1 00:00:00,280 --> 00:00:02,960 Speaker 1: Brought to you by the reinvented two thousand twelve Camray. 2 00:00:03,160 --> 00:00:08,920 Speaker 1: It's ready. Are you get in touch with technology? With 3 00:00:09,000 --> 00:00:17,840 Speaker 1: tech Stuff from how stuff works dot com. Hello again, everyone, 4 00:00:17,880 --> 00:00:20,320 Speaker 1: Welcome to tech Stuff. My name is Chris Poulett, and 5 00:00:20,320 --> 00:00:22,400 Speaker 1: I'm an editor at how stuff works dot com. Sitting 6 00:00:22,400 --> 00:00:25,239 Speaker 1: across from me as usual, its senior writer Jonathan Strickland. 7 00:00:25,360 --> 00:00:28,080 Speaker 1: All my bags are packed, I'm ready to go. I'm 8 00:00:28,120 --> 00:00:30,760 Speaker 1: standing here outside your door. I hate to wake you 9 00:00:30,840 --> 00:00:38,040 Speaker 1: up to say goodbye. Okay, clearly you have been seen Armagedon. Yeah, 10 00:00:38,080 --> 00:00:40,199 Speaker 1: I have. I just tried to put it out of 11 00:00:40,240 --> 00:00:43,360 Speaker 1: my head that that song's in it. And we're gonna 12 00:00:43,400 --> 00:00:47,680 Speaker 1: be talking about asteroids and preventing a collision with Earth 13 00:00:47,720 --> 00:00:49,839 Speaker 1: and what sort of tech would be involved with that. 14 00:00:50,159 --> 00:00:54,440 Speaker 1: And this comes courtesy of some Facebook requests and email requests. 15 00:00:54,480 --> 00:00:57,080 Speaker 1: I can't believe that we had people send us multiple 16 00:00:57,080 --> 00:01:01,360 Speaker 1: people sent us this request, which seems really specific for 17 00:01:01,600 --> 00:01:04,440 Speaker 1: more than one person. But hey, we're gonna do it. 18 00:01:05,760 --> 00:01:09,760 Speaker 1: And um, you know, if you have seen the documentary Armagedon, 19 00:01:10,560 --> 00:01:13,440 Speaker 1: you remember that we shot Bruce Willis up into space 20 00:01:14,040 --> 00:01:16,560 Speaker 1: um with Ben Affleck and some other folks like Steve 21 00:01:16,600 --> 00:01:19,880 Speaker 1: Bussemmy to scare an asteroid out of the way, because 22 00:01:19,920 --> 00:01:22,959 Speaker 1: Steve Bussummey is a scary guy. Uh wait, I think 23 00:01:22,959 --> 00:01:24,520 Speaker 1: I might be. I think I might be a little 24 00:01:24,560 --> 00:01:26,759 Speaker 1: off track. Oh well, anyway, the premise of the movie 25 00:01:26,840 --> 00:01:29,560 Speaker 1: was that there was this enormous asteroid the size of Texas, 26 00:01:29,800 --> 00:01:36,360 Speaker 1: which put the way, not that guy, do you do? Yeah? 27 00:01:36,440 --> 00:01:39,920 Speaker 1: That that's that's a reference that goes over everyone's head 28 00:01:40,040 --> 00:01:42,720 Speaker 1: because no one, none of our listeners have ever played 29 00:01:42,760 --> 00:01:46,160 Speaker 1: the game Asteroids. Any really, some of you have played 30 00:01:46,160 --> 00:01:51,160 Speaker 1: Asteroids and maybe maybe, uh maybe our our buddy Floyd 31 00:01:51,200 --> 00:01:54,240 Speaker 1: the truck driver, he might have hopefully not while driving. 32 00:01:54,440 --> 00:01:57,240 Speaker 1: Well I hope not. Anyway, we're getting off track already. 33 00:01:57,320 --> 00:02:00,120 Speaker 1: So the whole, the whole premise of the movie is 34 00:02:00,120 --> 00:02:02,360 Speaker 1: that there's this giant asteroid the size of Texas that's 35 00:02:02,360 --> 00:02:04,760 Speaker 1: going to be flying at Earth. And so they come 36 00:02:04,840 --> 00:02:07,880 Speaker 1: up with this idea where they scramble a bunch of 37 00:02:07,440 --> 00:02:13,000 Speaker 1: of uh minors essentially to shoot up into space, land 38 00:02:13,040 --> 00:02:16,360 Speaker 1: on the asteroid, and plant a nuclear device on the 39 00:02:16,400 --> 00:02:19,440 Speaker 1: asteroid that will blow it up to tiny little bits 40 00:02:19,480 --> 00:02:22,600 Speaker 1: and save the Earth. And so we want to address 41 00:02:22,720 --> 00:02:25,760 Speaker 1: this um this first, so let's let's get this all 42 00:02:25,800 --> 00:02:28,639 Speaker 1: the way. That would not work. That would that would 43 00:02:28,680 --> 00:02:32,600 Speaker 1: be a bad thing. First of all, the power of 44 00:02:32,639 --> 00:02:36,240 Speaker 1: such a device is hard to imagine. How would you 45 00:02:36,280 --> 00:02:40,800 Speaker 1: create a nuclear device powerful enough to explode texas into 46 00:02:40,840 --> 00:02:45,040 Speaker 1: tiny bits the equivalent of texas flying at you. Also, 47 00:02:45,080 --> 00:02:48,480 Speaker 1: by the way, an asteroid that size would pretty much 48 00:02:48,480 --> 00:02:52,079 Speaker 1: wipe out everybody. Um. You know, when we talk about 49 00:02:52,120 --> 00:02:55,680 Speaker 1: asteroids that are are dangerous enough to wipe out a city, 50 00:02:56,040 --> 00:02:59,880 Speaker 1: fifty yards is big enough. A fifty yard asteroid like 51 00:03:00,080 --> 00:03:05,760 Speaker 1: asteroid fifty yards across, we have enough power, enough enough 52 00:03:05,800 --> 00:03:10,000 Speaker 1: force to destroy a city if it impacted the city. Um. Now, 53 00:03:10,360 --> 00:03:15,360 Speaker 1: NASA classifies earth threatening asteroids as being a hundred and 54 00:03:15,400 --> 00:03:19,120 Speaker 1: forty meters or larger. But then that conveniently is about 55 00:03:19,120 --> 00:03:24,080 Speaker 1: the size that we can detect them. Well, it's uh, 56 00:03:24,200 --> 00:03:27,120 Speaker 1: it's important to note too that it's happened before. You know, 57 00:03:27,200 --> 00:03:30,920 Speaker 1: we have been hit with with many space objects in 58 00:03:30,960 --> 00:03:36,240 Speaker 1: the past, and I assume to some small degree continue 59 00:03:36,280 --> 00:03:38,800 Speaker 1: to do so, like something that we hear about in 60 00:03:38,800 --> 00:03:41,320 Speaker 1: the news every day, But every single day the Earth 61 00:03:41,440 --> 00:03:46,480 Speaker 1: is hit by by tiny little object. Granted we haven't 62 00:03:46,480 --> 00:03:49,400 Speaker 1: been hit by a massive asteroid in a really long time. 63 00:03:49,480 --> 00:03:52,920 Speaker 1: But meteorites hit the Earth every day. Sometimes they're so 64 00:03:52,960 --> 00:03:56,440 Speaker 1: small that you know, they're almost undetectable, but it does 65 00:03:56,560 --> 00:04:00,160 Speaker 1: happen the But yeah, they've happened in the past. I mean, 66 00:04:00,920 --> 00:04:04,560 Speaker 1: that's what wiped out the dinosaurs was an asteroid impact 67 00:04:04,720 --> 00:04:08,320 Speaker 1: or possibly common impact, but it was a massive impact 68 00:04:08,360 --> 00:04:11,520 Speaker 1: that that altered the Earth's climate, and dinosaurs did not 69 00:04:11,600 --> 00:04:16,120 Speaker 1: have air conditioning, so they were pretty much doomed. Doomed. 