1. Properties of Stars

2. How do we classify stars? A.Size B.Temperature and Color C.Brightness

3. Temperature and color The color of the star is dependent on the temp of the star. The color of the star is dependent on the temp of the star. Red – coolest stars Red – coolest stars Blue – hottest stars Blue – hottest stars Order from coolest to hottest Order from coolest to hottest Red, red-orange, yellow, white, blue Red, red-orange, yellow, white, blue 3000K 6000K 30,000K 3000K 6000K 30,000K Stars have Different colors which indicate different temperatures

4. Temperature and Color

5. Size Giants/supergiants- large and very large stars. Many of these are very far away White dwarfs- very small stars – about the size of the Earth Neutron stars- even smaller stars – only 20 km in diameter. Medium sized stars- many stars this size. The size of our Sun.

6. Binary star systems contain two stars that orbit around their common center of mass. Many of the stars in our galaxy are part of a binary system. Binary Stars are used to determine the mass of the star.

7. How do we measure stars? Parallax- the apparent change in position of an object when you look at it from different places.

8. Parallax The closer the star is to Earth, the larger the shift will be

9. Parallax Only good for measuring stars close to us. Not farther than 1000 light years away. Why? The movement would be too small to measure accurately.

10. Light travels at a speed of 186,000 miles a second or 300,000,000 meters per second or 700 million miles an hour. For scale, the distance from the Earth to the Moon is about 239,000 miles. The distance light can travel in a year is called a "light year." The light year is one of the basic measures of distance for astronomy. Nothing travels faster than the speed of light. SPEED OF LIGHT

11. Stellar Brightness=magnitude Apparent Brightness- the brightness as seen from Earth. The closer the star is to Earth, the brighter it will look. 3 factors that control: 1.How big it is 2.How hot it is 3.How far away it is

12. 2 stars with the same absolute magnitude do not have the same apparent magnitude Absolute Brightness – the amount of light the star actually gives off.

13. H-R Diagram- diagram showing the relationship between absolute magnitude/luminosi ty and temperature of the star *Temperature on the x axis *Luminosity/ absolute brightness on the y axis

14. H-R Diagram (sketch this) What kind of stars are cooler than, but brighter than the sun? What kind of stars are bluer than the sun but less bright & must be quite small? RED GIANTS WHITE DWARFS

15. Variable Stars Cepheid variables - pulsate in a regular way, rapidly increasing in brightness as they increase in size, then slowly decreasing in brightness as they decrease in size. The reason for this is slight instabilities in temperature and density Cepheid variables - pulsate in a regular way, rapidly increasing in brightness as they increase in size, then slowly decreasing in brightness as they decrease in size. The reason for this is slight instabilities in temperature and density Nova – sudden brightening of a star Nova – sudden brightening of a star

16. Interstellar Matter Between stars there are clouds of dust and gasses = nebulae (Greek for cloud) Between stars there are clouds of dust and gasses = nebulae (Greek for cloud) If next to a bright star it will light up and glow If not close to a star looks like a dark starless region