1 00:00:00,120 --> 00:00:01,960 Speaker 1: This Day in History Class is a production of I 2 00:00:02,040 --> 00:00:07,680 Speaker 1: Heart Radio Greetings, I'm Eves and welcome to This Day 3 00:00:07,680 --> 00:00:10,600 Speaker 1: in History Class, a show that believes no day in 4 00:00:10,680 --> 00:00:25,560 Speaker 1: history is a slow day. Today is November. The day 5 00:00:25,640 --> 00:00:31,200 Speaker 1: was November. Nineteen sixty seven, Astell physicist Jocelyn Bill Burnell 6 00:00:31,360 --> 00:00:34,880 Speaker 1: became the first person to detect a radio pulsar. A 7 00:00:34,960 --> 00:00:38,800 Speaker 1: pulsar is a celestial source of pulse stating electromagnetic radiation 8 00:00:39,200 --> 00:00:42,120 Speaker 1: that is thought to be a rapidly rotating neutron star. 9 00:00:43,120 --> 00:00:47,080 Speaker 1: Pulsars amit pulses of radiation like radio waves, at short, 10 00:00:47,360 --> 00:00:52,280 Speaker 1: relatively constant intervals. In nineteen sixty seven, Jocelyn Bell was 11 00:00:52,280 --> 00:00:55,480 Speaker 1: pursuing her doctorate at the University of Cambridge, where her 12 00:00:55,520 --> 00:01:00,640 Speaker 1: advisor was radio astronomer Anthony Hewish. That year, Huish and 13 00:01:00,840 --> 00:01:04,880 Speaker 1: his graduate students completed a radio telescope that was designed 14 00:01:04,920 --> 00:01:10,440 Speaker 1: to observe the scintillation of stars, particularly quasars. A quasar 15 00:01:10,520 --> 00:01:12,640 Speaker 1: is a region at the center of a galaxy that 16 00:01:12,720 --> 00:01:16,840 Speaker 1: omits an exceptionally large amount of energy. The first quasars 17 00:01:16,840 --> 00:01:21,279 Speaker 1: were discovered by the early nineteen sixties. Bill helped build 18 00:01:21,319 --> 00:01:25,240 Speaker 1: the telescope at the Millard Radio Astronomy Observatory. Once the 19 00:01:25,240 --> 00:01:28,679 Speaker 1: telescope went into operation in July of nineteen sixty seven, 20 00:01:29,040 --> 00:01:32,199 Speaker 1: Bill began operating it and analyzing the data by hand. 21 00:01:33,360 --> 00:01:36,520 Speaker 1: One day, she noticed a strange signal at a wavelength 22 00:01:36,640 --> 00:01:40,040 Speaker 1: of three point seven meters. The signal continued to appear 23 00:01:40,120 --> 00:01:44,520 Speaker 1: over the next several months. On November, she captured a 24 00:01:44,560 --> 00:01:48,160 Speaker 1: recording of the signal that gave more detail. Bill called 25 00:01:48,200 --> 00:01:50,760 Speaker 1: the reading a quote bit of scruff in the data. 26 00:01:51,920 --> 00:01:54,440 Speaker 1: It showed that the signal corresponded to a burst of 27 00:01:54,560 --> 00:01:57,880 Speaker 1: radio energy that came in regular intervals of about one 28 00:01:57,920 --> 00:02:01,680 Speaker 1: point three seconds. The re was sinked with sidereal time 29 00:02:01,800 --> 00:02:04,960 Speaker 1: rather than Earth time, and it consistently came from the 30 00:02:05,000 --> 00:02:08,640 Speaker 1: same part of the sky. So she set about determining 31 00:02:08,680 --> 00:02:11,440 Speaker 1: the source of the signal. It couldn't be coming from 32 00:02:11,480 --> 00:02:15,840 Speaker 1: any natural sources like stars, galaxies, or solar wind, and 33 00:02:15,919 --> 00:02:18,280 Speaker 1: it did not come from any human or human made 34 00:02:18,320 --> 00:02:22,639 Speaker 1: sources like radar reflected off the Moon, other radio astronomers, 35 00:02:22,760 --> 00:02:28,360 Speaker 1: television signals orbiting satellites, or buildings near the telescope. After 36 00:02:28,440 --> 00:02:31,359 Speaker 1: ruling out all those sources, she and Huish