:01:01,610 --> 00:00:59,940 scattered throughout the Universe and if 25 00:01:03,349 --> 00:01:01,620 you're looking at a distant light and 26 00:01:05,390 --> 00:01:03,359 trying to tell how far away it is dust 27 00:01:07,730 --> 00:01:05,400 can dim the light and fool you into the 28 00:01:09,410 --> 00:01:07,740 gates further away than it is Hubble has 29 00:01:11,450 --> 00:01:09,420 sort of all of these tools on its 30 00:01:14,810 --> 00:01:11,460 utility belt that allow us to measure 31 00:01:16,070 --> 00:01:14,820 the expansion rate as well as it's been 32 00:01:18,410 --> 00:01:16,080 measured to date 33 00:01:19,730 --> 00:01:18,420 Hubble found that the expansion rate of 34 00:01:22,730 --> 00:01:19,740 the universe is speeding up it's 35 00:01:24,380 --> 00:01:22,740 accelerating due to a new component of 36 00:01:26,270 --> 00:01:24,390 the universe that we call dark energy 37 00:01:29,390 --> 00:01:26,280 [Music] 38 00:01:32,270 --> 00:01:29,400 Dark Energy actually reverses the sign 39 00:01:34,550 --> 00:01:32,280 of gravity it actually gives rise to a 40 00:01:36,170 --> 00:01:34,560 repulsive gravity which is sounds very 41 00:01:38,149 --> 00:01:36,180 strange and it's not something that 42 00:01:40,789 --> 00:01:38,159 Isaac Newton would have understood but 43 00:01:42,649 --> 00:01:40,799 it is a feature in Einstein's theory of 44 00:01:44,870 --> 00:01:42,659 general relativity Einstein's theory of 45 00:01:47,210 --> 00:01:44,880 gravity that replacement theory of 46 00:01:50,149 --> 00:01:47,220 gravity and in that theory you can have 47 00:01:51,770 --> 00:01:50,159 such a material if you have a constant 48 00:01:54,230 --> 00:01:51,780 energy and empty space that's 49 00:01:56,450 --> 00:01:54,240 unavoidable then it will give rise to 50 00:01:59,870 --> 00:01:56,460 this repulsive gravity because gravity 51 00:02:02,569 --> 00:01:59,880 is weakest in the empty regions of space 52 00:02:04,490 --> 00:02:02,579 between galaxies dark energy has its 53 00:02:07,190 --> 00:02:04,500 most pronounced effect in deep space 54 00:02:10,449 --> 00:02:07,200 it's driving now pushing the inwards to 55 00:02:15,110 --> 00:02:13,190 the James Webb Space Telescope has 56 00:02:17,570 --> 00:02:15,120 certain capabilities that are even 57 00:02:20,390 --> 00:02:17,580 greater than Hubble's it will have 58 00:02:22,610 --> 00:02:20,400 greater resolution it can extend 59 00:02:25,070 --> 00:02:22,620 observations further to the room for red 60 00:02:28,729 --> 00:02:25,080 to even further diminish the impact of 61 00:02:32,089 --> 00:02:28,739 dust so it will both simultaneously give 62 00:02:33,890 --> 00:02:32,099 us a sharper view of these distant stars 63 00:02:35,510 --> 00:02:33,900 that are used to calibrate the expansion 64 00:02:38,030 --> 00:02:35,520 of the universe and it will also allow 65 00:02:41,089 --> 00:02:38,040 us to see through the last little wisps 66 00:02:43,250 --> 00:02:41,099 of dust in front of those our goal is to 67 00:02:46,369 --> 00:02:43,260 measure the Hubble constant to one 68 00:02:48,530 --> 00:02:46,379 percent precision and so we are using 69 00:02:50,509 --> 00:02:48,540 the Hubble Space Telescope and James 70 00:02:52,610 --> 00:02:50,519 Webb Space Telescope to refine those