Blogarchiv
Astronomie - How Vera Rubin broke barriers and convinced the astronomy community that dark matter exists

30.10.2023

vera-rubin

Lines of enquiry Vera Rubin measuring spectra at the Department of Terrestrial Magnetism at the Carnegie Institution in Washington, in about 1970. (Courtesy: AIP Emilio Segrè Visual Archives, Rubin Collection)

In the early 2000s, I sat down at a desk in Durham University library and, behind a tower of ageing books, I began researching my undergraduate dissertation. My topic was the discovery that the matter in the Milky Way galaxy, and indeed the universe, is mostly composed of a mysterious and invisible substance called “dark matter”. I chose the subject out of curiosity. Who had figured dark matter out? How could we have missed it? Well, the answer to the former is Vera Rubin, and the answer to the latter is that, in her words, the universe had been “unkind” and “played a trick” on us all.

But perhaps Rubin was the subject of another trick too. “A flip of a switch, and astronomer Vera Rubin disappeared.” This is the first line of the biography Bright Galaxies, Dark Matter, and Beyond: the Life of Astronomer Vera Rubin by Ashley Jean Yeager, associate news editor at Science News. The line directly refers to Rubin beginning a cold night of observations, but it also hints that the book will not shy away from Rubin’s struggle to gain visibility in the astronomical community. This is Yeager’s first book, and it benefits from her background in journalism and science writing, leaving no stone unturned as it rigorously illuminates Rubin and her discoveries.

As Yeager shows, Rubin – who died in 2016 at the age of 86 – was not a scientist who was content for her career path to be steered by more powerful figures, even her own supervisors. She declared she had no interest in the PhD project she was assigned, which was identifying the Sun’s spectral lines. Instead, Rubin wandered around for something else, searching out the infamous George Gamow and settling on exploring faraway galaxies. The subject of galaxies was one she would stick with long-term, eventually focusing on the motion of stars within them.

The stars in a galaxy orbit its centre of mass, which is usually a supermassive black hole, and Rubin could measure the speed at which those stars were orbiting using the spectrum of light they were emitting. The laws of gravity are clear on how the speeds should change: they should travel more slowly with increasing distance from the galactic centre, as the mass of luminous matter decreases. No-one was interested in proving something so obvious. Why would anyone question it?

Well, Rubin did, and for two reasons. First, she did not accept assumptions readily, and second, because it was a nice, quiet research topic. She liked to work at her own pace because she “would rather drop dead than have another astronomer find I made a mistake”. Rubin measured these stellar speeds with no small contribution from Kent Ford, who built the required technology and observed alongside her for years. What they found came as a shock: the plots of observable speeds versus distance (rotation curves) were flat, implying there was a lot of invisible mass at outer radii, changing the field of astronomy forever.

355 Views
Raumfahrt+Astronomie-Blog von CENAP 0