1 00:00:00,120 --> 00:00:05,080 Speaker 1: This Day in History Class is a production of iHeartRadio, 2 00:00:05,800 --> 00:00:09,559 Speaker 1: Hello and Welcome to This Day in History Class, a 3 00:00:09,600 --> 00:00:13,520 Speaker 1: show that uncovers a little bit more about history every day. 4 00:00:15,280 --> 00:00:18,840 Speaker 1: I'm Gabe Lucier, and in this episode, we're talking about 5 00:00:18,840 --> 00:00:22,599 Speaker 1: one of the most widely observed comets in history and 6 00:00:22,960 --> 00:00:33,520 Speaker 1: the two armchair astronomers who spotted it first. The day 7 00:00:33,920 --> 00:00:39,400 Speaker 1: was July twenty third, nineteen ninety five. Amateur astronomers Alan 8 00:00:39,520 --> 00:00:45,199 Speaker 1: Hale and Thomas Bop independently and simultaneously discovered a comet 9 00:00:46,159 --> 00:00:50,840 Speaker 1: officially designated Comet c SLASH nineteen ninety five oh one, 10 00:00:51,320 --> 00:00:55,000 Speaker 1: it was more commonly known as Comet hail Bop in 11 00:00:55,080 --> 00:00:59,880 Speaker 1: honor of its two discoverers. Hail Bop first became visible 12 00:01:00,040 --> 00:01:03,480 Speaker 1: without a telescope in May of nineteen ninety six, and 13 00:01:03,560 --> 00:01:07,039 Speaker 1: it didn't fade from view until December of the following year. 14 00:01:07,920 --> 00:01:12,200 Speaker 1: That eighteen month long appearance was double the nine month 15 00:01:12,280 --> 00:01:16,000 Speaker 1: record previously set in eighteen eleven, and at the time 16 00:01:16,040 --> 00:01:19,600 Speaker 1: of recording, it's still the longest period of time that 17 00:01:19,680 --> 00:01:23,920 Speaker 1: a comet has ever remained visible to the naked eye. 18 00:01:24,000 --> 00:01:27,240 Speaker 1: The reason for that high visibility is that Comet hail 19 00:01:27,360 --> 00:01:31,640 Speaker 1: Bop was an unusually bright comet. In fact, it appeared 20 00:01:31,760 --> 00:01:35,720 Speaker 1: one thousand times brighter than the famous Haley's Comet had 21 00:01:35,840 --> 00:01:38,840 Speaker 1: when it streaked by at roughly the same distance in 22 00:01:38,920 --> 00:01:43,000 Speaker 1: nineteen eighty six. As for why it was so bright, 23 00:01:43,360 --> 00:01:47,919 Speaker 1: that's because of the comet's abnormally large size. The nucleus 24 00:01:47,920 --> 00:01:51,560 Speaker 1: of a comet, that is, the solid core, is typically 25 00:01:51,600 --> 00:01:56,040 Speaker 1: about one to two miles across. The nucleus of Haley's 26 00:01:56,080 --> 00:02:00,400 Speaker 1: comet was an outlier at approximately ten miles across, But 27 00:02:00,560 --> 00:02:04,520 Speaker 1: hail Bop was on a whole other level. According to NASA, 28 00:02:04,840 --> 00:02:09,920 Speaker 1: its nucleus measured about thirty seven miles in diameter. Because 29 00:02:09,919 --> 00:02:12,799 Speaker 1: of that massive surface area and the huge amount of 30 00:02:12,880 --> 00:02:16,640 Speaker 1: light it reflected, hail Bop was highly visible in our 31 00:02:16,760 --> 00:02:19,799 Speaker 1: night skies, even though it was farther from the Earth 32 00:02:19,880 --> 00:02:23,520 Speaker 1: than the Earth is from the Sun. All the comets 33 00:02:23,560 --> 00:02:26,360 Speaker 1: in our Solar System, no matter how bright they are, 34 00:02:26,680 --> 00:02:30,680 Speaker 1: come from two specific regions in space, the Kuiper Belt 35 00:02:30,880 --> 00:02:34,720 Speaker 1: and the Ort Cloud. Both are debris fields made up 36 00:02:34,720 --> 00:02:37,840 Speaker 1: of small icy bodies on the edge of our Solar System, 37 00:02:38,240 --> 00:02:41,280 Speaker 1: and on occasion, one of those icy bodies will become 38 00:02:41,320 --> 00:02:44,880 