70 00:04:16,680 --> 00:04:21,120 Speaker 1: I figured it was their debaucherous lifestyle and it was unsustainable. 71 00:04:21,200 --> 00:04:24,240 Speaker 1: Now you're thinking of Rome, right, you know, I get 72 00:04:24,279 --> 00:04:26,280 Speaker 1: this confused a lot. Yeah, well, you know, if you've 73 00:04:26,279 --> 00:04:30,040 Speaker 1: ever seen a t rex in Atoga never mind, So 74 00:04:30,560 --> 00:04:34,680 Speaker 1: so why would this plan not work with destroying an 75 00:04:34,760 --> 00:04:38,200 Speaker 1: asteroid with a nuclear device. Let's assume that, for for 76 00:04:38,360 --> 00:04:43,040 Speaker 1: argument's sake, that somehow you managed to find a nuclear 77 00:04:43,080 --> 00:04:48,000 Speaker 1: device capable of breaking up a Texas sized asteroid while 78 00:04:48,000 --> 00:04:49,920 Speaker 1: it was hurtling towards Earth. And keep in mind this 79 00:04:49,960 --> 00:04:53,039 Speaker 1: was this this asteroid was close to Earth by the 80 00:04:53,080 --> 00:04:56,320 Speaker 1: time it blows up. Otherwise it's not nearly as dramatic 81 00:04:56,360 --> 00:04:58,560 Speaker 1: an ending. Right, of course, you've gotta have it close 82 00:04:58,640 --> 00:05:00,800 Speaker 1: enough to the Earth where people are starting really freak out. 83 00:05:01,080 --> 00:05:03,440 Speaker 1: Oh and how long exactly did they have to prepare 84 00:05:03,480 --> 00:05:05,520 Speaker 1: for this. It was like a couple of days or 85 00:05:05,560 --> 00:05:08,440 Speaker 1: something like that. It was crazy short time period. We 86 00:05:08,480 --> 00:05:12,200 Speaker 1: would know. Yeah, anything that's anything that that size, we 87 00:05:12,240 --> 00:05:15,400 Speaker 1: would be able to spot between Mars and Jupiter, giving 88 00:05:15,480 --> 00:05:19,520 Speaker 1: us years, literally years to prepare. It would not be 89 00:05:19,600 --> 00:05:21,719 Speaker 1: a last minute thing. And um, that's one of the 90 00:05:21,760 --> 00:05:24,560 Speaker 1: myths that movies perpetuate is that you know, you have 91 00:05:24,720 --> 00:05:28,840 Speaker 1: some uh, some some amateur astronomer out in the middle 92 00:05:28,880 --> 00:05:31,120 Speaker 1: of nowhere just looking up and saying, that's weird that 93 00:05:31,160 --> 00:05:35,160 Speaker 1: star wasn't there yesterday. And then and then that information 94 00:05:35,360 --> 00:05:38,480 Speaker 1: slowly filters its way to some official source, which immediately 95 00:05:38,480 --> 00:05:41,640 Speaker 1: clamps down and keeps it all secret so that nobody 96 00:05:41,720 --> 00:05:44,160 Speaker 1: knows that doom is on the way until it leaks 97 00:05:44,160 --> 00:05:46,520 Speaker 1: to the media causing a panic. Yeah, that we don't 98 00:05:46,560 --> 00:05:49,599 Speaker 1: want to cause a panic. That's definitely Hollywood related. So 99 00:05:49,839 --> 00:05:52,840 Speaker 1: why would blowing up the asteroid not be a good idea? Well, 100 00:05:53,520 --> 00:05:56,000 Speaker 1: that asteroids moving at a really fast speed and the 101 00:05:56,080 --> 00:05:58,920 Speaker 1: nuclear warhead is not going to slow it down. Okay, 102 00:05:58,920 --> 00:06:01,760 Speaker 1: so you've still got this this material moving at an 103 00:06:01,800 --> 00:06:06,479 Speaker 1: incredible speed, and the mass isn't gone. You haven't destroyed 104 00:06:06,480 --> 00:06:09,240 Speaker 1: the mass, You've just spread it out some So instead 105 00:06:09,240 --> 00:06:12,320 Speaker 1: of it being a one massive asteroid hitting the Earth, 106 00:06:12,360 --> 00:06:15,080 Speaker 1: it's a whole bunch of them hitting the Earth. And 107 00:06:15,120 --> 00:06:18,799 Speaker 1: it's like the difference between getting hit by a slug 108 00:06:18,880 --> 00:06:23,120 Speaker 1: and getting hit by um shotgun shot. You know, you 109 00:06:23,279 --> 00:06:26,320 Speaker 1: just spread out the area of impact, is what you've done. 110 00:06:26,920 --> 00:06:30,800 Speaker 1: This is mission control. We just wanted to say, Oops, yeah, 111 00:06:30,960 --> 00:06:34,719 Speaker 1: are bad so um so yeah, here's here's while this 112 00:06:34,760 --> 00:06:37,560 Speaker 1: stuff would really work in the real world. All Right, 113 00:06:37,720 --> 00:06:41,679 Speaker 1: We've got lots of powerful telescopes pointing in all sorts 114 00:06:41,680 --> 00:06:44,560 Speaker 1: of directions. Now, so the the the myths of the 115 00:06:44,600 --> 00:06:48,680 Speaker 1: amateur astronomer who detects uh something the size the size 116 00:06:48,680 --> 00:06:52,320 Speaker 1: that's in depicted an armageddon is really that's that's busted 117 00:06:52,680 --> 00:06:55,640 Speaker 1: because it would be detected by much more powerful telescopes 118 00:06:55,760 --> 00:07:01,080 Speaker 1: much earlier, and um that information would go to uh 119 00:07:01,200 --> 00:07:05,280 Speaker 1: it's kind of a clearing house for near Earth objects 120 00:07:05,320 --> 00:07:09,960 Speaker 1: that could potentially cause harm. It's called the Minor Planet Center. 