From Astronomy Magazine: Women in STEM- “Meet Henrietta Leavitt, the woman who gave us a universal ruler”

Astronomy magazine

From Astronomy Magazine

February 4, 2019
Korey Haynes

Henrietta Swan Leavitt (1868 – 1921) No image credit

Cepheid variable stars act as signposts to help astronomers build a 3D picture of the sky. Here’s the story of the woman who unlocked these stars’ secrets.

Henrietta Swan Leavitt’s work revealed the true size of the universe. A. Fujii NASA/ESA Hubble

Gazing up at the sky, it’s hard not to imagine the Sun, Moon, stars, and planets as part of an inverted bowl over our heads, even if we know that’s an antiquated way of viewing the heavens. These days, we understand it’s Earth that’s spinning daily like a ballerina, while also circling the Sun on its yearly journey. But the bowl imagery was and remains a reasonable way of envisioning how the skies appear to revolve around us, and why certain stars appear or disappear with the changing hour or season.

But to understand the universe as it really is, we need a three-dimensional picture of the skies. The Copernican revolution started this change in perspective, but it took until the 20th century for a true understanding of the universe’s scale and layout to evolve. The researcher who provided one of the biggest keys was a deaf woman who earned 30 cents an hour.

Changing Stars Unlock a Map

Leavitt’s work on variable stars allowed Edwin Hubble to deduce the distance to the Andromeda galaxy.

Using the Hooker Telescope at Mt. Wilson, Hubble identified Cepheid variables (a kind of star that is used as a means to determine the distance from the galaxy in several spiral nebulae, including the Andromeda Nebula and Triangulum).

Andromeda Nebula Clean by Rah2005 on DeviantArt

The Triangulum Galaxy via The VLT Survey Telescope (VST) at ESO’s Paranal Observatory in Chile. This beautifully detailed image of the galaxy Messier 33. This nearby spiral, the second closest large galaxy to our own galaxy, the Milky Way, is packed with bright star clusters, and clouds of gas and dust. This picture is amongst the most detailed wide-field views of this object ever taken and shows the many glowing red gas clouds in the spiral arms with particular clarity.

His observations, made in 1924, proved conclusively that these nebulae were much too distant to be part of the Milky Way and were, in fact, entire galaxies outside our own, suspected by researchers at least as early as 1755 when Immanuel Kant’s General History of Nature and Theory of the Heavens appeared.

Edwin Hubble at Caltech Palomar Samuel Oschin 48 inch Telescope, (credit: Emilio Segre Visual Archives/AIP/SPL)

Edwin Hubble looking through a 100-inch Hooker telescope at Mount Wilson in Southern California

Mt Wilson 100 inch Hooker Telescope Interior

Mt Wilson 100 inch Hooker Telescope, perched atop the San Gabriel Mountains outside Los Angeles, CA, USA, Mount Wilson, California, US, Altitude 1,742 m (5,715 ft)

Henrietta Swan Leavitt was one of many women “computers” who worked at Harvard University, cataloging stars around the turn of the last century. Women could be paid less than men, and were generally seen as detail-oriented and suited for the often boring and rote work of data analysis. They were also barred from operating Harvard’s telescopes, limiting their other astronomical options. Leavitt’s particular assignment was Cepheid variable stars. These stars change how bright they are from day to day or week to week. And she noticed that, in general, the brighter stars had longer periods – the brighter the star, the longer it took to cycle through its variability.

At first, this was nothing more than a curiosity. It didn’t mean anything to anyone. But Leavitt made it very meaningful with her follow-up work. She looked at a sample of variable stars that were all near the same location, in the Small Magellanic Cloud.

Small Magellanic Cloud. NASA/ESA Hubble and ESO/Digitized Sky Survey 2

This is a tiny dwarf galaxy very near to our own Milky Way. Here, with a smaller sample, her trend was even clearer. Brighter stars had longer periods.

Leavitt realized something very important here, though it’s not clear many others did at the time. Because the stars in her second study were all in the same place, they were all essentially the same distance from Earth. So her discovery was telling her something intrinsic to the stars themselves: the longer a star took to change brightness, the brighter it actually was. So, if another star took a long time to change brightness but didn’t appear brighter, then she concluded it must be farther away, thus dimming its true brightness. With this simple relationship, Leavitt turned a two-dimensional picture of the sky into a 3D one.

Finishing the Scale

Leavitt herself pointed out that someone merely needed to work out the parallax (a way of calculating distance that works only on very nearby stars) of a tiny handful of her variable stars to calibrate the system, and turn her rough picture of “near or far” into an accurate map complete with marked distances. Within a year, another astronomer named Ejnar Hertzsprung had done so.

Perhaps Leavitt was a few years too early for her brilliant observation. Perhaps it was overlooked because she was a woman, and not allowed the status of a full researcher (though her name is on her own published work). Whatever the cause, this observation sat quietly for over a decade, until after Leavitt had suffered an early death due to cancer. It was only then that Edwin Hubble used her work to show how large the universe was, and that many of the fuzzy “nebulae” astronomers had observed for so long were actually far more distant than the stars in the Milky Way, and were in fact entire galaxies themselves.

Leavitt never earned fame in her own lifetime, nor a fancy telescope namesake afterward. But when looking up at the night skies, it’s worth remembering that she is part of the reason we have a three-dimensional map of the skies, instead of the flat picture that sustained humans for so much of our history.

See the full article here .


Please help promote STEM in your local schools.

Stem Education Coalition