Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated:
1
00:00:01,934 --> 00:00:06,167
The sun, our nuclear powerhouse.
2
00:00:07,135 --> 00:00:16,231
Our star, its light powers our world...and us.
3
00:00:16,264 --> 00:00:19,632
Without light, we would not be alive.
4
00:00:20,698 --> 00:00:23,898
Starting deep inside the sun,
5
00:00:23,931 --> 00:00:26,131
We follow the brutal journey
6
00:00:26,163 --> 00:00:31,462
Of a single, tiny package of light -- A photon.
7
00:00:31,495 --> 00:00:34,663
The ride that any photon takes
to get to my eyes
8
00:00:34,694 --> 00:00:37,294
When i look up at the sun
is an amazing one.
9
00:00:37,328 --> 00:00:39,794
From its ancient birth
in the sun's core
10
00:00:39,828 --> 00:00:41,861
To its escape from the surface.
11
00:00:44,327 --> 00:00:45,961
The light reaching me
from the sun
12
00:00:45,993 --> 00:00:48,726
Was produced before there
was even human civilization.
13
00:00:48,760 --> 00:00:50,028
It's an incredible idea.
14
00:00:51,992 --> 00:00:53,459
Join our photon
15
00:00:53,492 --> 00:00:56,559
On its incredible
million-Year journey
16
00:00:56,593 --> 00:01:01,624
Through the most hostile
environment in the solar system
17
00:01:01,659 --> 00:01:05,124
To bring light and life
to earth.
18
00:01:20,953 --> 00:01:25,720
The universe,
home to billions of galaxies...
19
00:01:27,786 --> 00:01:30,719
...each made
of billions of stars.
20
00:01:33,885 --> 00:01:38,251
And, in an unremarkable corner
of our galaxy, the milky way,
21
00:01:38,284 --> 00:01:42,051
Lies the sun,
our closest star...
22
00:01:43,950 --> 00:01:48,149
...a dazzling sphere
of intense light,
23
00:01:48,182 --> 00:01:49,883
Too bright for the naked eye.
24
00:01:51,849 --> 00:01:57,149
But strip away that glare,
and the sun transforms
25
00:01:57,182 --> 00:01:59,147
Into a giant ball
26
00:01:59,182 --> 00:02:03,982
Of super heated gas
dominating our cosmic stage.
27
00:02:07,613 --> 00:02:09,612
The sun is really
the star of the show.
28
00:02:09,647 --> 00:02:13,179
The sun is the parent
of the whole solar system.
29
00:02:13,212 --> 00:02:16,712
It provides its children,
the planets,
30
00:02:16,745 --> 00:02:18,178
With everything they need.
31
00:02:18,212 --> 00:02:22,177
We depend on the sun for energy,
for light, for warmth.
32
00:02:22,211 --> 00:02:24,810
We would not exist
without the sun.
33
00:02:27,509 --> 00:02:30,275
The sun
generates heat and light,
34
00:02:30,310 --> 00:02:32,942
The energy source
for all life on earth.
35
00:02:32,975 --> 00:02:36,942
All of the energy
that my body uses,
36
00:02:36,974 --> 00:02:39,275
Literally what i'm doing
to talk to you right now,
37
00:02:39,307 --> 00:02:40,707
Came from the sun.
38
00:02:40,741 --> 00:02:43,741
The sun truly is the creator
of all of the life around us.
39
00:02:45,407 --> 00:02:48,106
The sun
is a constantly exploding
40
00:02:48,139 --> 00:02:51,506
Nuclear bomb,
violent and essential.
41
00:02:53,938 --> 00:02:57,737
Our entire existence
is powered by the energy
42
00:02:57,771 --> 00:02:59,770
Emitted in those
nuclear reactions in the sun.
43
00:02:59,805 --> 00:03:02,870
We are here because of the light
from the sun.
44
00:03:02,903 --> 00:03:05,037
We are here because
of those nuclear reactions,
45
00:03:05,070 --> 00:03:07,703
And no aspect of our existence
could persist
46
00:03:07,736 --> 00:03:08,969
If it wasn't there.
47
00:03:11,735 --> 00:03:14,501
Light is
one of the basic building blocks
48
00:03:14,536 --> 00:03:15,569
Of the universe.
49
00:03:20,301 --> 00:03:22,900
I find light to be probably
50
00:03:22,932 --> 00:03:24,566
The most amazing thing
in the universe.
51
00:03:24,599 --> 00:03:26,599
It's so important in everything.
52
00:03:26,633 --> 00:03:28,933
I mean, it's everything.
It's everywhere.
53
00:03:28,966 --> 00:03:32,466
So, it's such a fundamental part
of everything that exists.
54
00:03:32,498 --> 00:03:37,597
Fundamental and fast.
55
00:03:37,630 --> 00:03:39,830
The fastest thing
in the cosmos...
56
00:03:41,796 --> 00:03:45,829
...traveling at 186,000 miles
per second.
57
00:03:47,962 --> 00:03:50,428
The sun is about
93 million miles away from us.
58
00:03:50,462 --> 00:03:52,594
So, going at 186,000 miles
per second,
59
00:03:52,628 --> 00:03:53,728
That's about eight minutes.
60
00:03:53,761 --> 00:03:55,594
But those eight minutes
61
00:03:55,629 --> 00:03:59,262
Are just the brief last leg
of its incredible journey.
62
00:04:04,194 --> 00:04:06,926
It may have taken the light
as much as a million years
63
00:04:06,958 --> 00:04:09,326
To escape from
the sun's raging interior...
64
00:04:12,992 --> 00:04:15,758
...which means the light
we're seeing right now
65
00:04:15,790 --> 00:04:17,992
Was created long before
66
00:04:18,023 --> 00:04:20,158
Our ancestors
left the plains of africa.
67
00:04:23,557 --> 00:04:25,323
When i first learned this fact,
68
00:04:25,357 --> 00:04:27,356
I was already
a practicing scientist.
69
00:04:27,389 --> 00:04:29,355
I had never really
thought about that,
70
00:04:29,388 --> 00:04:31,922
And on first glance,
it just blew me away.
71
00:04:31,954 --> 00:04:34,088
Right now the light
reaching me from the sun
72
00:04:34,122 --> 00:04:37,021
Was produced before there
was even human civilization.
73
00:04:37,054 --> 00:04:39,388
And yet, the minute it gets
to the surface of the sun,
74
00:04:39,422 --> 00:04:42,521
It races away and is here
eight minutes after that.
75
00:04:42,554 --> 00:04:45,687
It's an incredible idea.
76
00:04:45,720 --> 00:04:48,619
The ride that any photon takes
to get to my eyes
77
00:04:48,653 --> 00:04:52,086
When i look up at the sun
is an amazing one.
78
00:04:52,119 --> 00:04:55,419
That ride starts
deep in the belly of our star.
79
00:04:56,817 --> 00:04:59,983
If we could open up the sun,
80
00:05:00,017 --> 00:05:03,650
We'd see layers
of dense hydrogen gas
81
00:05:03,683 --> 00:05:07,248
Hundreds of thousands
of miles deep.
82
00:05:07,283 --> 00:05:12,315
And at its center, the core,
the sun gives birth to light...
83
00:05:16,947 --> 00:05:19,479
...forged in one of the most
violent reactions
84
00:05:19,512 --> 00:05:23,280
In the universe, nuclear fusion.
85
00:05:29,646 --> 00:05:32,812
The specific nuclear reaction
that powers the sun is fusion,
86
00:05:32,846 --> 00:05:34,812
Fusion of hydrogen into helium.
