1 00:00:20,153 --> 00:00:21,654 So, what are zombie stars? 2 00:00:21,654 --> 00:00:23,223 This is kind of a nickname 3 00:00:23,223 --> 00:00:26,359 that we're giving the white dwarf in this particular system. 4 00:00:26,559 --> 00:00:28,495 So you can think of a white dwarf as a star 5 00:00:28,495 --> 00:00:30,263 that's kind of reached the end of its life. 6 00:00:30,263 --> 00:00:32,999 So you can think about that as it's like a zombie. 7 00:00:32,999 --> 00:00:35,635 And then what happens is it 8 00:00:35,635 --> 00:00:38,605 grabs material from the secondary star nearby, 9 00:00:38,605 --> 00:00:41,307 and that goes on the surface of the white dwarf. 10 00:00:41,307 --> 00:00:43,343 And then we have the explosion within that material. 11 00:00:43,343 --> 00:00:44,544 And that's the nova outburst. 12 00:00:44,544 --> 00:00:49,115 You can think about the zombie being reinvigorated and being much more active. 13 00:00:49,382 --> 00:00:52,385 And then after a while, when it doesn't get to eat anything, 14 00:00:52,719 --> 00:00:54,587 it goes a lot quiet again. 15 00:00:54,587 --> 00:00:56,656 And then with this particular system, in eight years, it 16 00:00:56,656 --> 00:00:59,692 will eat some more material and become re-energized again. 17 00:00:59,692 --> 00:01:01,261 So when we think about, 18 00:01:01,261 --> 00:01:04,431 Taco Bell and the White Dwarf, we give it the nickname of a zombie, 19 00:01:15,775 --> 00:01:18,578 So why are we interested in this particular system? 20 00:01:18,578 --> 00:01:21,714 Well, this is, only 3000 light years away, 21 00:01:22,015 --> 00:01:24,517 and the outburst is going to be particularly bright. 22 00:01:24,517 --> 00:01:29,789 It's going to be comparative to Polaris, which is, about about second magnitude. 23 00:01:30,056 --> 00:01:33,093 And so we're gonna be able to view it very well, and we're gonna be able 24 00:01:33,093 --> 00:01:36,596 to do that now with a bunch of different, telescopes and facilities. 25 00:01:36,596 --> 00:01:39,566 So we haven't really, used before on this object. 26 00:01:51,010 --> 00:01:54,781 So originally, scientists thought that this star was going to explode 27 00:01:54,781 --> 00:01:55,949 by September. 28 00:01:55,949 --> 00:01:59,385 Now, this is what we call a recurrent nova system. 29 00:01:59,385 --> 00:02:03,056 So what I mean by that is that it has to have an outburst. 30 00:02:03,123 --> 00:02:05,859 So that's when the material is ejected from the surface, 31 00:02:05,859 --> 00:02:07,727 the white dwarf from that explosion. 32 00:02:07,727 --> 00:02:11,197 And then what would happen is after all that matter was, you know, 33 00:02:11,197 --> 00:02:15,368 after that's been flung out, it will grab more material 34 00:02:15,368 --> 00:02:16,903 from the secondary star 35 00:02:16,903 --> 00:02:20,440 and then build up again, and then I'll have another eruption, another outburst, 36 00:02:20,440 --> 00:02:21,441 and that we'll see in the sky. 37 00:02:21,441 --> 00:02:23,143 Now, for this object. 38 00:02:23,143 --> 00:02:26,179 This happens every 80 years or so. 39 00:02:26,479 --> 00:02:31,017 So I believe the first record of this happening was in 1217. 40 00:02:31,551 --> 00:02:36,556 And then the last outburst that we saw here on earth was in 1946. 41 00:02:36,923 --> 00:02:39,759 And we kind of have seen as astronomers 42 00:02:39,759 --> 00:02:42,896 that this seems to have happened every 80 years or so. 43 00:02:43,363 --> 00:02:48,368 And previously before the outburst, we tended to see this kind of behavior 44 00:02:48,368 --> 00:02:51,771 where it's decreased in brightness very slowly. 45 00:02:52,071 --> 00:02:55,041 And then once we started to see that slight decrease in brightness. 46 00:02:55,175 --> 00:02:58,912 But a year or so later, we saw the outburst, the big eruption. 47 00:02:59,312 --> 00:03:01,614 Now this decrease in brightness started happening. 48 00:03:01,614 --> 00:03:05,285 Can't remember the top of my head, but it seemed to indicate that 49 00:03:05,685 --> 00:03:10,223 the next eruption should happen, before September of this year. 50 00:03:10,557 --> 00:03:13,560 Now we've already gone past September and it hasn't happened yet. 51 00:03:13,693 --> 00:03:16,062 But that's because this is kind of unpredictable science. 