1 00:00:01,920 --> 00:00:06,640 Speaker 1: Welcome to brain Stuff production of I Heart Radio. Hey 2 00:00:06,720 --> 00:00:10,680 Speaker 1: brain Stuff, Lauren Vogelbaum here. Given the vastness of the 3 00:00:10,760 --> 00:00:13,840 Speaker 1: universe and the few short millennia that humans have been 4 00:00:13,880 --> 00:00:17,800 Speaker 1: gazing star ward, it's no surprise that we're still discovering 5 00:00:17,960 --> 00:00:21,720 Speaker 1: how things work out there. One good example of this 6 00:00:21,800 --> 00:00:25,960 Speaker 1: ongoing process is the cosmic cow, which is the unofficial 7 00:00:26,000 --> 00:00:30,080 Speaker 1: name affectionately used by astronomers to refer to a t 8 00:00:30,600 --> 00:00:35,360 Speaker 1: cow or cow an unexplained X ray phenomenon that occurred 9 00:00:35,400 --> 00:00:40,519 Speaker 1: in the name was procedurally generated. The letters ceow just 10 00:00:40,640 --> 00:00:45,440 Speaker 1: happened to come together, but it's pretty cute. Today, researchers 11 00:00:45,479 --> 00:00:48,879 Speaker 1: have a strong hypothesis to explain the cosmic cow and 12 00:00:49,000 --> 00:00:53,000 Speaker 1: guide future research into black holes, neutron stars, and other 13 00:00:53,159 --> 00:00:56,680 Speaker 1: as yet unexplained events in the farthest reaches of the universe. 14 00:00:57,640 --> 00:01:00,880 Speaker 1: To understand why the cosmic cow caut us ronomers, attention, 15 00:01:01,320 --> 00:01:05,120 Speaker 1: let's talk about the life cycle of stars, including star death. 16 00:01:06,160 --> 00:01:09,319 Speaker 1: Of course, there's a whole range of star types and sizes, 17 00:01:09,520 --> 00:01:12,440 Speaker 1: which means there's no normal way for stars to die, 18 00:01:12,800 --> 00:01:16,840 Speaker 1: and even dying isn't an accurate word, as stars simply 19 00:01:16,920 --> 00:01:21,000 Speaker 1: move from one phase of life to another. In any case, 20 00:01:21,120 --> 00:01:24,840 Speaker 1: it's broadly accurate to say that when most massive stars, 21 00:01:25,280 --> 00:01:28,240 Speaker 1: that is, stars much larger than our Sun, reached the 22 00:01:28,319 --> 00:01:30,440 Speaker 1: end of their life cycle and have consumed all of 23 00:01:30,480 --> 00:01:34,040 Speaker 1: the fuel within their cores, they explode in a supernova 24 00:01:34,400 --> 00:01:37,399 Speaker 1: and then become either a black hole or a neutron star, 25 00:01:37,560 --> 00:01:42,200 Speaker 1: but depending on the star's original size. Astronomers have been 26 00:01:42,240 --> 00:01:46,160 Speaker 1: measuring supernovas for a long time. The first possible recorded 27 00:01:46,200 --> 00:01:50,040 Speaker 1: supernova dates back to Indian astronomers records around four thousand, 28 00:01:50,160 --> 00:01:54,640 Speaker 1: five hundred BC plus remind us about a thousand years. 29 00:01:54,640 --> 00:01:57,720 Speaker 1: Since then, there have been many notable supernovas, including one 30 00:01:57,760 --> 00:02:01,200 Speaker 1: recorded by Chinese astronomers in one eight five C and 31 00:02:01,320 --> 00:02:04,800 Speaker 1: another by Johanna's Kepler and many other astronomers across the 32 00:02:04,800 --> 00:02:08,840 Speaker 1: globe in sixteen o four, plus dozens more recently, thanks 33 00:02:08,840 --> 00:02:13,920 Speaker 1: to advancements in telescope science, so astronomers generally understand what 34 00:02:13,960 --> 00:02:18,639 Speaker 1: they're seeing when a particularly bright emission appears in the sky. 35 00:02:19,480 --> 00:02:22,440 Speaker 1: That's what was so baffling about this so called cosmic 36 00:02:22,520 --> 00:02:27,720 Speaker 1: cow when astronomers first observed it in June of astronomers 37 00:02:27,800 --> 00:02:31,280 Speaker 1: using a telescope at Helic Club Observatory in Hawaii noticed 38 00:02:31,320 --> 00:02:34,640 Speaker 1: the bright X ray emission, which persisted for three weeks 39 00:02:34,840 --> 00:02:38,399 Speaker 1: and glowed ten times more brightly than supernovas that astronomers 40 00:02:38,400 --> 00:02:42,600 Speaker 1: had previously studied. Only now years later do we have 41 00:02:42,639 --> 00:02:45,079 Speaker 1: a sense of what may have caused this bright emission, 42 00:02:45,600 --> 00:02:48,160 Speaker 1: A bouncing bundle of joy