87
00:05:34,845 --> 00:05:37,377
You take two hydrogen atoms,
you ram them together,
88
00:05:37,410 --> 00:05:39,778
And what's left over
is a helium atom.
89
00:05:39,810 --> 00:05:41,575
It sounds simple enough,
90
00:05:41,610 --> 00:05:43,877
But it's not.
91
00:05:43,910 --> 00:05:46,410
It's actually hard
to get two atoms to fuse.
92
00:05:46,442 --> 00:05:48,175
Two photons
have the same charge.
93
00:05:48,209 --> 00:05:50,909
They're both positively charged.
They want to repel each other.
94
00:05:52,608 --> 00:05:54,973
Protons don't like
to get close together.
95
00:05:55,007 --> 00:05:57,341
They have to come together
with a huge amount
96
00:05:57,374 --> 00:05:59,640
Of energy or velocity
97
00:05:59,673 --> 00:06:01,673
To get close enough
to begin to fuse,
98
00:06:01,706 --> 00:06:04,605
And that's very, very rare.
99
00:06:04,639 --> 00:06:06,805
To force protons together
100
00:06:06,838 --> 00:06:09,939
Takes immense amounts
of heat and pressure...
101
00:06:11,937 --> 00:06:15,903
...generated by
the invisible hand of gravity.
102
00:06:15,937 --> 00:06:19,536
The sun contains 99.8%
of all the matter
103
00:06:19,571 --> 00:06:21,037
In the solar system.
104
00:06:23,670 --> 00:06:25,968
That's a lot of mass.
105
00:06:26,002 --> 00:06:28,835
All that mass
pulls the sun together
106
00:06:28,867 --> 00:06:31,868
With unimaginable
gravitational force.
107
00:06:34,267 --> 00:06:36,333
With gravity
crushing things down,
108
00:06:36,367 --> 00:06:38,734
Things get close enough together
and nuclear fusion happens.
109
00:06:39,967 --> 00:06:43,233
In this nuclear compactor,
110
00:06:43,265 --> 00:06:44,898
Hydrogen atoms slam together
111
00:06:44,933 --> 00:06:49,466
100 million quadrillion
quadrillion times each second.
112
00:06:53,698 --> 00:06:59,198
Some of these collisions
are so powerful that atoms fuse,
113
00:06:59,230 --> 00:07:01,162
Releasing energy.
114
00:07:01,196 --> 00:07:04,996
When the protons
come together to bind together,
115
00:07:05,030 --> 00:07:06,662
They lose a little bit of mass,
116
00:07:06,695 --> 00:07:08,995
And that mass
gets converted into energy.
117
00:07:09,027 --> 00:07:11,660
And every second of every day,
118
00:07:11,695 --> 00:07:17,560
About five million tons of stuff
is being converted to energy.
119
00:07:17,594 --> 00:07:19,227
It's amazing.
120
00:07:24,426 --> 00:07:28,092
Each collision
creates a tiny burst of energy,
121
00:07:28,124 --> 00:07:34,057
A packet of light impossibly
small and incredibly powerful.
122
00:07:36,790 --> 00:07:40,889
Somehow, our photon
will deliver its energy to earth
123
00:07:40,924 --> 00:07:46,121
Where it will power the planet
and make life possible.
124
00:07:46,155 --> 00:07:50,388
But right now it's nothing like
the light we see.
125
00:07:50,422 --> 00:07:55,421
It has massive amounts
of energy, and it's deadly.
126
00:08:06,951 --> 00:08:11,451
The light we see
from our star is old...
127
00:08:11,484 --> 00:08:13,284
much older
than the eight minutes it takes
128
00:08:13,316 --> 00:08:15,184
To get from the sun to earth.
129
00:08:17,615 --> 00:08:22,116
That short leap across space is
the end of a long, hard journey
130
00:08:22,149 --> 00:08:24,449
That starts deep inside our sun.
131
00:08:24,482 --> 00:08:26,114
When we look at the sun,
132
00:08:26,149 --> 00:08:29,782
We say, "how beautiful,
how elegant, and how simple."
133
00:08:29,814 --> 00:08:30,914
Light is formed in the sun,
134
00:08:30,947 --> 00:08:33,780
And it shines
and lights up our world.
135
00:08:33,814 --> 00:08:35,247
Well, not so fast.
136
00:08:35,280 --> 00:08:37,146
It's actually very complex.
137
00:08:38,978 --> 00:08:40,112
The journey starts
138
00:08:40,146 --> 00:08:42,779
In the immense heat
of the sun's core.
139
00:08:48,478 --> 00:08:52,143
Crushed together
by the sun's enormous gravity,
140
00:08:52,176 --> 00:08:54,944
Atoms smash into each other
and fuse...
141
00:08:56,476 --> 00:09:01,775
...releasing a tiny packet
of energy, photon of light...
142
00:09:03,742 --> 00:09:07,974
...far smaller
than an atom with no mass.
143
00:09:08,007 --> 00:09:10,874
Photons travel
faster than anything else,
144
00:09:10,906 --> 00:09:15,607
And they never stop moving.
145
00:09:20,338 --> 00:09:24,039
Photons don't just come
from the core of stars.
146
00:09:26,205 --> 00:09:27,538
So, where does light come from?
147
00:09:27,572 --> 00:09:30,405
The short answer is,
matter makes it,
148
00:09:30,438 --> 00:09:32,271
And the amount of light
that it creates
149
00:09:32,304 --> 00:09:33,571
Depends on its temperature.
150
00:09:34,803 --> 00:09:36,670
Every piece of matter
in the universe
151
00:09:36,704 --> 00:09:39,170
Above absolute zero degrees
152
00:09:39,204 --> 00:09:42,003
Produces light,
including humans.
153
00:09:43,701 --> 00:09:46,200
We humans
are emitting light all the time
154
00:09:46,234 --> 00:09:49,633
Because we're alive, we're warm,
we're not at a zero temperature.
155
00:09:49,667 --> 00:09:52,967
So, in fact we are emitting
infrared radiation,
156
00:09:53,000 --> 00:09:54,999
Often called heat radiation.
157
00:09:55,032 --> 00:09:57,398
But all matter emits light.
158
00:09:57,431 --> 00:10:00,633
Even someone as cool as me,
i'm creating light right now.
159
00:10:02,931 --> 00:10:04,464
The light we see
160
00:10:04,498 --> 00:10:06,797
Can be split
into the colors of the rainbow.
161
00:10:06,830 --> 00:10:09,330
Each color is photons of light
162
00:10:09,364 --> 00:10:12,230
With slightly different amounts
of energy.
163
00:10:15,196 --> 00:10:16,562
And what we can see
164
00:10:16,595 --> 00:10:18,864
Is only a fraction
of the light spectrum.
165
00:10:21,027 --> 00:10:23,327
Our eyes are actually
imperfect detectors.
166
00:10:23,360 --> 00:10:24,628
We know about visible light,
167
00:10:24,662 --> 00:10:26,927
The type of light
that our eyes are sensitive to,
168
00:10:26,960 --> 00:10:28,693
But that's only a small range
of energies.
169
00:10:28,728 --> 00:10:33,327
Light comes at higher and lower
energies than we can detect.
170
00:10:33,359 --> 00:10:34,759
Using special cameras,
171
00:10:34,792 --> 00:10:38,393
We can see the infrared light
that humans emit.
