4.4: Wrapping It Up 4 - The Andromeda Shift
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In this part of the activity, you will make measurements of Andromeda’s motion using the Doppler shift. From those measurements you will determine Andromeda’s rotation speed and systemic velocity.
1. First you will look at spectra taken from opposite sides of the Andromeda Galaxy (M31), and compare them to a spectrum taken at rest to determine which way the galaxy is spinning. By observing the Doppler shift (either redshift or blueshift) of the spectra at either end, you can tell in which direction M31 is spinning. The spectrum being observed is a very small sliver of the galaxy’s actual spectrum. It is limited to the region around one of the most prominent lines of galaxy spectra, the Hß line.
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