121 00:07:10,440 --> 00:07:14,960 Speaker 1: It's in Cambridge, Massachusetts. Now, the Minor Planet Center would 122 00:07:14,960 --> 00:07:17,800 Speaker 1: then take the information that was sent to it, which 123 00:07:17,880 --> 00:07:21,480 Speaker 1: usually would involve the size of the asteroid and it's 124 00:07:21,480 --> 00:07:24,480 Speaker 1: its shape of orbit around the Sun and whether that 125 00:07:24,600 --> 00:07:27,840 Speaker 1: orbit could potentially uh collide with the Earth. Send that 126 00:07:27,880 --> 00:07:31,560 Speaker 1: information out to observatories all across the planet. Now, these 127 00:07:31,560 --> 00:07:35,560 Speaker 1: observatories would then train their telescopes onto the object to 128 00:07:35,640 --> 00:07:37,960 Speaker 1: try and make their own calculations based upon their own 129 00:07:38,520 --> 00:07:42,080 Speaker 1: their own perspective, to see if perhaps this would be 130 00:07:42,160 --> 00:07:47,960 Speaker 1: a quote unquote interesting object. Now, in astronomical terms, interesting 131 00:07:48,000 --> 00:07:52,360 Speaker 1: means holy crap, we're all going to die. That's the 132 00:07:52,440 --> 00:07:56,320 Speaker 1: that's what they mean by interesting as in potentially impact 133 00:07:56,360 --> 00:08:00,200 Speaker 1: the Earth interesting. And that information would then be shared 134 00:08:00,000 --> 00:08:05,160 Speaker 1: amongst those observatories, and the likelihood of a clamp down 135 00:08:05,320 --> 00:08:07,320 Speaker 1: is really low, just because you have so many people 136 00:08:07,320 --> 00:08:09,880 Speaker 1: who would be involved in this and have the information, 137 00:08:09,920 --> 00:08:12,960 Speaker 1: and lots of them were gonna talk. A lot of 138 00:08:12,960 --> 00:08:14,880 Speaker 1: them we're gonna talk and say we gotta prepare now, 139 00:08:14,920 --> 00:08:16,720 Speaker 1: because if we don't, we're all going to die, or 140 00:08:17,160 --> 00:08:20,400 Speaker 1: a significant number of people are going to die. Because 141 00:08:20,480 --> 00:08:23,920 Speaker 1: if this asteroid hits a land mass, then it's gonna 142 00:08:24,000 --> 00:08:27,640 Speaker 1: be like, depending on the size of the asteroid, it 143 00:08:27,640 --> 00:08:31,040 Speaker 1: could be like the entire world's nuclear arsenal exploding in 144 00:08:31,040 --> 00:08:35,520 Speaker 1: a single point. Um. If it hits the ocean, then 145 00:08:35,600 --> 00:08:41,440 Speaker 1: it could generate a tsunami of unprecedented uh force that 146 00:08:41,520 --> 00:08:46,640 Speaker 1: could wipe out an entire coast of a of a continent. Um. 147 00:08:46,679 --> 00:08:50,760 Speaker 1: So I mean this is serious business. Uh. Fortunately, we 148 00:08:50,800 --> 00:08:54,600 Speaker 1: haven't discovered anything so far that would cause that much 149 00:08:54,600 --> 00:08:57,440 Speaker 1: of a problem. But again, our ability to detect these 150 00:08:57,480 --> 00:09:02,040 Speaker 1: objects is limited. Most of the objects that NASA concentrates 151 00:09:02,040 --> 00:09:04,079 Speaker 1: on is anything that's a higher and forty meters or 152 00:09:04,240 --> 00:09:07,640 Speaker 1: across or larger. And uh. The problem is that smaller 153 00:09:07,679 --> 00:09:10,959 Speaker 1: objects could cause significant harm. But finding those objects is 154 00:09:10,960 --> 00:09:15,600 Speaker 1: a lot trickier because space is big. Really, Yeah, and 155 00:09:15,640 --> 00:09:19,920 Speaker 1: in relation to space, fifty yard across asteroid or is nothing. 156 00:09:20,640 --> 00:09:25,360 Speaker 1: It's it's you know, you you it's it's impossible to 157 00:09:25,400 --> 00:09:30,120 Speaker 1: exaggerate how tiny that is. Yeah, it's like a it's 158 00:09:30,160 --> 00:09:34,480 Speaker 1: like a germ on a bug. And and and you 159 00:09:34,559 --> 00:09:38,240 Speaker 1: happen to be like a blue whale. That's kind of 160 00:09:38,760 --> 00:09:42,800 Speaker 1: and even then that's not even close that Yeah, I 161 00:09:42,840 --> 00:09:44,960 Speaker 1: can't get my mind around it. That's that's how it is. 162 00:09:45,000 --> 00:09:48,800 Speaker 1: So so all right, So nuking a an asteroid directly 163 00:09:49,000 --> 00:09:51,679 Speaker 1: as in trying to blow it up is not a 164 00:09:51,720 --> 00:09:55,840 Speaker 1: feasible option. So let's let's assume for the moment that 165 00:09:55,880 --> 00:09:58,600 Speaker 1: we have developed technology that helps us, that has improved 166 00:09:58,640 --> 00:10:02,000 Speaker 1: our ability to detect asteroids to the point where any 167 00:10:02,040 --> 00:10:06,400 Speaker 1: asteroid that could potentially cause significant harm to people on Earth, 168 00:10:06,440 --> 00:10:09,160 Speaker 1: to life on Earth, that we have somehow managed to 169 00:10:09,160 --> 00:10:12,840 Speaker 1: to create the technology to detect it. Yeah, all right, 170 00:10:12,960 --> 00:10:14,880 Speaker 1: and it's and it's important to do so because it 171 00:10:15,000 --> 00:10:18,439 Speaker 1: is probable that we will be hit by something largish 172 00:10:18,640 --> 00:10:23,200 Speaker 1: again at some point, essentially, like it's worthwhile to to 173 00:10:23,400 --> 00:10:27,040 Speaker 1: develop this technology exactly. So yeah, the the risk might 174 00:10:27,080 --> 00:10:30,640 Speaker 1: be low, but the impact would be huge. So you know, 175 00:10:30,679 --> 00:10:34,600 Speaker 1: even taking a low risk perspective of it, the actual 176 00:10:34,640 --> 00:10:38,600 Speaker 1: impact would be so enormous that it is a good argument, 177 00:10:38,720 --> 00:10:40,480 Speaker 1: and a lot of people have made this argument to 178 00:10:41,200 --> 00:10:44,760 Speaker 1: UM to invest in technology to help prevent it from happening. 179 00:10:45,120 --> 00:10:47,720 Speaker 1: So let's assume that we have improved technology so we 180 00:10:47,760 --> 00:10:50,760 Speaker 1: can actually detect these asteroids from a pretty good distance. 181 00:10:50,760 --> 00:10:52,920 Speaker 1: Like I said, it might be years before they get here, 182 00:10:53,160 --> 00:10:54,959 Speaker 1: or we're gonna need that time because we're gonna need 183 00:10:54,960 --> 00:10:59,959 Speaker 1: that time to develop the actual vehicles that the tools 184 00:11:00,280 --> 00:11:03,120 Speaker 1: that we're going to use in order to intercept that asteroid. 185 00:11:03,200 --> 00:11:07,400 Speaker 1: So by intercepting it, what could we do to to 186 00:11:08,240 --> 00:11:12,559 Speaker 1: avoid a collision. Well, the real key is deflecting the asteroid. 187 00:11:13,559 --> 00:11:16,160 Speaker 1: You just have to move it a tiny bit, especially 188 00:11:16,160 --> 00:11:17,920 Speaker 1: the further out you go. The further out you go, 189 00:11:18,000 --> 00:11:21,920 Speaker 1: the tinier that that adjustment needs to be, because by 190 00:11:21,920 --> 00:11:24,240 Speaker 1: the time it gets to the Earth, it's going to 191 00:11:24,280 --> 00:11:27,160 Speaker 1: be the distance is going to be much more enormous. 