172
00:10:39,993 --> 00:10:41,825
This infrared light
173
00:10:41,859 --> 00:10:44,825
Has less energy
than the visible light we see.
174
00:10:48,224 --> 00:10:52,924
Some light is too energetic
to see,
175
00:10:52,956 --> 00:10:56,989
Like ultraviolets,
x-Rays, and gamma rays.
176
00:11:01,689 --> 00:11:07,187
The vast, hot sun
generates all forms of light.
177
00:11:07,221 --> 00:11:10,787
But in the nuclear furnace
of the sun's core,
178
00:11:10,819 --> 00:11:14,718
Every photon starts out
as a gamma ray,
179
00:11:14,752 --> 00:11:19,451
The most energetic form
of light in the universe.
180
00:11:19,484 --> 00:11:20,619
And when
a nuclear reaction happens,
181
00:11:20,652 --> 00:11:22,951
It emits
an amazing amount of energy,
182
00:11:22,984 --> 00:11:25,651
The energy much, much bigger
than visible light --
183
00:11:25,684 --> 00:11:28,218
Gamma rays, we call them.
184
00:11:28,251 --> 00:11:30,617
Literally almost a million times
185
00:11:30,650 --> 00:11:35,449
Or at least 10,000 times
the energy of the light we see.
186
00:11:35,782 --> 00:11:39,015
Gamma rays
can transform and even kill.
187
00:11:39,149 --> 00:11:40,649
There's a reason why gamma rays
188
00:11:40,682 --> 00:11:42,481
Turned bruce banner
into the hulk.
189
00:11:42,514 --> 00:11:45,147
Gamma rays are a very dangerous
form of light.
190
00:11:45,179 --> 00:11:46,813
They can travel into your body
191
00:11:46,846 --> 00:11:48,414
And when they interact
with the matter,
192
00:11:48,447 --> 00:11:51,278
They can break apart atoms.
193
00:11:51,312 --> 00:11:53,080
Fortunately for us,
194
00:11:53,113 --> 00:11:57,079
Our gamma-Ray photon can't
head straight out of the sun.
195
00:12:04,110 --> 00:12:07,211
If the sun
were not this hot ball of gas,
196
00:12:07,245 --> 00:12:09,076
Then upon being created,
197
00:12:09,110 --> 00:12:12,576
A photon would immediately
escape from the sun
198
00:12:12,609 --> 00:12:14,043
And it would be
a gamma-Ray photon,
199
00:12:14,076 --> 00:12:19,109
A very energetic photon,
not very good for life on earth.
200
00:12:19,142 --> 00:12:21,709
After its birth as a gamma ray,
201
00:12:21,743 --> 00:12:25,075
Our photon starts
to race out from the sun's core
202
00:12:25,107 --> 00:12:26,141
At the speed of light.
203
00:12:30,440 --> 00:12:34,474
But it encounters an obstacle
course of epic proportions.
204
00:12:36,273 --> 00:12:38,639
A journey
that should take seconds
205
00:12:38,672 --> 00:12:40,904
Slows to a cosmic crawl.
206
00:12:42,403 --> 00:12:46,571
It takes on average
about 100,000 years
207
00:12:46,604 --> 00:12:49,737
For a photon to make it
from the middle of the sun,
208
00:12:49,770 --> 00:12:52,471
Where it was created,
to the outermost edge,
209
00:12:52,504 --> 00:12:55,802
Where it gets emitted
into space -- 100,000 years.
210
00:12:55,836 --> 00:12:58,768
If it had traveled
in a straight line unimpeded,
211
00:12:58,801 --> 00:13:00,968
It would have taken two seconds.
212
00:13:01,001 --> 00:13:04,334
What could possibly
slow a photon
213
00:13:04,368 --> 00:13:08,001
Moving at the speed of light?
214
00:13:08,033 --> 00:13:16,533
Something slams on the brakes --
Huge, hot, dense.
215
00:13:16,566 --> 00:13:21,465
So powerful,
it doesn't just slow light,
216
00:13:21,498 --> 00:13:23,165
It transforms it.
217
00:13:34,994 --> 00:13:36,863
In the sun's core,
218
00:13:36,896 --> 00:13:41,428
Nuclear fusion releases
a tiny bundle of energy...
219
00:13:43,594 --> 00:13:45,660
...a photon of light.
220
00:13:46,560 --> 00:13:51,426
It races outwards
at 186,000 miles per second.
221
00:13:54,825 --> 00:13:57,526
At that speed,
it should take two seconds
222
00:13:57,557 --> 00:14:00,591
To travel through the
sun's interior to the surface.
223
00:14:04,724 --> 00:14:09,689
But something turns seconds
into an eternity.
224
00:14:09,723 --> 00:14:11,090
The sun is so dense
225
00:14:11,123 --> 00:14:13,689
That to get through all
of the different layers of gas,
226
00:14:13,723 --> 00:14:16,189
This poor little piece of light
takes hundreds of thousands,
227
00:14:16,221 --> 00:14:18,254
If not a million years,
to get to the surface.
228
00:14:20,888 --> 00:14:22,687
So,
when you're looking at the sun,
229
00:14:22,720 --> 00:14:23,921
You're looking at the light
230
00:14:23,953 --> 00:14:27,252
Emitted from reactions
a million years ago.
231
00:14:27,285 --> 00:14:28,752
Our newborn photon
232
00:14:28,787 --> 00:14:30,586
Leaves the core
at the speed of light
233
00:14:30,620 --> 00:14:33,885
Only to run smack
into a dense soup
234
00:14:33,918 --> 00:14:37,918
Of hydrogen atoms,
a photon's nightmare,
235
00:14:37,951 --> 00:14:42,984
That stretches
for over 400,000 miles.
236
00:14:43,018 --> 00:14:45,350
If you're a photon
born in the center of the sun,
237
00:14:45,383 --> 00:14:47,550
You have a heck of a journey
ahead of you.
238
00:14:47,582 --> 00:14:48,916
It's actually pretty hard
239
00:14:48,950 --> 00:14:51,749
For light generated in
the core of the sun to get out
240
00:14:51,782 --> 00:14:54,083
Because there's a lot of sun
in the way,
241
00:14:54,115 --> 00:14:55,581
And it's extremely dense.
242
00:14:55,615 --> 00:14:59,914
The radiation zone
surrounds the core of the sun.
243
00:15:02,913 --> 00:15:05,646
The zone is made
of hydrogen gas,
244
00:15:05,679 --> 00:15:07,912
But not a gas as we think of it.
245
00:15:10,379 --> 00:15:13,346
The sheer weight
of all the material above
246
00:15:13,379 --> 00:15:18,711
Compresses the radiation zone
until it's denser than lead
247
00:15:18,745 --> 00:15:21,077
And nearly impossible
to pass through.
248
00:15:24,876 --> 00:15:27,242
A photon produced
in the center of the sun
249
00:15:27,275 --> 00:15:29,142
Knows where it wants to go.
250
00:15:29,175 --> 00:15:32,009
It wants to go to the edge
where it's cool,
251
00:15:32,043 --> 00:15:33,875
And it wants to get out.
252
00:15:33,909 --> 00:15:36,842
But it's got 400,000 miles
253
00:15:36,875 --> 00:15:39,775
Of all these opaque gases
blocking its way.
254
00:15:39,808 --> 00:15:45,206
These gases aren't
just dense -- They're hot,
255
00:15:45,240 --> 00:15:50,639
Superheated to over 12 1/2
million degrees fahrenheit.