Speaker 1: dislodged and be sent hurtling on an elliptical orbit around 39 00:02:44,919 --> 00:02:49,400 Speaker 1: the Sun. These are what we call comets, large dirty 40 00:02:49,440 --> 00:02:54,000 Speaker 1: snowballs composed of densely packed ice and dust. They become 41 00:02:54,120 --> 00:02:56,960 Speaker 1: visible as they approach the Sun and begin to warm up. 42 00:02:57,440 --> 00:03:01,600 Speaker 1: The nucleus starts to evaporate, creating a hazy cloud around it, 43 00:03:01,840 --> 00:03:04,720 Speaker 1: as well as tales of gases and dusts that streak 44 00:03:04,800 --> 00:03:09,480 Speaker 1: out behind. Of the two comet producing regions, the Kuiper 45 00:03:09,520 --> 00:03:13,320 Speaker 1: Belt is significantly closer to Earth and is located between 46 00:03:13,360 --> 00:03:17,919 Speaker 1: Neptune and Pluto, so still pretty far away. The comets 47 00:03:17,960 --> 00:03:21,119 Speaker 1: that hail from here are known as short period comets, 48 00:03:21,280 --> 00:03:23,680 Speaker 1: as it takes them less than two hundred years to 49 00:03:23,720 --> 00:03:27,840 Speaker 1: make one orbit around the Sun. Haley's Comet is perhaps 50 00:03:27,880 --> 00:03:30,760 Speaker 1: the most well known in this class. It was last 51 00:03:30,800 --> 00:03:33,960 Speaker 1: seen from Earth in nineteen eighty six and is expected 52 00:03:33,960 --> 00:03:37,880 Speaker 1: to return to our view in twenty sixty one. As 53 00:03:37,920 --> 00:03:41,000 Speaker 1: you've probably worked out by now, comets that originate in 54 00:03:41,040 --> 00:03:44,760 Speaker 1: the Ort Cloud begin their journey from beyond Neptune and 55 00:03:44,840 --> 00:03:49,360 Speaker 1: are known as long period comets. Their orbits take anywhere 56 00:03:49,400 --> 00:03:53,840 Speaker 1: from several hundred to several thousand years to complete, making 57 00:03:53,880 --> 00:03:57,840 Speaker 1: their sightings a true once in a lifetime experience for humans. 58 00:03:58,880 --> 00:04:02,640 Speaker 1: Comet hail Ba is a long period comet that's believed 59 00:04:02,640 --> 00:04:06,240 Speaker 1: to have formed some four billion years ago. It's made 60 00:04:06,240 --> 00:04:09,240 Speaker 1: the trip around the Sun numerous times since then, but 61 00:04:09,320 --> 00:04:11,800 Speaker 1: it won't be seen this way again for at least 62 00:04:11,840 --> 00:04:16,400 Speaker 1: another twenty five hundred years. It's rare for a comet 63 00:04:16,440 --> 00:04:19,320 Speaker 1: to be large, close and bright enough to be seen 64 00:04:19,400 --> 00:04:23,200 Speaker 1: with the naked eye, but dimmer comets are fairly common, 65 00:04:23,440 --> 00:04:25,640 Speaker 1: and at least a few of them are discovered each year, 66 00:04:26,160 --> 00:04:31,760 Speaker 1: some by human observers, but most by automated spacecraft. Comet 67 00:04:31,800 --> 00:04:35,080 Speaker 1: hail Bop was an exception in this regard as well. 68 00:04:35,680 --> 00:04:39,080 Speaker 1: It was discovered not just by an amateur astronomer, but 69 00:04:39,120 --> 00:04:42,240 Speaker 1: by two of them. It was on a clear night 70 00:04:42,360 --> 00:04:45,719 Speaker 1: in late July of nineteen ninety five that Alan Hale 71 00:04:45,880 --> 00:04:48,840 Speaker 1: set up his personal telescope in the driveway of his 72 00:04:48,880 --> 00:04:53,320 Speaker 1: new Mexico home. He worked professionally in space research, but 73 00:04:53,520 --> 00:04:57,640 Speaker 1: comet spotting was just his late night hobby. That night, 74 00:04:57,800 --> 00:05:01,120 Speaker 1: he was planning to observe known comic that were expected 75 00:05:01,160 --> 00:05:03,880 Speaker 1: to come into view, but as he waited for them 76 00:05:03,920 --> 00:05:07,279 Speaker 1: to appear, he pointed his telescope at a globular cluster 77 00:05:07,440 --> 00:05:11,520 Speaker 1: in the Sagittarius system just to see what he could see. 78 00:05:11,600 --> 00:05:14,520 Speaker 1: To Hale's surprise, there was a fuzzy object in the 79 00:05:14,560 --> 00:05:17,080 Speaker 1: field that hadn't been there when he checked the same 80 00:05:17,120 --> 00:05:21,720 Speaker 1: location two weeks earlier. He consulted his deep sky catalogs 81 00:05:21,760 --> 00:05:24,760 Speaker 1: and star charts to make sure he wasn't mistaken, and 82 00:05:24,839 --> 00:05:28,000 Speaker 1: after confirming that he had indeed found something new, he 83 00:05:28,120 --> 00:05:32,520 Speaker 1: shot off an email to the International Astronomical Union informing 84 00:05:32,560 --> 00:05:37,200 Speaker 1: them of his discovery. Meanwhile, one stayed away in Arizona, 85 00:05:37,400 --> 00:05:40,760 Speaker 1: a factory manager named Thomas Bob had cited the comet 86 00:05:40,800 --> 00:05:45,160 Speaker 1: as well. He had spent decades observing deep sky objects 87 00:05:45,160 --> 00:05:47,839 Speaker 1: in his spare time, and on that fateful night, he 88 00:05:47,880 --> 00:05:50,560 Speaker 1: had gone out comet hunting with a group of friends. 89 00:05:51,120 --> 00:05:54,200 Speaker 1: Bob didn't actually own a telescope of his own at 90 00:05:54,240 --> 00:05:57,280 Speaker 1: the time, but as he peered into a friend's telescope, 91 00:05:57,360 --> 00:06:00,800 Speaker 1: he saw a strange, fuzzy object past into his field 92 00:06:00,800 --> 00:06:04,720 Speaker 1: of view. After having his friends verify what he had seen, 93 00:06:05,040 --> 00:06:09,120 Speaker 1: Bop also fired off a message to the IAU sharing 94 00:06:09,120 --> 00:06:12,400 Speaker 1: his observations. In the early morning of July twenty third, 95 00:06:13,400 --> 00:06:17,520 Speaker 1: the Central Bureau verified both men's finding shortly after, and 96 00:06:17,600 --> 00:06:20,599 Speaker 1: when comparing the times of the discovery, they were shocked 97 00:06:20,640 --> 00:06:23,640 Speaker 1: to find that Hale and Bop had cited the comet 98 00:06:23,720 --> 00:06:27,240 Speaker 1: at the same time. The news of the comet was 99 00:06:27,279 --> 00:06:31,640 Speaker 1: officially announced about twelve hours after its initial discovery, with 100 00:06:31,800 --> 00:06:37,040 Speaker 1: Hale and Bop sharing the credit by sheer coincidence. According 101 00:06:37,120 --> 00:06:39,960 Speaker 1: to NASA, at a distance of about six hundred and 102 00:06:40,040 --> 00:06:43,359 Speaker 1: sixty five million miles from our Sun, it was the 103 00:06:43,560 --> 00:06:48,359 Speaker 1: farthest comet ever to be discovered by amateur astronomers for 104 00:06:48,440 --> 00:06:56,080 Speaker 1: at least so far. I'm Gay, Bluesyay, and hopefully you 105 00:06:56,200 --> 00:06:59,279 Speaker 1: now know a little more about history today than you 106 00:06:59,320 --> 00:07:02,440 Speaker 1: did yesterday. If you'd like to keep up with the show, 107 00:07:02,600 --> 00:07:05,960 Speaker 1: you can follow us on Twitter, Facebook, and Instagram at 108 00:07:06,000 --> 00:07:10,600 Speaker 1: TDI HC Show, and if you have any comments or suggestions, 109 00:07:10,760 --> 00:07:13,080 Speaker 1: feel free to send them my way by writing to 110 00:07:13,160 --> 00:07:18,080 Speaker 1: this Day at iHeartMedia dot com. Thanks to Casby Bias 111 00:07:18,160 --> 00:07:20,720 Speaker 1: for producing the show, and thanks to you for listening. 112 00:07:21,080 --> 00:07:24,000 Speaker 1: I'll see you back here again tomorrow for another day 113 00:07:24,320 --> 00:07:36,160 Speaker 1: in History Class