192 00:11:27,520 --> 00:11:31,360 Speaker 1: You know. Just think about like you're walking to have 193 00:11:31,440 --> 00:11:34,560 Speaker 1: a friend standing across from you across a football field, 194 00:11:34,760 --> 00:11:38,240 Speaker 1: and you're both facing each other exactly. Now, imagine that 195 00:11:38,280 --> 00:11:40,719 Speaker 1: your friend just turns slightly a little bit to the 196 00:11:40,800 --> 00:11:44,400 Speaker 1: left and starts walking forward. Well, from a distance, it 197 00:11:44,440 --> 00:11:48,040 Speaker 1: looks like there that your friend may actually meet up 198 00:11:48,080 --> 00:11:50,040 Speaker 1: with you once they get all the way across the 199 00:11:50,040 --> 00:11:52,520 Speaker 1: football field. But as they continue, you see that they're 200 00:11:52,520 --> 00:11:56,040 Speaker 1: getting further and further away until they reach essentially a 201 00:11:56,040 --> 00:11:59,560 Speaker 1: point parallel to you, and they are a good distance 202 00:11:59,640 --> 00:12:02,360 Speaker 1: from you right there, further down the field, like further 203 00:12:02,400 --> 00:12:03,959 Speaker 1: to the right or to the left, whichever way that 204 00:12:04,120 --> 00:12:07,679 Speaker 1: the person turned. Um, that's kind of the idea here 205 00:12:07,720 --> 00:12:09,600 Speaker 1: is that if you can catch an asteroid early enough 206 00:12:09,920 --> 00:12:13,520 Speaker 1: and deflect it just a couple of degrees. Then you've 207 00:12:13,559 --> 00:12:15,240 Speaker 1: solved the problem because it's going to miss the Earth 208 00:12:15,280 --> 00:12:19,600 Speaker 1: by millions of miles. But how do you deflect it? Well, 209 00:12:19,640 --> 00:12:23,280 Speaker 1: there's a lot of different options. Yeah, I read uh 210 00:12:23,559 --> 00:12:27,600 Speaker 1: too specifically, that seemed to be the options people are 211 00:12:27,640 --> 00:12:32,640 Speaker 1: thinking of most what's that um One of them, ironically enough, 212 00:12:32,960 --> 00:12:36,840 Speaker 1: was to use nuclear devices, but not to destroy, but 213 00:12:36,920 --> 00:12:39,079 Speaker 1: to nudge. Right. Yeah, the idea is being that you 214 00:12:39,120 --> 00:12:43,120 Speaker 1: would you would detonate the device over the asteroid. This 215 00:12:43,160 --> 00:12:46,800 Speaker 1: would actually um cause a couple of things to happen, 216 00:12:47,160 --> 00:12:50,559 Speaker 1: and it's you know, it's interesting that again that we're 217 00:12:50,559 --> 00:12:52,280 Speaker 1: talking about something. You know, you might say, hey, you 218 00:12:52,360 --> 00:12:54,520 Speaker 1: just said nuking is bad. Well, in this case, what 219 00:12:54,559 --> 00:12:57,679 Speaker 1: would happen is that you would uh create an uh 220 00:12:58,000 --> 00:13:01,640 Speaker 1: A nuclear radiation would create this this vaporizing energy and 221 00:13:01,800 --> 00:13:04,400 Speaker 1: vaporize the surface or a section of the surface of 222 00:13:04,440 --> 00:13:08,160 Speaker 1: the asteroid. Now that's going to cause that part of 223 00:13:08,160 --> 00:13:11,600 Speaker 1: the surface to eject material into space. And you know, 224 00:13:11,640 --> 00:13:14,199 Speaker 1: for a react action, there's an equal and opposite reaction, 225 00:13:14,280 --> 00:13:16,600 Speaker 1: So that ejection from space is actually going to act 226 00:13:16,640 --> 00:13:21,480 Speaker 1: as a pushing force on the asteroid and it's tiny, 227 00:13:21,520 --> 00:13:23,800 Speaker 1: but that's all you need necessarily know, that might be 228 00:13:23,840 --> 00:13:25,959 Speaker 1: all you need to move that asteroid out of the 229 00:13:26,000 --> 00:13:29,560 Speaker 1: pathway of the Earth. So yeah, you, um you're just 230 00:13:29,679 --> 00:13:34,360 Speaker 1: using it again to to give the asteroid a little push. Um. Actually, 231 00:13:34,400 --> 00:13:38,160 Speaker 1: most of the the options I've seen are some variation 232 00:13:38,280 --> 00:13:41,680 Speaker 1: on pushing the asteroid. It's just lots of different potential 233 00:13:41,679 --> 00:13:45,160 Speaker 1: ways we could do that. Well, that's true. I did read, uh, Yeah, 234 00:13:45,200 --> 00:13:47,160 Speaker 1: to be fair, I did read of the possibility of 235 00:13:47,240 --> 00:13:51,640 Speaker 1: using an inert uh device, nothing that explodes, but basically 236 00:13:51,679 --> 00:13:56,280 Speaker 1: a bullet if you will, to shove. Yeah, using using 237 00:13:56,360 --> 00:14:00,240 Speaker 1: kinetic force to push the asteroid out of the way. Yeah, 238 00:14:00,240 --> 00:14:07,400 Speaker 1: that is another potential UM solution, although it's it's again 239 00:14:07,480 --> 00:14:11,120 Speaker 1: one of those that that has its own set of difficulties. 240 00:14:11,520 --> 00:14:14,280 Speaker 1: But yeah, that's that is what I've also heard, where 241 00:14:14,280 --> 00:14:16,960 Speaker 1: you're just using a kinetic force to to tap the 242 00:14:17,000 --> 00:14:20,360 Speaker 1: asteroid out of the way. And it's it's important to 243 00:14:20,440 --> 00:14:25,400 Speaker 1: note that. Um. What we really can't stress how much 244 00:14:25,640 --> 00:14:30,720 Speaker 1: detection and identifying the the object path how important that is. 245 00:14:30,760 --> 00:14:34,680 Speaker 1: Because um, there there's an effect called the Yarkovsky effect. 246 00:14:34,720 --> 00:14:38,760 Speaker 1: Did you read about this, um as the object gets 247 00:14:38,760 --> 00:14:41,560 Speaker 1: close to the Sun, closer to the Sun UM. And 248 00:14:41,600 --> 00:14:43,720 Speaker 1: I'm not talking about directly on a path too, but 249 00:14:43,800 --> 00:14:46,080 Speaker 1: you know, as it gets closer and closer to the 250 00:14:46,080 --> 00:14:48,040 Speaker 1: Sun in the center of our solar system, it's going 251 00:14:48,080 --> 00:14:53,040 Speaker 1: to heat up. UM. And for a larger object it 252 00:14:53,120 --> 00:14:58,080 Speaker 1: doesn't matter so much UM. But according uh to an 253 00:14:58,160 --> 00:15:01,360 Speaker 1: article that I um than in an article I read, 254 00:15:01,400 --> 00:15:05,560 Speaker 1: the Arkovsky effect basically means that once the the object 255 00:15:05,640 --> 00:15:09,640 Speaker 1: starts to heat up, the heat can affect its path. 256 00:15:10,240 --> 00:15:13,360 Speaker 1: It can basically start it to move in a slightly 257 00:15:13,360 --> 00:15:16,080 Speaker 1: different direction. So you need to be able to We 258 00:15:16,120 --> 00:15:18,960 Speaker 1: would need to be able to know exactly