256
00:15:50,672 --> 00:15:52,606
The gas in the radiation zone
257
00:15:52,640 --> 00:15:56,739
Is transformed into
what scientists call plasma.
258
00:15:59,669 --> 00:16:02,871
Plasma is the fourth state
of matter.
259
00:16:02,904 --> 00:16:07,703
Atoms in normal matter have a
nucleus with orbiting electrons.
260
00:16:07,836 --> 00:16:11,169
In plasma, the atoms
have been torn apart
261
00:16:11,202 --> 00:16:15,035
And the electrons ripped away.
262
00:16:15,068 --> 00:16:19,067
Here on earth, we're familiar
with the three main states
263
00:16:19,101 --> 00:16:21,168
Of matter
that we're taught in school --
264
00:16:21,201 --> 00:16:23,834
Solids, liquids, and gases.
265
00:16:23,866 --> 00:16:27,000
You know, we have the atmosphere
as a gas, the oceans are water,
266
00:16:27,033 --> 00:16:29,533
The ground
that i stand on is solid.
267
00:16:29,566 --> 00:16:31,433
But in fact,
most of the universe,
268
00:16:31,466 --> 00:16:35,265
Including stars,
consists of plasma.
269
00:16:37,831 --> 00:16:39,664
Compared to
the rest of the universe,
270
00:16:39,698 --> 00:16:43,063
Earth is a calm place.
271
00:16:43,096 --> 00:16:44,396
Most of the time,
272
00:16:44,429 --> 00:16:47,663
It's not hot or violent enough
here to create plasma.
273
00:16:49,928 --> 00:16:54,694
The best place to witness
the power of plasma on earth
274
00:16:54,728 --> 00:16:56,395
Is inside a lightning strike.
275
00:16:59,427 --> 00:17:05,658
Temperatures inside a bolt can
reach 53,000 degrees fahrenheit,
276
00:17:05,693 --> 00:17:08,725
Enough to momentarily
rip a few atoms apart.
277
00:17:10,759 --> 00:17:13,258
The plasma lasts an instant.
278
00:17:13,291 --> 00:17:17,059
Then the electrons rebind
and it's gone.
279
00:17:19,890 --> 00:17:22,355
But in our massive sun,
280
00:17:22,390 --> 00:17:25,290
The plasma
lasts for billions of years
281
00:17:25,323 --> 00:17:26,489
And makes up
282
00:17:26,524 --> 00:17:30,089
The entire 200,000-Mile-Deep
radiation zone.
283
00:17:32,588 --> 00:17:34,688
Worse for our photon,
284
00:17:34,720 --> 00:17:40,253
The plasma is electrically
charged, forming a cosmic trap.
285
00:17:43,953 --> 00:17:46,418
And a plasma
is opaque to radiation
286
00:17:46,452 --> 00:17:49,385
Because light
interacts much more strongly
287
00:17:49,417 --> 00:17:51,083
With electronically charged
objects
288
00:17:51,118 --> 00:17:52,783
Than with neutral objects.
289
00:17:52,818 --> 00:17:54,318
So, when you
have a neutral atom,
290
00:17:54,350 --> 00:17:56,217
Light in general can pass by.
291
00:17:56,251 --> 00:17:57,817
But when you separated
the charges
292
00:17:57,850 --> 00:17:59,284
And you have positive
and negative charges
293
00:17:59,318 --> 00:18:03,384
Located everywhere,
the light can't make it through.
294
00:18:03,417 --> 00:18:06,215
Our photon,
in the form of a gamma ray,
295
00:18:06,248 --> 00:18:08,181
Has entered the radiation zone
296
00:18:08,215 --> 00:18:11,881
And smashed
into a charged plasma particle.
297
00:18:11,915 --> 00:18:13,380
For a fraction of a second,
298
00:18:13,415 --> 00:18:18,347
The particle absorbs the photon,
then spits it back out,
299
00:18:18,379 --> 00:18:22,113
And the photon collides
with another particle.
300
00:18:25,244 --> 00:18:27,513
Every time it goes
a little bit of a distance,
301
00:18:27,545 --> 00:18:29,245
It basically slams into an atom,
302
00:18:29,279 --> 00:18:32,545
Is absorbed and readmitted
in some random direction.
303
00:18:32,579 --> 00:18:34,378
So, instead of just flying out,
304
00:18:34,410 --> 00:18:37,443
It's bouncing around countless,
countless, countless times
305
00:18:37,476 --> 00:18:39,277
Until finally, it reaches
the edge of the star.
306
00:18:40,776 --> 00:18:44,042
It's an atomic game
of basketball
307
00:18:44,074 --> 00:18:47,975
With a court
representing the radiation zone.
308
00:18:48,009 --> 00:18:51,942
The players stand in
for the particles and the plasma
309
00:18:51,975 --> 00:18:53,774
And the ball is the photon.
310
00:18:55,406 --> 00:18:56,941
So, the basketball
311
00:18:56,973 --> 00:19:00,840
Is being thrown from one player
to another seemingly randomly.
312
00:19:00,874 --> 00:19:04,173
It's not making a lot
of progress down the court,
313
00:19:04,205 --> 00:19:07,173
But it is gradually
making progress.
314
00:19:07,205 --> 00:19:09,438
Gradually over time, it is going
315
00:19:09,472 --> 00:19:12,538
From the hotter parts
of the core outward
316
00:19:12,570 --> 00:19:14,503
Toward cooler temperatures.
317
00:19:14,537 --> 00:19:16,271
That's where it wants to get.
318
00:19:16,303 --> 00:19:18,204
It's a random-Looking process,
319
00:19:18,238 --> 00:19:22,736
But it's directed in
a certain direction with time.
320
00:19:25,901 --> 00:19:28,468
The photon wants
to go straight up the court --
321
00:19:28,502 --> 00:19:31,435
Its quickest route --
322
00:19:31,467 --> 00:19:34,033
But is bounced and thrown
around the radiation zone,
323
00:19:34,068 --> 00:19:36,268
Slowing to a crawl.
324
00:19:38,899 --> 00:19:43,864
This bruising process
transforms the photon.
325
00:19:43,898 --> 00:19:45,931
When a photon,
a little packet of light,
326
00:19:45,965 --> 00:19:47,665
Is created
in the center of the star,
327
00:19:47,697 --> 00:19:50,931
It's actually a gamma ray,
super high energy bit of light.
328
00:19:50,965 --> 00:19:53,898
And it can't go very far
because as soon as it does,
329
00:19:53,932 --> 00:19:56,365
Boom, it hits another atom
and gets absorbed.
330
00:19:58,663 --> 00:19:59,797
Every time it does this,
331
00:19:59,830 --> 00:20:02,629
It loses
a little bit of that energy.
332
00:20:04,628 --> 00:20:06,462
Over several
hundred thousand years,
333
00:20:06,495 --> 00:20:10,794
Sometimes even a million,
the photon keeps bouncing
334
00:20:10,829 --> 00:20:15,128
Through the dense
radiation zone.
335
00:20:15,160 --> 00:20:20,059
Each collision saps
a tiny bit of energy,
336
00:20:20,092 --> 00:20:23,560
Transforming it
from a lethal gamma-Ray photon
337
00:20:23,592 --> 00:20:25,627
To a lower energy x-Ray.
338
00:20:27,825 --> 00:20:31,292
Nearly a million years
after its creation in the core,
339
00:20:31,325 --> 00:20:35,789
The photon has made it
through the radiation zone,
340
00:20:35,824 --> 00:20:38,690
But its quest to escape
is not over yet.
