In short
StarTalk Radio Episode Notes: Things You Thought You Knew – The Color of the Sun
Episode Overview This episode features Neil deGrasse Tyson and co-host Chuck Nice discussing the true color of the sun, the acoustic effects in weather, and the importance of friction. The conversation blends science with humor and insights from pop culture.
Key Themes and Discussions
The Color of the Sun
- Common Misconception: The sun is often depicted as yellow, particularly in children's drawings.
- Truth Revealed: The sun appears white, especially when viewed directly overhead. The yellow or red hues observed during sunrise and sunset are optical effects caused by atmospheric filtering.
- Atmospheric Effects:
- Scattering of Light: Blue light is scattered more than other colors due to the atmosphere's particles, leading to a blue sky.
- Sunset Colors: As the sun lowers in the sky, its light must pass through more atmosphere, scattering more blue light, leaving reds and oranges visible.
- Visual Experiment: When the sun is obscured by thin clouds, it appears dim but remains white, contradicting the belief that it becomes yellow when covered.
Weather Acoustics
- Thunder and Lightning:
- Lightning creates a shockwave, resulting in thunder, which can vary in sound quality due to the lightning's non-linear path.
- The intervals between seeing lightning and hearing thunder can help gauge distance (5 seconds = 1 mile).
- Sounds of Snow:
- Freshly fallen snow absorbs sound, creating a noticeable silence in urban environments.
- The temperature affects sound; colder temperatures lead to crunching sounds when walking on snow, while warmer temperatures yield silence as snow compresses without breaking.
Friction
The Unsung Hero
- Importance of Friction:
- Friction is essential for movement, driving, walking, and even staying seated at a table.
- Without friction, cars wouldn't move, and walking would be impossible on slippery surfaces.
- Everyday Examples:
- Friction generates heat, making it useful in cold weather to warm hands.
- Friction is essential for the operation of vehicles, where tires grip the road.
- Friction in Space:
- Rockets use thrust to propel, unlike vehicles that rely on friction with the ground.
- Discussed the need for friction in spacecraft re-entry; it dissipates the heat generated by rapid movement through the atmosphere.
Interesting Tidbits
- Sound Propagation: Sound travels slower at lower frequencies, which affects how we perceive thunder sounds at various distances.
- Cultural References: The conversation incorporates cultural and humorous references, making complex scientific concepts more relatable.
Conclusion Neil deGrasse Tyson emphasizes that friction is a friend in the physical world, aiding in various processes from daily activities to the complexities of space travel. The discussion encourages listeners to appreciate the science behind common misconceptions and everyday phenomena.
---
Key Takeaways
- Misconceptions about the sun's color are rooted in childhood perceptions and atmospheric effects.
- Weather sounds are influenced by physical phenomena like lightning and snow, altering our auditory experience.
- Friction is crucial for movement and everyday life, often overlooked but fundamentally important in both terrestrial and space contexts.
Keep looking up!
Written by AI. May contain mistakes. Listen to the episode to check what was said.
Chapters
Tap a time to open that second in VOThe Color of the Sun: A Childhood Misconception
0:45 to 2:48
Discussing common perceptions of the sun's color and the reality behind it.
“So I want to talk about the sun, the color of the sun.”
Atmospheric Effects on Sunlight
2:48 to 4:48
Explaining how the atmosphere alters our perception of the sun's color at different elevations.
“Sometimes it's so deep it can be red, amber into red.”
Understanding Sunlight and Color
4:48 to 7:31
Delving into the science of light and its impact on the sun's appearance from Earth.
“So let's see what the atmosphere is doing when the sun is overhead.”
The Relationship Between Light Bulbs and Sunlight
7:31 to 12:39
Comparing the color temperature of incandescent bulbs with sunlight and its implications for photography.
“So that when they reflect up, you see white.”
Artistic Interpretations of Color
12:39 to 14:02
Exploring how art and emotional perceptions of color influence our understanding of light.
“If an artist draws an Arctic scene, what color is prevalent?”
Understanding Light Bulbs and Scene Settings
14:02 to 14:40
Learn how art and technology influence lighting in scenes.
“They had to have a colder bulb to do that.”
The Science Behind Thunder and Lightning
14:58 to 17:20
Explore the relationship between lightning and the sound of thunder.
“really yeah yeah i i just thought just thought about that okay it sounds um like something that But if somebody said to me at a cocktail party, I'd be like, I got to get a drink.”
Intriguing Facts About Lightning Sounds
17:20 to 18:18
Discover how lightning produces different sounds and why they vary.
“So the sound will hit you at different times.”
The Acoustic Experience of Thunder
18:18 to 21:03
Learn how the acoustics of lightning affect the sounds we hear.
“By the way, there's certain frequencies of sound that are longer, sorry, there's certain wavelengths of sound that are longer than what will fit in your eardrum.”
Calculating Distance Using Sound
21:03 to 23:16
Find out how to estimate the distance of a storm using sound.
“So, so that's what's, that's what's going on there.”
Show all 21 chapters
Snow and Its Unique Acoustic Properties
23:16 to 24:40
Understand how snow affects sound and creates a quieter environment.
