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Table of contents

The Nature of the Stars

Guiding Questions

Parallax

Slide 4

Slide 5

Careful measurements of the parallaxes of stars reveal their distances

Barnard’s star has a parallax of 0.54 arcsec

Slide 8

If a star’s distance is known, its luminosity can be determined from its brightness

Slide 10

The Population of Stars

Stellar Motions

Astronomers often use the magnitude scale to denote brightness

Slide 14

A star’s color depends on its surface temperature

Slide 16

Photometry and Color Ratios

Slide 18

The spectra of stars reveal their chemical compositions as well as surface temperatures

Slide 20

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Slide 22

Relationship between a star’s luminosity, radius, and surface temperature

Finding Key Properties of Nearby Stars

Hertzsprung-Russell (H-R) diagrams reveal the different kinds of stars

Slide 26

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Slide 28

Spectroscopic Parallax

A Binary Star System

Binary Stars

Slide 32

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Slide 34

Binary star systems provide crucial information about stellar masses

Mass-Luminosity Relation for Main-Sequence Stars

Slide 37

Spectroscopy makes it possible to study binary systems in which the two stars are close together

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Light curves of eclipsing binaries provide detailed information about the two stars

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Key Words

Author: Michael Cohen

E-mail: mrcohe@ship.edu

Homepage: http://physics.ship.edu/~mrc/