3. EARTH SUN (SOL)
Radius = 1 Radius = 109
Density =1 Density = 0.255
Gravity =1 Gravity = 28.0
Temperature ~ 300K Temperature ~ 5,800K

4. Photosphere

5. Photosphere Very thin Emits Radiation
"Photo" means "light". This is the light sphere

6. Chromosphere Photosphere Thin layer Cooler than Photosphere
"Chromo" means "color". This is the color sphere
Chromosphere
Photosphere
Very thin
Emits Radiation
"Photo" means "light". This is the light sphere

7. Chromosphere Transition zone Starts getting warm in a hurry
Transitions from cool to hot, from Sun to Outer space.
Chromosphere
Thin layer
Cooler than Photosphere
"Chromo" means "color". This is the color sphere

8. Solar Wind,
2,000,000 K
0.000,000,000,000,000,000,000,02 g / m3
Corona, very hot and very low density
1,000,000 K
.000,009 g / m3

9. Heat moves through convection (movement of material itself)
2,000,000 K
NO fusion
NO light given off

10. Heat moves through convection (movement of material itself)
2,000,000 K
NO fusion
NO light given off
Heat moves through Radiation (movement through radiation)
7,000,000 K
NO fusion
NO light given off
Energy is created through fusion of hydrogen in to helium
15,000,000 K
Getting hotter over time, started out at about 10,000,000 K

13. Granulation is the tops of the convection currents

15. Based on the total number of atoms, NOT mass. By MASS, 71% H, 27 % He

17. One of those protons became a neutron, so in order to keep the Conservation of Energy happy, a positron is ejected from its nucleus.

18. One of those protons became a neutron, so in order to keep the Conservation of Energy happy, a positron is ejected from its nucleus.
This Helium only has one neutron.

19. One of those protons became a neutron, so in order to keep the Conservation of Energy happy, a positron is ejected from its nucleus.
This Helium only has one neutron.
Left side has 6P and 2N Right side has 6P and 2N (& repeat)

21. Sunspot is a cool place on the Sun
Sunspot is a cool place on the Sun. Convection is not working because of magnetism decay in that area. Heat not rising.

22. Prominences connect sunspots, and are really big.

23. Sunspot cycle is 11 years
Solar Cycle is 22 years

25. Solar flares are outward bursts.

26. Coronal Mass Ejections are bigger than huge.
One per day at solar minimum, two or three per day at solar maximum.

31. True or False
1. The Sun is a rather normal star ________
The Sun’s average density is less than that of Earth ________
The Sun’s diameter is about 10 times that of Earth ________
Sunspots show that the Sun’s poles spin faster than the equator ________
Convection currents in the Sun involve cool gas rising toward the surface, and hot gas sinking to the interior ________
The temperature of the solar atmosphere decreases with increasing altitude ________
Prominences are large flames erupting from the burning surface of the Sun ________
Positrons are the antiparticles of electrons ________
Nuclei are held together by the strong force ________
Self-Test: Fill in the Blank
The part of the Sun that we see is called the ________
Traveling outward from the surface of the Sun, the main regions of the solar atmosphere are the ________, the ________, and the ________.
Below the surface of the Sun, lie the ________ zone, the ________ zone and the ________ zone.
The most abundant element of the Sun is ________________ followed by ________________.
The two most abundant elements of the Sun make up about ________ percent of its composition (by number of atoms)
Sunspots appear dark because they are ________ than the surrounding gas of the photosphere.
The Sunspot cycle is ________ years long, but the solar cycle is ________ years long
The net result of the proton-proton chain is that ________ protons are fused into a nucleus of ________, two ________ are emitted, and energy is released in the form of ________________. Mass is ________.