341
00:20:40,655 --> 00:20:42,822
It's about to hitch a wild ride
342
00:20:42,856 --> 00:20:46,189
On the sun's ferocious
internal roller coaster...
343
00:20:47,922 --> 00:20:51,621
...a place so violent,
it makes the sun roar.
344
00:21:10,850 --> 00:21:14,282
A photon,
nature's energy-Delivery system,
345
00:21:14,317 --> 00:21:16,717
Has spent up to a million years
346
00:21:16,750 --> 00:21:18,715
In the maze
of the sun's interior
347
00:21:18,748 --> 00:21:20,782
On its journey toward the earth.
348
00:21:23,015 --> 00:21:27,114
The photon has fought its way
through 3/4 of the sun's radius.
349
00:21:29,647 --> 00:21:31,848
Battered and sapped of energy,
350
00:21:31,880 --> 00:21:35,281
It is morphed from
a deadly gamma ray to an x-Ray.
351
00:21:37,980 --> 00:21:42,412
But now it enters the mysterious
boiling layer of the sun,
352
00:21:42,444 --> 00:21:44,146
The convection zone.
353
00:21:48,310 --> 00:21:51,711
The convection zone
lies between the radiation zone
354
00:21:51,744 --> 00:21:57,309
And the sun's surface
and is 125,000 miles deep.
355
00:21:59,542 --> 00:22:03,408
We can't see
the convection zone directly.
356
00:22:03,442 --> 00:22:08,406
This region of the sun is still
opaque to our telescopes,
357
00:22:08,441 --> 00:22:10,475
But we can hear it.
358
00:22:14,573 --> 00:22:19,805
Nasa's solar dynamics
observatory listens to the sun.
359
00:22:19,839 --> 00:22:23,771
The sound it picks up
is too deep for humans to hear,
360
00:22:23,805 --> 00:22:27,338
But if you speed up
40 days' recording
361
00:22:27,370 --> 00:22:31,503
Into a few seconds,
this is what you get.
362
00:22:35,236 --> 00:22:38,603
It's the sound of chaos.
363
00:22:41,567 --> 00:22:43,968
Since we can't see into the sun,
364
00:22:44,001 --> 00:22:46,769
Its sound
is vital to scientists.
365
00:22:50,000 --> 00:22:55,165
When a gun fires, the bullet
rushes out and smashes into air,
366
00:22:55,199 --> 00:22:57,767
Creating waves of turbulence.
367
00:23:00,897 --> 00:23:02,865
When we hear the gun firing,
368
00:23:02,898 --> 00:23:06,231
These waves
vibrate our eardrums.
369
00:23:09,396 --> 00:23:11,931
What we see here is sound.
370
00:23:11,962 --> 00:23:16,696
The sun works the same way
on a much larger scale.
371
00:23:18,996 --> 00:23:21,961
When we see these waves
moving across,
372
00:23:21,995 --> 00:23:24,962
What we're looking at
is when material moves up
373
00:23:24,995 --> 00:23:27,562
From inside the sun
and it makes noise.
374
00:23:27,594 --> 00:23:29,026
It just, like,
ran into a surface.
375
00:23:29,059 --> 00:23:32,259
It just ran into a wall,
and it generates sound.
376
00:23:32,294 --> 00:23:35,826
And we see that sound
moving all around the sun.
377
00:23:35,860 --> 00:23:38,659
Sound waves
crashing through the plasma
378
00:23:38,691 --> 00:23:42,124
Create ripples
in the sun's surface.
379
00:23:42,159 --> 00:23:44,425
And all we see
are these ripples.
380
00:23:44,458 --> 00:23:47,325
Those are the actual sound waves
of the sun,
381
00:23:47,357 --> 00:23:49,356
And they move
around the entire sun.
382
00:23:49,390 --> 00:23:50,956
They move down inside the sun.
383
00:23:50,989 --> 00:23:52,923
They move back up
to the surface.
384
00:23:52,956 --> 00:23:54,956
By tracking the sound,
385
00:23:54,990 --> 00:23:57,489
Scientists
can see the invisible.
386
00:23:59,954 --> 00:24:01,521
They pick up sound waves
387
00:24:01,553 --> 00:24:04,021
Smashing
against the sun's surface
388
00:24:04,055 --> 00:24:06,988
And resonating
throughout the solar interior...
389
00:24:08,886 --> 00:24:12,587
...revealing a violent,
boiling convection zone.
390
00:24:16,786 --> 00:24:20,485
The sun can be said
to be ringing.
391
00:24:20,518 --> 00:24:22,818
You have this hot gas rising.
392
00:24:22,851 --> 00:24:24,716
You have cool gas falling.
393
00:24:24,750 --> 00:24:26,517
You have all this turbulence.
394
00:24:26,550 --> 00:24:30,050
You have so much action going on
that it causes the sun to ring.
395
00:24:30,082 --> 00:24:34,182
Columns of gases rise and fall,
396
00:24:34,215 --> 00:24:39,281
Churned by heat from below.
397
00:24:39,315 --> 00:24:40,948
If you look at water boiling,
398
00:24:40,981 --> 00:24:44,881
Bubbles of gas or water are
rising up because they're hot.
399
00:24:44,915 --> 00:24:47,047
And then they cool off,
and then they sink back down.
400
00:24:47,079 --> 00:24:49,512
And if you look
at a pot of boiling water,
401
00:24:49,546 --> 00:24:52,547
That's the same phenomena
that's going on the sun,
402
00:24:52,579 --> 00:24:55,878
But with hot plasma
instead of water.
403
00:24:55,913 --> 00:24:58,245
At the bottom
of the convection zone,
404
00:24:58,279 --> 00:25:01,612
Photons smash
into atoms in the plasma,
405
00:25:01,645 --> 00:25:03,212
Heating them to a boil.
406
00:25:04,244 --> 00:25:07,644
But this time, the photons
are absorbed by the atoms.
407
00:25:09,510 --> 00:25:12,609
The hot atoms ride
the boiling current to the top,
408
00:25:12,641 --> 00:25:15,142
Dragging the photons with them.
409
00:25:18,242 --> 00:25:21,207
So, it's almost like
this conveyor belt of material.
410
00:25:21,241 --> 00:25:24,141
Photons are actually
hitchhiking a ride on the atoms
411
00:25:24,174 --> 00:25:27,574
That are traveling upward
through this heat transfer.
412
00:25:27,607 --> 00:25:29,906
So, it's a much easier ride
in the convection layer
413
00:25:29,939 --> 00:25:31,639
Than it is
in the radiation zone.
414
00:25:36,473 --> 00:25:39,338
It's as if our photon
were now in the hands
415
00:25:39,371 --> 00:25:42,404
Of a single player
making a fast break.
416
00:25:44,704 --> 00:25:48,735
In the convection
layer, it's a direct path.
417
00:25:48,770 --> 00:25:52,235
One player can actually hold on
to this basketball or photon
418
00:25:52,269 --> 00:25:54,636
For a lot longer
in a direct path.
419
00:25:56,901 --> 00:25:58,134
By not passing,
420
00:25:58,167 --> 00:26:01,135
The atom takes the ball
quickly up the court.
421
00:26:04,167 --> 00:26:06,766
The photon's journey
through the convection zone
422
00:26:06,801 --> 00:26:09,699
Takes just one week.
423
00:26:09,733 --> 00:26:13,565
But in that time,
the photon is transformed.
