1 00:00:00,520 --> 00:00:03,400 Speaker 1: Welcome to brain Stuff from house Stuff works dot com, 2 00:00:03,600 --> 00:00:15,400 Speaker 1: where smart happens Him Marshall Brain with today's question, how 3 00:00:15,440 --> 00:00:18,040 Speaker 1: big does a meteor have to be to make it 4 00:00:18,079 --> 00:00:21,439 Speaker 1: to the ground. If you've spent much time looking up 5 00:00:21,440 --> 00:00:25,400 Speaker 1: at the night sky, you've probably seen some spectacular meteors 6 00:00:25,480 --> 00:00:29,080 Speaker 1: and meteor showers. One of the most amazing things about 7 00:00:29,120 --> 00:00:31,840 Speaker 1: these displays is that the majority of the space does 8 00:00:31,960 --> 00:00:36,839 Speaker 1: that causes visible meteors is tiny, between the size of 9 00:00:36,880 --> 00:00:39,920 Speaker 1: a grain of sand and the size of a small pebble. 10 00:00:40,640 --> 00:00:44,839 Speaker 1: Discussing meteor activity can be tricky because the terminology is 11 00:00:44,880 --> 00:00:49,280 Speaker 1: pretty confusing. The term meteor actually refers to the streak 12 00:00:49,360 --> 00:00:52,720 Speaker 1: of light caused by a piece of space debris burning 13 00:00:52,760 --> 00:00:57,240 Speaker 1: up in the atmosphere. The pieces of debris are called meteoroids, 14 00:00:57,720 --> 00:01:01,120 Speaker 1: and remnants of the debris that actually each Earth's surface 15 00:01:01,600 --> 00:01:06,680 Speaker 1: or another planets for that matter, are called meteorites. Meteoroids 16 00:01:06,840 --> 00:01:10,440 Speaker 1: have a pretty big size range. They include any space 17 00:01:10,520 --> 00:01:14,280 Speaker 1: debris bigger than a molecule and smaller than about three 18 00:01:14,760 --> 00:01:18,720 Speaker 1: thirty feet or a hundred meters in diameter. Space debris 19 00:01:18,760 --> 00:01:22,160 Speaker 1: bigger than this is considered an asteroid, but most of 20 00:01:22,200 --> 00:01:25,760 Speaker 1: the debris the Earth comes into contact with is dust 21 00:01:26,000 --> 00:01:30,279 Speaker 1: shed by comets traveling through the Solar System. This dust 22 00:01:30,480 --> 00:01:33,480 Speaker 1: tends to make up the small particles that we see 23 00:01:33,880 --> 00:01:37,600 Speaker 1: as meteors. So how can we see a meteor caused 24 00:01:37,640 --> 00:01:40,679 Speaker 1: by such a small bit of matter. It turns out 25 00:01:40,760 --> 00:01:44,160 Speaker 1: that what these meteoroids lack in mass, they make up 26 00:01:44,200 --> 00:01:47,040 Speaker 1: for in speed, and this is what causes the flash 27 00:01:47,080 --> 00:01:50,600 Speaker 1: of light in the sky. Meteoroids enter the atmosphere at 28 00:01:50,640 --> 00:01:55,240 Speaker 1: extremely high speeds seven to forty five miles per second 29 00:01:55,480 --> 00:01:59,120 Speaker 1: or eleven to seventy two kilometers per second. They can 30 00:01:59,160 --> 00:02:01,960 Speaker 1: travel at this rate very easily in the vacuum of 31 00:02:02,000 --> 00:02:05,920 Speaker 1: space because there's nothing to stop them. Earth's atmosphere, on 32 00:02:06,000 --> 00:02:08,760 Speaker 1: the other hand, is full of matter, which creates a 33 00:02:08,800 --> 00:02:12,640 Speaker 1: great deal of friction on the traveling object. This friction 34 00:02:12,760 --> 00:02:16,440 Speaker 1: generates enough heat up to three thousand degrees fahrenheit or 35 00:02:17,600 --> 00:02:22,120 Speaker 1: degrees celsius, to raise the meteoroid surface to its boiling point, 36 00:02:22,440 --> 00:02:26,800 Speaker 1: so the meteoroid is vaporized layer by layer. The friction 37 00:02:26,880 --> 00:02:30,280 Speaker 1: breaks the molecules of both the meteoroid material and the 38 00:02:30,320 --> 00:02:36,600 Speaker 1: atmosphere into glowing ionized particles, which then recombine, releasing light energy. 