1 00:00:05,930 --> 00:00:04,430 over the last two decades scientists 2 00:00:07,670 --> 00:00:05,940 have found thousands of planets 3 00:00:09,710 --> 00:00:07,680 elsewhere in the universe these are 4 00:00:11,509 --> 00:00:09,720 called exoplanets as we get better and 5 00:00:13,249 --> 00:00:11,519 better at finding them we need ways to 6 00:00:14,509 --> 00:00:13,259 narrow down the ones most likely to 7 00:00:16,730 --> 00:00:14,519 support life 8 00:00:18,650 --> 00:00:16,740 two NASA rocket teams are working to do 9 00:00:21,170 --> 00:00:18,660 just that from Australia 10 00:00:22,490 --> 00:00:21,180 their mission study a special pair of 11 00:00:24,890 --> 00:00:22,500 stars best seen in the Southern 12 00:00:27,589 --> 00:00:24,900 Hemisphere and Propel Humanity's search 13 00:00:29,570 --> 00:00:27,599 for habitable worlds into the future I'm 14 00:00:31,310 --> 00:00:29,580 miles Hadfield and I'm following these 15 00:00:33,410 --> 00:00:31,320 rocket teams to Australia to show you 16 00:00:34,610 --> 00:00:33,420 what it takes to launch a rocket and 17 00:00:37,250 --> 00:00:34,620 make groundbreaking scientific 18 00:00:39,420 --> 00:00:37,260 measurements hang on tight we're going 19 00:00:45,069 --> 00:00:39,430 on an adventure High Above Down Under 20 00:00:45,079 --> 00:00:50,209 Earth is packed with life 21 00:00:54,350 --> 00:00:52,010 some environments are more habitable 22 00:00:56,869 --> 00:00:54,360 than others so what makes an environment 23 00:01:00,770 --> 00:00:56,879 or a planet a good place for life to 24 00:01:03,650 --> 00:01:00,780 thrive well one thing is 25 00:01:05,210 --> 00:01:03,660 water and in fact that's what the search 26 00:01:07,550 --> 00:01:05,220 for life elsewhere in the universe is 27 00:01:09,950 --> 00:01:07,560 focused on so far finding planets where 28 00:01:11,990 --> 00:01:09,960 water can exist in liquid form there's a 29 00:01:14,390 --> 00:01:12,000 region around every Star that scientists 30 00:01:16,190 --> 00:01:14,400 call the Goldilocks zone a planet in 31 00:01:19,130 --> 00:01:16,200 this Zone has the right temperature for 32 00:01:21,590 --> 00:01:19,140 water to remain liquid too close and the 33 00:01:24,350 --> 00:01:21,600 water will evaporate away too far and 34 00:01:27,410 --> 00:01:24,360 it'll freeze the distance has to be just 35 00:01:29,510 --> 00:01:27,420 right this Zone has been the basis for 36 00:01:31,490 --> 00:01:29,520 the search for habitable worlds but just 37 00:01:33,469 --> 00:01:31,500 because a plant is inside the Goldilocks 38 00:01:35,870 --> 00:01:33,479 zone doesn't mean it can sustain life 39 00:01:38,450 --> 00:01:35,880 take for example the closest known 40 00:01:40,490 --> 00:01:38,460 exoplanet to Earth At just 4.2 light 41 00:01:42,649 --> 00:01:40,500 years away it's located in the 42 00:01:44,569 --> 00:01:42,659 Goldilocks zone but scientists think the 43 00:01:46,310 --> 00:01:44,579 star's frequent eruptions might have 44 00:01:48,469 --> 00:01:46,320 blown away any atmosphere the planet 45 00:01:50,810 --> 00:01:48,479 might have had in other words the 46 00:01:52,789 --> 00:01:50,820 Goldilocks zone is just a first guess to 47 00:01:54,649 --> 00:01:52,799 truly tell whether an exoplanet is 48 00:01:57,410 --> 00:01:54,659 habitable we need to look at the star 49 00:01:59,810 --> 00:01:57,420 it's orbiting unfortunately we can't 50 00:02:01,789 --> 00:01:59,820 just observe a planet and understand it 51 00:02:03,649 --> 00:02:01,799 at face value we have to understand it 52 00:02:07,010 --> 00:02:03,659 in the context of what its parent star 53 00:02:08,809 --> 00:02:07,020 is giving it so scientists have been 54 00:02:10,790 --> 00:02:08,819 collecting data from different types of 55 00:02:12,470 --> 00:02:10,800 stars to learn how they affect their 56 00:02:15,190 --> 00:02:12,480 planets we would like to be able to 57 00:02:18,110 --> 00:02:15,200 create a menu of star planet 58 00:02:22,130 --> 00:02:18,120 possibilities that our future missions 59 00:02:25,250 --> 00:02:22,140 can draw from and prioritize the most 60 00:02:27,350 --> 00:02:25,260 promising places to find habitable 61 00:02:29,750 --> 00:02:27,360 environments the next item to be added 62 00:02:32,089 --> 00:02:29,760 to the menu yellow stars we're looking 63 00:02:35,449 --> 