424
00:26:13,599 --> 00:26:16,165
The bottom
of the convection zone
425
00:26:16,197 --> 00:26:20,065
Is around
360,000 degrees fahrenheit.
426
00:26:20,996 --> 00:26:23,264
The top -- Just 10,000.
427
00:26:26,630 --> 00:26:31,529
So, as the photon rises up,
it cools, losing energy,
428
00:26:31,562 --> 00:26:35,262
Changing from an energetic x-Ray
to visible light.
429
00:26:39,626 --> 00:26:42,161
So, it starts
as a high-Energy x-Ray
430
00:26:42,194 --> 00:26:44,792
At the bottom of the convection
zone, moves its way up,
431
00:26:44,827 --> 00:26:46,827
It loses a little bit
of that energy.
432
00:26:46,859 --> 00:26:48,225
By the time it leaves there,
433
00:26:48,259 --> 00:26:50,527
It's closer to the kind of light
that we see,
434
00:26:50,559 --> 00:26:51,826
Which is visible light.
435
00:26:55,492 --> 00:26:57,524
At the top
of the convection zone,
436
00:26:57,558 --> 00:26:59,825
The atom releases the photon,
437
00:26:59,857 --> 00:27:02,823
Which shoots out
as visible light.
438
00:27:04,490 --> 00:27:05,990
This cools the atoms,
439
00:27:06,023 --> 00:27:09,223
Which fall back down
to absorb more photons,
440
00:27:09,257 --> 00:27:11,190
Heat up, and rise again.
441
00:27:12,889 --> 00:27:16,289
The photon is now
just below the sun's surface.
442
00:27:18,854 --> 00:27:24,252
But the churning convection zone
unleashes another force --
443
00:27:24,285 --> 00:27:27,152
A force that powers huge storms,
444
00:27:27,187 --> 00:27:31,386
Detonates bombs, and threatens
to stop light's escape.
445
00:27:48,916 --> 00:27:51,649
In the sun's core,
446
00:27:51,682 --> 00:27:54,414
Nuclear fusion has created
a photon, a packet of light.
447
00:27:54,848 --> 00:27:58,780
It has battled
through the radiation zone,
448
00:27:58,815 --> 00:28:01,581
Been dragged up
through the convection zone
449
00:28:01,614 --> 00:28:06,614
On columns of hot plasma,
hurdling towards its escape.
450
00:28:09,546 --> 00:28:11,712
On this million-Year journey,
451
00:28:11,744 --> 00:28:16,411
The photon has changed from
an invisible deadly gamma ray
452
00:28:16,444 --> 00:28:19,811
To the kind of life-Giving light
we see here on earth.
453
00:28:24,942 --> 00:28:29,241
Finally,
it has reached the surface --
454
00:28:29,276 --> 00:28:32,975
The visible shell of the sun,
the photosphere.
455
00:28:35,773 --> 00:28:36,974
The photosphere,
456
00:28:37,008 --> 00:28:38,575
Which is basically
the visible part of the sun,
457
00:28:38,607 --> 00:28:42,140
Or the surface, is what we see
when we look up at the sun.
458
00:28:42,174 --> 00:28:45,240
We're seeing visible light
coming from that very layer,
459
00:28:45,273 --> 00:28:46,339
The photosphere.
460
00:28:49,472 --> 00:28:52,904
The ball
of blinding light we perceive
461
00:28:52,938 --> 00:28:57,472
Hides a spectacular
and savage world.
462
00:28:59,971 --> 00:29:03,537
The sun from a distance
looks quiet and serene,
463
00:29:03,569 --> 00:29:06,636
But if you take a close-Up
of the surface of the sun,
464
00:29:06,668 --> 00:29:09,602
You see that it's churning
with activity.
465
00:29:11,402 --> 00:29:14,869
It's beautiful and
terrifying at the same time --
466
00:29:14,902 --> 00:29:18,034
Huge storms of material
bubbling and boiling.
467
00:29:18,067 --> 00:29:19,534
It looks like a witch's brew,
468
00:29:19,568 --> 00:29:21,567
Except the bubbles
in the witch's brew
469
00:29:21,600 --> 00:29:23,632
Are larger
than the size of the earth.
470
00:29:25,567 --> 00:29:28,933
The surface of the sun
is a turbulent barrier.
471
00:29:30,799 --> 00:29:34,764
And once again,
our photon gets taken hostage.
472
00:29:44,996 --> 00:29:48,561
At kitt peak observatory
in arizona,
473
00:29:48,594 --> 00:29:53,060
Solar astronomer matt penn
studies this solar surface
474
00:29:53,093 --> 00:29:57,093
To discover how photons of light
get trapped.
475
00:29:57,127 --> 00:29:58,860
There's a bunch of cirrus today,
476
00:29:58,894 --> 00:30:00,694
But hopefully,
we'll get some data.
477
00:30:04,627 --> 00:30:06,592
Using
the mcmath-Pierce telescope,
478
00:30:06,626 --> 00:30:10,759
He focuses the sun's light to
scan the photosphere in detail.
479
00:30:11,991 --> 00:30:14,491
So, what we've got
are a few small sun spots
480
00:30:14,525 --> 00:30:15,824
On a disc of the sun.
481
00:30:15,857 --> 00:30:19,255
We've got two sun spots,
two large ones.
482
00:30:19,289 --> 00:30:20,822
They're heading off
to the edge of the sun,
483
00:30:20,855 --> 00:30:22,289
To the limb of the sun.
484
00:30:22,323 --> 00:30:24,723
But they're all accompanied
by a smaller sun spots,
485
00:30:24,756 --> 00:30:26,390
Groups of smaller ones,
following them.
486
00:30:29,189 --> 00:30:32,721
Sun spots mark areas
where light is trapped.
487
00:30:34,886 --> 00:30:36,986
So, a sun spot forms a dark spot
488
00:30:37,020 --> 00:30:39,421
By removing energy
from that part of the sun.
489
00:30:39,453 --> 00:30:42,052
It's blocking the convective
flows that transport the heat
490
00:30:42,086 --> 00:30:44,519
And the light
from inside the sun to space.
491
00:30:44,553 --> 00:30:46,320
So, what we see then
is a cooler region
492
00:30:46,353 --> 00:30:47,786
That appears dark to us.
493
00:30:50,385 --> 00:30:54,750
A powerful force stops
our photon dead in its tracks,
494
00:30:54,784 --> 00:30:58,651
Preventing its light and energy
from leaving the sun's surface.
495
00:31:00,983 --> 00:31:03,384
That force is magnetism.
496
00:31:07,615 --> 00:31:10,814
Sun spots take shape
where intense magnetism
497
00:31:10,849 --> 00:31:15,548
From deep inside the sun blasts
up through the photosphere.
498
00:31:19,514 --> 00:31:22,647
The magnetic fields
are so strong that it actually
499
00:31:22,679 --> 00:31:27,411
Stops the convective motion
of hot inner material
500
00:31:27,445 --> 00:31:28,678
From flowing to the surface.
501
00:31:28,711 --> 00:31:31,010
So, you actually get
what looks like a cool spot
502
00:31:31,044 --> 00:31:32,111
On the surface of the sun.
503
00:31:32,943 --> 00:31:34,776
They can be huge,
504
00:31:34,809 --> 00:31:37,844
The largest over 10 times
the size of earth.
505
00:31:44,642 --> 00:31:47,275
The magnetism
that generates these sun spots
506
00:31:47,308 --> 00:31:50,541
Forms field lines
covering the sun.