“If that time delay keeps getting shorter and shorter and shorter, watch out, watch out.”
The Science of Walking on Snow
24:40 to 26:17
Learn why snow crunches underfoot at certain temperatures.
“Because you're just pressing down snowflakes because they landed softly and now you're just sort of compressing them.”
Hail and Weather Dynamics
26:17 to 28:01
Explore the phenomenon of hail and its relationship with summer storms.
“So, these are some interesting sort of sound things to look out for when this happens.”
The Dynamics of Hail Formation
28:01 to 30:50
Discover how hail forms and the role of unstable air columns in weather.
“Ice falling out of the sky in the summertime.”
The Silence Under Overpasses
30:51 to 31:46
Learn about the perception of sound and silence while driving in the rain.
“You ever been driving a car and it's raining and it's raining, you know, the whole time you're driving and then you come under an overpass and it's silent.”
Introducing 'Down Pause'
31:47 to 32:26
Explore the intriguing term 'down pause' to describe silence during rain.
Understanding Friction's Importance
32:27 to 35:24
Examine how friction is essential for movement and everyday activities.
“when people talk about friction, it's bad.”
Friction and Earth's Rotation
35:25 to 38:36
Learn about the relationship between friction, human movement, and Earth's rotation.
“So with a rocket, however, by the way, it's why rockets work in space where there's no air, there's nothing rubbing against anything else.”
Galileo vs. Aristotle on Motion
38:37 to 42:01
Discover how Galileo's experiments challenged Aristotle's views on motion.
“So all of we humans run forward and add up all our mass and get our velocities, add it all up.”
Understanding Friction and Motion
42:01 to 43:27
Learn how friction affects the movement of heavy objects and vehicles.
“You sit on a couch, the couch would just slide back.”
Re-entry Physics: The Role of Friction
43:27 to 46:38
Discover how astronauts survive re-entry and the importance of friction in this process.
“Because all they would have to do, all they would have to do, we don't do this, but what they could do is bring enough fuel.”
Transcript
Automatic transcript. May contain errors.0:00Hey everybody in the StarTalkiverse, we've got yet another Things You Thought You Knew episode. This time, Chuck and I get into the color of the sun, weather acoustics, and friction. Check it out. Welcome to StarTalk, your place in the universe where science and pop culture collide. StarTalk begins right now. Welcome to the Explainer Zone. Yes, the Explainer Zone. Yeah, yeah. Not the Twilight Zone. Not the Twilight Zone. We are confused at the end. Right. The explainer zone. Where you come out knowing more than you did when you went in. Knowing some stuff. Right. And so I think there's no end to this, just so you know.
0:48Good. I will be calling you forever. All right. So I want to talk about the sun, the color of the sun. Okay. All right. Well, you know me. I don't see color. You don't see color. Sorry. We're already done here. Um, so, so, so here's the thing. If you're a school child and you to draw a scene and you want to put the sun in the sky, what crayon do you reach for? Um, well, I was a very depressed child. So black. Black. Okay. No, you knew about black holes. Yes, exactly. No. Oh, it's always a big yellow ball. It's always yellow. And this notion has been with us since childhood, that the sun is yellow.
1:34Yes. And that's not true. It's not even close to being true. Uh-oh. And so, yeah, I'm sorry. You know, I don't want to. Are there any kids watching? Please. you might want to leave the room right now because we're not sure if there's a Crayola available for you to draw your little scenes with the house and the grass. Okay. So here's the thing. The sun in broad daylight is too bright to look at. All right. Without risking damaging your eyes. So unless of course you have perfect eyes. Okay. So, so you don't do it. All right. So when is the time most people ever find themselves looking directly at the sun?
2:27When is that? Well, the only times I've ever done it is sunset and sunrise. Exactly. Exactly. So not only do we have the yellow crayon in our crayon box from childhood, anytime we actually ever find ourselves looking at the sun, either on purpose or by accident, It's low on the horizon. The sun is rising or setting. Right. And it has a deep yellow color. Sometimes it's so deep it can be red, amber into red. Yeah. So, and we know the sun isn't red. Of course it's not red. We know that's an optical effect. Now, this isn't Krypton. It's not Krypton. Exactly. I had a red sun. So, you know intuitively it's not red, but somehow you don't know intuitively that it's also not yellow.
3:13Okay. what color is the sun it is white now now come on man why you gotta do that white see what what just like everything else all of a sudden chuck not everything we got a race commentary you know what seriously we gotta must we whitewash all of history including the sun really so yeah so it's not yellow okay it's not yellow now i can give you evidence of this if you need evidence but i'm simply saying that as the sun gets let's look at earth and and there's the atmosphere wrapped around the earth if the sun is directly overhead or anywhere near directly overhead it goes to sort of let's call that one thickness of atmosphere okay top to bottom as the sun gets lower and lower in the sky the path of light through the atmosphere is longer okay because now you got there's that angle through it and the lower the sun gets on the sky the more and more atmosphere it has to pass through and in fact you can calculate how many equivalent atmospheres it went through okay and you just need a little bit of trigonometry it's a simple calculation.
