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CH. 29.1 – THE SUN Chapter 29 – March 13 th , 2015

CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

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Page 1: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

CH. 29.1 – THE SUNChapter 29 – March 13th, 2015

Page 2: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

VOCABULARY TO KNOW…

Photosphere – Chromosphere – Corona – Convection Zone – Radiative Zone – Nuclear Fusion -

Page 3: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

CONTENTS OF THE SUN

The sun is made up of…75% Hydrogen 24% Helium 1% Other Gases

It is powered by FUSION = where lighter nuclei is combine to make heavier ones

Thus, releasing LOTS of ENERGY!

Page 4: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

** EACH STEP RELEASES ENERGY **

#1. 2 hydrogens ( protons) fuse, the second p+ is neutralized by emitting a positron…so that proton becomes a neutron (p+ no pair created)

Page 5: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

2. Another H proton combines with the first p+no pair…creates a helium isotope (2 p+, 1 no)

Page 6: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

3. These helium isotopes, each with 2p+ 1no, fuse and release two protons leaving behind a “common” helium atom.

Page 7: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

** EACH STEP RELEASES ENERGY **

Page 8: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

ABOUT ENERGY…

Neutrinos (uncharged “electrons”… 1/10,000 the size of an e-) are also released and reach Earth in 8 minutes

Helium (He) product is 0.7% less massive than the Hydrogen (H) that formed it….

--that MASS is converted into ENERGYTHIS energy causes intense shine and heat.

 

Page 9: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

MASS -> ENERGY

1905:Nucleus of atom/fusion unknown…Einstein proposed: small mass yields large energy

This is known as the Theory of RelativityE=mc2

Scientists used E=mc2 to explain the sun’s huge quantities of E.

E = mc²E = energy M = mass of matter changedC = speed of light

Page 10: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

SUN’S STRUCTURE

1. Core gaseous25% of sun’s diametertemp 15,000,000 oC)

Super dense (10x that of ironheat & pressure cause atoms to separate into nuclei and e-s. (remember, nuclei are +)

Nuclei try to repel but heat/pressure force them to fuse.

Page 11: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

2. Radiative - Outside core 2-7,000,000oC E moving as EM waves3. Convection (30% of Sun) 2,000,000 oC E moving as convection (hot gases move out,

expand, lose E…become dense and sink back down in convective zone…repeats)

Corona is seen during solar eclipses

Page 12: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015
Page 13: CH. 29.1 – THE SUN Chapter 29 – March 13 th, 2015

ATMOSPHERE OF THE SUN…

4. Photosphere gases risen out of convective (6,000oC)

5. Chromosphere color sphere 6-50,000oC g as shoots up from photosphere

6. CoronaTemps. spikes here (above 1,000,000 oC) ions can escape---this is solar wind.