507
00:31:50,575 --> 00:31:53,440
On our solid earth,
the whole planet
508
00:31:53,473 --> 00:31:59,207
Rotates together,
including its magnetic field.
509
00:31:59,240 --> 00:32:02,605
But the sun
is a big ball of gas,
510
00:32:02,640 --> 00:32:05,505
And the same rules don't apply.
511
00:32:05,538 --> 00:32:07,837
You see, there's nothing solid
about the sun.
512
00:32:07,871 --> 00:32:09,038
It's a big ball of gas.
513
00:32:09,072 --> 00:32:10,872
It turns on its axis,
514
00:32:10,904 --> 00:32:13,537
But the equator
rotates faster than the poles.
515
00:32:13,571 --> 00:32:14,937
The sun twists itself up,
516
00:32:14,970 --> 00:32:17,238
And the magnetic field
twists with it.
517
00:32:18,903 --> 00:32:22,935
It rotates faster at
the equator than at the poles,
518
00:32:22,969 --> 00:32:26,235
Twisting and tangling
its magnetic field
519
00:32:26,269 --> 00:32:27,902
With each rotation.
520
00:32:29,201 --> 00:32:33,067
The result -- Magnetic mayhem.
521
00:32:36,866 --> 00:32:39,765
So, when these fields emerge
from the surface of the sun,
522
00:32:39,798 --> 00:32:41,866
They have all this stored energy
in them.
523
00:32:41,998 --> 00:32:43,932
They're, like,
all twisted and knotted,
524
00:32:43,966 --> 00:32:45,998
Like rubber bands
you just twist and knot
525
00:32:46,032 --> 00:32:47,332
With all this energy in it.
526
00:32:47,364 --> 00:32:48,931
If you ever twist and twist
and twist a rubber band
527
00:32:48,965 --> 00:32:50,097
And pull it straight,
528
00:32:50,131 --> 00:32:52,532
You can tell,
you can feel that tension in it.
529
00:32:54,796 --> 00:32:57,262
Where the magnetic lines twist,
530
00:32:57,296 --> 00:33:00,329
Flows of plasma
containing our photon
531
00:33:00,363 --> 00:33:01,863
Can't reach the surface.
532
00:33:03,662 --> 00:33:05,961
So, what happens is you have
these packets of gas
533
00:33:05,995 --> 00:33:08,661
Which reach the surface,
cool off,
534
00:33:08,694 --> 00:33:11,061
But are trapped right there
by the magnetism.
535
00:33:13,994 --> 00:33:15,993
A patch of the sun goes dark
536
00:33:16,026 --> 00:33:18,759
Where light can't escape.
537
00:33:18,794 --> 00:33:20,794
A sun spot is born.
538
00:33:22,393 --> 00:33:24,926
But in that tangle
of magnetic lines,
539
00:33:24,960 --> 00:33:26,691
Something
eventually has to snap.
540
00:33:26,925 --> 00:33:29,990
The magnetic fields
are very unhappy.
541
00:33:30,023 --> 00:33:31,656
They don't like
the state that they're in,
542
00:33:31,689 --> 00:33:33,890
And all they want to do
is unravel.
543
00:33:38,356 --> 00:33:40,655
Huge loops of magnetic energy
544
00:33:40,689 --> 00:33:43,056
Arch out over the sun spots.
545
00:33:46,023 --> 00:33:50,421
Twisted and unstable,
desperate to spew their energy,
546
00:33:50,454 --> 00:33:54,820
They create a magnetic bomb
primed to explode.
547
00:33:56,919 --> 00:33:58,852
And so, if one magnetic
field with stored energy
548
00:33:58,886 --> 00:34:02,451
Sees another magnetic field,
those two look at each other
549
00:34:02,486 --> 00:34:05,786
And say, "hey, if we connect, we
can get rid of a lot of energy."
550
00:34:05,819 --> 00:34:07,151
They do so, they reconnect.
551
00:34:07,183 --> 00:34:08,618
Baddow!
552
00:34:18,082 --> 00:34:21,115
It's a huge explosion,
and we call it a solar flare.
553
00:34:23,515 --> 00:34:27,147
And this can be equivalent
to millions of nuclear weapons
554
00:34:27,181 --> 00:34:29,915
Exploding simultaneously.
555
00:34:31,213 --> 00:34:35,945
Solar flares
erupt outwards into space
556
00:34:35,980 --> 00:34:38,579
At up to 4 1/2 million miles
an hour...
557
00:34:40,646 --> 00:34:43,079
...releasing massive amounts
of energy.
558
00:34:47,411 --> 00:34:49,311
Magnetic fields
are throwing plasma
559
00:34:49,344 --> 00:34:51,443
From the surface of the sun.
560
00:34:51,476 --> 00:34:54,010
Suddenly, there's a large
outpouring of light.
561
00:34:57,710 --> 00:34:59,442
After nearly a million years,
562
00:34:59,476 --> 00:35:02,675
Our packet of light
finally makes its escape.
563
00:35:06,907 --> 00:35:08,174
It's free,
564
00:35:08,206 --> 00:35:12,940
Catapulting out along
with trillions of other photons,
565
00:35:12,974 --> 00:35:15,574
But their journey
is far from over.
566
00:35:17,206 --> 00:35:22,072
Most hurdle onwards to
the far reaches of the cosmos,
567
00:35:22,105 --> 00:35:24,771
To strange, new worlds.
568
00:35:34,401 --> 00:35:38,368
After a nearly
million-Year journey
569
00:35:38,401 --> 00:35:42,968
Through the most hostile
environment in the solar system,
570
00:35:43,001 --> 00:35:45,801
Tiny parcels of light --
571
00:35:45,834 --> 00:35:49,667
Photons -- Finally burst
from the sun's surface.
572
00:35:56,464 --> 00:35:57,999
They're free.
573
00:35:58,033 --> 00:36:01,931
They basically are free
to leave this arduous journey
574
00:36:01,964 --> 00:36:03,464
That they've been on in the sun.
575
00:36:03,497 --> 00:36:05,830
And then they fly out
at the speed of light.
576
00:36:07,997 --> 00:36:11,763
So, it's kind of a "breaking
out of prison" type of feeling
577
00:36:11,796 --> 00:36:13,595
For those poor photons.
578
00:36:14,996 --> 00:36:17,961
They speed out into empty space
579
00:36:17,994 --> 00:36:21,028
At 186,000 miles per second.
580
00:36:22,960 --> 00:36:26,327
And just 8.3 minutes
after it leaves the sun,
581
00:36:26,360 --> 00:36:28,592
Our photon reaches earth.
582
00:36:28,626 --> 00:36:30,858
The next time
you look at a star in the sky,
583
00:36:30,893 --> 00:36:33,425
You might consider
the amazing journey
584
00:36:33,458 --> 00:36:37,058
The photons have taken on
their way to reaching your eye.
585
00:36:40,291 --> 00:36:42,525
They were created
by nuclear reactions
586
00:36:42,557 --> 00:36:46,458
Deep in the core of the stars,
and then they bounced around
587
00:36:46,490 --> 00:36:50,422
And got degraded
into lower energy photons.
588
00:36:50,456 --> 00:36:52,523
And then in the convective zone,
589
00:36:52,556 --> 00:36:55,855
They were carried
by mass motions of gas.
590
00:36:55,889 --> 00:36:59,122
And finally, at the edge,
they were set free.