4:30And if it's low on the horizon, it goes through five, six, ten equivalent atmospheres when it's low on the horizon. So whatever the atmosphere is doing to the sun when it's high up overhead, it's doing it ten times that and more when it goes lower on the horizon. Okay. So let's see what the atmosphere is doing when the sun is overhead. In comes white light. okay and white light is composed of colors as isaac newton demonstrated all the colors of the rainbow red orange yellow green blue indigo if you must violet violet okay so in it comes particles in earth's atmosphere that happen to be the same size as the wavelength of light of the blue side of the spectrum the blue indigo purple a violet side of the spectrum Those particles preferentially scatter the blue out of the sunlight.
5:32Preferentially scatters it. So it subtracts away a little bit, just a little bit. All right? The rest of the light makes it all the way to Earth's surface. But some of the blue gets scattered, and that's why we have a blue sky. Nice. The blue sky is stolen sunlight that would have otherwise passed straight through. Look at that. Okay. Right. Because the sky is really clear, right? Okay, so now watch. How beautiful is that? Now let's have the sun get a little lower in the sky. Well, there'll be more of this going on. Okay, more of the sky. That's why on cloudless days into sunset, the sun gets deeper and deeper and deeper blue.
6:15The bluest sky. That's why sky blue is light blue. Right. All right. You want to talk about serious right home to mama blue is the blue sky that surrounds the twilight curtain of a sunset. Now you're talking blue. Right. Okay. So, so much blue is taken out that we now, Roy G. Biv, red, orange, yellow, green, blue, and he took out blue, indigo, violet. What's left? Red, orange, yellow, green. Okay. If you add those colors together, you're going to get an amber sun. And depending on how many particles there are, you'll get a red sun or you'll get a simple yellow sun on the horizon. And so you now look at, oh, we have a yellow star.
7:04Look, it's yellow. No, the atmosphere made it yellow. Okay? Wow. It's lying to you. And here's what you do. broad daylight if there's thin cirrus clouds okay so it's safer to look up to the sun look up to the sun in the middle of the day is it yellow no no it is white this is very disturbing it's this is very very disturbing because the clouds themselves don't change the color of the sun it'll just it just dims it so you look at a slightly dimmer sun uh behind the thin clouds as they pass it's not yellow it's not yellow not only that consider the following all right now this takes a little extra thinking put your thinking cap on okay and we in another explainer we address this but now there's a different reason for it if i have a sheet of paper and it's white that means light reflected of it from it is an even mixture an equal mixture of red orange yellow green blue violet all those colors together in optics makes white don't tell this to an artist right it doesn't doesn't work on the easy no it's they you do it's just the opposite and all right it's just the opposite you don't get black but you'll get like sludge you'll get sludge right all right so the fact that the page is white means all of those colors of light are hitting that page.
8:36Correct. So that when they reflect up, you see white. Okay. So a white light illuminating a white piece of paper shows up to you as a white piece of paper. There you go. Okay. Now white reflects all colors. Let me put a red gel in front of the light. Now look at the paper. What color is it? It's red. It's red. We kind of pinkish, but yeah. That's right. So it reflects all colors, but now it's only getting red. It's going to reflect the red. It reflects all colors. The page is red to your eye. Let's put a blue gel. What happens to the page? The page is blue. Same thing. Yeah. Okay. So if the sun were yellow, then snow would be yellow.
9:24yellow which by the way sometimes snow is yellow and it's not from the sun and whatever you do whatever you do stay away from that snow the fact that snow looks white right is evidence that it's being illuminated by white light wow that white light is either sunlight or a moonlight that's right which is also a reflection of sunlight it's just reflected sunlight there you go this is so disturbing so so so i'm just trying to be honest i'm just trying to put it out there and just and by the way let me take you want to go up a notch are you ready to go up a notch on this i don't know if i'm ready to go up and i don't think you're ready okay so um white is the sun I hate where this is going already.
10:20Relative to incandescent bulbs. Right. Okay. Your kids will have no memory of incandescent bulbs, but old timers, if you're over 25, you're an old timer. You remember bulbs that would get hot when you put them in. It was a bulb with a little piece of wire in it. Okay. That wire used to light up. You hear me? That sounds like a Ken Burns special. The guy on the porch. Right. I remember the days when it had a bulb with a little piece of wire now that wire would light up and get hot and we pulled the switch we pulled the switch and it gave off light now first it looked like magic
11:07okay we gotta put you on the list of the next Ken Burns special the origin of the light bulb so alright So where was it? I forgot. Okay. He's saying incandescent bulbs. Incandescent bulbs. Incandescent bulbs, when you turn them on, the temperature of the filament is not as high as the temperature of the surface of the sun. And so the higher the temperature, the more full that spectrum becomes. So if you looked at the spectrum of a bulb in your house or an incandescent bulb, it's very weak in the blue section. There's some blue there, which is why blue still looks blue under that light. But the blue is very weak under an incandescent light bulb.
11:47Okay? So if you bring out film that needs the full complement of blue, and you take a picture under incandescent lights, everything is going to be red. That film, if it needed the blue, is called daylight film. This is why there was a difference. Again, I'm only talking old timers here. There was indoor film and tungsten film and outdoor film. And the outdoor film was color balanced to get the entire spectrum of the sunlight. If you took indoor film and put it outside, that indoor film is too sensitive to blue because it's making up for the feeble blue coming out of a bulb. And it goes out, it's getting all the blue it ever wanted.
