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12/14 Name ___________________________________________ Block ________ Chapter 28 Stars and Galaxies Reading Guide Pages 612 – 630 Before you read: 1. Think about a fire you may have seen before. What color are the hottest flames? Blue 2. Why do you think some objects in the sky are brighter than others? Hotter, closer While you read: Page 612 1. What is the electromagnetic spectrum? List the types of electromagnetic radiation in order from longest of the left to shortest on the right. Radiation arranged in a continuum. Radio waves, Microwaves, Infrared, Visible Light, Ultra Violet, X-Rays, Gamma Rays Page 613614 2. What is a spectroscope and what does it tell us about stars? Separates visible white light into its colors, like a prism or rainbow Tells astronomer the composition of a star (elements and proportions) Page 615 3. What is the Doppler Effect? Tendency for light and sound waves to become longer when moving away and shorter when moving towards an observer. For example, you hear the high pitch of the siren of the approaching ambulance, and notice that its pitch drops suddenly as the ambulance passes you. Page 619 2. Why is Hipparchus important to astronomers? He devised a system to classify stars based on their brightness from Earth. Page 619 3. What is the apparent magnitude of a star? Measure of how bright a star appears from Earth 12/14 Page 619 3. Explain the difference between the two stars listed below: Star #1 – apparent magnitude = 1.67 Star #2 – apparent magnitude = -1.67 #2 is brighter as seen from Earth because it has a lower apparent magnitude Page 619 4. How do we measure distances to stars? Light Years Page 619 5. What is the closest star to Earth (besides the Sun)? Proxima Centauri Page 620 6. Why are light-years used to measure distances in space? Because of the vast distances Page 620 7. What is parallax? (Use your thumb to demonstrate it to yourself) Apparent shift in position due to the location of the observer. Used to measure the distance of stars Page 620 8. Why do astronomers call star spectra the “fingerprints of stars”? Each star has a unique spectrum Page 621 9. What color are the hottest stars? Blue Page 622 10. What color is our Sun? (make sure you read, it is NOT yellow!) White with a twinge of yellow Page 623 11. Luminosity is the actual brightness of a star. What two factors determine luminosity? Size and temperature 12/14 Page 623 12. A star’s absolute magnitude is how bright it would be if all stars were the same distance (10 parsecs) from Earth. If the apparent magnitude of Sirius is –1.44 and the absolute magnitude is +1.42, what does this tell you about the distance of Sirius from the Earth? Sirius is closer to Earth than 10 parsecs. Even though it is the brightest star in the sky as seen from Earth, it is close to earth, but relatively dim. Page 626 13. What is the H-R diagram? Plots luminosity and temperature of stars. Page 626 14. Look at the H-R diagram. What is unusual about labeling of the x- and y-axes? (Think about how we normally number an axis.) The hotter temperatures are to the left of the X-axis and the cooler temperatures are towards the right. After you read: 15. The Sun has an apparent magnitude of –26.7. A friend tells you about a star that also has a magnitude of –26.7. How could this be true? The friend can be referring to absolute magnitude and not apparent magnitude 16. We are not able to visit distant stars, yet we can determine how far away they are. How do parallax and math help us do this? A nearby star's apparent movement against the background of more distant stars as the Earth revolves around the Sun is referred to as stellar parallax. Nearby objects have a larger parallax than more distant objects when observed from different positions, so parallax can be used to determine distances. By observing parallax, measuring angles, and using geometry, one can determine distance.