The Glass Universe: How the Ladies of the Harvard Observatory Took the Measure of the Stars
#1 New York Times bestselling author Dava Sobel returns with the captivating, little-known true story of a group of women whose remarkable contributions to the burgeoning field of astronomy forever changed our understanding of the stars and our place in the universe
 
In the mid-nineteenth century, the Harvard College Observatory began employing women as calculators, or “human computers,” to interpret the observations made via telescope by their male counterparts each night. At the outset this group included the wives, sisters, and daughters of the resident astronomers, but by the 1880s the female corps included graduates of the new women's colleges—Vassar, Wellesley, and Smith. As photography transformed the practice of astronomy, the ladies turned to studying the stars captured nightly on glass photographic plates. The “glass universe” of half a million plates that Harvard amassed in this period—thanks in part to the early financial support of another woman, Mrs. Anna Draper, whose late husband pioneered the technique of stellar photography—enabled the women to make extraordinary discoveries that attracted worldwide acclaim. They helped discern what stars were made of, divided the stars into meaningful categories for further research, and found a way to measure distances across space by starlight. Their ranks included Williamina Fleming, a Scottish woman originally hired as a maid who went on to identify ten novae and more than three hundred variable stars, Annie Jump Cannon, who designed a stellar classification system that was adopted by astronomers the world over and is still in use, and Dr. Cecilia Helena Payne-Gaposchkin, who in 1956 became the first ever woman professor of astronomy at Harvard—and Harvard’s first female department chair. Elegantly written and enriched by excerpts from letters, diaries, and memoirs, The Glass Universe is the hidden history of a group of remarkable women who, through their hard work and groundbreaking discoveries, disproved the commonly held belief that the gentler sex had little to contribute to human knowledge.


From the Hardcover edition.
"1124022683"
The Glass Universe: How the Ladies of the Harvard Observatory Took the Measure of the Stars
#1 New York Times bestselling author Dava Sobel returns with the captivating, little-known true story of a group of women whose remarkable contributions to the burgeoning field of astronomy forever changed our understanding of the stars and our place in the universe
 
In the mid-nineteenth century, the Harvard College Observatory began employing women as calculators, or “human computers,” to interpret the observations made via telescope by their male counterparts each night. At the outset this group included the wives, sisters, and daughters of the resident astronomers, but by the 1880s the female corps included graduates of the new women's colleges—Vassar, Wellesley, and Smith. As photography transformed the practice of astronomy, the ladies turned to studying the stars captured nightly on glass photographic plates. The “glass universe” of half a million plates that Harvard amassed in this period—thanks in part to the early financial support of another woman, Mrs. Anna Draper, whose late husband pioneered the technique of stellar photography—enabled the women to make extraordinary discoveries that attracted worldwide acclaim. They helped discern what stars were made of, divided the stars into meaningful categories for further research, and found a way to measure distances across space by starlight. Their ranks included Williamina Fleming, a Scottish woman originally hired as a maid who went on to identify ten novae and more than three hundred variable stars, Annie Jump Cannon, who designed a stellar classification system that was adopted by astronomers the world over and is still in use, and Dr. Cecilia Helena Payne-Gaposchkin, who in 1956 became the first ever woman professor of astronomy at Harvard—and Harvard’s first female department chair. Elegantly written and enriched by excerpts from letters, diaries, and memoirs, The Glass Universe is the hidden history of a group of remarkable women who, through their hard work and groundbreaking discoveries, disproved the commonly held belief that the gentler sex had little to contribute to human knowledge.


