DLAP questions | universe10e_ch6_1_dlap.xml | 53486f26757a2ef364000000 |
6-1 A refracting telescope uses a lens to concentrate incoming light at a focus
| universe10e_ch6_2.html | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_2_dlap.xml | 53486f26757a2ef364000000 |
6-2 A reflecting telescope uses a mirror to concentrate incoming light at a focus
| universe10e_ch6_3.html | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_3_dlap.xml | 53486f26757a2ef364000000 |
6-3 Telescope images are degraded by the blurring effects of the atmosphere and by light pollution
| universe10e_ch6_4.html | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_4_dlap.xml | 53486f26757a2ef364000000 |
6-4 A charge-coupled device is commonly used to record the image at a telescope’s focus
| universe10e_ch6_5.html | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_5_dlap.xml | 53486f26757a2ef364000000 |
6-5 Spectrographs record the spectra of astronomical objects
| universe10e_ch6_6.html | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_6_dlap.xml | 53486f26757a2ef364000000 |
6-6 A radio telescope uses a large concave dish to reflect radio waves to a focus
| universe10e_ch6_7.html | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_7_dlap.xml | 53486f26757a2ef364000000 |
6-7 Telescopes in orbit around Earth detect radiation that does not penetrate the atmosphere
| universe10e_ch6_8.html | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_8_dlap.xml | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_9_dlap.xml | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_10_dlap.xml | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_11_dlap.xml | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_12_dlap.xml | 53486f26757a2ef364000000 |
DLAP questions | universe10e_ch6_13_dlap.xml | 53486f26757a2ef364000000 |