12:29If you have indoor film, took a picture outside, everything looks blue because it was hypersensitive to blue. And the sun has plenty of it. okay so to a photographer sunlight is blue it's highly blue and they have to correct for that if they're going from indoors to outdoors they have to redo the color balance on a white sheet of paper to account for the difference between indoor lighting and outdoor lighting now here's where they all got it wrong but they're not going to change it because they're deep into it you ready Now we have the blending of science and technology with art. You ready? Here it is.
13:10If an artist draws an Arctic scene, what color is prevalent? White. And what color? Blue. Blue. Right. If an artist draws Dante's hell, what color is prevalent? Red and orange. Red and orange. Okay, so emotionally, we think of blue as cold and red as hot. Photographers will tell you we need to reduce the temperature of the light, which means make it colder emotionally. functionally. But the only way to do that is to get more blue in it, which means upping the temperature of the tungsten that they have shining on you or to put more blue into it. And in the old days, that meant a hotter light bulb.
14:04So they said, we need a cooler scene. They had to have a hotter bulb. We need a warmer scene. They had to have a colder bulb to do that. Wow. And that language is still embedded in that entire profession. Yep. That is true. The opposites. And they meet in the middle and they deal with it. The opposites of art and technology. And science. And the physics of light.
14:39I'm Ali Khan Hemraj. And I support StarTalk on Patreon. This is StarTalk with Neil deGrasse Tyson.
14:57so i got one for you how about acoustic effects in climactic phenomenon really yeah yeah i i just thought just thought about that okay it sounds um like something that But if somebody said to me at a cocktail party, I'd be like, I got to get a drink. I'll be right back. But they will come back because it's intriguing enough, but they got to get prepped. First, they got to get prepped. They're chemically prepped for it. Exactly. All right. So let's start out with thunder and lightning, for example. So lightning, in its path between the ground and the clouds, or between a cloud and the cloud, never goes in a straight line.
15:39because it's finding the path of least resistance the entire time unknown to you. This is what it's doing. And then when you see the lightning strike, it is already a predetermined path between one point and another. All right. Now, it turns out the sound of lightning is simply the shock wave of rapidly heated air by the bolt of electricity moving through the air, which is extremely hot. Right. It's thousands of degrees. But what matters is that the air is some other temperature, and then it is instantaneously made extremely hot. This creates an expanding shockwave that we hear as thunder. Okay.
16:27Now, because the path of the lightning is not straight, Right. There are kinks in the root. So each segment of that kinky lightning has its own generated shockwave. Okay. Right. So now you have multiple kinks generating their shockwaves and you can have constructive and destructive interference of competing shockwaves. that makes so much sense which is oh go ahead okay okay oh this is good okay so our researchers just found the the lightning 50 000 degrees 50 000 degrees fahrenheit yes okay that that's hot okay all right i'll send it so now watch so with these different segments that's why a single lightning bolt and by the way the lightning bolt is not all the same distance from you okay the parts that are a little closer that are on the ground if it's cloud to cloud The part directly above you is closer than farther away.
17:30So the sound will hit you at different times. But it's one generated event. Right. So that's why the lightning can go, snap, quackle, pop. Okay? That's why it's not just one acoustic experience. It is a highly... I love your thunder. Okay. You like my thunder? We have to isolate. No. What just happened? If I see that on a meme, I'm going to kick you. Oh, my God. I am so. I'm going to kick. That is so going to be a meme. So here's the lightning. And it's because of the acoustical configuration of the lightning bolt itself. That is wonderful. I'm serious. That is so great because one of my favorite things in the world is to hear lightning, to hear thunder.
18:25but not the rumbling thunder the thunder that sounds as if it is tearing the sky yeah because that it's okay i'm getting there that's my next point okay so so that so i'm just simply accounting for oh by the way constructive and destructive interference if you're not familiar with that so so sound travels in waves so it crests and troughs and that's this is a pressure wave through the air it hits your eardrum your eardrum vibrates we interpret that as sound So does your body too. By the way, there's certain frequencies of sound that are longer, sorry, there's certain wavelengths of sound that are longer than what will fit in your eardrum.
19:08So your eardrum will have a hard time communicating it to your brain. But the length of the wavelength is about the size of your chest cavity. That's the low frequency, long wavelength. And so there are some sounds that you feel more than you hear.
19:28that's the rhythm section of the beat well what do they call the beat the the the beat boppers what do they call the beat batzers yes yeah yeah yeah but if i heard lightning starting to do that it was like whoa There is a God. God is a DJ. So here's what happens. The lightning sound is a huge cacophony of frequencies of sound energy. Okay. High frequency, low frequency. But here's the problem. High frequency doesn't travel very far. It's easily disrupted. It's easily, lose its energy relative to the energy that it started with. And if high frequency sound loses its energy, it becomes lower frequency sounds.
