Great Debate (astronomy)

The debate was the topic of that year's William Ellery Hale lecture during a meeting of the National Academy of Sciences in the Baird Auditorium of the U.S. National Museum in Washington, D.C.(now the Smithsonian Museum of Natural History). Most of the Academy members in attendance that night were not astronomers. The topics considered for that year's meeting included Einstein's theory of relativity, glaciers, and even zoological or biological subjects, before a debate on "The Distance Scale of the Universe" was chosen. Shapley and Curtis agreed to a format where each would present their opposing views in back-to-back 40-minute lectures. Shapley worked from a typed script and presented a general background introduction to astronomy before going on to his views on the size of the universe. Curtis worked from a set of notes and presented his lecture points in type written projected photographic slides. No transcript of the debate exists; its content has been pieced together over the years from Shapley's original annotated typewritten script, Curtis's slides (his script was discarded after the lecture), and both participants' letters. ==The debate==

(1902 photograph). The Debate was over whether this was a cloud of gas and dust or a distant galaxy. Shapley presented the case that the Milky Way is the entirety of the Universe. In his astronomical work he had been coming up with estimates for the size of the Milky Way using globular clusters and the Cepheid variables found within them. He presented the audience with a "universe" 300,000 light-years in diameter with the Sun off to one side. He spent most of his lecture describing the vast size of the Milky Way and towards the end argued that "spiral nebulae" such as Andromeda were simply objects on the edge of the Milky Way itself. He backed up this claim by appealing to their relative sizes—if Andromeda and other spiral nebulae were not part of the Milky Way but were in fact similar island universes, then, given the vast size of the Milky Way, the distance to them would be a span most contemporary astronomers would not accept. Curtis, on the other hand, described a Milky Way 30,000 light-years across, one tenth the size of the one postulated by Shapley, and contended that Andromeda and other such "nebulae" were similarly smaller separate galaxies, or "island universes" (a term invented by the 18th-century philosopher Immanuel Kant, who also argued that the "spiral nebulae" were extragalactic). He showed that there were more novae in Andromeda than in the Milky Way. From this, he could ask why there were more novae in one small section of the Milky Way than the other sections of the Milky Way, if Andromeda were not a separate galaxy but simply a nebula within Earth's galaxy. This led to supporting Andromeda as a separate galaxy with its own signature age and rate of nova occurrences. Curtis also noted the large radial velocities of spiral nebulae that suggested they could not be gravitationally bound to the Milky Way in a single island universe model universe. Curtis pointed out a similarity in structure that explained why there were no spiral nebulae visible along the plane of the Milky Way (referred to as the Zone of Avoidance); both the Milky Way and the spiral nebulae had similar dust clouds along their plane, and that dust in the Milky Way blocked our view of the spiral nebulae. ==The followup paper==

In a May 1921 issue of the Bulletin of the National Research Council Harlow Shapley and Heber Curtis sides of the debate were presented and expanded on in independent technical papers under the title "The Scale of the Universe". Shapley and Curtis were able to read each other's paper and edit their final published papers so that that they could present more refined counterarguments. Expanding on his comments at the debate, Shapley argued that "spiral nebulae" such as Andromeda were simply part of the Milky Way. He backed up this claim by appealing to their relative sizes—if Andromeda were not part of the Milky Way, then its distance must have been on the order of 108 light years—a span most contemporary astronomers would not accept. Shapley's paper cited the work of Adriaan van Maanen, a well-respected astronomer of the time, as providing evidence supporting Shapley's argument. Van Maanen had claimed he had observed the Pinwheel Galaxy rotating, ==Aftermath==

Later in the 1920s, Edwin Hubble showed that Andromeda was far outside the Milky Way by measuring Cepheid variable stars, proving that Curtis was correct. It is now known that the Milky Way is only one of as many as an estimated 200 billion () to 2 trillion () or more galaxies in the observable Universe. Also, astronomers generally accept that the nova Shapley referred to in his arguments was in fact a supernova, which does indeed temporarily outshine the combined output of an entire galaxy. On other points, the results were mixed (the actual size of the Milky Way is in between the sizes proposed by Shapley and Curtis), or in favor of Shapley (the Sun was near the center of the galaxy in Curtis's model, while Shapley correctly placed the Sun in the outer regions of the galaxy). It later became apparent that van Maanen's observations were incorrect—one cannot actually see the Pinwheel Galaxy rotate during a human lifespan. == Other Great Debates ==

The format of the great debate has been used subsequently to argue the nature of fundamental questions in astronomy. In honor of the first Great Debate's diamond jubilee (75th anniversary) in 1995 the Smithsonian hosted another debate on "The Distance Scale to Gamma-ray Bursts," between Bohdan Paczyński and Donald Q. Lamb. == Notes ==