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You're Technically HOTTER Than The Sun (with XKCD!)
You're Technically HOTTER Than The Sun (with XKCD!)
minutephysics
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3:40 · Sep 8, 2022
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Spoiler alert: this won't end well.
0:04
There are five large worlds that share names with chemical elements: the planets Mercury,
0:08
Uranus, and Neptune, and the dwarf planets Ceres and Pluto.
0:12
What if - 2 have some fun - each world suddenly became composed of
0:16
its corresponding element?
0:17
Mercury and cerium are metals,
0:19
so Mercury and Ceres would mostly just get slightly heavier and shinier.
0:22
From earth they'd look a bit brighter in the night sky,
0:25
enough that Ceres would become visible to the naked eye.
0:28
Unfortunately, the night sky - and human eyes - would get a little harder to find,
0:32
thanks to the other planets.
0:34
Plutonium, uranium and neptunium are radioactive;
0:37
plutonium and uranium do have (non-fissile) isotopes
0:40
which decay slowly and mainly produce a bit of heat.
0:43
A small lump of Uranium’s most common
0:45
and stable isotope wouldn’t even be hot to the touch.
0:47
But if you collected it into a planet-size ball,
0:49
the tiny amount of heat produced by each part would add up to heat
0:52
up the planet to thousands of degrees.
0:54
* It might seem strange
0:55
that something that's cool in small amounts would be hot
0:58
when collected together in a big ball,
0:59
but this is just a consequence of geometry and the physics of radiating heat.
1:03
Since volume grows faster than surface area,
1:05
and the volume is where the heat is produced,
1:07
the interiors of large heat-producing objects produce more heat relative to their surface areas.
1:12
But thermodynamics doesn't allow objects to just radiate more heat - they have to
1:16
get hotter to do
1:17
so;
1:17
the hotter they are, the more heat they're allowed to radiate.
1:20
So a large heat-producing object will produce more heat than it can radiate away
1:24
until that heat builds up (enough)
1:25
and the object gets hot - hot enough
1:27
that it can radiate away enough heat.
1:29
Really big objects can get extremely hot from just a tiny amount of heat
1:33
production per unit of volume.
1:34
Like, the Sun.
1:35
A cup of the sun's core * produces about 60 milliwatts of thermal energy.
1:39
By volume, that’s about the same heat production rate
1:41
as the body of a lizard,
1:42
and substantially less than that of a human.
1:44
In a sense, you are hotter than the Sun—there’s just not
1:48
as much of you.
1:48
But we were talking about Uranus, which there is a lot of,
1:51
and which would get really really hot if made from uranium.
1:54
The real Uranus, lit by the sun,
1:56
is too dim to see with the naked eye.
1:58
But the superhot uranium Uranus would glow bright enough to be visible like an
2:01
ordinary star in the night sky.
2:03
And plutonium Pluto would heat up
2:05
and glow enough that from earth it would also be visible to the naked
2:08
eye - though just barely.
2:09
Except you wouldn't be spending much time looking at the night sky anymore,
2:12
thanks to neptunium Neptune.
2:14
Even the most stable neptunium isotope is fissile,
2:17
so 237Neptune would instantly undergo a runaway fission chain reaction,
2:20
converting the planet into an expanding cloud of high-energy particles and X-rays.
2:24
Around four hours later, the shock wave would reach—and completely obliterate—the Earth,
2:29
stripping away its surface and everything on it and leaving behind a molten blob.
2:32
We'd have gotten similar results for Uranus
2:34
and Pluto if we'd instead used fissile isotopes of uranium
2:37
or plutonium,
2:38
though as a bonus Uranus' shock wave would reach
2:40
(and destroy) us about an hour faster than Neptune's.
2:43
There's a simple takeaway from all this:
2:45
If you have a choice between isotopes
2:47
and you’re not sure
2:48
which to pick,
2:48
go for the most stable one.
2:50
And just stay away from neptunium altogether.
2:53
Ok - I'll avoid neptunium.
2:55
But what if to be silly we filled the solar system with soup out
2:58
to Jupiter?
2:59
Or what if to pass the time we spun the earth up
3:01
so that a day lasted a second?
3:03
Or what if to avoid getting in trouble you tried to read every single
3:06
law that applies to you?
3:07
What if to answer these questions you could just read a book called What
3:11
if 2,
3:11
that this video is based on and supported by?
3:13
What if two reasons to read what
3:15
if 2 are that it was written by Randall Munroe
3:18
and that it has over 60 answers to important "what
3:22
if" questions like "what
3:23
if Japan disappeared?"
3:24
What if to read what
3:24
if 2 you just had to look at the information in the description of
3:27
this video?
3:27
What if two be clear, is available wherever books are sold,
3:32
and when you get yourself a copy, then you can ask "what if," too.
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