Procedure: 1. Plot the stars listed in the data table at right on the graph paper provided. 2. Draw a circle around each grouping of stars on your graph. How many groups did you circle? 3. Label the following on your graph: main sequence, red giants, white dwarfs, supergiants. 4. Circle the dot representing the sun. What type of star is the sun?
Procedure: 1. Plot the stars listed in the data table at right on the graph paper provided. 2. Draw a circle around each grouping of stars on your graph. How many groups did you circle? 3. Label the following on your graph: main sequence, red giants, white dwarfs, supergiants. 4. Circle the dot representing the sun. What type of star is the sun?
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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Transcribed Image Text:HERTZSPRUNG-RUSSELL DIAGRAM
100,000
40,000
20,000
10,000
4000
2000
1000
400
200
100
40
20
10
4.0
2.0
1.0
.4
.1
.04
.02
.01
.004
.002
.001
35
30
25
20
18
16
14
12
10
8.
7
6.
4.
Surface Temperature ( x 1000°C )
2.
3.
2.
Luminosity ( x Sun)

Transcribed Image Text:Astronomers use two basis properties of stars to classify them. These two properties are
luminosity and surface temperature. Luminosity usually refers to the brightness of the star relative to
the brightness of our sun. Astronomers will often use a star's color to measure its temperature. Stars
with low temperature produce a reddish light while stars with high temperatures shine with a brilliant
blue-white light. Surface temperatures of stars range from 3000 degrees Celsius to 50,000 degrees
Celsius. When these surface temperatures are plotted against luminosity, the stars fall into groups.
Using data similar to what you will plot in this activity, Danish astronomer Ejnar Hertzsprung and US
astronomer Henry Norris Russell independently arrived at similar results in what is now commonly
referred to as the HR diagram.
Purpose: To make a Hertzsprung-Russell diagram.
Procedure:
1. Plot the stars listed in the data table at right on the graph paper provided.
2. Draw a circle around each grouping of stars on your graph.
How many groups did you circle?
3. Label the following on your graph: main sequence, red giants, white dwarfs, supergiants.
4. Circle the dot representing the sun. What type of star is the sun?
LUMINOSITY
(X SUN)
STAR
SURFACE
STAR
LUMINOSITY
SURFACE
TEMPERATURE
TEMPERATURE
(Х 1000°C)
(X 1000°C)
20
1. Orion
3. Polaris
5. Antares
7. Spica
9. Vega
11. Procyon A
13. Regulus
15. Lacaille
2. Betelgeuse
4. Achemar
6. Aldebaran
8. Ceti
10,000
20,000
3
6
5.9
2,000
100
24
1,000
3
4
800
25
.1
4.5
40
12
10. Sirius A
20
11
50
6.9
12. Sun
1
5.7
1,000
18
14. Procyon B
.004
6.6
.02
4.5
16. Altair
.01
9
17. Sirius B
.01
18. Alpha Centauri
1.6
5.7
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