20:21So the farther away you are from a lightning strike, the lower is the total cacophony of frequencies that reach you. uh-huh so lightning on the horizon is all right okay if you have a pet dog they'll they hear that and they notice that and they might start trembling and you don't even know why because that frequency is below what you can hear the dogs hear it all right as the storm gets closer and closer the higher frequencies become more and more part of what you what you hear and if you hear a lightning strike where that sounds of like it's ripping the fabric of the space-time continuum. It meant it hits your house.
21:08All right. So, so that's what's, that's what's going on there. Sound moves through air at about 700 miles an hour, plus or minus depends on the density of the air. But I like easy math. So let's just declare that the sound is moving at 600 miles an hour. Okay. 600 miles an hour is the speed of sound in air, how far does sound go in a minute? 600 divided by 60. That's how far? I don't know. You've just set up the verbal math problem in my computer. No, that's not allowed. I don't know, 120 miles. So if it's 600 miles an hour and you divide by 60 minutes, okay? Then sound will move 10 miles in a minute.
22:0010 miles in a minute. In a minute. Right. Okay. So if sound moves 10 miles in a minute, how many seconds does it take the sound to move one mile? 10 seconds. Or six. Six seconds, right? Six seconds. So it moves a mile every six seconds so that after a minute, it moves 10 miles. Right. And after an hour, it moves 600 miles. right so so basically if you want to know how far away the rain is from you
22:37time get the time difference between when you see a lightning strike and when you hear it so you see the flash and then you count 1001 one down mississippi 2003 so if it's five seconds let's say that's almost six seconds so the storm is about a mile away mile away yeah about a mile away. And so, and the real number is 700 miles an hour. So it's, you know, you make a small adjustment, but you get the basic idea. Okay. Sound lose a mile every six seconds. And so just for your habits, if, and if you hear the thunder and it never gets closer than that, the rain is not headed towards you. Don't worry about it.
23:13Go home, go back to sleep. Nice. If that time delay keeps getting shorter and shorter and shorter, watch out, watch out. Yep. Yeah. I'm going to lose your house. Yeah. Dorothy, you're not in Kansas anymore. There you go. Nice. So a couple of other acoustic things. So for example, a snowflake is very, is highly variegated, right? It's got six sides. It's got a lot of texture. And if you have snow that's descending and it's just softly landing on blankets on a surface, okay? Now you have sound. Generally, when you hear someone from a distance, you are relying on the fact that the sound is bouncing off the pavement, off the walls.
23:57We don't think often about this, but reflected sound is a big part of how we interact with our world around us. All right. If you have snow everywhere, the surface of the snow is not rigid. It's not highly reflective. In fact, it's highly absorbent. So particularly for city people know this. If all of a sudden the city gets quiet and you don't hear anything, look out the window, chances are it's snowing. Nice. Because the sound of the cars and all the normal sounds that reach you by reflecting off of steel and glass and concrete and cement is no longer reflecting. It's all muffled. Yeah. And so the song, the Christmas song, Silent Night, Holy Night, um whatever other reasons you want to think of it as a silent night if it has just snowed guaranteed to be more silent than it otherwise would have ever been snow is nature soundproofing and they are soundproofing now when you're walking on snow okay as opposed to walking on sunshine okay if it's just snowed and you're walking on it okay and that will normally be a silent exercise, okay?
25:16Because you're just pressing down snowflakes because they landed softly and now you're just sort of compressing them. Fine. If it's colder, I forgot the temperatures. If it's colder than like 25 degrees, low 20s, definitely if it's in the teens or lower, if you then step on the snow. Okay. The snow says, I will not yield under your boot print. I'm going to hold my shape because it is cold enough that we are all solid and rigid. And what happens? The snow crunches. Yeah. Then you crunch on snow. So if you're filming a movie or if you're observing a scene and you hear people crunching on the snow, guarantee the temperatures in the low twenties are in the teens or or there's a guy in a booth with some cornflakes and he's just matching the sound to the people walking is the sound studios have all those sweat the sound effects in them right so so that's why snow crunches at cold temperatures and does not crunch at warmer temperatures by the way at the warmer temperatures your pressure is enough to melt the snow okay to bring it immediately below the freezing point that's a whole other star talk explainers that we've done, what ice will do under pressure.
26:30Under pressure. Yeah. So, these are some interesting sort of sound things to look out for when this happens. Now, it has been rumored that Aurora, that you can hear Aurora. And I'm not convinced of that. Really? Yeah. Yeah. Because it happens, it, you know, it's, it happens 50 ,000 feet up, you know, 10 miles away and farther up in the atmosphere where the atmosphere is really thin, right? It is electrical. So it could be that it's creating other electrical phenomenon in your environment. But to say that you heard sound that comes from that high, I'm not convinced of that. I don't believe, but people say it.
27:14So it's worth the essays it sings yeah yeah yeah it's worth investigating i think so yeah yeah and so let me think any other sounds you've heard in weather that you wonder about i mean you know aside from the fact that uh my uncle used to like to make his own sounds and then blame it on me while we were walking in the cold other than that now and here's another one um you know the sound of hail hitting right these are basically these These are like marbles falling out of the sky. I know what that sound is. That is the sound of a call to the insurance adjustment.
