The Shapley – Curtis Debate 26 Apr 1920
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Transcript of The Shapley – Curtis Debate 26 Apr 1920
The Shapley – Curtis Debate 26 Apr 1920Center of the Galaxy How big is the universeNebula vs. Galaxies Are “nebula” local or distant
Heber Curtis
• Degree in Classical Languages
• Amateur Astronomer @ Napa College
• Ph.D. in Astro from UVa in 1902
• Director of Allegheny Observatory @ Pitt
Heber Curtis
• Sun is at the center of the Milky Way—oops
• Cepheids are not good for distance measurements—oops
• Milky Way size about 10K parsecs—oops
• Nebula are Galaxies beyond the MW--yea
Harlow Shapley
• Missouri to study journalism
• Switched to astronomy• Ph.D. 1913 @ Princeton
under H.N. Russell• Director of Harvard
Observatory• Founder of UNESCO• FBI Investigation
Harlow Shapley
• Galaxy 100K parsecs—oops (too big)
• Sun is 20K parsecs from the center—yea
• Nebula minor gaseous populations in the Milky Way--oops
The Distance Ladder
• Photometric parallax--using geometry to measure distance to nearby stars
• Standard Candles—using decreasing brightness from certain stars to measure distance to nearby galaxies
Cepheid Variables
• Class of stars whose brightness varies with time
• Period is proportional to intrinsic brightness
• Using inverse square law and knowing period distance can be calculated
Cepheid Variables
• Period vs. luminosity discovered by Henrietta Swan Leavitt
• Worked at Harvard classifying stars
• Opened the way for Hubble, Hurtzsprung and Russell
The Great Debate--Resolved
Edwin Hubble• Used Cepheids to show
Andromeda was beyond the Milky Way
• Discovered “Red Shift”—evidence of an expanding universe
• Erased Einstein’s “Cosmological Constant”