1 00:00:01,920 --> 00:00:04,320 Speaker 1: Welcome to brain Stuff, a production of I Heart Radio, 2 00:00:06,200 --> 00:00:10,720 Speaker 1: Hey brain Stuff Lauren Vogelbon. Here, imagine the number four. 3 00:00:11,680 --> 00:00:14,400 Speaker 1: Now imagine that it's at the head of a number 4 00:00:14,520 --> 00:00:18,720 Speaker 1: with eighty four zeros behind it. And that is the 5 00:00:18,840 --> 00:00:21,759 Speaker 1: number of photons emitted by all of the stars in 6 00:00:21,800 --> 00:00:25,640 Speaker 1: the observable universe, going back to when the now thirteen 7 00:00:25,680 --> 00:00:28,360 Speaker 1: point seven billion year old universe had been around for 8 00:00:28,520 --> 00:00:31,639 Speaker 1: just a billion years or so. And that's according to 9 00:00:31,680 --> 00:00:34,600 Speaker 1: a team of researchers headed by one Marco A. YAlO, 10 00:00:34,920 --> 00:00:38,560 Speaker 1: an astrophysicist in the College of Science at Clemson University. 11 00:00:39,080 --> 00:00:41,959 Speaker 1: It's based on an analysis of data from NASA's ten 12 00:00:42,040 --> 00:00:45,839 Speaker 1: year old Fermie Gamma Rays space telescope, which enabled the 13 00:00:45,880 --> 00:00:49,640 Speaker 1: researchers to compile a history of star formation over most 14 00:00:49,680 --> 00:00:53,159 Speaker 1: of the universe's lifetime. The scientists detailed their findings in 15 00:00:53,159 --> 00:00:57,840 Speaker 1: a paper published in eighteen in the journal Science. Measuring 16 00:00:57,880 --> 00:01:02,920 Speaker 1: starlight for most of the universe's history required considerable ingenuity 17 00:01:03,320 --> 00:01:05,480 Speaker 1: for the article. This episode is based on hows To 18 00:01:05,560 --> 00:01:09,280 Speaker 1: Forks obtained prepared remarks from a yellow via email. He 19 00:01:09,360 --> 00:01:12,320 Speaker 1: explained that the total amount of light emitted by stars 20 00:01:12,480 --> 00:01:16,520 Speaker 1: is comprised of two types. Quote. One is stellar light 21 00:01:16,640 --> 00:01:19,920 Speaker 1: that survives absorption by dust. This is what we measured. 22 00:01:20,440 --> 00:01:23,160 Speaker 1: The rest is stellar light absorbed by dust and re 23 00:01:23,240 --> 00:01:26,240 Speaker 1: emitted in the infrared. We are not sensitive to that. 24 00:01:26,680 --> 00:01:29,400 Speaker 1: It turns out half of the energy emitted by stars 25 00:01:29,440 --> 00:01:32,800 Speaker 1: across the history of the universe is reprocessed by stars. 26 00:01:32,840 --> 00:01:38,800 Speaker 1: At longer infrared wavelengths, the sky is filled with photons 27 00:01:38,840 --> 00:01:42,440 Speaker 1: emitted long ago by distant stars. This is called the 28 00:01:42,520 --> 00:01:47,000 Speaker 1: extra galactic background light, or e b L. And nevertheless, 29 00:01:47,240 --> 00:01:49,680 Speaker 1: except for the Moon and stars from our own galaxy, 30 00:01:50,080 --> 00:01:53,280 Speaker 1: the sky appears dark to our eyes according to a 31 00:01:53,400 --> 00:01:56,559 Speaker 1: yellow that's because most of the starlight that reaches Earth 32 00:01:56,600 --> 00:01:59,559 Speaker 1: from the rest of the vast universe is extremely faint, 33 00:02:00,240 --> 00:02:03,520 Speaker 1: the equivalent of a sixty watt lightbulb viewed in complete 34 00:02:03,600 --> 00:02:08,400 Speaker 1: darkness from about two point five million miles away. To 35 00:02:08,720 --> 00:02:12,119 Speaker 1: get around that problem, A. YAlO and his team perused 36 00:02:12,200 --> 00:02:15,480 Speaker 1: ten years of data from the FAMI telescope and looked 37 00:02:15,480 --> 00:02:18,280 Speaker 1: at the e b LS interaction with gamma rays emitted 38 00:02:18,320 --> 00:02:22,639 Speaker 1: by distant blazers. Blazers being black holes that can send 39 00:02:22,680 --> 00:02:27,320 Speaker 1: powerful streams of radiation out into the universe. The researchers 40 00:02:27,360 --> 00:02:30,079 Speaker 1: calculated the extent to which the gamma rays from those 41 00:02:30,080 --> 00:02:33,320 Speaker 1: blazers had been absorbed or altered by collisions with the 42 00:02:33,360 --> 00:02:38,040 Speaker 1: e b l's photons. A. Yelo describes tracking the e 43 00:02:38,160 --> 00:02:42,400 Speaker 1: b L as the astrophysicists equivalent of quote following the 44 00:02:42,520 --> 00:02:45,200 Speaker 1: rainbow and discovering a pot of gold. The e b 45 00:02:45,400 --> 00:02:48,440 Speaker 1: L is the rainbow, and its knowledge can finally disclose 46 00:02:48,600 --> 00:02:53,720 Speaker 1: a lot of useful information. The researchers technique enabled them 47 00:02:53,760 --> 00:02:56,320 Speaker 1: to see the history of star formation in the universe, 48 00:02:56,600 --> 00:02:59,560 Speaker 1: which they found had peaked about three billion years after 49 00:02:59,600 --> 00:03:04,040 Speaker 1: the Big Bang and has slowed dramatically since then. Slowed 50 00:03:04,080 --> 00:03:07,560 Speaker 1: but never completely stopped. The Milky Way, for example, creates 51 00:03:07,600 --> 00:03:12,360 Speaker 1: about seven new stars each year. A note that the 52 00:03:12,480 --> 00:03:15,680 Speaker 1: researchers count does not include the amount of starlight emitted 53 00:03:15,720 --> 00:03:19,720 Speaker 1: in the first billion years of the universe's existence. Yelo said, 54 00:03:20,160 --> 00:03:24,320 Speaker 1: this is an epoch we can't really probe yet. That's 55 00:03:24,400 --> 00:03:27,400 Speaker 1: one reason he and other scientists are looking forward to 56 00:03:27,440 --> 00:03:30,360 Speaker 1: the launch of the James Webb Space Telescope, which NASA 57 00:03:30,400 --> 00:03:33,840 Speaker 1: says will be sufficiently sensitive to detect the first stars. 58 00:03:34,480 --> 00:03:44,280 Speaker 1: It's currently set to launch on December. Today's episode is 59 00:03:44,320 --> 00:03:47,000 Speaker 1: based on the article how much starlight has been omitted 60 00:03:47,040 --> 00:03:49,440 Speaker 1: since the beginning of time on house to works dot com, 61 00:03:49,560 --> 00:03:52,360 Speaker 1: written by Patrick da Tiger Brainstuff is production of I 62 00:03:52,400 --> 00:03:54,520 Speaker 1: Heart Radio in partnership with house to works dot com, 63 00:03:54,600 --> 00:03:57,440 Speaker 1: and it's produced by Tyler Klang. For four more podcasts 64 00:03:57,440 --> 00:04:00,600 Speaker 1: from my heart Radio, visit the heart Radio app, Apple Podcasts, 65 00:04:00,720 --> 00:04:13,800 Speaker 1: or wherever you listen to your favorite shows. H