27:56So people say, you know, when do you get hailed most? You get it in the summertime. All right. That's weird. Ice falling out of the sky in the summertime. Well, it's a reminder that the sun is not heating the air. The air is transparent to sunlight. That's why you can see the sun from Earth's surface through the air. So the septum of Los Angeles. The septum of Los Angeles and Beijing and Mexico City. Right. So those are inversion layers. So they're climactically susceptible to trapping smog. Both those three areas. You notice they're all in basins. Oh, yeah. Santiago de Chile as well. So here's what happens.
28:38The sun heats the ground. The ground heats the air. But if you go high above the ground, it gets very, very cold very, very quickly, no matter the time of year. But in the summertime, you have the most ground heating, and so you have the most unstable air columns. So the biggest, thickest, juiciest cumulonimbus clouds, which we all learned about in elementary school, the big puffy ones, you find those in the summertime. And you look at them and you think the cloud is just sitting there. But if you look for long enough, you will see that it is roiling. And in the roiling, there is very highly unstable air rising within it.
29:19The more unstable the air is in the upwardly rising columns, the harder it is for whatever is hanging out in there to fall out of the cloud. Wow. Because it's kept buoyant by these upwardly moving air columns. Right. So you first nucleate a little droplet of ice. It wants to fall. I say, no, you're not. And it comes back out and it nucleates with more moisture. Because what is a cloud? It's a big pocket of moisture. Droplets. Droplets. Water drops. So it gathers more moisture. And, uh-huh, no, you're not. And it keeps doing this. It keeps doing this. Until the frozen ball says, you ain't holding me this time.
30:05And that's why all of hail is about the same size. Because it had to get to that size to overcome the highly unstable air columns that were supporting it. And so the more turbulent is the air, the louder they will be when they hit the ground. And then there it is. And we always reference the size of hail to some other object, which I find interesting. It was softball-sized hail. It was baseball-sized hail. I've never seen anybody talk about hail-sized golf balls. Right. Maybe it's obvious why, but I don't know. But anyhow, so Chuck, that's a little bit of the sound of weather. I love it. So, so very cool.
30:51Oh, and one other thing. One last thing. You ever been driving a car and it's raining and it's raining, you know, the whole time you're driving and then you come under an overpass and it's silent. Yes. Okay. Just silent. That's an interesting phenomenon because what your brain had done was create the sound of rain as the normal so that when you go under the underpass, it's the absence of rain that you take notice of. See, and that happens in my everyday life where the normal sound is a house full of annoying children running around. And when you step out the house, you say, what was that? I was surprised.
31:34When you step out, it's a silence. You wonder, you look around. So silent out here. What's relevant? What happened? And I'm like, God, did we move to the country? so there's a word i've seen and it hasn't caught on but i think it should it's the sound of the absence of rain under an overpass okay and it's called a down pause oh instead of a downpour yes down pause down pause there oh that's lovely i'm gonna leave you with
Read the full transcript
32:26that friction oh my goodness yes friction friction now friction usually when when people talk about friction, it's bad. All right. You can bring out the WD-40. It's squeaking. It's friction. And let's burn friction burn. Right. Right. Right. But let me tell you without friction, life as we know it would not be possible. Friction is your friend. See, I have lots of missing skin on my knees with that to differ. So, so friction, I mean, just think about it. If you just sort of put your elbow on the table, right? And you just rest it there. Yes. And then you want to listen to me. If there was no friction, you would just slide off the table.
33:22There'd be nothing keeping your elbow there. That's why I stopped wearing silk shirts.
33:29So, so, and let's say you wanted to drive your car. You need the friction between your tires and the road so that you will move forward. If there were zero friction between your car and the road, the wheels would just spin and nothing would happen. Okay. You would go nowhere. You wouldn't be able to start the car, to move the car, slow down the car, stop the car, or even steer the car. All of that requires friction. to walk, to walk. You put a foot down, there is friction there. You press back and your next foot moves forward in advance of it. That required friction. This is why on slippery ice where there is no friction, you can't walk, you can't run.
34:19And you say, this is bad. Put me back on regular ground. What you're really pleading for is give me some friction. You don't say that because friction has a bad name. And what do you do when it's cold out and you're not wearing gloves? What do you do?
34:36Hands get hot. I just realized it's cold in my house. Okay. So you do that. Okay. Friction is your friend. Oh, that's nice. So we'll do a whole other thing on friction becoming heat. That's a whole other explainer that needs its own time for that. Oh. But friction can help get you warm. All right. So the only thing that really does not use friction is rockets. All other transportation requires friction. Bicycles, trains, planes in order to take off. Okay. Oh my goodness. That's right. All of this requires friction. Interesting. The planes need it to take off. Oh. So with a rocket, however, by the way, it's why rockets work in space where there's no air, there's nothing rubbing against anything else.
35:34It sends material out the back and it recoils forward. Right. So all rockets that are accelerating are losing mass in order to do it in a recoil. Whereas you don't have to lose mass to do it. You just have to press against the earth. Right. Well, Newton told us for every action is an equal and opposite reaction. So if you are stand still and you start moving forward, actually something has to start moving backwards. And it's communicated that way through friction. So what happens? You move forward with a certain momentum. What are you pushing against? The ground. The ground. The ground has to move backwards.