39 00:02:36,680 --> 00:02:40,760 Speaker 1: To form a bright tail. A meteor tail caused by 40 00:02:40,800 --> 00:02:44,640 Speaker 1: a grain sized meteoroid is a few feet wide about 41 00:02:44,639 --> 00:02:47,960 Speaker 1: a meter, but because of the high speed of the debris, 42 00:02:48,240 --> 00:02:52,760 Speaker 1: maybe many miles long. So how big does a meteoroid 43 00:02:52,880 --> 00:02:54,520 Speaker 1: have to be to make it to the surface of 44 00:02:54,520 --> 00:02:58,440 Speaker 1: the Earth. Surprisingly, most of the meteoroids that reach the 45 00:02:58,480 --> 00:03:02,880 Speaker 1: ground are a specially small, from microscopic debris to dust 46 00:03:02,919 --> 00:03:07,320 Speaker 1: size particle pieces. They don't get vaporized because they're light 47 00:03:07,440 --> 00:03:11,120 Speaker 1: enough that they slow down very easily, moving about one 48 00:03:11,280 --> 00:03:13,799 Speaker 1: inch or two and a half centimeters per second through 49 00:03:13,840 --> 00:03:18,399 Speaker 1: the atmosphere. They don't experience the intense friction that larger 50 00:03:18,440 --> 00:03:23,600 Speaker 1: meteoroids do. In this sense, most all meteoroids that enter 51 00:03:23,680 --> 00:03:26,080 Speaker 1: the atmosphere make it to the ground in the form 52 00:03:26,160 --> 00:03:30,400 Speaker 1: of microscopic dust. As for the meteoroids big enough to 53 00:03:30,480 --> 00:03:35,200 Speaker 1: form visible meteors, estimates for the minimum size vary. This 54 00:03:35,280 --> 00:03:39,760 Speaker 1: is because there are factors other than size involved. Most notably, 55 00:03:40,040 --> 00:03:43,800 Speaker 1: a meteoroid's entry speed affects its chances of reaching the 56 00:03:43,880 --> 00:03:49,360 Speaker 1: surface because it determines the amount of friction the meteoroid experiences. Typically, 57 00:03:49,400 --> 00:03:52,320 Speaker 1: though a meteoroid would have to be about the size 58 00:03:52,320 --> 00:03:54,920 Speaker 1: of a marble or a portion of it to reach 59 00:03:55,000 --> 00:03:58,760 Speaker 1: the Earth's surface. Smaller particles burn up in the atmosphere 60 00:03:58,840 --> 00:04:02,560 Speaker 1: about fifty seven five miles above the Earth. The fist 61 00:04:02,640 --> 00:04:05,480 Speaker 1: size meteorites a person is likely to find on the 62 00:04:05,480 --> 00:04:09,920 Speaker 1: ground probably came from something significantly larger pieces of debris 63 00:04:10,000 --> 00:04:13,440 Speaker 1: at least the size of a basketball. Since larger meteoroids 64 00:04:13,640 --> 00:04:16,920 Speaker 1: usually break up into smaller chunks as they travel through 65 00:04:16,960 --> 00:04:21,400 Speaker 1: the atmosphere, you can actually find and collect tiny meteorites 66 00:04:21,440 --> 00:04:23,680 Speaker 1: that have made it through the Earth's atmosphere. With this 67 00:04:23,800 --> 00:04:27,320 Speaker 1: simple experiment, put a pan on your back porch or 68 00:04:27,440 --> 00:04:30,120 Speaker 1: deck and catch them. You can find sites on the 69 00:04:30,120 --> 00:04:33,120 Speaker 1: web that will show you how to identify the difference 70 00:04:33,120 --> 00:04:39,040 Speaker 1: between meteorites and bits of sand and dust. For more 71 00:04:39,040 --> 00:04:41,600 Speaker 1: illness and thousands of other topics. Does that how stuff 72 00:04:41,640 --> 00:04:43,720 Speaker 1: works dot com and don't forget to check out the 73 00:04:43,760 --> 00:04:45,800 Speaker 1: brain stuff blog on the house stuff works dot com 74 00:04:45,839 --> 00:04:48,680 Speaker 1: home page. You can also follow brain stuff on Facebook 75 00:04:48,760 --> 00:04:53,920 Speaker 1: or Twitter at brain stuff HSW. The house Stuff Works 76 00:04:53,920 --> 00:04:57,160 Speaker 1: I fine app has arrived down at it today on iTunes, 77 00:05:00,080 --> 00:05:00,120 Speaker 1: m