where the 259 00:15:19,680 --> 00:15:23,960 Speaker 1: or as least as close enough to uh, where the 260 00:15:24,040 --> 00:15:26,560 Speaker 1: object is going to be, so that we can accurately 261 00:15:27,160 --> 00:15:28,760 Speaker 1: hit it with something if we're going to try to 262 00:15:28,840 --> 00:15:32,360 Speaker 1: use a brute force method of moving the the asteroid 263 00:15:32,360 --> 00:15:34,760 Speaker 1: out of the way, And a lot of the attempts 264 00:15:34,760 --> 00:15:38,640 Speaker 1: to move asteroids may depend upon sun, the sunlight and 265 00:15:39,000 --> 00:15:41,640 Speaker 1: the Sun's power because um, there are a lot of 266 00:15:41,640 --> 00:15:44,440 Speaker 1: different options that would harness the power of the Sun 267 00:15:44,480 --> 00:15:48,600 Speaker 1: in order to create a pulling effect or pushing effect 268 00:15:49,120 --> 00:15:54,080 Speaker 1: on the the asteroid. For example, there's one UM. One 269 00:15:54,400 --> 00:15:59,560 Speaker 1: possible technique where we would coat the asteroid with white 270 00:15:59,760 --> 00:16:05,200 Speaker 1: and dark coating like paint or dust or whatever, and 271 00:16:05,480 --> 00:16:09,560 Speaker 1: that would uh cause it to move because the Sun's 272 00:16:09,640 --> 00:16:12,840 Speaker 1: energy would actually push against the asteroid. And if we 273 00:16:13,000 --> 00:16:15,880 Speaker 1: coded the rights the correct side, not the right side, 274 00:16:15,880 --> 00:16:18,400 Speaker 1: I mean there's no real right or left, but the 275 00:16:18,480 --> 00:16:21,840 Speaker 1: correct side of the asteroid, it could push the asteroid 276 00:16:22,120 --> 00:16:24,320 Speaker 1: those couple of degrees. By the time it gets to 277 00:16:24,360 --> 00:16:26,400 Speaker 1: where the Earth is, it's millions of miles away, you know, 278 00:16:26,400 --> 00:16:30,680 Speaker 1: it's it's millions of miles off course from hitting the Earth. Um. Similarly, 279 00:16:31,680 --> 00:16:34,840 Speaker 1: there were suggestions that maybe we could create a solar 280 00:16:34,880 --> 00:16:38,520 Speaker 1: sale that would attach we we would use a like 281 00:16:38,560 --> 00:16:41,800 Speaker 1: a probe to attach a solar sale to an asteroid, 282 00:16:41,800 --> 00:16:45,480 Speaker 1: and the solar sale would catch the Sun's energy and 283 00:16:46,040 --> 00:16:49,640 Speaker 1: be propelled by the solar wind, essentially to pull the 284 00:16:49,680 --> 00:16:55,480 Speaker 1: asteroid again outside of its pathway. UM. That that's kind 285 00:16:55,480 --> 00:16:58,000 Speaker 1: of a far fetched one. Really, It's definitely a lot 286 00:16:58,040 --> 00:17:01,520 Speaker 1: more challenging than say, coding an asteroid with a light 287 00:17:01,600 --> 00:17:05,600 Speaker 1: colored material. UM. But then there's also the idea of 288 00:17:05,680 --> 00:17:10,040 Speaker 1: using a net, an enormous net to encapsulate the the 289 00:17:10,200 --> 00:17:13,320 Speaker 1: asteroid and the net would again act as almost like 290 00:17:13,320 --> 00:17:16,720 Speaker 1: a solar sail. It would it would react against you know, 291 00:17:16,800 --> 00:17:19,360 Speaker 1: the sun. The Sun's energy would push against the net, 292 00:17:19,400 --> 00:17:23,760 Speaker 1: which again would alter the course of the asteroid. UM. 293 00:17:23,960 --> 00:17:29,479 Speaker 1: Mirrors are another potential UH solution, where you you launch 294 00:17:29,760 --> 00:17:33,040 Speaker 1: a device that is going to deploy mirrors around the 295 00:17:33,080 --> 00:17:36,800 Speaker 1: asteroid to direct sunlight to specific points in the asteroid 296 00:17:36,800 --> 00:17:39,920 Speaker 1: to again push it out of the way. Um. Well, 297 00:17:39,960 --> 00:17:42,600 Speaker 1: everyone knows that asteroids are veins. If you, you know, 298 00:17:42,800 --> 00:17:44,520 Speaker 1: put the mirrors on the far side of the Earth, 299 00:17:44,560 --> 00:17:47,159 Speaker 1: they'll go toward the mirrors and go, oh, just my 300 00:17:47,200 --> 00:17:51,879 Speaker 1: best side, I look good. Um. But then there are 301 00:17:51,920 --> 00:17:53,440 Speaker 1: a couple of other elements. There are a couple of 302 00:17:53,480 --> 00:17:55,320 Speaker 1: other ways of nudging an asteroid all the way that 303 00:17:55,400 --> 00:17:59,200 Speaker 1: don't involve sunlight at all. Uh. And one of them, 304 00:17:59,400 --> 00:18:03,040 Speaker 1: one of them's strapping a rocket to it. So essentially 305 00:18:03,080 --> 00:18:06,320 Speaker 1: you have a UM, we have to land somebody on 306 00:18:06,359 --> 00:18:09,400 Speaker 1: the asteroid. No, not necessarily, you'd have to have some 307 00:18:09,440 --> 00:18:16,840 Speaker 1: sort of of remotely operated probe that could embed into 308 00:18:16,880 --> 00:18:21,119 Speaker 1: the asteroid itself and then use um, have enough fuel 309 00:18:21,160 --> 00:18:24,560 Speaker 1: in it to be able to push as a rocket 310 00:18:24,640 --> 00:18:26,720 Speaker 1: to push the asteroid out of the way of the 311 00:18:26,760 --> 00:18:31,240 Speaker 1: pathway of collision. Now it doesn't have to push very hard, 312 00:18:31,280 --> 00:18:33,080 Speaker 1: it doesn't have to push for very long. Again, as 313 00:18:33,080 --> 00:18:35,520 Speaker 1: long as you catch the asteroid early enough that we 314 00:18:35,560 --> 00:18:37,480 Speaker 1: have to keep stressing that this is. This is assuming 315 00:18:37,520 --> 00:18:40,640 Speaker 1: that we capture, that we detect the asteroid and years 316 00:18:40,640 --> 00:18:42,520 Speaker 1: and years and years in advance, and that we're able 317 00:18:42,520 --> 00:18:44,720 Speaker 1: to react quickly enough so that by the time the 318 00:18:44,720 --> 00:18:46,960 Speaker 1: probe reaches the asteroid. Because you remember, this isn't gonna 319 00:18:46,960 --> 00:18:49,240 Speaker 1: be overnight. It's gonna take time for the for whatever 320 00:18:49,280 --> 00:18:53,040 Speaker 1: solution we deploy to get to the asteroid. Like it, 321 00:18:53,080 --> 00:18:55,000 Speaker 1: maybe you know, we launched something and we don't know 322 00:18:55,040 --> 00:18:56,919 Speaker 1: if it's going to work for another two years or 323 00:18:57,000 --> 00:18:59,440 Speaker 1: three years. I mean, it's kind of scary to think about, 324 00:18:59,480 --> 00:19:04,240 