52 00:03:16,062 --> 00:03:18,998 You know, it might be it will happen before the end of the year. 53 00:03:18,998 --> 00:03:20,533 It might actually happen next year. 54 00:03:20,533 --> 00:03:22,502 It's all really an estimate. And it keeps us, 55 00:03:24,470 --> 00:03:25,972 second guessing what we see. 56 00:03:25,972 --> 00:03:28,575 So we'll see some trend, but it might not happen. 57 00:03:28,575 --> 00:03:31,744 And if it doesn't happen by next year, that also gives us some other 58 00:03:32,078 --> 00:03:34,547 interesting information about the system as well. 59 00:03:34,547 --> 00:03:36,649 So either way, we'll find out something really interesting 60 00:03:36,649 --> 00:03:38,952 about what's going on in the system, whether we see an outburst 61 00:03:38,952 --> 00:03:41,955 in the next few months or maybe later on next year. 62 00:03:53,800 --> 00:03:54,334 So this, 63 00:03:54,334 --> 00:03:57,337 Nova event happens about every 80 years. 64 00:03:57,403 --> 00:04:02,041 And it is only 3000 light years away from us in the Northern Crown constellation. 65 00:04:02,575 --> 00:04:04,410 And because it's so close 66 00:04:04,410 --> 00:04:08,047 and because it gets so bright, we can learn a lot from this system. 67 00:04:08,047 --> 00:04:13,987 But also most importantly is since 1946, we actually have new facilities, 68 00:04:13,987 --> 00:04:17,257 which will observe x rays and gamma rays, 69 00:04:17,490 --> 00:04:21,194 and we can coordinate all of our observations together on this object. 70 00:04:21,227 --> 00:04:22,996 So we're going to really understand the physics 71 00:04:22,996 --> 00:04:24,897 of what's happening in the explosion. 72 00:04:24,897 --> 00:04:28,801 Get a better understanding of the dynamics between the two stars, and learn 73 00:04:28,801 --> 00:04:31,170 about the composition of the stars themselves. 74 00:04:42,849 --> 00:04:43,783 So how can you 75 00:04:43,783 --> 00:04:46,886 see this, new star when it does go nova? 76 00:04:46,886 --> 00:04:48,688 And what can you do to prepare? 77 00:04:48,688 --> 00:04:53,293 So essentially, this, Nova, this bright, this new star is going to happen 78 00:04:53,293 --> 00:04:57,864 in the Northern Crown constellation or Corona Borealis, and that's near Hercules. 79 00:04:58,197 --> 00:05:00,600 And the way in which we'll be able to view it. 80 00:05:00,600 --> 00:05:04,370 Well, if you have, a dark night sky, you'll see a, 81 00:05:04,570 --> 00:05:08,074 brighter star in that constellation, and it's going to be 82 00:05:08,074 --> 00:05:11,711 comparatively bright to Polaris, which is a second magnitude star. 83 00:05:12,145 --> 00:05:14,881 Additionally, what you can do if you don't have dark Sky 84 00:05:14,881 --> 00:05:18,751 is you can also, you know, use various apps on your phone like Sky view 85 00:05:18,751 --> 00:05:22,055 or to make sure you know what that, where that region is 86 00:05:22,055 --> 00:05:25,058 and also when you found it, know what it should look like. 87 00:05:25,191 --> 00:05:29,395 And then when it goes into the outburst, you'll see that slightly brighter 88 00:05:29,529 --> 00:05:30,697 star in that region. 89 00:05:30,697 --> 00:05:34,067 You're not going to see a huge explosion in space, obviously, but you will see 90 00:05:34,067 --> 00:05:37,537 a slight brightening of a star in that constellation. 91 00:05:47,914 --> 00:05:49,515 So what am I most excited about? 92 00:05:49,515 --> 00:05:50,683 This event? 93 00:05:50,683 --> 00:05:53,086 This is something that I'm never going to get to go see. 94 00:05:53,086 --> 00:05:56,622 And once it's, really is every 80 years or so. 95 00:05:57,156 --> 00:06:00,493 And I think for this event, because we're going to have so 96 00:06:00,493 --> 00:06:04,197 many facilities observing it, we're going to learn so much more 97 00:06:04,197 --> 00:06:07,200 about what's happening and the physics in the system. 98 00:06:07,500 --> 00:06:11,404 And I like to think of novae as mini laboratories 99 00:06:11,404 --> 00:06:14,874 for other more, energetic events. 100 00:06:15,208 --> 00:06:19,212 So now we really help us to understand the physics that are going on 101 00:06:19,212 --> 00:06:22,715 in these binary systems and what we call accretion. 102 00:06:22,715 --> 00:06:27,120 So the way in which we grab material from one star and put it onto another. 