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slater2e_ch10_1.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_1_dlap.xml53922a64757a2e4848000002
10-1 Measuring the distances to nearby stars utilizes an effect called parallax slater2e_ch10_2.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_2_dlap.xml53922a64757a2e4848000002
10-2 A star’s brightness can be described in terms of luminosity or magnitude slater2e_ch10_3.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_3_dlap.xml53922a64757a2e4848000002
10-3 A star’s distance can be determined by comparing its luminosity and brightness slater2e_ch10_4.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_4_dlap.xml53922a64757a2e4848000002
10-4 A star’s color depends on its surface temperature slater2e_ch10_5.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_5_dlap.xml53922a64757a2e4848000002
10-5 The spectra of stars reveal their chemical compositions as well as surface temperatures and sizes slater2e_ch10_6.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_6_dlap.xml53922a64757a2e4848000002
10-6 Stars come in a wide variety of sizes and masses slater2e_ch10_7.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_7_dlap.xml53922a64757a2e4848000002
10-7 Hertzsprung-Russell (H-R) diagrams reveal the different kinds of stars slater2e_ch10_8.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_8_dlap.xml53922a64757a2e4848000002
Key Ideas and Termsslater2e_ch10_9.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_9_dlap.xml53922a64757a2e4848000002
Questionsslater2e_ch10_10.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_10_dlap.xml53922a64757a2e4848000002
Answersslater2e_ch10_11.html53922a64757a2e4848000002
DLAP questionsslater2e_ch10_11_dlap.xml53922a64757a2e4848000002