Speaker 1: but that's true. So um, yeah, you have to figure 325 00:19:04,240 --> 00:19:07,240 Speaker 1: out away where you have this this device, and it 326 00:19:07,440 --> 00:19:09,000 Speaker 1: has to be able to carry enough fuel so that 327 00:19:09,040 --> 00:19:12,320 Speaker 1: it can actually deploy properly. A lot of people suggest 328 00:19:12,359 --> 00:19:14,560 Speaker 1: that this kind of approach would be best if it 329 00:19:14,600 --> 00:19:17,520 Speaker 1: were already space born. So in other words, we already 330 00:19:17,520 --> 00:19:22,000 Speaker 1: had some sort of launching platform in space, so that 331 00:19:22,359 --> 00:19:26,680 Speaker 1: the uh, the individual probes would not need so much 332 00:19:26,720 --> 00:19:29,479 Speaker 1: fuel to both escape the arts gravity and land on 333 00:19:29,520 --> 00:19:33,399 Speaker 1: an asteroid and then propel it away. Um. That that 334 00:19:33,520 --> 00:19:36,600 Speaker 1: does prose a problem. But then another one is the 335 00:19:36,720 --> 00:19:40,840 Speaker 1: gravity tractor. Ah, yes, and I when I looked up 336 00:19:40,880 --> 00:19:43,760 Speaker 1: the gravity tractor, I had to check just a moment ago. 337 00:19:43,880 --> 00:19:47,960 Speaker 1: And yes, someone has named their band gravity Tractor. Good 338 00:19:47,960 --> 00:19:53,760 Speaker 1: for them, Yeah, lead singer John Dear, nice, thank you. Um, 339 00:19:54,040 --> 00:19:59,400 Speaker 1: but yeah, the gravity tractor is fascinating, um, because this 340 00:19:59,600 --> 00:20:04,760 Speaker 1: is essentially using a different body and the gravity of 341 00:20:04,800 --> 00:20:08,119 Speaker 1: another body and body that we would launch into space 342 00:20:08,680 --> 00:20:12,560 Speaker 1: to pull the asteroid away without even I mean it's 343 00:20:12,560 --> 00:20:15,080 Speaker 1: not the point here is not even a touch the asteroid. 344 00:20:15,119 --> 00:20:18,680 Speaker 1: It's to get something near enough to it to affect 345 00:20:19,280 --> 00:20:22,760 Speaker 1: um the asteroids path with another gravitational field, right, Because 346 00:20:22,800 --> 00:20:26,960 Speaker 1: you gotta remember everything in the universe exerts a gravitational 347 00:20:27,000 --> 00:20:30,040 Speaker 1: pull on everything else. It's just that that poll is 348 00:20:30,080 --> 00:20:33,399 Speaker 1: dependent upon distance and mass and lots of other stuff. 349 00:20:33,880 --> 00:20:35,960 Speaker 1: But they you know, so if you were able to 350 00:20:36,000 --> 00:20:39,359 Speaker 1: put a massive enough object close enough to the asteroid, 351 00:20:39,600 --> 00:20:41,760 Speaker 1: you could alter its pathway. There is there are some 352 00:20:41,800 --> 00:20:46,240 Speaker 1: problems with the gravity tractor, really, Yeah. One of them 353 00:20:46,320 --> 00:20:47,840 Speaker 1: is that you have to figure out all a. Well, 354 00:20:48,640 --> 00:20:51,560 Speaker 1: you want the gravity tractor to pull the asteroid away 355 00:20:51,600 --> 00:20:53,359 Speaker 1: from the path of collision. You don't want the asteroid 356 00:20:53,400 --> 00:20:56,160 Speaker 1: to pull the gravity tractor into the path of collision. 357 00:20:56,640 --> 00:20:59,040 Speaker 1: So so that means that you would have to have 358 00:20:59,080 --> 00:21:02,120 Speaker 1: some sort of propole sustion system aboard the gravity tractor 359 00:21:02,480 --> 00:21:06,760 Speaker 1: to make little course corrections and continue to gently pull 360 00:21:06,840 --> 00:21:09,800 Speaker 1: the asteroid out of its pathway. Well, if you have propulsion, 361 00:21:09,960 --> 00:21:12,560 Speaker 1: then there's the possibility of that propulsion that you're going 362 00:21:12,600 --> 00:21:16,399 Speaker 1: to when you fire your rockets to to give it 363 00:21:16,400 --> 00:21:19,920 Speaker 1: a boost, that force may push against the asteroid, thus 364 00:21:20,000 --> 00:21:23,240 Speaker 1: negating the gravity pull that you are exerting upon it. 365 00:21:23,320 --> 00:21:28,399 Speaker 1: So essentially you're getting a net zero result because that 366 00:21:28,560 --> 00:21:30,639 Speaker 1: you're you're pulling on it with gravity, but you're pushing 367 00:21:30,640 --> 00:21:33,240 Speaker 1: on it with your propulsion system. So finding a way 368 00:21:33,240 --> 00:21:37,320 Speaker 1: where you could create some sort of gravity tractor where 369 00:21:37,720 --> 00:21:41,720 Speaker 1: the propulsion system would not actually push against the asteroid 370 00:21:41,760 --> 00:21:44,879 Speaker 1: itself is would be part of the solution. Plus this 371 00:21:44,880 --> 00:21:47,879 Speaker 1: would be really really expensive. It's a much more costly 372 00:21:48,359 --> 00:21:52,960 Speaker 1: approach and not necessarily uh the most easy to implement 373 00:21:53,440 --> 00:21:56,880 Speaker 1: compared to other approaches. So I don't know that this 374 00:21:56,920 --> 00:22:00,640 Speaker 1: is necessarily likely to happen. I mean, if if enough 375 00:22:00,640 --> 00:22:02,520 Speaker 1: research goes into it where it proves that this is 376 00:22:02,560 --> 00:22:07,520 Speaker 1: the most effective way, then sure I can see it happening, 377 00:22:07,560 --> 00:22:09,679 Speaker 1: just because people would finally say, all right, well, you know, 378 00:22:09,720 --> 00:22:12,919 Speaker 1: we have to invest in it, because we can't. We 379 00:22:12,960 --> 00:22:17,919 Speaker 1: can't just play roulette all our existence. We have to 380 00:22:17,960 --> 00:22:21,080 Speaker 1: prepare for this. But I would imagine that we'd probably 381 00:22:21,080 --> 00:22:26,000 Speaker 1: go with some other route before we tried this one. Yeah. 382 00:22:26,600 --> 00:22:29,879 Speaker 1: An article I read suggested that the the gravity tractor 383 00:22:29,920 --> 00:22:34,320 Speaker 1: would have to be at least uh twenty tons in 384 00:22:34,400 --> 00:22:38,600 Speaker 1: order to safely to you know, effectively to I should say, 385 00:22:38,640 --> 00:22:43,520 Speaker 1: not safely effectively to and an asteroid away from the Earth. Um, 386 00:22:43,600 --> 00:22:47,600 Speaker 1: and I can't you know, I just imagine that's going 387 00:22:47,640 --> 00:22:50,680 Speaker 1: to be very hard to get out of the Earth's orbit. 