1 00:00:02,040 --> 00:00:06,720 Speaker 1: Welcome to brain Stuff from How Stuff Works Pay brain 2 00:00:06,760 --> 00:00:10,520 Speaker 1: Stuff Lauren Vogel bomb Here many mysteries hide beneath Jupiter's 3 00:00:10,600 --> 00:00:13,840 Speaker 1: beautifully chaotic clouds, But with the help of some clever 4 00:00:13,920 --> 00:00:17,960 Speaker 1: astronomical techniques and NASA's Juno spacecraft, one of the giant 5 00:00:18,000 --> 00:00:21,160 Speaker 1: planet's biggest puzzles may be closer than ever to being solved. 6 00:00:21,800 --> 00:00:24,720 Speaker 1: As we know, water is the key to life on Earth. 7 00:00:25,040 --> 00:00:27,639 Speaker 1: Our efforts therefore to seek out life on other worlds 8 00:00:27,800 --> 00:00:31,880 Speaker 1: hinges on the detection of this important compound. Though scientists 9 00:00:31,920 --> 00:00:35,440 Speaker 1: don't think that life inhabits Jupiter, finding a Jovian reservoir 10 00:00:35,560 --> 00:00:38,479 Speaker 1: is one of the most pressing issues in planetary science. 11 00:00:39,040 --> 00:00:41,520 Speaker 1: Locating this water would help us understand how the Solar 12 00:00:41,560 --> 00:00:46,520 Speaker 1: System and Jupiter itself evolved. Unfortunately, Jupiter has been notoriously 13 00:00:46,680 --> 00:00:50,080 Speaker 1: unhelpful at revealing any water deep in its thick atmosphere, 14 00:00:50,360 --> 00:00:54,800 Speaker 1: leaving scientists and their models of planetary formation high and dry. 15 00:00:55,320 --> 00:00:58,920 Speaker 1: Before we sent spacecraft to investigate Jupiter, scientists assumed the 16 00:00:59,000 --> 00:01:01,480 Speaker 1: gas giant would contain encopious amounts of H two O. 17 00:01:02,040 --> 00:01:04,600 Speaker 1: The logic was simple, Earth is covered in the wet stuff, 18 00:01:04,800 --> 00:01:07,160 Speaker 1: and there's lots of water in the various moons that 19 00:01:07,280 --> 00:01:11,039 Speaker 1: orbit the giant planets. Therefore, Jupiter, the most massive and 20 00:01:11,120 --> 00:01:14,399 Speaker 1: most gravitationally dominant planet in the Solar System, must have 21 00:01:14,480 --> 00:01:17,320 Speaker 1: trapped the lion's share of our Solar System's water as 22 00:01:17,360 --> 00:01:20,840 Speaker 1: it formed billions of years ago. That logic was shattered 23 00:01:20,880 --> 00:01:24,800 Speaker 1: in when NASA's Galileo mission dropped a probe into the 24 00:01:24,800 --> 00:01:28,840 Speaker 1: planet's atmosphere to measure its composition. Much to everyone's surprise, 25 00:01:29,040 --> 00:01:32,560 Speaker 1: there was an astonishing lack of water. But the Galileo 26 00:01:32,600 --> 00:01:35,479 Speaker 1: probe may not have detected water simply because it wasn't 27 00:01:35,520 --> 00:01:37,920 Speaker 1: dropped in the right place. It could be as if 28 00:01:37,920 --> 00:01:40,600 Speaker 1: the probe parachuted over a desert on Earth. It's not 29 00:01:40,640 --> 00:01:43,000 Speaker 1: that there's no water on Earth, it's just that deserts 30 00:01:43,000 --> 00:01:46,320 Speaker 1: aren't known for being awash with the stuff. Jupiter's atmosphere 31 00:01:46,360 --> 00:01:50,080 Speaker 1: is dynamic, with jet stream storms and a non homogeneous composition. 32 00:01:50,520 --> 00:01:53,240 Speaker 1: The probe could only sample the atmosphere it was traveling 33 00:01:53,240 --> 00:01:56,200 Speaker 1: through in that one location, and that location might have 34 00:01:56,240 --> 00:01:59,600 Speaker 1: been as dry as a desert. The situation changed, however, 35 00:01:59,640 --> 00:02:03,400 Speaker 1: when we searchers used the powerful wm Keck observatory and 36 00:02:03,560 --> 00:02:07,560 Speaker 1: NASA infrared telescope facility on Hawaii's Mona Kea to stare 37 00:02:07,600 --> 00:02:11,520 Speaker 1: deep into Jupiter's biggest storm, the Great Red Spot. They 38 00:02:11,560 --> 00:02:15,400 Speaker 1: released their water filled news in an August study published 39 00:02:15,440 --> 00:02:18,600 Speaker 1: in the Astrophysical Journal and led by Gordon L. Bulaker 40 00:02:18,720 --> 00:02:21,960 Speaker 1: of NASA's Goddard Space Flight Center. Bure Aker said in 41 00:02:21,960 --> 00:02:25,080 Speaker 1: a NASA statement, the moons that orbit Jupiter are mostly 42 00:02:25,120 --> 00:02:27,880 Speaker 1: water ice, so the whole neighborhood has plenty of water. 