36:15And it does. So the entire earth is responding to the fact that you moved in one direction. Okay. Okay. Oh, man. Could we all get together, every human being, just in one group, and start running in one direction? Will we speed up the Earth? Yes. Or slow it down, depending on which direction. And it has to be due east or due west. Correct. It has to be due east or due west. Yes. What? So if everyone lined up, okay, and started running due east, okay, so that will sort of spin. Wait, which way are we turning? returning this way. So you have to run and run due west. And if everybody does that with their scurrying feet, you will speed up the rotation of the earth.
37:02What? That is the response of the earth to you propelling yourself forward by way of friction connecting you to the earth itself. It's true with cars. It's true with everything. Now, I once did a calculation and I said, let's get our most powerful rocket engines, bench mount them at the equator where you have sort of maximum torque on the earth and can we use that to either speed up or slow down the earth and i did the math on that and it's hopeless okay it's like a gnat flying full speed into the side of an elephant and believing the elephant even took notice okay sorry confident very confident nat very confident it's a very confident nat in fact it's less than that so but but take that dumbo what i'm saying is the momentum that we all gave each other by putting ourselves into motion you can write down that number momentum is your mass times your velocity that you gave yourself okay earth's rotation increase or decrease will have changed by exactly that same amount of momentum so that they both cancel because you started out both not moving relative to each other so if one thing starts moving the other thing has to recoil the other way so that they balance out that's physics 101 so if you go forward earth goes backwards by the exact same total momentum but earth has so much mass relative to all the mass of the humans, that your momentum, which is mass times velocity, that's the only quantity that has to be the same.
38:41All right. So all of we humans run forward and add up all our mass and get our velocities, add it all up. And we got this honkering earth with this really large mass and it gets a teeny little bitty velocity to balance us out. So if you don't notice it, but you can calculate what that effect is and it is real. It is real. Wow. Excellent. And it's friction. It's all friction. So I just want you to think of friction as a good thing. It's more good than bad. One thing friction does is it slows down things that were put into motion. And Aristotle, not really understanding friction. Aristotle got most of his physics wrong, by the way.
39:24He's no hero in physics and astrophysics. Thank God he had philosophy. philosophers like him uh and he did important things but there's stuff he could have really checked and he didn't and so it's it's before experimental philosophy kicked in as opposed to thinking philosophy and and and so the experimental philosophers bacon had a whole book just on experiments that he said he conducted but there's like a thousand experiments in it and that's what all he'd be doing every day for the rest of his life so i don't think he did them all but it's a there's a book that we collected them and so he and galileo they do the experiment if you have an idea okay so because otherwise and no disrespect aristotle you're just bullshit you're just you're just thinking stuff up that you think should be true because it makes sense to you we could all do that in the armchair so he said things in motion tend to come to rest okay so that's true right all right but Galileo said wait a minute if I wax the track you know I have a thing I roll it down the hill and it stops like here now I make it smoother it stops a little farther away make it even smoother it starts even farther away and he said wait a minute What would happen if there was no friction on this track?
40:53Where will it stop? And he concluded that things in motion will tend to stay in. He fed Newton's things in motion tend to stay in motion. It's the opposite of Aristotle, unless acted on by an outside. Look at that. And so Galileo was the bridge between Aristotle and Newton. and doing the experiments by waxing the track, making it ever more smooth, reducing the friction coming, that enabled him to establish a fundamental truth about nature, going beyond just what your life experience is. Look at that. Galileo, the Mr. Miyagi of physics. Who knew? Wax on. Wax off.
41:44So I just want you to appreciate friction. You know, I will not. No. I still can't get my head around liking friction. But it is necessary. Without friction, everything would just be floating. Would be gliding. Sliding around. Sliding around. You sit on a couch, the couch would just slide back. By the way, you could push very heavy things. If there's a freight train, I don't care what it weighed. If it's on frictionless tracks, let's say it's a maglev frictionless track and you have a little handle, just take it and start pulling. So you can put a force on it. And yes, it's way more mass than you are.
42:27So the velocity will be small, but it'll have some velocity. So you can just start pushing it. And this is why those strong men in competitions, okay, where they pull with it in the old days. they pull the train with their teeth okay it's because trains are on steel rolling wheels on steel tracks which has very low friction okay if you took it off the tracks and let it sit there in the mud and then haven't tried to tug the train that ain't happening that's that's kind of funny though you could pull things that have wheels on them because wheels have very low friction in the transmission of the movement of that object to the ground because you're not dragging it on the ground right but the wheel itself still needs a little bit of friction in order to not spin spin out that's all that's so cool oh you know i i have to say i i will never think of friction in the same way uh one last thing okay one last thing uh when astronauts re-enter the atmosphere and they have that you know the the burning phase you know yes the flames and the thing all right we say oh my gosh will they survive this is bad how good no you need that the astronauts coming out of orbit are going 17 000 miles an hour and they didn't bring fuel to break.
