1 00:00:01,840 --> 00:00:07,280 Speaker 1: Welcome to brain Stuff, a production of iHeartRadio, Hey brain 2 00:00:07,280 --> 00:00:12,800 Speaker 1: Stuff Lauren vogelbom Here. A water surrounds us, falling from 3 00:00:12,880 --> 00:00:16,200 Speaker 1: rain clouds, rushing down river beds, and pouring from faucets, 4 00:00:16,840 --> 00:00:19,400 Speaker 1: and yet many of us have never stopped to wonder 5 00:00:20,120 --> 00:00:24,480 Speaker 1: where does water come from? The answer is a complicated one, 6 00:00:24,760 --> 00:00:27,480 Speaker 1: stretching way beyond the water cycle and all the way 7 00:00:27,480 --> 00:00:32,280 Speaker 1: back to the very origins of the universe. It's essential 8 00:00:32,320 --> 00:00:35,720 Speaker 1: to understand that water isn't just a liquid that happens 9 00:00:35,720 --> 00:00:38,800 Speaker 1: to cover our planet. It's a medium for pretty much 10 00:00:38,840 --> 00:00:42,280 Speaker 1: all life as we know it. A water's unique properties, 11 00:00:42,320 --> 00:00:45,720 Speaker 1: such as its ability to dissolve many substances and its 12 00:00:45,760 --> 00:00:49,080 Speaker 1: solid state being less dense than its liquid state, which 13 00:00:49,120 --> 00:00:51,720 Speaker 1: is why ice expands as it freezes and floats in 14 00:00:51,720 --> 00:00:56,920 Speaker 1: liquid water, make it invaluable. A water acts as a solvent, 15 00:00:57,080 --> 00:00:59,920 Speaker 1: a temperature regulator, and a means of transportation for new 16 00:00:59,880 --> 00:01:03,200 Speaker 1: tents and waste. And devoid of the water cycle, the 17 00:01:03,280 --> 00:01:06,520 Speaker 1: complex chain of life on Earth from microbes to mammals 18 00:01:06,720 --> 00:01:12,039 Speaker 1: would cease to exist. But let's go back, like way back. 19 00:01:12,920 --> 00:01:16,840 Speaker 1: Shortly after the Big Bang, neutrons and electrons swarmed in 20 00:01:17,040 --> 00:01:21,920 Speaker 1: ten billion degree heat within minutes, hydrogen and then helium 21 00:01:22,080 --> 00:01:25,039 Speaker 1: unknown as the lighter elements had taken shape from these 22 00:01:25,080 --> 00:01:29,720 Speaker 1: atomic building blocks in a process called nucleosynthesis. Lithium made 23 00:01:29,760 --> 00:01:32,679 Speaker 1: a cameo as well, but generally the heavier elements didn't 24 00:01:32,680 --> 00:01:36,280 Speaker 1: appear until much later, when the lighter elements underwent fusion 25 00:01:36,400 --> 00:01:41,479 Speaker 1: inside of stars and during supernova Over time, stars sent 26 00:01:41,600 --> 00:01:45,520 Speaker 1: wave after wave of these heavier elements, including oxygen, out 27 00:01:45,560 --> 00:01:50,160 Speaker 1: into space, where they mixed with the lighter elements. Of course, 28 00:01:50,360 --> 00:01:53,480 Speaker 1: the mixing of hydrogen and oxygen atoms and the subsequent 29 00:01:53,560 --> 00:01:57,720 Speaker 1: formation of water are two different things. That's because even 30 00:01:57,760 --> 00:02:01,200 Speaker 1: when hydrogen and oxygen atoms get together, they still need 31 00:02:01,240 --> 00:02:05,080 Speaker 1: a spark of energy to form water. The process is 32 00:02:05,120 --> 00:02:07,760 Speaker 1: a violent one, and so far nobody has found a 33 00:02:07,800 --> 00:02:13,240 Speaker 1: way to safely create water on Earth. So how did 34 00:02:13,240 --> 00:02:15,880 Speaker 1: our planet come to be covered with the stuff. The 35 00:02:15,960 --> 00:02:18,640 Speaker 1: simple answer is we still don't know, but we have 36 00:02:18,680 --> 00:02:22,959 Speaker 1: a few ideas. One theory states that nearly four billion 37 00:02:23,040 --> 00:02:26,960 Speaker 1: years ago, the early Solar System was overrun by