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QUESTIONS/ANALYSIS: 1) Given the data in Table F, plot the stars on your HR diagram, label them by name, and estimate their complete spectral type. Star # Betelgeuse The Sun Arcturus Polaris Pollux Vega Table F: Stellar photometric data B-V My 1.85 0.63 1.23 0.60 1.00 0.00 -5.85 4.83 -0.30 -3.60 1.08 0.58 Spectral Type

QUESTIONS/ANALYSIS: 1) Given the data in Table F, plot the stars on your HR diagram, label them by name, and estimate their complete spectral type. Star # Betelgeuse The Sun Arcturus Polaris Pollux Vega Table F: Stellar photometric data B-V My 1.85 0.63 1.23 0.60 1.00 0.00 -5.85 4.83 -0.30 -3.60 1.08 0.58 Spectral Type

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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Hello sir, can I get some help with table F please?
3. Draw a smooth, curving line through your points to indicate the main sequence. (Do not "connect-the-dots" with a zig-zag line!). Label it "Main Sequence (V)." 4. Table D gives the B-V colors, and absolute magnitudes (M) for a set of giant stars. Plot the stars on Figure 1. Number each point you plot! 5. You should see two new groupings of stars. Draw a smooth, curving line through your points on the upper group to indicate the supergiants. (Do not "connect-the- dots" with a zig-zag line!). Label it "Supergiants (I).” 6. Draw a smooth, curving line through your points on the lower group to indicate the giants. (Do not "connect-the-dots" with a zig-zag line!). Label it "Giants (III)." 7. Table E gives the B-V colors, and absolute magnitudes (M) for a set of white dwarfs. Plot the stars on Figure 1. Number each point you plot! 8. Draw a smooth, curving line through your new points. (Do not "connect-the-dots" with a zig-zag line!). Label it "White Dwarfs (VII)." VOCABULARY: Apparent magnitude (m) Absolute magnitude (M) Distance modulus (m-M) Parsec Wavelength band Luminosity classes QUESTIONS/ANALYSIS: 1) Given the data in Table F, plot the stars on your HR diagram, label them by name, and estimate their complete spectral type. Star # Betelgeuse The Sun Arcturus Polaris Pollux Vega Table F: Stellar photometric data B-V Mv 1.85 0.63 1.23 0.60 1.00 0.00 -5.85 4.83 -0.30 -3.60 B-V color index Spectral classes Spectral classes Luminosity classes Spectral type HR Diagram 1.08 0.58 Spectral Type
Transcribed Image Text:3. Draw a smooth, curving line through your points to indicate the main sequence. (Do not "connect-the-dots" with a zig-zag line!). Label it "Main Sequence (V)." 4. Table D gives the B-V colors, and absolute magnitudes (M) for a set of giant stars. Plot the stars on Figure 1. Number each point you plot! 5. You should see two new groupings of stars. Draw a smooth, curving line through your points on the upper group to indicate the supergiants. (Do not "connect-the- dots" with a zig-zag line!). Label it "Supergiants (I).” 6. Draw a smooth, curving line through your points on the lower group to indicate the giants. (Do not "connect-the-dots" with a zig-zag line!). Label it "Giants (III)." 7. Table E gives the B-V colors, and absolute magnitudes (M) for a set of white dwarfs. Plot the stars on Figure 1. Number each point you plot! 8. Draw a smooth, curving line through your new points. (Do not "connect-the-dots" with a zig-zag line!). Label it "White Dwarfs (VII)." VOCABULARY: Apparent magnitude (m) Absolute magnitude (M) Distance modulus (m-M) Parsec Wavelength band Luminosity classes QUESTIONS/ANALYSIS: 1) Given the data in Table F, plot the stars on your HR diagram, label them by name, and estimate their complete spectral type. Star # Betelgeuse The Sun Arcturus Polaris Pollux Vega Table F: Stellar photometric data B-V Mv 1.85 0.63 1.23 0.60 1.00 0.00 -5.85 4.83 -0.30 -3.60 B-V color index Spectral classes Spectral classes Luminosity classes Spectral type HR Diagram 1.08 0.58 Spectral Type
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