103 00:06:27,453 --> 00:06:30,356 They really help us understand that process, 104 00:06:30,356 --> 00:06:33,693 and they can help us to understand it on a bigger scale as well. 105 00:06:33,726 --> 00:06:36,729 So I'm really excited about the new physics that we're going to learn 106 00:06:36,729 --> 00:06:39,065 with all these amazing facilities that we now have. 107 00:06:50,410 --> 00:06:52,445 So will our star. 108 00:06:52,445 --> 00:06:56,215 Our sun ends up like this system will have the same fate. 109 00:06:56,249 --> 00:06:57,950 The answer is no. 110 00:06:57,950 --> 00:07:01,254 All star is a, a star in isolation. 111 00:07:01,721 --> 00:07:03,956 And it doesn't have that secondary companion 112 00:07:03,956 --> 00:07:05,658 from which you can steal material. 113 00:07:05,658 --> 00:07:07,460 So it could have a Nova event. 114 00:07:07,460 --> 00:07:10,830 So eventually Asan is going to become a white dwarf, 115 00:07:11,097 --> 00:07:14,100 and it will spend the rest of his time just cooling down. 116 00:07:24,444 --> 00:07:26,446 So the last time that this nova went into 117 00:07:26,446 --> 00:07:29,749 eruption was in 1946, and we didn't some have 118 00:07:29,749 --> 00:07:32,752 some of the facilities that we now have today with NASA. 119 00:07:32,819 --> 00:07:38,424 Essentially we can use facilities like Fermi and Sby and James 120 00:07:38,424 --> 00:07:44,297 Webb and Hubble to do a multi wavelength, campaign on this object. 121 00:07:44,297 --> 00:07:46,632 We can observe it in the visible. 122 00:07:46,632 --> 00:07:48,501 So what you view with your eyes, 123 00:07:48,501 --> 00:07:52,705 but we can observe it with gamma ray detectors and x ray detectors. 124 00:07:52,905 --> 00:07:56,776 And this is really important to gain a full understanding of the system itself. 125 00:07:56,776 --> 00:08:01,881 So the composition of things, the, the accretion processes that's dragging 126 00:08:01,881 --> 00:08:05,785 material from one star on to another and the explosion mechanism itself. 127 00:08:17,864 --> 00:08:20,666 so what is the difference between a nova and a supernova? 128 00:08:20,666 --> 00:08:22,201 Well, a nova system. 129 00:08:22,201 --> 00:08:23,870 And that could happen multiple times 130 00:08:23,870 --> 00:08:27,139 because the system isn't destroyed once the explosion happens. 131 00:08:27,306 --> 00:08:31,978 It's just an explosion on the surface of the white dwarf in a supernova system. 132 00:08:32,245 --> 00:08:34,113 Well, the the system is destroyed. 133 00:08:34,113 --> 00:08:36,616 That white dwarf is destroyed in the explosion. 134 00:08:36,616 --> 00:08:39,185 And you cannot have a recurrence happen again. 135 00:08:39,185 --> 00:08:41,153 A supernova event is much more energetic. 136 00:08:41,153 --> 00:08:44,156 And a one time thing 137 00:08:52,832 --> 00:08:53,399 So why are 138 00:08:53,399 --> 00:08:56,702 nova important and what role do they play in solar system development? 139 00:08:57,069 --> 00:09:01,607 Well, Nova are actually quite frequent events in our galaxy. 140 00:09:01,607 --> 00:09:03,042 And another galaxies. 141 00:09:03,042 --> 00:09:05,978 And by observing them we can get a lot of insight 142 00:09:05,978 --> 00:09:08,981 into other, other, energetic events. 143 00:09:09,148 --> 00:09:14,120 They also produce a lot of lithium, which is really important for, our galaxy. 144 00:09:14,120 --> 00:09:17,089 And, you know, having what we call heavier elements. 145 00:09:17,189 --> 00:09:20,359 So novae are frequent, bright. 146 00:09:20,593 --> 00:09:24,564 And we can also, observe them from the ground in some cases, 147 00:09:24,564 --> 00:09:25,998 which makes them even more exciting. 148 00:09:37,343 --> 00:09:39,078 so what are scientists doing 149 00:09:39,078 --> 00:09:42,515 to observe the system and getting prepared for its explosion? 150 00:09:43,015 --> 00:09:47,186 Well, there are several telescopes, I believe, which are still observing. 151 00:09:47,186 --> 00:09:50,189 It's to check when it will go into outburst. 152 00:09:50,222 --> 00:09:54,493 But typically we get a lot of information from, the amateur astronomer communities 153 00:09:54,627 --> 00:09:59,599 who tend to focus on a region in the night sky and then send out alerts 154 00:09:59,599 --> 00:10:02,868 the broader community to let us know that this event has been happening. 155 00:10:02,868 --> 00:10:07,006 That's how, actually, a lot of novae have been detected in the past. 156 00:10:07,406 --> 00:10:10,409 And so when one of those alerts are sent out to the community, 157 00:10:10,509 --> 00:10:14,614 everybody else will jump on board and start observing with their own facilities 158 00:10:14,614 --> 00:10:16,616 and with the space based facilities as well.