00:02:32,099 for something around 5 billion years old 64 00:02:37,670 --> 00:02:35,459 an average sized wait a second don't we 65 00:02:40,790 --> 00:02:37,680 have one right here so why not use the 66 00:02:43,809 --> 00:02:40,800 sun we've thought that our sun is the 67 00:02:46,729 --> 00:02:43,819 prototype for kind of 5 billion year old 68 00:02:49,009 --> 00:02:46,739 average yellow stars what we've learned 69 00:02:51,949 --> 00:02:49,019 recently is that our stun is actually 70 00:02:54,890 --> 00:02:51,959 quite inactive for a 5 billion year old 71 00:02:56,750 --> 00:02:54,900 yellow star typical Earthling Behavior 72 00:02:58,970 --> 00:02:56,760 really thinking we're the example for 73 00:03:01,130 --> 00:02:58,980 the entire universe but it turns out 74 00:03:03,110 --> 00:03:01,140 yellow stars are found throughout our 75 00:03:05,150 --> 00:03:03,120 galaxy and they tend to erupt with 76 00:03:07,550 --> 00:03:05,160 life-altering activity more often than 77 00:03:09,650 --> 00:03:07,560 our sun does so if we want to understand 78 00:03:11,570 --> 00:03:09,660 if they can still support life we'll 79 00:03:13,790 --> 00:03:11,580 need more data than our son can give us 80 00:03:16,670 --> 00:03:13,800 that's why two rocket teams are looking 81 00:03:18,949 --> 00:03:16,680 to Alpha Centauri A and B the reason why 82 00:03:22,009 --> 00:03:18,959 we're targeting Alpha Centauri is that 83 00:03:24,229 --> 00:03:22,019 it's our nearest solar twin so in many 84 00:03:26,509 --> 00:03:24,239 many ways it's just like the sun it has 85 00:03:28,369 --> 00:03:26,519 almost the same mass it's a very similar 86 00:03:30,589 --> 00:03:28,379 age and it's nearby which is always 87 00:03:32,270 --> 00:03:30,599 great and with the help of NASA sounding 88 00:03:33,710 --> 00:03:32,280 Rockets they'll capture light from those 89 00:03:35,869 --> 00:03:33,720 stars that doesn't make it to the ground 90 00:03:37,490 --> 00:03:35,879 this range of Highly energetic 91 00:03:40,009 --> 00:03:37,500 ultraviolet light has never been 92 00:03:42,110 --> 00:03:40,019 measured before for these Stars even 93 00:03:44,089 --> 00:03:42,120 small differences in this UV light from 94 00:03:47,210 --> 00:03:44,099 a star can determine whether a nearby 95 00:03:49,250 --> 00:03:47,220 planet can support life or not but the 96 00:03:51,890 --> 00:03:49,260 Alpha Centauri system isn't visible from 97 00:03:53,930 --> 00:03:51,900 most places in the U.S it's best studied 98 00:03:55,670 --> 00:03:53,940 from the southern hemisphere 99 00:03:57,470 --> 00:03:55,680 that's why we're here in Northern 100 00:03:59,030 --> 00:03:57,480 Australia in the traditional homelands 101 00:04:00,710 --> 00:03:59,040 of the yongyu people they've been 102 00:04:02,990 --> 00:04:00,720 observing the Stars here for tens of 103 00:04:05,449 --> 00:04:03,000 thousands of years I'm here with two 104 00:04:07,910 --> 00:04:05,459 rocket science teams Sistine and deuce 105 00:04:11,149 --> 00:04:07,920 and a crew of about 50 NASA Engineers 106 00:04:12,649 --> 00:04:11,159 rocket Specialists and support staff in 107 00:04:14,449 --> 00:04:12,659 partnership with equatorial launch 108 00:04:16,909 --> 00:04:14,459 Australia and the gumach corporation 109 00:04:18,710 --> 00:04:16,919 they have created an entire rocket range 110 00:04:20,870 --> 00:04:18,720 from scratch to help the scientists 111 00:04:22,730 --> 00:04:20,880 achieve their goals in this series 112 00:04:24,530 --> 00:04:22,740 you're going to meet these teams and 113 00:04:26,570 --> 00:04:24,540 follow their Quest high above the 114 00:04:28,310 --> 00:04:26,580 Australian Outback to see what it takes 115 00:04:30,530 --> 00:04:28,320 to make these first ever measurements 116 00:04:32,090 --> 00:04:30,540 from our closest Stellar neighbors we 117 00:04:33,770 --> 00:04:32,100 are going behind the scenes to learn 118 00:04:35,810 --> 00:04:33,780 more about the science of habitability 119 00:04:37,909 --> 00:04:35,820 and what goes into launching a rocket 120 00:04:40,310 --> 00:04:37,919 dodging venomous snakes and crocodiles 121 00:04:42,170 --> 00:04:40,320 along the way but first we'll take a 122 00:04:43,969 --> 00:04:42,180 look at how this brand new rocket range 123 00:04:45,890 --> 00:04:43,979 came to life with the help of the