591
00:37:02,155 --> 00:37:07,121
And they traveled unimpeded
and finally reached your eyes.
592
00:37:08,919 --> 00:37:12,252
Our photon finally arrives,
593
00:37:12,287 --> 00:37:16,752
Smashes into a leaf,
and passes on its energy.
594
00:37:16,785 --> 00:37:18,885
This is photosynthesis,
595
00:37:18,919 --> 00:37:21,252
The fundamental link
in our food chain.
596
00:37:25,151 --> 00:37:29,450
Finally, carrying energy
born inside the sun's core,
597
00:37:29,482 --> 00:37:32,415
Our photon and billions like it
598
00:37:32,448 --> 00:37:36,914
Ignite the primal fires
of life on our planet.
599
00:37:36,948 --> 00:37:42,247
The sun's light creates
our fuel, drives our weather,
600
00:37:42,281 --> 00:37:43,680
Churns our seas.
601
00:37:46,913 --> 00:37:50,246
Every single day,
enough photons hit the earth
602
00:37:50,279 --> 00:37:53,245
To power our civilization
for 27 years.
603
00:37:55,346 --> 00:37:59,210
The sun's light is more
than just warmth and heat.
604
00:37:59,243 --> 00:38:02,910
It provides everything
we need to survive.
605
00:38:02,944 --> 00:38:06,476
Without light, we are nothing.
606
00:38:06,511 --> 00:38:09,543
All of the energy
that powers our biology,
607
00:38:09,576 --> 00:38:12,243
The thing that makes our planet
warm, that makes life possible,
608
00:38:12,275 --> 00:38:13,808
That all comes from the sun.
609
00:38:16,340 --> 00:38:20,241
Trillions of photons
hit the earth every second,
610
00:38:20,273 --> 00:38:22,473
Each delivering
life-Giving energy.
611
00:38:25,974 --> 00:38:30,039
But for the unimaginable number
who pass us by,
612
00:38:30,072 --> 00:38:33,239
The journey is far from over.
613
00:38:33,273 --> 00:38:36,472
Around 80 minutes
after leaving the sun,
614
00:38:36,505 --> 00:38:38,903
They reach saturn.
615
00:38:38,938 --> 00:38:41,371
After four hours, neptune.
616
00:38:43,771 --> 00:38:46,070
Once a photon
leaves the surface of the sun,
617
00:38:46,103 --> 00:38:48,470
It's free to travel
as far as it can,
618
00:38:48,503 --> 00:38:52,001
And as far as it can can be
literally across the universe,
619
00:38:52,034 --> 00:38:54,301
Billions of light years away.
620
00:38:55,668 --> 00:38:57,468
They shoot
past the outer reaches
621
00:38:57,501 --> 00:39:01,534
Of our solar system
in just 18 hours.
622
00:39:01,567 --> 00:39:06,300
Here, the sun is a dim speck
in the distance.
623
00:39:06,333 --> 00:39:10,865
But the photons keep on going,
out into deep space.
624
00:39:13,931 --> 00:39:16,564
In 1,200 years,
some of the photons
625
00:39:16,598 --> 00:39:21,065
Reach the red dwarf star system
kepler-62,
626
00:39:21,096 --> 00:39:25,529
A solar system with potentially
habitable earth-Like planets.
627
00:39:25,563 --> 00:39:28,330
In our galaxy,
628
00:39:28,362 --> 00:39:32,628
There are billions
of earth-Like planets.
629
00:39:32,661 --> 00:39:37,994
If there is life out there, can
it see the light from our sun?
630
00:39:38,029 --> 00:39:39,993
If aliens exist out there,
631
00:39:40,027 --> 00:39:42,560
They could easily
see the light from our sun.
632
00:39:42,594 --> 00:39:44,525
If they're sufficiently nearby,
633
00:39:44,560 --> 00:39:48,058
The sun might be
a naked-Eye star in their sky
634
00:39:48,092 --> 00:39:49,426
Or with telescopes,
635
00:39:49,458 --> 00:39:51,058
They would be able
to detect the sun
636
00:39:51,092 --> 00:39:53,725
Even from
vastly greater distances.
637
00:39:53,757 --> 00:39:55,725
So,
there's a distinct possibility
638
00:39:55,757 --> 00:40:00,656
That aliens are studying our sun
right now without realizing
639
00:40:00,690 --> 00:40:03,790
That we're here trying
to study the universe, as well.
640
00:40:05,855 --> 00:40:07,322
Hurdling on,
641
00:40:07,355 --> 00:40:12,656
The photons pass the horsehead
nebula in 1,500 years
642
00:40:12,688 --> 00:40:15,721
And the pillars of creation
in 7,000.
643
00:40:17,822 --> 00:40:20,387
At these distances,
the light from our star
644
00:40:20,420 --> 00:40:23,721
Is too small to be seen
with the naked eye,
645
00:40:23,753 --> 00:40:26,219
But it would be visible
with a powerful telescope.
646
00:40:26,253 --> 00:40:27,952
And with the biggest telescopes
647
00:40:27,985 --> 00:40:29,885
That we can create here on earth
or in space,
648
00:40:29,918 --> 00:40:32,550
We can actually see
the light from stars
649
00:40:32,585 --> 00:40:34,217
At the other end
of the universe,
650
00:40:34,251 --> 00:40:36,184
Over 10 billion light years
away.
651
00:40:36,217 --> 00:40:40,050
And so the light from our sun is
traveling across the universe.
652
00:40:42,384 --> 00:40:43,682
So, the light from our sun,
653
00:40:43,715 --> 00:40:47,014
The light from the earth,
travels essentially forever.
654
00:40:47,048 --> 00:40:49,481
The next time you're out
under a clear sky
655
00:40:49,516 --> 00:40:50,749
And you look up,
656
00:40:50,782 --> 00:40:52,980
You might want to wave
because somebody out there
657
00:40:53,014 --> 00:40:55,349
Might be able to see you
and wave back.
658
00:40:57,648 --> 00:41:01,847
Our tiny star
is visible across the universe
659
00:41:01,880 --> 00:41:04,380
If someone is looking.
660
00:41:04,413 --> 00:41:07,778
There isn't a single
place in our visible universe
661
00:41:07,813 --> 00:41:09,813
That you wouldn't be able
to see the sun from,
662
00:41:09,846 --> 00:41:11,445
And maybe that's heartening.
663
00:41:11,478 --> 00:41:13,510
Maybe there's some evidence
of our existence
664
00:41:13,545 --> 00:41:14,677
At the other end
of the universe.
665
00:41:14,711 --> 00:41:16,577
Won't get there
for billions of years,
666
00:41:16,610 --> 00:41:19,277
But at least
maybe we won't be forgotten.
667
00:41:19,311 --> 00:41:24,143
A journey that started
deep inside the core of the sun
668
00:41:24,177 --> 00:41:27,309
With a photon,
a million-Year struggle
669
00:41:27,342 --> 00:41:29,708
To finally escape
the sun's grip.
670
00:41:32,442 --> 00:41:34,641
Once free, our photon
671
00:41:34,675 --> 00:41:39,307
Brought energy, heat,
and life to our world.
672
00:41:41,574 --> 00:41:47,338
Light from our sun joins light
from trillions of other stars
673
00:41:47,371 --> 00:41:49,806
Journeying through the universe,
674
00:41:49,838 --> 00:41:53,072
Spreading energy
throughout the cosmos.
53664
Can't find what you're looking for?
Get subtitles in any language from opensubtitles.com, and translate them here.