Michael here. And my tea is quite hot, but it's not the hottest thing in the

universe.

So what is? I mean, we know that there is an absolute zero,

but is there an absolute hot? A point at which something is so hot

it can't get any hotter. Well to find out, let's begin

with the human body. Your internal temperature

is not constant. 37 degrees, 98.6.

Sure. But those are averages. Your body's internal temperature fluctuates

by about one degree Fahrenheit -

half a degree Celsius - throughout the day in a cycle.

Assuming you sleep at night, at 4:30 in the morning

your body reaches its coolest natural healthy temperature.

And at 7 p.m. it reaches its highest.

But a dangerous fever is not good.

108 degrees Fahrenheit is almost always

lethal. The highest recorded air temperature across

all of Earth has happened four times in Death

Valley, where it has reached 129

degrees Fahrenheit. 180 degrees Fahrenheit is the recommended

temperature for water

when brewing coffee. And at 210 degrees Fahrenheit,

a cake is done.

2,000 degrees Fahrenheit is the temperature of lava

fresh outta the ground. But come on. Make your own lava

like Green Science Pro. This guy uses Fresnel lenses to focus the sun's

energy onto whatever he wants. This is a small piece of obsidian,

volcanic glass, which he can melt into actual lava

right in his backyard. Keep in mind that the Sun is having that effect

even though it is 93 million miles away from

Earth. Right up on the surface of the Sun is a different story.

The surface clocks in at 10,000 degrees Fahrenheit,

but the centre, where fusion occurs, is ridiculous.

Temperatures there reach 28

million degrees Fahrenheit, which is also known

as 15 million Kelvin. The Kelvin scale

has units that are the same size as a Celsius degree,

but it's an absolute scale, where 0 is

absolute zero. When matter reaches temperatures as high as those found in

the centre of the Sun,

an enormous amount of energy is radiated

away. If you were to heat only the head

of a pin to the temperature of the centre of the Sun,

it would kill any person within 1,000 miles of it.

Speaking of which, the energy emitted by an object

often tells us a lot about the temperature

of that object. Any object over absolute zero

emits some form of electromagnetic radiation.

You and me, we don't glow visibly, but we do emit

infrared light. We can't see it, but infrared cameras

can. WBT has great videos

and here he is, hiding inside an opaque black

trash bag. Now, we can't see him, but his body is

infra-redly glowing through it. If you want something to be the right

temperature to glow in the

visible spectrum, you'll have to reach the Draper point,

about 798 Kalvin. At this point almost any object

will begin to glow a dead red.

We can calculate the expected wavelength of radiation

coming off of an object because of its temperature and that wavelength

gets smaller and smaller the hotter and hotter the object gets.

It goes from radio waves to microwaves up through infrared divisible,

all the way to x-rays and gamma-rays, which are created in the middle

of our Sun. At temperatures as hot as the Sun,

matter exists in a fourth state. Not solid, not liquid, not gas,

but instead, a state where the electrons wander away from the nuclei

plasma. If you've watched my temperature lean back you know that you could make

plasma by microwaving fire

But don't do it. Besides, our Sun isn't even close to being the hottest thing in

the universe.

I mean, sure, 15 million Kelvin is pretty incredible,

but the peak temperature reached during a thermonuclear explosion

is 350 million

Kelvin, which hardly counts, because the temperature is achieved

so briefly. But inside the core of a star,

8 times larger than our Sun,

on the last day of its life, as it collapses in on itself,

you would reach a temperature of 3

billion Kelvin. Or if you wanna be cool,

3 GigaKelvin. But let's get hotter.

At 1 TeraKelvin, things get weird.

Remember that plasma we were talking about that the Sun is made of?

Well, at 1 TeraKelvin, the electrons aren't the only thing that wander away.

The hedrons themselves, the protons and neutrons in the nucleus

melt into quirks and gluons,

a sort of soup. But how hot

is a TeraKelvin? Frighteningly hot.

There's a star named WR

104, about 8,000 light years away from us.

Its mass is the equivalent of 25

of our Suns, and when it dies,

when it collapses, its internal temperature will be so great

that the energy emitted, the gamma radiation it flings out into space

will be stronger than the entire amount of energy our Sun

will ever create in its entire lifetime.

Gamma ray bursts are quite narrow,

so Earth is most likely safe, but what if it wasn't?

Well, when WR 104 collapses,

even though Earth is 4,702 trillion miles away,

the energy it releases

would still be bad news. Exposure for 10 seconds

would mean losing a quarter of Earth's ozone layer,

resulting in mass extinction, food chain depletion

and starvation

from 8,000 light years away. Closer to home,

right here on earth in Switzerland, scientists have been able to smash

protons

into nuclei, resulting in temperatures much

larger than 1 TeraKelvin. They've been able to reach the

2 to 13 ExaKelvin range.

But we are okay, because those temperatures last

for an incredibly brief moment and only involve a small number

of particles. Remember how we could calculate the wavelength of the

radiation emitted by an object based on its temperature?

Well, if an object were to reach a temperature

of 1.41 times 10 to the 32

Kelvin, the radiation it would admit would have a wavelength of 1.616

times 10 to the -26th nano meters,

which is tiny.

Like so tiny, it actually has a special name.

It is the Planck distance, which according to quantum mechanics

is the shortest distance possible in our universe.

Okay, well what if we added

even more energy? Wouldn't the wavelength get smaller? It's supposed to,

but yet it can't. This is where we've got a problem.

Above 1.41 times 10 to 32 Kelvin,

the Planck temperature, our theories don't work.

The object would become hotter than

temperature. It would be so hot

that what it is would not be considered a

temperature. Theoretically, there is no limit to the amount of energy we could

keep

adding into the system. We just don't know what would happen

if it got hotter than the Planck temperature. Classically,

you could argue that that much energy in one place would instantly cause a black

hole to form.

And a black hole formed from energy has a special name -

a Kugelblitz. So basically, what I'm trying to say

is when you want to tell someone you like that you think they are

hot, so hot that not even science can understand it,

just call them a Kugelblitz. Finally,

here is something fun. The Sun

is about 4.7 billion years old, about halfway through its life cycle

and so far it has burned 100

Earths worth

of fuel, which sounds like a lot, but the Sun

is the size of 300,000 Earths.

Because of that discrepancy, you can have a lot of mathematical fun comparing

your energy output to the Sun's. The Sun is way hotter than us

and it puts out way more energy than us. Bad Astronomy had a lot of fun with this one

and although it doesn't really mean anything, it is technically true,

because of the Sun's enormous size, that one

cubic centimeter of human puts out more

energy than an average cubic centimetre of

the Sun. Which should make you feel

quite warm inside.

И, как всегда, спасибо за смотрящий. [I, kak vsegda , spasibo za smotryashchiy.] [And as always, thanks for watching.]