Upload
jack-greenhouse
View
216
Download
0
Embed Size (px)
Citation preview
8/7/2019 chapter14 pp lecture 1
1/63
1
8/7/2019 chapter14 pp lecture 1
2/63
2
8/7/2019 chapter14 pp lecture 1
3/63
3
8/7/2019 chapter14 pp lecture 1
4/634
8/7/2019 chapter14 pp lecture 1
5/63
5
8/7/2019 chapter14 pp lecture 1
6/63
6
8/7/2019 chapter14 pp lecture 1
7/63
7
8/7/2019 chapter14 pp lecture 1
8/63
8
8/7/2019 chapter14 pp lecture 1
9/63
9
8/7/2019 chapter14 pp lecture 1
10/63
10
8/7/2019 chapter14 pp lecture 1
11/63
11
8/7/2019 chapter14 pp lecture 1
12/63
12
8/7/2019 chapter14 pp lecture 1
13/63
13
8/7/2019 chapter14 pp lecture 1
14/63
14
8/7/2019 chapter14 pp lecture 1
15/63
15
8/7/2019 chapter14 pp lecture 1
16/63
16
Good Sun movies to download:
http://es.rice.edu/ES/humsoc/Galileo/Things/g_sunspots.html
Images compiled from Owen Gingerichs copy of the first edition of Istoria e
Dimostrazioni
Wave_fade.mpg photosphere:chromosphere:corona, optical:UV:X-ray
http://www.lmsal.com/YPOP/FilmFestival/index.html
C2_1mth.mpghttp://lasco-www.nrl.navy.mil/
8/7/2019 chapter14 pp lecture 1
17/63
17
8/7/2019 chapter14 pp lecture 1
18/63
18
8/7/2019 chapter14 pp lecture 1
19/63
19
8/7/2019 chapter14 pp lecture 1
20/63
20
8/7/2019 chapter14 pp lecture 1
21/63
21
8/7/2019 chapter14 pp lecture 1
22/63
22
8/7/2019 chapter14 pp lecture 1
23/63
23
8/7/2019 chapter14 pp lecture 1
24/63
24
8/7/2019 chapter14 pp lecture 1
25/63
25
8/7/2019 chapter14 pp lecture 1
26/63
26
8/7/2019 chapter14 pp lecture 1
27/63
Nuclear Fusion only occurs in the core. The core is only about 25% of the radius
of the sun. The core is essentially the oven of the sun.
27
8/7/2019 chapter14 pp lecture 1
28/63
Two different types. The sun ONLY does Fusion.
28
8/7/2019 chapter14 pp lecture 1
29/63
When two protons try to approach they repel because they have the same charge.
BUT in the core of the sun the temperatures due to the gravity of all the weight
applies enough pressure to get the core hot enough to allow kinetic energy which
means high velocity. The protons get close enough for a nuclear reaction to
occur.
29
8/7/2019 chapter14 pp lecture 1
30/63
4 protons combine to form a helium 4 particle and ENERGY. Energy is equal to
the difference of the mass of the 4 protons and helium 4.
30
8/7/2019 chapter14 pp lecture 1
31/63
Deuteron is a heavy hydrogen. Positron is a positive electron it is a beta ray.
Helium 3 is a helion which is a little lighter than regular helium. Gamma rays
and photons are the same thing at this given energy.
HIGH ENERGY- GAMMA
MEDIUM- x- Ray
LOWER- COLORS
UV
VIGYOR
IR
MICROWAVE
RADIO
31
8/7/2019 chapter14 pp lecture 1
32/63
Total mass is less than 1% lower. You need 6 protons to make the reaction go but
you get 2 back.
32
8/7/2019 chapter14 pp lecture 1
33/63
The sun would expand and cool down because the excess heat makes it expand
then it cools down as it expands.
33
8/7/2019 chapter14 pp lecture 1
34/63
If things get too hot the sun will expand. As it expands it will cool. If the sun
gets too cold it will shrink and warm up.
34
8/7/2019 chapter14 pp lecture 1
35/63
35
8/7/2019 chapter14 pp lecture 1
36/63
Photons are very energetic so they can go through very thick/very dense material.
Bounce of and goes in different directions. VERYLONG PROCESS TO GET
THROUGH. This is called the radiation zone because there is no mass
movement of particles. Fusion will not necessarily occur.
