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Nearest Stars Alpla Cenmur Barnard's STAL WET 359 Calande 21185 Sirius Luyten 726-8 Ross 154 Ross 248 5800 2800 2700 3200 10400 2700 2800 2700 Temperattir Absoforo Magnited the 20 Brightest Stars as seen Eura (8) +13.2 +16.8 - 10.S +15.4 +13.3 Sirius Canopus Alpha Centauri Arcturus Vega Capella Rigel 10400 7400 $800 4500 10700 5900 11800 414 -31 <-44 -0.3 +0.5 -0.7 -6.8

Nearest Stars Alpla Cenmur Barnard's STAL WET 359 Calande 21185 Sirius Luyten 726-8 Ross 154 Ross 248 5800 2800 2700 3200 10400 2700 2800 2700 Temperattir Absoforo Magnited the 20 Brightest Stars as seen Eura (8) +13.2 +16.8 - 10.S +15.4 +13.3 Sirius Canopus Alpha Centauri Arcturus Vega Capella Rigel 10400 7400 $800 4500 10700 5900 11800 414 -31 <-44 -0.3 +0.5 -0.7 -6.8

Applications and Investigations in Earth Science (9th Edition)
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
Problem 1LR
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POM The 20 Nearest Stars Barnard's to Star LAN WON 359 Calande 211853 Sirrus Luyten 726-8 Ross 154 Ross 248 Temperato Absolute Epsilon Eridani Ross 128 Luyten 789-6 61 Cygni Procyon Epsilon Indi Sigma 2398 3800 2800 2700 3200 10400 2700 2800 2700 4500 2800 2700 2800 6800 4200 3000 3200 BD +43-441 Tau Ceti 5200 CD-36 15693 3100 BD+5-1668 3000 CD-39-14192 3500 Name Temperatur Absoture Magnited the 20 Brightest Stars as seen fourth 444 +16.8 +10 S +14 +15.4 +13.3 +14.7 -6.1 -13.5 +14.9 +7.5 +2.7 +7.0 +11.1 +10.3 +5.7 +9.6 +11.9 +8.7 Sirius Canopus Alpha Centauri Arcturus Vega Capella Rigel Procyon Betelgeuse Achernar Beta Centauri Altair Alpha Crucis Aldebaran Spica Antares Pollux Fomalhaut Deneb Beta Crucis 10400 7400 $800 4500 10700 5900 11800 6800 3200 14000 21000 8000 21000 4200 21000 3400 4900 9500 9900 22000 414 -31 +44 -03 +0.5 -0.7 -6.8 +2.7 -5.5 -1.0 41 +2.2 -4.0 -0.2 -3.6 -4.5 +0.8 +2.0 -6.9 -4.6 1. Compare the two lists above, how many stars appear on both lists? Name the stars that you can find on both lists. 2. Are the nearest stars ALWAYS the brightest? Is the list on the left the same as the right? 3. A star located in the lower right portion of the HR Diagram is cool and dini. What are the characteristics of a star in the upper left? What about the stars in the upper right? 4 Look on page 819 of the textbook, in which group do most of the stars belong? 5. According to your diagram, are any of these stars white dwarfs? Explain how you know. 6. In order to be a star, it must burn gas through a process called fusion. What is fusion?
Transcribed Image Text:POM The 20 Nearest Stars Barnard's to Star LAN WON 359 Calande 211853 Sirrus Luyten 726-8 Ross 154 Ross 248 Temperato Absolute Epsilon Eridani Ross 128 Luyten 789-6 61 Cygni Procyon Epsilon Indi Sigma 2398 3800 2800 2700 3200 10400 2700 2800 2700 4500 2800 2700 2800 6800 4200 3000 3200 BD +43-441 Tau Ceti 5200 CD-36 15693 3100 BD+5-1668 3000 CD-39-14192 3500 Name Temperatur Absoture Magnited the 20 Brightest Stars as seen fourth 444 +16.8 +10 S +14 +15.4 +13.3 +14.7 -6.1 -13.5 +14.9 +7.5 +2.7 +7.0 +11.1 +10.3 +5.7 +9.6 +11.9 +8.7 Sirius Canopus Alpha Centauri Arcturus Vega Capella Rigel Procyon Betelgeuse Achernar Beta Centauri Altair Alpha Crucis Aldebaran Spica Antares Pollux Fomalhaut Deneb Beta Crucis 10400 7400 $800 4500 10700 5900 11800 6800 3200 14000 21000 8000 21000 4200 21000 3400 4900 9500 9900 22000 414 -31 +44 -03 +0.5 -0.7 -6.8 +2.7 -5.5 -1.0 41 +2.2 -4.0 -0.2 -3.6 -4.5 +0.8 +2.0 -6.9 -4.6 1. Compare the two lists above, how many stars appear on both lists? Name the stars that you can find on both lists. 2. Are the nearest stars ALWAYS the brightest? Is the list on the left the same as the right? 3. A star located in the lower right portion of the HR Diagram is cool and dini. What are the characteristics of a star in the upper left? What about the stars in the upper right? 4 Look on page 819 of the textbook, in which group do most of the stars belong? 5. According to your diagram, are any of these stars white dwarfs? Explain how you know. 6. In order to be a star, it must burn gas through a process called fusion. What is fusion?
7. On your diagram, put a large star where the sun is located. Describe the approximate temperature and brightness of our sun, compared to other stars. 8. Which is farther along in its life cycle: Betelgeuse or our sun? How do you know? 9. Describe what will eventually happen to our sun. What stages will it go through after it burns up its hydrogen and is no longer a main sequence star? :::: 8. 10.10
Transcribed Image Text:7. On your diagram, put a large star where the sun is located. Describe the approximate temperature and brightness of our sun, compared to other stars. 8. Which is farther along in its life cycle: Betelgeuse or our sun? How do you know? 9. Describe what will eventually happen to our sun. What stages will it go through after it burns up its hydrogen and is no longer a main sequence star? :::: 8. 10.10
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