called the 37 00:02:31,400 --> 00:02:34,519 Speaker 1: signal l g M one because they couldn't rule out 38 00:02:34,680 --> 00:02:38,760 Speaker 1: little green men a k a. Aliens, But soon Bill 39 00:02:38,840 --> 00:02:41,600 Speaker 1: found another signal, this one pulsing at one point to 40 00:02:41,800 --> 00:02:45,200 Speaker 1: second intervals. This signal was coming from a different part 41 00:02:45,200 --> 00:02:48,280 Speaker 1: of the sky. That meant that the signal was likely 42 00:02:48,360 --> 00:02:53,200 Speaker 1: not sent by extraterrestrial beings. Later that year, Bill noticed 43 00:02:53,240 --> 00:02:56,760 Speaker 1: a couple more of these unusual signals. In January nineteen 44 00:02:56,880 --> 00:03:01,160 Speaker 1: sixty eight, Bell Hwish in colleagues submitted paper describing their 45 00:03:01,160 --> 00:03:05,760 Speaker 1: discovery to the journal Nature, and the paper, Observation of 46 00:03:05,800 --> 00:03:11,640 Speaker 1: a Rapidly Pulsating Radio Source was published on February. The 47 00:03:11,680 --> 00:03:15,280 Speaker 1: paper noted that they had recorded unusual signals from pulsating 48 00:03:15,360 --> 00:03:19,480 Speaker 1: radio sources and positive that the radiation may be associated 49 00:03:19,480 --> 00:03:24,040 Speaker 1: with oscillations of white dwarf or neutron stars. But even 50 00:03:24,120 --> 00:03:27,080 Speaker 1: though they had announced the discovery, they still didn't know 51 00:03:27,160 --> 00:03:31,200 Speaker 1: the source of the signal. That didn't stop other scientists 52 00:03:31,280 --> 00:03:34,560 Speaker 1: from trying to discover more of these pulsating sources and 53 00:03:34,600 --> 00:03:37,280 Speaker 1: where they were coming from. By the end of nineteen 54 00:03:37,360 --> 00:03:40,200 Speaker 1: sixty eight, more had been discovered, and it had been 55 00:03:40,240 --> 00:03:45,080 Speaker 1: suggested that neutron stars were a source. Hewish first used 56 00:03:45,120 --> 00:03:48,000 Speaker 1: the word pulsar in an interview with the Daily Telegraph. 57 00:03:48,080 --> 00:03:52,200 Speaker 1: In nineteen sixty, Bell and Hwish changed the name of 58 00:03:52,200 --> 00:03:55,760 Speaker 1: the signal from l g M to CP or Cambridge Pulsar, 59 00:03:56,120 --> 00:03:59,160 Speaker 1: and the first radio pulsar they detected was dubbed CP. 60 00:03:59,440 --> 00:04:04,040 Speaker 1: Nineteen eighteen, he was received the nineteen seventy four Nobel 61 00:04:04,120 --> 00:04:07,360 Speaker 1: Prize in Physics for his role in the discovery of pulsars, 62 00:04:07,800 --> 00:04:13,400 Speaker 1: a controversial decision because Bill's contributions were not recognized. Since 63 00:04:13,400 --> 00:04:16,640 Speaker 1: their discovery, pulsars have been used to study extreme states 64 00:04:16,720 --> 00:04:21,840 Speaker 1: of matter and search for gravitational waves. I'm Eve Jeffcote, 65 00:04:21,880 --> 00:04:24,320 Speaker 1: and hopefully you know a little more about history today 66 00:04:24,360 --> 00:04:28,120 Speaker 1: than you did yesterday. Send your best history memes to 67 00:04:28,240 --> 00:04:34,039 Speaker 1: us at t d I h B Podcast on Facebook, Instagram, 68 00:04:34,080 --> 00:04:38,000 Speaker 1: and Twitter. Email still works. Send us a note at 69 00:04:38,040 --> 00:04:41,320 Speaker 1: this day at i heeart media dot com. Thanks for 70 00:04:41,400 --> 00:04:51,240 Speaker 1: listening and we'll see you tomorrow. For more podcasts from 71 00:04:51,279 --> 00:04:54,080 Speaker 1: I Heart Radio, visit the iHeart Radio app, Apple Podcasts, 72 00:04:54,160 --> 00:04:55,839 Speaker 1: or wherever you listen to your favorite shows.