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ASTR 1020 - Lab 9:  Cepheids - Part B
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In Part B, we will use a Python computer coding script to obtain a spectral redshift of a galaxy (M100). From this redshift, we will use the Doppler formula to find a recession speed. From this speed, we will apply Hubble’s Law to obtain the Hubble Constant.---------------------------------------Distant Nature: Astronomy Exercises 2016 by Stephen Tuttle under license "Creative Commons Attribution Non-Commercial Share Alike".

Subject:
Astronomy
Material Type:
Activity/Lab
Author:
Hollyanna White
Date Added:
05/13/2022