36
8/7/2019 chapter14 pp lecture 1
37/63
Here the material is fluid enough that it can move around. THERE IS MASS
MOVEMENT! The photons move quicker and brings the heat to the surface. As
it comes up (rises) it cools down on the way. Forms like cells.
37
8/7/2019 chapter14 pp lecture 1
38/63
Looking at the surface.
38
8/7/2019 chapter14 pp lecture 1
39/63
We tried to take what we know on earth, made a model and compared it to what
is actually going on.
39
8/7/2019 chapter14 pp lecture 1
40/63
We think we know about neutrinos. If the reaction occurs we can calculate it.
We know enough to count.
40
8/7/2019 chapter14 pp lecture 1
41/63
41
Download a movie to illustrate solar oscillations from:
http://science.nasa.gov/ssl/pad/solar/p_modes.htm
8/7/2019 chapter14 pp lecture 1
42/63
42
Download a movie to illustrate solar oscillations from:
http://science.nasa.gov/ssl/pad/solar/p_modes.htm
Compare data to how hot and dense each layer is. We have a good idea of what
is going on in the sun.
8/7/2019 chapter14 pp lecture 1
43/63
43
John Updike poem - permissions needed ?
8/7/2019 chapter14 pp lecture 1
44/63
Ray Davis detector uses cleaning fluid because it has a lot of chlorine in it.
Always get about 1/3 the number they are looking for. Build these under
mountains to get rid of everything else nd you need something hard enough to
beem a little.
44
8/7/2019 chapter14 pp lecture 1
45/63
Neutrinos- only one out of a very large number reacts in the detector. What
theorist have conjectured is that neutrinos from electron processes as it travels
the distance of sun to earth they change.
45
8/7/2019 chapter14 pp lecture 1
46/63
46
8/7/2019 chapter14 pp lecture 1
47/63
47
8/7/2019 chapter14 pp lecture 1
48/63
Magnetic fields- Behaves in such a way that opposite poles of magnets attract
visa versa. The south pole is in the north of the earth.
Sun is made of plasma Mostly hydrogen. Moving charged particles cause I
magnetic field. Changing magnetic fields make charged particles move.
48
8/7/2019 chapter14 pp lecture 1
49/63
Massive movements of charged particles gang together make regions of space
where magnetic field lines that particles like to follow. Sunspots are just cool
spaces on the sun. During times where there are a lot of sunspots, since the spots
are cause my strong magnetic fields they can cause problems on earth. Causedisruptions on Earth.
49
8/7/2019 chapter14 pp lecture 1
50/63
Separations of spectra lines are caused by a strong magnetic field inside a
sunspot.
50
8/7/2019 chapter14 pp lecture 1
51/63
Electron would get caught up on field lines. The charged particles follow the
magnetic field lines.
51
8/7/2019 chapter14 pp lecture 1
52/63
Providence cause by charged particles being attracted through field lines.
52
8/7/2019 chapter14 pp lecture 1
53/63
53
8/7/2019 chapter14 pp lecture 1
54/63
Field so strong that it captures the entire flare is called a solar prominence. HIGH
MAGNETIC FIELDS
54
8/7/2019 chapter14 pp lecture 1
55/63
55
Wave_fade.mpg photosphere:chromosphere:corona, optical:UV:X-ray
http://www.lmsal.com/YPOP/FilmFestival/index.html
8/7/2019 chapter14 pp lecture 1
56/63
56
8/7/2019 chapter14 pp lecture 1
57/63
When the corona has a solar prominence energy makes its way through the solar
system. Becomes solar storm.
57
8/7/2019 chapter14 pp lecture 1
58/63
If there is a solar ejections the field only gets a certain proportion of the particals
and the particles could get closer and closer to the Earth to affect satellites or
knock out power grids.
58
8/7/2019 chapter14 pp lecture 1
59/63
59
8/7/2019 chapter14 pp lecture 1
60/63
60
8/7/2019 chapter14 pp lecture 1
61/63
Equator rotates faster than the north and south pole. Sunspots tend to follow
these field lines
61
8/7/2019 chapter14 pp lecture 1
62/63
Fission and Fusion DO NOT occur at the surface of the sun.
62
8/7/2019 chapter14 pp lecture 1
63/63
63