FileTitleManuscript Id
[Unknown Title]universe10e_ch17_1.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_1_dlap.xml534c6a91757a2ed532000002
17-1 Careful measurements of the parallaxes of stars reveal their distances universe10e_ch17_2.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_2_dlap.xml534c6a91757a2ed532000002
17-2 If a star’s distance is known, its luminosity can be determined from its apparent brightness universe10e_ch17_3.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_3_dlap.xml534c6a91757a2ed532000002
17-3 Astronomers often use the magnitude scale to denote brightness universe10e_ch17_4.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_4_dlap.xml534c6a91757a2ed532000002
17-4 A star’s color depends on its surface temperature universe10e_ch17_5.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_5_dlap.xml534c6a91757a2ed532000002
17-5 The spectra of stars reveal their chemical compositions as well as their surface temperatures universe10e_ch17_6.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_6_dlap.xml534c6a91757a2ed532000002
17-6 Stars come in a wide variety of sizes and temperatures universe10e_ch17_7.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_7_dlap.xml534c6a91757a2ed532000002
17-7 Hertzsprung-Russell (H-R) diagrams reveal different kinds of stars universe10e_ch17_8.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_8_dlap.xml534c6a91757a2ed532000002
17-8 Details of a star’s spectrum reveal whether it is a giant, a white dwarf, or a main-sequence star universe10e_ch17_9.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_9_dlap.xml534c6a91757a2ed532000002
17-9 Observing binary star systems reveals the masses of stars universe10e_ch17_10.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_10_dlap.xml534c6a91757a2ed532000002
17-10 Spectroscopy makes it possible to study binary systems in which the two stars are close together universe10e_ch17_11.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_11_dlap.xml534c6a91757a2ed532000002
17-11 Light curves of eclipsing binaries provide detailed information about the two stars universe10e_ch17_12.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_12_dlap.xml534c6a91757a2ed532000002
Key Wordsuniverse10e_ch17_13.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_13_dlap.xml534c6a91757a2ed532000002
Key Ideasuniverse10e_ch17_14.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_14_dlap.xml534c6a91757a2ed532000002
Questionsuniverse10e_ch17_15.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_15_dlap.xml534c6a91757a2ed532000002
Activitiesuniverse10e_ch17_16.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_16_dlap.xml534c6a91757a2ed532000002
Answersuniverse10e_ch17_17.html534c6a91757a2ed532000002
DLAP questionsuniverse10e_ch17_17_dlap.xml534c6a91757a2ed532000002