for the universe in the 43 00:02:48,240 --> 00:02:51,520 Speaker 1: form of either a newborn black hole or neutron star. 44 00:02:52,760 --> 00:02:56,040 Speaker 1: Astronomers at m I T, led by research scientist dear 45 00:02:56,120 --> 00:02:59,600 Speaker 1: Rage DJ Pashum at the Covley Institute for Astrophysics and 46 00:02:59,639 --> 00:03:03,800 Speaker 1: Space Research in Cambridge, Massachusetts, studied the emissions from the 47 00:03:03,919 --> 00:03:06,959 Speaker 1: cow for several months and published their findings in the 48 00:03:07,040 --> 00:03:12,440 Speaker 1: journal Nature Astronomy in December. They determined it's likely the 49 00:03:12,520 --> 00:03:15,400 Speaker 1: result of a massive energy output caused by a black 50 00:03:15,440 --> 00:03:19,079 Speaker 1: hole or neutron star enjoying its first meal of its 51 00:03:19,080 --> 00:03:23,160 Speaker 1: origin star. Unlike other supernovas, the energy emitted by the 52 00:03:23,280 --> 00:03:27,200 Speaker 1: Cow occurred a bit differently, hence the bright, long lasting 53 00:03:27,200 --> 00:03:31,360 Speaker 1: glow observed in the sky. Given the unique data his 54 00:03:31,400 --> 00:03:34,480 Speaker 1: team was studying, Pashum admitted he was hoping that the 55 00:03:34,520 --> 00:03:37,960 Speaker 1: explanation would point to a black hole eating an exotic star. 56 00:03:38,760 --> 00:03:41,520 Speaker 1: He told Science News. I was a little bit disappointed, 57 00:03:41,680 --> 00:03:43,880 Speaker 1: but I'm more blown away that this could be direct 58 00:03:43,960 --> 00:03:46,280 Speaker 1: evidence of the birth of a black hole. This is 59 00:03:46,320 --> 00:03:49,480 Speaker 1: an even cooler result. The results of this m I 60 00:03:49,520 --> 00:03:53,320 Speaker 1: T study suggest that astrophysicists might use a similar protocol 61 00:03:53,440 --> 00:03:57,840 Speaker 1: to examine the data from other unexplained origin phenomena, for example, 62 00:03:58,080 --> 00:04:02,240 Speaker 1: fast blue optical transient phenomen enough. There are about a 63 00:04:02,240 --> 00:04:05,040 Speaker 1: dozen of these that have been recorded, and astronomers may 64 00:04:05,080 --> 00:04:07,280 Speaker 1: now be able to come up with new hypotheses to 65 00:04:07,320 --> 00:04:10,240 Speaker 1: explain these events which happened in the distant reaches of 66 00:04:10,280 --> 00:04:15,280 Speaker 1: the universe. Additionally, the cosmic cow now gives astronomers a 67 00:04:15,280 --> 00:04:17,839 Speaker 1: guide when it comes to looking for new neutron stars 68 00:04:17,920 --> 00:04:21,560 Speaker 1: and baby black holes. Studying black holes is a big 69 00:04:21,560 --> 00:04:24,520 Speaker 1: priority for NASA right now, and it's always good to 70 00:04:24,520 --> 00:04:26,680 Speaker 1: have a better idea of what to look for and 71 00:04:26,800 --> 00:04:30,880 Speaker 1: to gain a better understanding of the life cycle. If 72 00:04:31,000 --> 00:04:32,560 Speaker 1: you want to keep an eye on black holes to 73 00:04:33,200 --> 00:04:36,479 Speaker 1: look into the Imaging X ray polar Imatry Explorer, which 74 00:04:36,560 --> 00:04:41,200 Speaker 1: NASA launched in December, and the Chandra X ray Observatory. 75 00:04:41,800 --> 00:04:45,200 Speaker 1: These two space telescopes are gazing across the vast reaches 76 00:04:45,200 --> 00:04:48,120 Speaker 1: of our galaxy and universe to measure the X ray 77 00:04:48,160 --> 00:04:52,080 Speaker 1: emissions of typical black holes, though, as we're learning, there 78 00:04:52,120 --> 00:05:03,239 Speaker 1: are a typical black holes too m HM. Today's episode 79 00:05:03,240 --> 00:05:05,400 Speaker 1: is based on the article what is a Cosmic Cow? 80 00:05:05,560 --> 00:05:08,120 Speaker 1: On how stuff Works dot Com written by Valerie Stymond. 81 00:05:08,600 --> 00:05:10,760 Speaker 1: Brain Stuff is production of by Heart Radio in partnership 82 00:05:10,760 --> 00:05:12,640 Speaker 1: with how stuff Works dot Com and is produced by 83 00:05:12,640 --> 00:05:15,760 Speaker 1: Tyler Clang and Ramsay Young. Four more podcasts from my 84 00:05:15,760 --> 00:05:18,640 Speaker 1: heart Radio, visit the i heart Radio app, Apple Podcasts, 85 00:05:18,720 --> 00:05:20,520 Speaker 1: or wherever you listen to your favorite shows