1. Chapter 13
Stars and Galaxies

2. Section 1 Stars Patterns of Stars- constellations
1. Ancient cultures used mythology or everyday items to name constellations
2. Modern day astronomy studies 88 constellations
3. Some constellations are not visible all year because Earth revolves around the Sun
4. Circumpolar constellations in the northern sky appear to circle around Polaris and are visible all year

5. B. Star Magnitude
Absolute magnitude- measure of the amount of light a star actually gives off
Apparent magnitude- measure of the amount of a star’s light received on Earth

6. light-year =
C. Space measurement
Astronomers measure a star’s parallax- shift in its position when viewed from two different angles
Distance is measured in light-years- the distance that light travels in a year
SI units
9.461×10^12 km
9.461×10^15 m
Astronomical units
63.24×10^3 AU
0.3066 pc
US customary / Imperial units
5.879×10^12 mi
31.04×10^15 ft

7. D. Star properties Color indicates temperature
Hot stars are blue-white
Cool stars look orange or red
Yellow stars, like the Sun, are medium in temperature

8. 2. A spectroscope breaks the visible light from a star into a spectrum a. Spectrum indicates elements in the star’s atmosphere

9. Section 2 The Sun
Sun’s layers- energy created in the core moves outward through radiation zone and the convection zone and into the Sun’s atmosphere

10. B. Sun’s Atmosphere 1. Photosphere- lowest layer gives off light and is about 6,000 K 2. Chromosphere- the next layer about 2,000 km above the photosphere
The photosphere is the visible part of the star that we can see. It is characterised by emission spectra. A rarefied chromosphere, characterised by selective absorption surrounds the photosphere

11. Sunspots- areas of the sun that appear dark because they are cooler than surrounding areas. Sun spot cycle?

12. Solar Flares-occur when magnetic energy that has built up in the solar atmosphere is suddenly released.

13. Prominence- A solar prominence is an arc of gas that erupts from the surface of the Sun. Prominences can loop hundreds of thousands of miles into space

14. 3. Unusual- The Sun is not part of a multiple star system or cluster.

15. Section 3 Evolution of Stars
Classifying stars
Ejnar Hertzsprung and Henry Russell graphed stars by temperature and absolute magnitude in a H-R diagram
Main Sequence- diagonal band on H-R diagram
Upper left- hot, blue, bright stars
Lower right- cool, red, dim stars
Middle- average yellow stars like the Sun
Dwarfs and Giants- the ten percent of stars that don’t fall in the main sequence

17. B. Fusion of hydrogen occurs in star cores releasing huge amounts of energy Fusion in the core of the stars is achieved when the density and temperature arising from the gravitational pressure are high enough. There are different fusion cycles that occur in different phases of the life of a star . The first stage is the fusion of Hydrogen into Helium. This is the stage that our Sun is in.

19. C. Evolution of Stars 1. A nebula contracts and breaks apart from the instability caused by gravity a. Temperatures in each nebula chunk as particles move closer together. b. At 10 million K fusion begins and energy from a new star radiates into space

20. 2. The new main sequence star balances pressure from fusion heat with gravity a. Balance is lost when core hydrogen fuel is used up b. Core contracts and heats up causing outer layers to expand and cool c. Star becomes a giant as it expands and outer layers cool d. Helium nuclei fuse to form core of carbon

21. 3. A white dwarf forms from the giant star a
3. A white dwarf forms from the giant star a. Helium is exhausted and outer layers escape into space b. core contracts into hot, dense, small star Also called a degenerate dwarf, is a small star composed mostly of electron-degenerate matter. Because a white dwarf's mass is comparable to that of the Sun and its volume is comparable to that of the Earth, it is very dense

22. 4. In massive stars fusion causes higher temperatures and greater expansion into a supergiant a. Eventually fusion stops as iron is formed b. the core crashes inward causing the outer part to explode as an incredibly bright supernova

23. 5. The collapsed core of a supernova may form a neutron star of extremely high density 6. The mass of a tremendously big supernova core can collapse to a point, forming a black hole. a. gravity is so strong not even light can escape. b. Beyond a black hole’s event horizon gravity operates as it would before the mass collapsed

24. 7. Matter emitted by a star over its life time is recycled and can become part of a nebula

25. Section 4 Galaxies and the Universe
Galaxy- gravity holds together a large collection of stars, gas and dust.
1. Earth’s galaxy is Milky Way which is part of a galaxy cluster named the Local Group

26. 2. Spiral galaxies- spiral arms wind out from inner section; some have barred spirals with stars and gas in a central bar

27. 3. Elliptical galaxies- large 3-dimensional ellipses; most common shape

28. 4. Irregular galaxies-smaller, less common galaxies with various different shapes

29. B. The Milky Way May contain one trillion stars
About 100,000 light years wide
Sun orbits galaxies core every 225 million years

31. C. Theories on the origin of the universe 1
C. Theories on the origin of the universe 1. Steady state theory universe has always existed just as it is now 2. Oscillating model- universe expands and contracts repeatedly over time

32. D. Universe is expanding 1
D. Universe is expanding 1. Doppler shift- light changes as it moves toward or away from an object a. Starlight moving toward Earth shifts to blue-violet end of spectrum b. Starlight moving away from Earth shifts to red end of spectrum 2. All galaxies outside the local group indicate a red shift in their spectra indicating they are moving away from Earth

33. E. Big Bang Theory- holds that the universe began 13
E. Big Bang Theory- holds that the universe began 13.7 billion years ago with a huge explosion that caused the expansion everywhere at the same time. 1. Galaxies more than 10 billion light years away give information about a young universe. 2. Whether the universe may eventually stop expanding and begin contracting is unknown.