millions 38 00:02:26,960 --> 00:02:30,080 Speaker 1: of asteroids and comets, which slammed into the surface of 39 00:02:30,120 --> 00:02:34,040 Speaker 1: our relatively young planet. A quick glance at the Moon's 40 00:02:34,120 --> 00:02:37,400 Speaker 1: crater pocked surface gives us an idea of what conditions 41 00:02:37,400 --> 00:02:41,280 Speaker 1: of early Earth might have been. The theory goes that 42 00:02:41,320 --> 00:02:45,320 Speaker 1: these crash landing celestial bodies weren't solid rock, but rather 43 00:02:45,480 --> 00:02:48,880 Speaker 1: the equivalent of cosmic sponges, loaded with water that was 44 00:02:48,919 --> 00:02:54,560 Speaker 1: released on impact. While astronomers have confirmed that water rich 45 00:02:54,600 --> 00:02:58,239 Speaker 1: asteroids and comets exist, some scientists think that the theory 46 00:02:58,560 --> 00:03:03,079 Speaker 1: doesn't hold water huh. They question whether enough collisions could 47 00:03:03,080 --> 00:03:08,480 Speaker 1: have taken place to account for all of Earth's water. Also, 48 00:03:08,639 --> 00:03:11,960 Speaker 1: a researchers from the California Institute of Technology found that 49 00:03:12,080 --> 00:03:15,760 Speaker 1: water from the comet hail Bop is different from normal 50 00:03:15,760 --> 00:03:19,960 Speaker 1: Earth water. Ours has the chemical formula H two OH. 51 00:03:20,560 --> 00:03:23,639 Speaker 1: It's one atom of oxygen linked together with two atoms 52 00:03:23,680 --> 00:03:27,200 Speaker 1: of the common hydrogen one isotope, which has in its 53 00:03:27,280 --> 00:03:32,080 Speaker 1: nucleus only one proton a butt. Most of the water 54 00:03:32,160 --> 00:03:35,120 Speaker 1: on the hail Bop is what's called semi heavy water, 55 00:03:35,680 --> 00:03:38,120 Speaker 1: a form of water in which there's still one atom 56 00:03:38,120 --> 00:03:41,200 Speaker 1: of oxygen, but one of the atoms of hydrogen is 57 00:03:41,280 --> 00:03:45,960 Speaker 1: a different isotope called hydrogen two or deuterium. It has 58 00:03:46,000 --> 00:03:49,840 Speaker 1: a proton and a neutron in its nucleus. The semi 59 00:03:49,840 --> 00:03:53,640 Speaker 1: heavy water's chemical formula is h DO, and its higher 60 00:03:53,680 --> 00:03:58,360 Speaker 1: mass gives it slightly different chemical and physical properties. So 61 00:03:59,080 --> 00:04:02,400 Speaker 1: either the comets asteroids that hit Earth were very different 62 00:04:02,400 --> 00:04:05,480 Speaker 1: from the hail BOP or Earth got its H two 63 00:04:05,560 --> 00:04:10,840 Speaker 1: oh some other way. More recently, astronomers may have revealed 64 00:04:10,920 --> 00:04:15,040 Speaker 1: that the former may actually be true. Using observations from 65 00:04:15,080 --> 00:04:19,480 Speaker 1: the Stratospheric Observatory for Infrared Astronomy or SOPHIA, which is 66 00:04:19,520 --> 00:04:22,120 Speaker 1: a converted seven to forty seven aircraft that flies at 67 00:04:22,200 --> 00:04:24,880 Speaker 1: high altitude with an infrared telescope sticking out of the 68 00:04:24,880 --> 00:04:28,440 Speaker 1: tail section. A researchers found that when the comet Wordinin 69 00:04:28,600 --> 00:04:31,560 Speaker 1: made its closest approach with Earth in December of twenty eighteen, 70 00:04:32,120 --> 00:04:35,440 Speaker 1: it was venting very ocean like water vapor into space. 71 00:04:37,240 --> 00:04:40,840 Speaker 1: Wordenin belongs to a specific family of comets called hyperactive 72 00:04:40,880 --> 00:04:44,040 Speaker 1: comets that vent more water vapor into space than others. 