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29:50 MODERN ASTRONOMY
Fifth Homework Set...October 27, 1999

Note: Having problems? Don't go around confused and despondent! Ask for help! The purpose of these problem sets is to help you learn something.

(1) A galaxy is observed to be receding from us at a velocity of 50,000 km/sec. How far away is it?
tex2html_wrap_inline15 Megaparsecs

(2) A spectral line which has a ``rest wavelength'' of 600 nanometers is observed in a radio galaxy at a wavelength of 660 nanometers. What is the velocity of recession of the galaxy?
tex2html_wrap_inline17 km/sec

(3) For the problem immediately above, what is the distance of the galaxy?
tex2html_wrap_inline19 Megaparsecs

(4) The redshift of 3C79 is 0.264. What would be the apparent magnitude of the most luminous star we see in the night sky? Check Appendix 12 for data. Would we be able to see it with the Hubble Space Telescope?
tex2html_wrap_inline21 Velocity of recession tex2html_wrap_inline23 . Therefore distance = 1131 Mpc, so distance modulus = 40 magnitudes. Most luminous stars tex2html_wrap_inline27 for absolute magnitude, so their apparent magnitude would be tex2html_wrap_inline29 .

(5) Quasars with a redshift of 2.0 are very common. When we see the light from such objects, how long ago was it produced in the quasar galaxy (i.e. what is the lookback time?)
tex2html_wrap_inline21 From Figure 24.4 we see that z=2.0 corresponds to a ``look-back time'' of 80 % of the age of the universe. For an age of the universe of 12 - 14 GYr, this means the look back time is 9.6 - 11.2 Gyr.




Steve Spangler
Wed Dec 8 13:42:38 CST 1999