388 00:22:51,200 --> 00:22:52,960 Speaker 1: I mean, you know, our gravity. I'm sorry to leave 389 00:22:52,960 --> 00:22:55,080 Speaker 1: the gravitational field of the Earth to launch something that 390 00:22:55,160 --> 00:22:58,760 Speaker 1: big in the space. But you know, I'm not a 391 00:22:58,880 --> 00:23:03,360 Speaker 1: rocket scientist, so nor are you a brain surgeon. Now 392 00:23:03,760 --> 00:23:07,040 Speaker 1: I'm not a rocket surgeon either, so um, well that's good. 393 00:23:07,960 --> 00:23:10,480 Speaker 1: I can just imagine that going wrong. So I've got 394 00:23:10,480 --> 00:23:15,760 Speaker 1: another another potential, although it's far fetched possibility of getting 395 00:23:15,840 --> 00:23:18,119 Speaker 1: rid of an asteroid that um that's coming at you. 396 00:23:19,520 --> 00:23:23,640 Speaker 1: You let robots eat it. Really, Yeah, that's Robert Lamb 397 00:23:23,680 --> 00:23:26,119 Speaker 1: actually wrote about this. He has a great article on 398 00:23:27,000 --> 00:23:31,040 Speaker 1: the Our Our Discovery news site called top ten ways 399 00:23:31,080 --> 00:23:33,920 Speaker 1: to stop an asteroid, and one of them is talking 400 00:23:34,000 --> 00:23:39,040 Speaker 1: about using them robots that would actually essentially kind of 401 00:23:39,119 --> 00:23:43,560 Speaker 1: chew up the asteroid and then shoot out the tiny 402 00:23:43,640 --> 00:23:50,040 Speaker 1: bits of asteroid uh into space electromagnetically UM and essentially 403 00:23:50,040 --> 00:23:53,600 Speaker 1: disperse the asteroid while it's still really, really really far 404 00:23:53,640 --> 00:23:55,560 Speaker 1: away from the Earth. Because keep in mind, if it's 405 00:23:55,560 --> 00:23:57,840 Speaker 1: really far away from the Earth, then not all of 406 00:23:57,880 --> 00:23:59,920 Speaker 1: that mass is going to hit the Earth the way 407 00:24:00,040 --> 00:24:04,159 Speaker 1: it would in the beginning of UM the or or 408 00:24:04,280 --> 00:24:08,560 Speaker 1: at the end of arm again rather So, Yeah, these 409 00:24:08,720 --> 00:24:12,720 Speaker 1: these robots UH eating poop, They eat asteroids and they 410 00:24:12,760 --> 00:24:16,600 Speaker 1: poop asteroid dust. I am. I wanted to go there, 411 00:24:16,600 --> 00:24:18,399 Speaker 1: and I said, no, I'm not gonna say it. You're 412 00:24:18,400 --> 00:24:20,520 Speaker 1: not gonna say they eating poop. Nope, But you did 413 00:24:20,520 --> 00:24:22,399 Speaker 1: it for me. So I can see the look on 414 00:24:22,440 --> 00:24:24,159 Speaker 1: your face, and I knew that you were thinking that. 415 00:24:24,240 --> 00:24:27,280 Speaker 1: So I was like, I'm going to do it. Um, Well, 416 00:24:27,400 --> 00:24:31,000 Speaker 1: I wanted to. Yeah, so this is this is definitely 417 00:24:31,040 --> 00:24:32,760 Speaker 1: something that we need to think about. I mean, it's 418 00:24:32,760 --> 00:24:35,480 Speaker 1: it's true that we need to think about invest in it. 419 00:24:35,520 --> 00:24:39,840 Speaker 1: There are some talks about private companies actually investing in 420 00:24:39,880 --> 00:24:43,479 Speaker 1: this UM sort of technology, this sort of approach UM, 421 00:24:43,520 --> 00:24:45,160 Speaker 1: which is kind of cool that you know, it's not 422 00:24:45,240 --> 00:24:49,120 Speaker 1: just not just depending upon governmental agencies that have lots 423 00:24:49,119 --> 00:24:52,520 Speaker 1: of different you know, things pulling on them. Um. I 424 00:24:52,560 --> 00:24:55,840 Speaker 1: did read that UM scientists don't seem to believe that 425 00:24:55,840 --> 00:24:58,879 Speaker 1: there's anything likely to hit us in the next hundred 426 00:24:58,960 --> 00:25:01,680 Speaker 1: years or so at the earliest, well at least nothing 427 00:25:01,680 --> 00:25:04,560 Speaker 1: that we can see. Yeah, exactly. So there's still the 428 00:25:04,600 --> 00:25:07,440 Speaker 1: possibility that something smaller it could hit and still cause 429 00:25:07,600 --> 00:25:11,040 Speaker 1: massive damage. It's just not gonna necessarily cause global damage, 430 00:25:11,119 --> 00:25:15,600 Speaker 1: but it could cause catastrophic local damage, you know. Um. Yeah, 431 00:25:15,600 --> 00:25:19,040 Speaker 1: there's some interesting organizations out there that are dedicated to 432 00:25:19,080 --> 00:25:21,359 Speaker 1: trying to fix this problem. There's one called the B 433 00:25:21,600 --> 00:25:26,359 Speaker 1: six one to Foundation, uh, and they their goal is 434 00:25:26,400 --> 00:25:31,280 Speaker 1: to have a workable solution by So that's coming up 435 00:25:31,320 --> 00:25:34,280 Speaker 1: pretty pretty soon. Um. If you guys want to learn 436 00:25:34,359 --> 00:25:36,920 Speaker 1: more about the topic, well, I can recommend a couple 437 00:25:36,960 --> 00:25:39,160 Speaker 1: of things and how stuff works. We actually have two 438 00:25:39,280 --> 00:25:41,680 Speaker 1: articles that you go into more detail about the stuff 439 00:25:41,680 --> 00:25:44,400 Speaker 1: we've talked about. One is called could we really blow 440 00:25:44,520 --> 00:25:47,640 Speaker 1: up an incoming asteroid with a nuclear bomb? And one 441 00:25:47,760 --> 00:25:49,880 Speaker 1: is called could we stop an asteroid on a collision 442 00:25:49,880 --> 00:25:54,080 Speaker 1: course towards the Earth? And also, uh, there's a great 443 00:25:54,080 --> 00:25:58,719 Speaker 1: program that aired on Discovery UM called Bad Universe, and 444 00:25:58,840 --> 00:26:01,680 Speaker 1: it was It's hosted by Phil Play the Bad Astronomer. 