Name______Period______
Hertzsprung-Russell Diagram
Purpose: Use provided data and your own observations to identify the characteristics used to classify stars and place them on the H-R Diagram
Materials: Planetarium dome, HR diagram, colored pencils
Procedure:
- Observe stars on dome andwrite apparent magnitude, color, distance, and spectral class on data table 7-1.
Table 7-1: Star Temperature and Luminosity
Star Name / # / Color / Spectral Type / Apparent
magnitude / Distance
(l.y.) / Temperature
(K) / Luminosity
(relative to sun) / Mass
(solar mass)
Rigel / 1 / 14 000 / 66 000 / 20
Betelgeuse / 2 / 3 500 / 12 000 / 20
Polaris / 3 / 6 500 / 1 000 / 6
Aldebaran / 4 / 4 000 / 100 / 1.7
Sun / 5 / 6 000 / 1 / 1
Regulus / 6 / 12 300 / 300 / 3.5
Vega / 7 / 9 700 / 60 / 2.3
Spica / 8 / 19 700 / 10 000 / 10
Procyon / 9 / 6530 / 7.3 / 1.4
Pollux / 10 / 4865 / 43 / 1.8
Sirius A / 11 / 10,000 / 25 / 2
Bellatrix / 12 / 22,000 / 6,400 / 8.4
Sirius B / 13 / x / x / x / 8.6 / 25,000 / .03 / 1
Tau Ceti / 14 / x / x / x / 12 / 5 000 / 0.50 / 0.8
Alpha Centauri B / 15 / x / x / x / 4.3 / 4 300 / 0.3 / 0.9
Barnard’s Star / 16 / x / x / x / 5.98 / 3 000 / 0.002 / .17
Procyon B / 17 / x / x / x / 11.5 / 7 740 / 0.01 / 0.6
- On the final page of this packet, label each axis of the HR Diagram correctly (temperature or luminosity)
- Using the data from table 7-1, plot the position of each star using its approximate temperature and luminosity by writing its number in the correct location on the H-R diagram
- In the “COLOR” box at the bottom of your HR Diagram,shade in each temperature region of the with the correct star color, using the information on table 7-2 below.
Table 7-2 Star Temperature, Spectral Class, and Color
Star Temperature (oK) / Spectral Class / Star Color
Less than 3,600 / M / Red
3,6000 – 5,000 / K / Orange
5,000 - 6,000 / G / Yellow
6,000 – 7,500 / F / Yellow-White (pale yellow)
7,500 – 10,000 / A / White
10,000-28,000 / B / Blue-White (pale blue)
Greater than 28,000 / O / Blue
- In bold letters, label the following regions of your HR diagram with the following terms:
White DwarfRed DwarfsGiants Main Sequence Supergiants
- In the “SPECTRAL CLASS” box at the bottom of the HR diagram, write the spectral class that coincides with each temperature range, using table 7-2 above.
Analysis questions:
1. As stars change color from red to blue, what happens to its surface temperature?
2. A main sequence star that is 100 times more luminous than the sun most likely has a temperature of
______.
4. A main sequence star that has a luminosity of 10 is most likely to be what color? ______
5. Name a white dwarf star that you plotted on your HR diagram:
- A massive star with a temperature of 20,000K and a luminosity of nearly 100,000 would be classified as what
type of star? ______
7. Our sun has a Luminosity of ______and a temperature of ______
8. Other than the sun, name two other Main Sequence stars that you plotted on your HR diagram:
9. Why do you think we could not observe stars #13-17 on the dome?
10. Compare the apparent magnitudes, luminosities, and distances for Pollux (#10) and Bellatrix (#12). Why does
Pollux appear brighter in the sky when Bellatrix is so much more luminous?
- Label each axis
- Plot the stars by number
- Use colored pencils in the “color box” near the bottomto indicate the data shown on table 7-2
- Label these regions of the diagram: White Dwarf, Red Dwarfs, Main Sequence,Giants, Supergiants
- In the “Spectral Class” box, write the letters of spectral classes in the order that corresponds with each temperature.
HR Diagram