Ninety seven years ago, #OTD in 1925, Edwin Hubble announced that our Milky Way was just one of many lonely little islands of stars sprinkled throughout the Universe. Andromeda and all the other “spiral nebulae” were in fact separate galaxies, outside the Milky Way.
Hubble’s announcement — other galaxies exist! — was made on the third day of the 33rd Meeting of the American Astronomical Society, in a paper read by H.N. Russell. The meeting started on December 30th; I don’t know if Hubble waited for New Year’s Day to be dramatic.
Hubble’s work, conducted with the 100-inch Hooker Telescope at Mount Wilson observatory, relied on earlier measurements by Vesto Slipher and Henrietta Swan Leavitt’s results on Cepheid variable stars.
Image: Huntington Library
It’s hard to imagine the pre-Hubble view of the Universe, though it was less than 100 years ago. Many (if not most) astronomers believed that the collection of stars we now recognize as our galaxy was… everything.
But there had always been astronomers who suspected that the Milky Way was just one of many galaxies. This view goes at least as far back as Immanuel Kant’s “Universal Natural History and Theory of the Heavens,” which he published anonymously in 1755.
The astronomer Harlow Shapley was perhaps the leading proponent of the establishment view at the time of Hubble’s announcement. He had long argued that spiral nebulae seen by astronomers — shapes any kid would now recognize as galaxies — were dust clouds inside the Milky Way.
Hubble kept Shapley in the loop as he built his case for separate galaxies, alerting him to the discovery of Cepheid variables in M31, M33, and other spiral nebulae throughout 1924.
It was the identification of Cepheid variables that allowed Hubble to prove that M31 and other spiral nebulae were so far away that they must be outside the Milky Way.
A Cepheid variable is a type of star whose brightness waxes and wanes over a period of time that tightly correlates with its maximum brightness. If you measure that period then you know its absolute brightness. Then if you know how bright it appears you can estimate its distance.
This important relationship, one of our primary tools in establishing the scale of the Universe, was first laid out by astronomer Henrietta Swan Leavitt:
Anyway, Shapley doubted Hubble’s claims at first, but eventually relented in the face of growing evidence.
Upon receiving one of Hubble's letters, Shapley remarked to doctoral student Cecilia Payne-Gaposchkin “Here is the letter that destroyed my universe.”
It seems hard to believe, but there are people alive today who were born into what scientists thought was a much smaller universe.
Alas, I had been planning on using Betty White here. She was born almost three years before Hubble’s announcement.
Astronomically speaking, January 1st is a meaningless date. However, today is also the 97th anniversary of humanity taking a monumental step towards understanding our place in a Universe that is vast and puzzling, but ultimately knowable.
Happy New Year!
Image: Richard Powell
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Kumlien’s Gull is a sub-species of the Iceland Gull. I’m not a bird person, but I understand there’s some controversy. Anyway, it’s named after Ludwig Kumlien.
Yvonne Madelaine Brill was born #OTD in 1924. She was a rocket scientist who invented the hydrazine resistojet, which increased the payload capacity of satellites by reducing the weight of propellant they require. JWST (@NASAWebb) uses hydrazine thrusters!
Photo: W. McNamee/Getty
Here is the JWST propulsion page describing its SCAT and MRE-1 thrusters which use hydrazine as a fuel and propellant, respectively. jwst-docs.stsci.edu/jwst-observato…
Yvonne Madelaine Brill studied Chemistry and Math at the University of Manitoba. She wanted to study engineering, but women weren't allowed at the time.
Mathematical physicist Cécile DeWitt-Morette, who made foundational contributions to the study of Feynman functional integrals, organized the first American conference on general relativity, and founded the Les Houches Summer School, was born #OTD in 1922.
Images: UT-Austin
Cécile Morette grew up in Normandy, studying math and physics at the University of Caen. Her graduate work, on quantum mechanics, took place at the University of Paris. Much of her education took place during the German occupation of WWII.
While in Paris, she worked with Irène and Frédéric Joliot-Curie. After finishing her doctorate in 1947, she moved to Copenhagen to work with Neils Bohr. Her next stop was the Institute for Advanced Study, where she worked with Robert Oppenheimer.
Physicist David Bohm, who developed a non-local formulation of quantum mechanics that he hoped would evade some of the conceptually thorny aspects of the Copenhagen Interpretation, and would later inspire the work of John Bell, was born #OTD in 1917.
Bohm’s quantum mechanics textbook was published in 1951. It was very successful, and is still available from Dover as an inexpensive reprint. Here’s my copy: