Great Debate (astronomy)
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In astronomy, the Great Debate, also called the Shapley–Curtis Debate, was an influential debate, held on 26 April 1920 at the Smithsonian Museum of Natural History, between the astronomers Harlow Shapley and Heber Curtis.
The debate concerned the nature of so-called spiral nebulae and the size of the universe, specifically whether distant nebulae were relatively small and lay within the outskirts of the Earth's home galaxy or whether they were in fact independent galaxies, implying that they were exceedingly large and distant.
The two scientists first presented independent technical papers about "The Scale of the Universe" during the day and then took part in a joint discussion that evening. Much of the lore of the Great Debate grew out of two papers published by Shapley and by Curtis in the May 1921 issue of the Bulletin of the National Research Council. The published papers each included counter arguments to the position advocated by the other scientist at the 1920 meeting.
Shapley was arguing in favor of the Milky Way as the entirety of the then known universe. He believed that "spiral nebulae" such as Andromeda were simply part of the Milky Way. He could back up this claim by citing 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 astronomers would not accept. Adriaan van Maanen was also providing evidence to Shapley's argument. Van Maanen was a well-respected astronomer of the time who claimed he had observed the Pinwheel Galaxy rotating. If the Pinwheel Galaxy were in fact a distinct galaxy and could be observed to be rotating on a timescale of years, its orbital velocity would be enormous and there would clearly be a violation of the universal speed limit, the speed of light. Also used to back up his claims was the observation of a nova in the Andromeda "nebula" that had briefly outshone the entire nebula, constituting a seemingly impossible output of energy were Andromeda in fact a separate galaxy.
Curtis on the other side contended that Andromeda and other such "nebulae" were separate galaxies, or "island universes" (a term invented by the 18th-century philosopher Immanuel Kant, who also believed 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 galaxy than the other sections of the galaxy, if Andromeda was not a separate galaxy but simply a nebula within the Earth's galaxy. This led to supporting Andromeda as a separate galaxy with its own signature age and rate of nova occurrences. He also cited dark lanes present in other galaxies similar to the dust clouds found in the Earth's own galaxy and massive doppler shifts found in other galaxies.
Curtis stated that if van Maanen's observation of the Pinwheel Galaxy rotating were correct, he himself would have been wrong about the scale of the universe and that the Milky Way would fully encompass it.
After the debateEdit
Due to the work of Edwin Hubble, it is now known that the Milky Way is only one of as many as an estimated 200 billion (×1011) 2 to 2 trillion (×1012) or more galaxies 2 (containing more stars than all the grains of sand on planet Earth), proving Curtis the more accurate party in the debate. Also, astronomers generally accept that the nova Shapley referred to in his arguments was in fact a supernova, which do 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 (Curtis' galaxy was centered on the Sun, while Shapley correctly placed the Sun in the outer regions of the galaxy).
Other Great DebatesEdit
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", the Smithsonian has hosted 4 more events.
- Gott III, J. R.; et al. (2005). "A Map of the Universe". The Astrophysical Journal. 624 (2): 463–484. Bibcode:2005ApJ...624..463G. arXiv: . doi:10.1086/428890.
- Christopher J. Conselice; et al. (2016). "The Evolution of Galaxy Number Density at z < 8 and its Implications". The Astrophysical Journal. 830 (2): 83. arXiv: . doi:10.3847/0004-637X/830/2/83.
- Fountain, Henry (17 October 2016). "Two Trillion Galaxies, at the Very Least". The New York Times. Retrieved 17 October 2016.
- Mackie, Glen (1 February 2002). "To see the Universe in a Grain of Taranaki Sand". Centre for Astrophysics and Supercomputing. Retrieved 28 January 2017.
- "Why the 'Great Debate' was important". NASA/Goddard Space Flight Center. Retrieved 2009-10-16.
- Shapley, H.; Curtis, H. D (1921). "The scale of the universe". Bulletin of the National Research Council. 2 (Part 3, Issue 11): 171–217. Bibcode:1921BuNRC...2..171S. (The original publication of the debate.)
- "The Shapley–Curtis Debate in 1920". (Resources related to the debate at the NASA website)
- Trimble, V. (1995). "The 1920 Shapley–Curtis Discussion: Background, Issues, and Aftermath". Publications of the Astronomical Society of the Pacific. 107: 1133. Bibcode:1995PASP..107.1133T. doi:10.1086/133671.