445 00:26:01,840 --> 00:26:05,000 Speaker 1: Phil Plate, by the way, one of my favorite bloggers 446 00:26:05,400 --> 00:26:07,960 Speaker 1: and scientists out there, because he's one of those scientists 447 00:26:08,640 --> 00:26:11,879 Speaker 1: who really dedicates his work to explaining science to the 448 00:26:11,960 --> 00:26:15,399 Speaker 1: layman in terms that are easy, easy to understand. It 449 00:26:15,440 --> 00:26:19,400 Speaker 1: makes science fun and exciting, and he does not shy 450 00:26:19,440 --> 00:26:23,159 Speaker 1: away from topics like this, where you know, he's like, yeah, 451 00:26:23,200 --> 00:26:25,359 Speaker 1: it'll kill you, so that's why I gotta fix it. 452 00:26:26,320 --> 00:26:29,160 Speaker 1: So he's very matter of fact about it. UM. Really 453 00:26:29,200 --> 00:26:32,000 Speaker 1: intelligent guy, very entertaining guy. So if you have not 454 00:26:32,160 --> 00:26:35,560 Speaker 1: read his stuff or watched his show, I do recommend 455 00:26:35,600 --> 00:26:38,400 Speaker 1: trying to catch that because it's he's a great guy. 456 00:26:38,400 --> 00:26:41,439 Speaker 1: And he also has a really amusing Twitter feed and 457 00:26:41,480 --> 00:26:44,960 Speaker 1: he interacts with a lot of other uh Twitter Wisenheimer's 458 00:26:45,000 --> 00:26:48,199 Speaker 1: out there. Like Jonathan Colton, Paul and Storm you know, 459 00:26:48,400 --> 00:26:51,840 Speaker 1: um will be eaten. There's there's this kind of Twitter 460 00:26:51,920 --> 00:26:55,800 Speaker 1: rottie that have have formed up and uh and so 461 00:26:56,280 --> 00:27:00,880 Speaker 1: um he often will chat with those oaks and in 462 00:27:00,880 --> 00:27:03,040 Speaker 1: interesting and entertaining ways. And he's and he shares a 463 00:27:03,040 --> 00:27:06,040 Speaker 1: lot of really cool science news through his Twitter feed 464 00:27:06,040 --> 00:27:09,280 Speaker 1: as well. I showed you that that amazing photo of 465 00:27:09,560 --> 00:27:14,159 Speaker 1: the Space Shuttle Endeavor across the sun. Yeah, yeah, that 466 00:27:14,240 --> 00:27:17,280 Speaker 1: was that was courtesy of of Mr Phil Plate. So yeah, 467 00:27:17,359 --> 00:27:20,120 Speaker 1: he's written extensively about this and he's he's talked about 468 00:27:20,160 --> 00:27:22,160 Speaker 1: it in his blogs and on on on the show 469 00:27:22,200 --> 00:27:26,280 Speaker 1: Bad Universe. Um, so I recommend that as well. And uh, well, 470 00:27:26,359 --> 00:27:29,920 Speaker 1: I don't have any other potential solutions off the top 471 00:27:29,960 --> 00:27:31,320 Speaker 1: of my head. Do you have anything else you want 472 00:27:31,320 --> 00:27:35,080 Speaker 1: to add before we conclude? Not in particular? Now, Well, then, um, 473 00:27:35,119 --> 00:27:37,760 Speaker 1: I would suggest we all just take a moment to 474 00:27:38,000 --> 00:27:44,160 Speaker 1: uh to to ridicule the documentary Armageddon, uh for its 475 00:27:44,480 --> 00:27:48,760 Speaker 1: portrayal of how we would uh alter the course of 476 00:27:48,800 --> 00:27:51,120 Speaker 1: a of an asteroid by blowing it up real good, 477 00:27:51,720 --> 00:27:53,720 Speaker 1: uh Texas style. But you have to land a space 478 00:27:53,720 --> 00:27:56,800 Speaker 1: shuttle on it first. Yeah, and you have to sing 479 00:27:57,080 --> 00:27:59,359 Speaker 1: the song I quoted at the beginning at some point 480 00:27:59,520 --> 00:28:05,239 Speaker 1: and uh, and Bruce Willis has to die of spoiler alert. Yeah. Um. 481 00:28:05,760 --> 00:28:08,600 Speaker 1: I was interested in though, that scientists are also talking 482 00:28:08,640 --> 00:28:13,119 Speaker 1: about the possibility of of mining asteroids in a in 483 00:28:13,160 --> 00:28:16,360 Speaker 1: a in an attempt to understand them better. Um. Yeah, 484 00:28:16,400 --> 00:28:19,240 Speaker 1: I did read that. Uh. You know, although we may 485 00:28:19,280 --> 00:28:23,600 Speaker 1: not necessarily be ready to to destroy one just yet, 486 00:28:23,680 --> 00:28:28,600 Speaker 1: that scientists even alter its path, right right, Um, but 487 00:28:29,080 --> 00:28:31,920 Speaker 1: scientists are considering the possibility if uh, you know, since 488 00:28:31,960 --> 00:28:35,239 Speaker 1: they are tracking some asteroids that are coming near to 489 00:28:35,359 --> 00:28:38,480 Speaker 1: Earth and near and again space is big, so near 490 00:28:38,520 --> 00:28:41,960 Speaker 1: as a relative term. Um. But they're talking about the 491 00:28:42,000 --> 00:28:47,760 Speaker 1: idea of visiting some near Earth asteroids with the possibility 492 00:28:47,760 --> 00:28:51,120 Speaker 1: of mining, you know, taking some samples of the rocks 493 00:28:51,360 --> 00:28:53,240 Speaker 1: that are there on the asteroid to get a better 494 00:28:53,320 --> 00:28:56,600 Speaker 1: understanding of elements in the universe and bringing them back 495 00:28:56,640 --> 00:28:59,720 Speaker 1: to Earth, which, uh is a really cool idea. I 496 00:28:59,720 --> 00:29:03,440 Speaker 1: don't I don't imagine they would send people to do that. Um. 497 00:29:03,480 --> 00:29:07,960 Speaker 1: So the idea of doing the complex calculation necessary to 498 00:29:08,480 --> 00:29:12,040 Speaker 1: hit a moving object you know that's coming around, um, 499 00:29:12,240 --> 00:29:14,880 Speaker 1: take samples and then return to Earth. That's that's really 500 00:29:14,960 --> 00:29:18,280 Speaker 1: fascinating stuff. And that's not exactly the same topic, but 501 00:29:18,400 --> 00:29:22,040 Speaker 1: I think it's a really cool application of science and 502 00:29:22,120 --> 00:29:24,480 Speaker 1: hope that if they can do that that it will 503 00:29:24,520 --> 00:29:26,680 Speaker 1: be fruitful and we'll learn a lot from it. Yeah, 504 00:29:26,720 --> 00:29:29,680 Speaker 1: and asteroid mining may actually lead to other things as well, like, 505 00:29:29,720 --> 00:29:32,080 Speaker 1: for example, if we find an asteroid that has ice 506 00:29:32,120 --> 00:29:35,160 Speaker 1: deposits on it, that could be a way of finding 507 00:29:35,160 --> 00:29:40,960 Speaker 1: not just water, but actually generating oxygen for other space missions. 508 00:29:41,160 --> 00:29:43,360 Speaker 1: So yeah, they're the asteroid mining is one of those 509 00:29:43,360 --> 00:29:45,520 Speaker 1: other things. We could probably do a full episode about 510 00:29:45,560 --> 00:29:47,720 Speaker 1: asteroid mining as well, just because there's so many other 511 00:29:48,320 --> 00:29:52,520 Speaker 1: possible applications for it that would be fun. Yep, I agree, 512 00:29:52,800 --> 00:29:55,680 Speaker 1: So let us wrap this one up. Guys. If you 513 00:29:55,720 --> 00:29:58,360 Speaker 1: have any topics you want us to cover, there's something 514 00:29:58,400 --> 00:30:00,680 Speaker 1: that's uh, it's got an ast right heading straight for 515 00:30:00,760 --> 00:30:03,000 Speaker 1: your brain, and you want us to nudge it all 516 00:30:03,040 --> 00:30:05,600 Speaker 1: the way. Let us know. You can send us a 517 00:30:05,640 --> 00:30:09,160 Speaker 1: message on email. 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