43:58Oh. Okay. Because all they would have to do, all they would have to do, we don't do this, but what they could do is bring enough fuel. While you're in orbit at 17 ,000 miles an hour, because that's orbital speed, turn their ship around and fire it backwards. Right. That will slow you down. And you keep doing that until you like have zero velocity. And then you just drop out of the sky. If you drop out of the sky, you're not going to be burning up because what's burning up is the kinetic energy of having gone 17 ,000 miles an hour in the first place. I saw a movie, I think it was, it was one of these Mars movies, one of the earlier ones that came and went, where there's something happening on a platform and the guy falls off the platform, but it's a stable platform up there above the ground.
44:48And as he falls, we see him just burn up. It's like, no, no. The act of falling through the atmosphere alone is not what burns you up. It's the fact that you are going from 17 ,000 miles an hour to zero. And where does all that kinetic energy go? There is friction between you and the air molecules passing across your surface. There's also shockwaves that communicate as you're going faster than the speed of sound. Shockwaves take all this energy that you have and convert it into heat. and then the heat dissipates and then you fall down out of the sky alive because you have special heat shields that protect you uh-huh there you go and before we perfected the the tiles that we used on the shuttle we had the heat shield was astronauts we they weren't really shields a shield is something that protects you we call them shields but that's not what they were you know what they were they're like onion layers of burnable material oh so they just burned off Exactly.
45:51But you had to go through enough of them to get to the crispy center. Where the astronauts are. Where the astronauts are. So it turns out coming out of orbit, you need more of these layers than when you come back from the moon. So coming back from the moon, you just make that layer thicker. And then it ablates and it heats, it burns off and goes out. That takes the heat away and eats as these layers go. So it was a very blunt, effective heat shield, but it's really a shield that dissolves away in the heat. All of that, the friction, the shockwaves, and that allows you to not have to take fuel in order to slow down using fuel because you're basically aerobraking.
46:35Sweet. That's what reentry is. It's a form of aerobraking. That is fascinating. Friction is your friend. That's all I'm trying to tell you, Chuck. Every astronaut loves friction. Otherwise, they can't come home. or you need fuel to slow down that's all i'm saying you want to exploit to exploit what you got and so you should say great they're burning up their heat shields that's a good thing sweet all right all right i'm liking it chuck friction is your friend all right i i got a new friend today that makes one all right makes one one one french chuck and his one friend i got my one friend All right.
47:18Neil deGrasse Tyson here, your personal astrophysicist. Keep looking up.
From the publisher
What’s the true color of the sun? Neil deGrasse Tyson and comic co-host Chuck Nice discuss things you thought you knew about the color of the Sun, the sound of weather, and why friction is our friend.
NOTE: StarTalk+ Patrons can listen to this entire episode commercial-free here:
https://startalkmedia.com/show/things-you-thought-you-knew-the-color-of-the-sun/
Thanks to our Patrons Jorge Aguirre, C&C Angeli, Len Brandis, Alan Parker, Aaron Ivey, AA-ron or just "AI", MD Bartlett, Nox, Nicholas Crayford, Adam Collins, Deep Patel, RAHIM THERIOT, Dan Abrams, Dan Thomas, Tig, Gloria Michelle Shirley, Mike Horvath, Daniel Brannon, Tonieh Ellis, Camila Von Malice, Kat, Nickolas Madeo, Marcus Phelps, Daniela Eneva, AndyF, Paul Purington, Paul, Mark Fowler, Thomas Freridge, Corey Ferrell, Mo O, Jacob Johnson, Matt Newcomb, Vladimir Antonovich, Steffen Sommers, Joan Morrissey, yared ts, Danielle Seitz, Edmond Fondahn, Blythe Lucas, Richard Adam, Bryant McFayden, Nayah Sci Fi, Lissett Lamboy, John Lujan, Marie Mckenna, Kaustav Chakravarthy, Hannah Bradley, Joshua Jones, EVA, Gail Knapp, Gavin Dunagan, Decoy, Athena Ozanich, Dakota Barron, William Gibson, Eleanor Dewitt, Tru Shadow, MorningSong, Matt Delashaw, Angela Woods, Eric Gorohoff, Zakary Tackett, Carmen Fragapane, Kristián Žuffa, Michael Dunsavage, Mark Bradshaw, Kelsey Harkness-Jones, Mark Rose, Brent, Mohammed Hamdy, Baz, Andrew Stevens, Rachel Jacobsen, Rick Dawson, Tibor Szabo, Raven Knight, McMarklar, Chris Cummings, FromLongIsland, Wendy Parsons, Denise Asmus, Brad, JimPP, Lauren Cooper, Juan Jove, Brent Bailey, Watts Wire Extension Cords, Graham, sean aley, NotAnotherMike, Robert Currier, Steve Vanspall, Alex Nuss, Thomas PASCAL, Antonín Karásek, Mikayla Trousdale, MC, 22 Simulations, Kasey Marsland, and Stevie for supporting us this week.
Subscribe to SiriusXM Podcasts+ to listen to new episodes of StarTalk Radio ad-free and a whole week early.
Start a free trial now on Apple Podcasts or by visiting siriusxm.com/podcastsplus.
Hosted by Simplecast, an AdsWizz company. See pcm.adswizz.com for information about our collection and use of personal data for advertising.
