Ch. 6: The Sun - PowerPoint PPT Presentation

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Ch. 6: The Sun

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Title: Testing Author: Mark Voit Last modified by: Monika Kress Created Date: 9/29/1999 2:52:42 PM Document presentation format: On-screen Show Company – PowerPoint PPT presentation

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Title: Ch. 6: The Sun


1
Ch. 6 The Sun
2
The Suns luminosity is about 4x1026 joules per
second. Its mass is about 2x1030 kg. What is its
energy source?
Chemical energy?
3
The Suns luminosity is about 4x1026 joules per
second. Its mass is about 2x1030 kg. What is its
energy source?
Chemical energy?
4
10 Cal/g 108 J/kg
2x1030 kg
5
Is it CONTRACTING?
6
E mc2 - Einstein, 1905
It can be powered by NUCLEAR ENERGY!
Nuclear Potential Energy (core)
10 billion years
Luminosity
7
The fusion of hydrogen via the proton-proton chain
  • Neutrinos created during fusion fly directly
    through the Sun
  • Observations of these solar neutrinos can tell us
    whats happening in core

8
Weight of upper layers compresses lower layers
9
The Sun is in hydrostatic equilibrium Gravity
pushes inward Fusion generates energy - heats
the gas - increases the pressure - balances
the inward force of gravity
10
Core Energy generated by nuclear fusion 15
million K
11
Radiation Zone Photons dont know which way is
up - they escape by a random walk Energy
gradually leaks out of radiation zone
12
Convection Zone Energy transported upward by
rising hot gas
13
Photosphere Visible surface of Sun 6,000 K
14
Chromosphere Middle layer of solar atmosphere
104 - 105 K
15
Corona Outermost layer of solar atmosphere 1
million K
16
Solar wind A flow of charged particles from the
surface of the Sun
17
Limb darkening
18
Radiation transport (radiative transfer)
The layers of the Sun are determined by how
energy is transported through and out of that
layer
19
Sunspots cooler than other parts of the Suns
surface (4000 K) Contain strong magnetic
fields cool gas is sinking
20
41.2 Zeeman effect
Atomic energy levels, and their spectral lines,
are split when the atoms are in a magnetic field
Experimental confirmation of the quantization of
angular momentum
21
Why do the lines split?
  • Electrons are moving charges
  • They respond to external B
  • Their energy levels change when in a B

22
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23
X-ray emission
Loops of bright gas often connect sunspot pairs
24
Magnetic activity causes solar flares that send
bursts of X-rays and charged particles into space
25
Magnetic activity also causes solar prominences
that erupt high above the Suns surface
26
Corona appears bright in X-ray photos in places
where magnetic fields trap hot gas
Insert TCP 5e Figure 14.20
27
Coronal mass ejections send bursts of energetic
charged particles out through the solar system
28
Charged particles streaming from Sun can disrupt
electrical power grids and can disable
communications satellites
29
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30
Solar activity varies with time
Number of sunspots rises and falls in 11-year
cycle
31
Little Ice Age 1300-1850
Winter sports became very popular!
32
  • Historical implications of the Little Ice Age
  • Greenland settlement collapsed in 1400
  • Glaciers advanced, crushing villages in
    Switzerland
  • 1780 New York Harbor froze
  • Stradivari built his famous violins
  • Armies could march acropss frozen rivers and
    straits
  • Snow fell in summer in Northern Europe famine
    ensued
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