73 00:04:45,200 --> 00:04:48,479 Speaker 1: The researchers deduced that its water is ocean like by 74 00:04:48,520 --> 00:04:52,200 Speaker 1: comparing the ratio of observed H two O and HDO 75 00:04:52,720 --> 00:04:56,720 Speaker 1: in that water vapor. Earth's oceans have a very specific 76 00:04:56,800 --> 00:05:01,160 Speaker 1: ratio of those two hydrogen isotopes. And here's that wordinan 77 00:05:01,360 --> 00:05:06,120 Speaker 1: shares that same ratio as Observing infrared wavelengths from the 78 00:05:06,200 --> 00:05:10,240 Speaker 1: ground is impossible because Earth's atmosphere blocks these wavelengths. Only 79 00:05:10,279 --> 00:05:14,080 Speaker 1: space telescopes and Sophia, which flies above most of the atmosphere, 80 00:05:14,279 --> 00:05:20,039 Speaker 1: can make reliable observations of comets. Another theory states that 81 00:05:20,120 --> 00:05:23,159 Speaker 1: a young Earth was bombarded by oxygen and other heavy 82 00:05:23,160 --> 00:05:26,839 Speaker 1: elements produced within the Sun. The idea is that the 83 00:05:26,839 --> 00:05:29,960 Speaker 1: oxygen combined with hydrogen and other gases released from the 84 00:05:30,000 --> 00:05:33,800 Speaker 1: Earth itself in a process known as degassing, thus forming 85 00:05:33,839 --> 00:05:39,480 Speaker 1: Earth's oceans and atmosphere along the way. And a team 86 00:05:39,480 --> 00:05:43,040 Speaker 1: of scientists from Japan's Tokyo Institute of Technology has devised 87 00:05:43,080 --> 00:05:45,920 Speaker 1: yet another theory, which states that a thick layer of 88 00:05:46,000 --> 00:05:50,000 Speaker 1: hydrogen may have once covered Earth's surface, eventually interacting with 89 00:05:50,040 --> 00:05:55,000 Speaker 1: oxides in the crust to form our planet's oceans. Finally, 90 00:05:55,160 --> 00:05:59,359 Speaker 1: computer simulations reported on in twenty seventeen suggested a closer 91 00:05:59,400 --> 00:06:03,240 Speaker 1: origin or at least some water on our planet. This 92 00:06:03,320 --> 00:06:06,919 Speaker 1: theory states that water could develop deep inside Earth's mantle 93 00:06:07,240 --> 00:06:13,760 Speaker 1: and eventually escape via earthquakes or other geological processes. Water 94 00:06:13,839 --> 00:06:16,360 Speaker 1: is so essential to life on Earth that a lot 95 00:06:16,360 --> 00:06:19,200 Speaker 1: of research is devoted to finding it on other planets 96 00:06:19,200 --> 00:06:22,679 Speaker 1: and moons, because where we find it, we may find 97 00:06:22,760 --> 00:06:27,880 Speaker 1: alien life. However, here on our planet, a water's availability 98 00:06:28,000 --> 00:06:32,640 Speaker 1: and quality are under threat. Pollution, over extraction, and climate 99 00:06:32,720 --> 00:06:35,560 Speaker 1: change are just some of the challenges facing our planet's 100 00:06:35,600 --> 00:06:41,360 Speaker 1: water resources. Addressing these issues is not only a scientific endeavor, 101 00:06:41,400 --> 00:06:45,559 Speaker 1: but also a societal one. After all, while we can't 102 00:06:45,560 --> 00:06:48,760 Speaker 1: say with certainty how water came to Earth, we are 103 00:06:48,880 --> 00:06:56,680 Speaker 1: fortunate it did. Today's episode is based on the article 104 00:06:56,760 --> 00:06:59,640 Speaker 1: where does water come From? On howstiffworks dot com, written 105 00:06:59,640 --> 00:07:03,000 Speaker 1: by job An Adabury and Ian O'Neil. Brain Stuff is 106 00:07:03,000 --> 00:07:05,760 Speaker 1: production of iHeartRadio in partnership with ho stuffworks dot Com 107 00:07:05,760 --> 00:07:08,560 Speaker 1: and was produced by Tyler Klang. For four more podcasts 108 00:07:08,560 --> 00:07:11,880 Speaker 1: from my heart Radio, visit the iHeartRadio app, Apple Podcasts, 109 00:07:11,960 --> 00:07:13,800 Speaker 1: or wherever you listen to your favorite shows.