43 00:02:28,280 --> 00:02:30,880 Speaker 1: Why wouldn't the planet, which is this huge gravity well 44 00:02:30,919 --> 00:02:35,080 Speaker 1: where everything falls into it, be water rich too. To investigate, 45 00:02:35,240 --> 00:02:39,120 Speaker 1: Bureaker's team measured the infrared radiation leaking from deep beneath 46 00:02:39,120 --> 00:02:43,280 Speaker 1: the clouds. Specifically, they studied the infrared absorption spectrum of 47 00:02:43,320 --> 00:02:45,400 Speaker 1: a certain type of methane, which is known to exist 48 00:02:45,480 --> 00:02:49,520 Speaker 1: in a vapor throughout the planet. This infrared radiation should 49 00:02:49,680 --> 00:02:53,360 Speaker 1: leak through the clouds unimpeded, but should any water vapor 50 00:02:53,400 --> 00:02:57,360 Speaker 1: clouds be present, this radiation would be blocked. During analysis 51 00:02:57,360 --> 00:03:00,960 Speaker 1: of observations from Jupiter's Great Red Spot, the researchers found 52 00:03:01,080 --> 00:03:04,360 Speaker 1: three distinct cloud layers were blocking this infrared signal from 53 00:03:04,400 --> 00:03:08,200 Speaker 1: passing through the atmosphere, thus agreeing with the theoretical predictions 54 00:03:08,200 --> 00:03:11,560 Speaker 1: for the presence of water rich clouds. They also detected 55 00:03:11,639 --> 00:03:14,880 Speaker 1: large quantities of carbon monoxide, suggesting that there's lots of 56 00:03:14,880 --> 00:03:18,560 Speaker 1: oxygen available in Jupiter's atmosphere to chemically bond with molecular 57 00:03:18,639 --> 00:03:22,000 Speaker 1: hydrogen to form water if the temperature and pressure is 58 00:03:22,040 --> 00:03:25,120 Speaker 1: just right. The next step will be to use these 59 00:03:25,200 --> 00:03:29,720 Speaker 1: data to complement the Juno spacecraft's observations of Jupiter. JUNO 60 00:03:29,800 --> 00:03:33,880 Speaker 1: can make spectroscopic observations even deeper into Jupiter's atmosphere, and 61 00:03:33,919 --> 00:03:36,160 Speaker 1: it will do so for the entire planet, not just 62 00:03:36,320 --> 00:03:39,480 Speaker 1: the Great Red Spot. But should Juno also detect this 63 00:03:39,560 --> 00:03:43,040 Speaker 1: possible water cloud layer. The techniques developed by Bureaker's team 64 00:03:43,160 --> 00:03:45,760 Speaker 1: using telescopes on Earth will have been proven effective at 65 00:03:45,760 --> 00:03:49,080 Speaker 1: finding water deep inside Jupiter, thereby solving the gas giants 66 00:03:49,080 --> 00:03:51,960 Speaker 1: watery mystery, and these techniques could then be used to 67 00:03:52,000 --> 00:03:55,000 Speaker 1: probe deep into the atmospheres of other planets like Saturn, Urinus, 68 00:03:55,080 --> 00:03:58,080 Speaker 1: or Neptune without having to send a probe into them. 69 00:03:58,240 --> 00:04:00,480 Speaker 1: NASA named the Juno mission, by the way, after the 70 00:04:00,600 --> 00:04:03,480 Speaker 1: Roman goddess Juno, who was married to Jupiter and had 71 00:04:03,520 --> 00:04:11,640 Speaker 1: the handy ability to see through clouds. Today's episode was 72 00:04:11,680 --> 00:04:14,480 Speaker 1: written by Ian O'Neill and produced by Tyler Clang. To 73 00:04:14,520 --> 00:04:17,560 Speaker 1: find brain stuff, notebooks, and other brainy stuff, visit our 74 00:04:17,640 --> 00:04:20,960 Speaker 1: online shop at t public dot com slash brain stuff, and, 75 00:04:21,080 --> 00:04:22,920 Speaker 1: of course, for more on this and lots of other 76 00:04:23,000 --> 00:04:26,279 Speaker 1: perceptive topics, visit our home planet, how stuff works dot 77 00:04:26,279 --> 00:04:37,640 Speaker 1: com