From the Hardcover edition.
10.99 In Stock
The Glass Universe: How the Ladies of the Harvard Observatory Took the Measure of the Stars

The Glass Universe: How the Ladies of the Harvard Observatory Took the Measure of the Stars

by Dava Sobel
The Glass Universe: How the Ladies of the Harvard Observatory Took the Measure of the Stars

The Glass Universe: How the Ladies of the Harvard Observatory Took the Measure of the Stars

by Dava Sobel

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Overview

#1 New York Times bestselling author Dava Sobel returns with the captivating, little-known true story of a group of women whose remarkable contributions to the burgeoning field of astronomy forever changed our understanding of the stars and our place in the universe
 
In the mid-nineteenth century, the Harvard College Observatory began employing women as calculators, or “human computers,” to interpret the observations made via telescope by their male counterparts each night. At the outset this group included the wives, sisters, and daughters of the resident astronomers, but by the 1880s the female corps included graduates of the new women's colleges—Vassar, Wellesley, and Smith. As photography transformed the practice of astronomy, the ladies turned to studying the stars captured nightly on glass photographic plates. The “glass universe” of half a million plates that Harvard amassed in this period—thanks in part to the early financial support of another woman, Mrs. Anna Draper, whose late husband pioneered the technique of stellar photography—enabled the women to make extraordinary discoveries that attracted worldwide acclaim. They helped discern what stars were made of, divided the stars into meaningful categories for further research, and found a way to measure distances across space by starlight. Their ranks included Williamina Fleming, a Scottish woman originally hired as a maid who went on to identify ten novae and more than three hundred variable stars, Annie Jump Cannon, who designed a stellar classification system that was adopted by astronomers the world over and is still in use, and Dr. Cecilia Helena Payne-Gaposchkin, who in 1956 became the first ever woman professor of astronomy at Harvard—and Harvard’s first female department chair. Elegantly written and enriched by excerpts from letters, diaries, and memoirs, The Glass Universe is the hidden history of a group of remarkable women who, through their hard work and groundbreaking discoveries, disproved the commonly held belief that the gentler sex had little to contribute to human knowledge.


From the Hardcover edition.

Product Details

ISBN-13: 9780698148697
Publisher: Penguin Publishing Group
Publication date: 12/06/2016
Sold by: Penguin Group
Format: eBook
Pages: 336
Sales rank: 333,857
Lexile: 1330L (what's this?)
File size: 12 MB
Note: This product may take a few minutes to download.

About the Author

About The Author
DAVA SOBEL is the author of five books, including the New York Times bestsellers Longitude, Galileo’s Daughter, The Planets, and The Glass Universe. A former New York Times science reporter and longtime contributor to The New Yorker, AudubonDiscover, and Harvard Magazine, she is the recipient of the National Science Board’s Individual Public Service Award and the Boston Museum of Science’s Bradford Washburn Award, among others.

Read an Excerpt

Miss Cannon had classified one hundred thousand stars when she set the work aside to spend the summer of 1913 in Europe with her sister, Mrs. Marshall. They planned to attend three major astronomy meetings on the continent, plus all the banquets, garden parties, excursions, and entertainments that such international congresses entailed. On her previous trip to Europe, with her friend and Wellesley classmate Sarah Potter in 1892, Miss Cannon had made the grand tour of popular tourist destinations, camera in hand. This time she would go as a respected astronomer and the only female officer in her professional organization. At the 1912 meeting of the Astronomical and Astrophysical Society of America, the members had voted to change their name to the American Astronomical Society and to make her their treasurer. Now she would seek out her foreign colleagues, many of whom she knew only by reputation or correspondence, in their native settings.
 
“There are no women assistants,” Miss Cannon noted of the Royal Observatory, Greenwich. Travel broadened her appreciation for the singularity of Harvard’s large female staff, although she easily befriended men wherever she went. At Greenwich, “Without the slightest feeling of being out of place, without the smallest tinge of embarrassment, I discussed absorbing work with one and another.” That evening the astronomer royal, Frank Dyson, called for Miss Cannon and Mrs. Marshall at their London hotel and escorted them to a soiree at Burlington House, the headquarters of the Royal Astronomical Society and four other scientific fraternities. “Never has it been my good fortune to have such a kindly greeting, such hearty good will, such wonderful feeling of equality in the great world of research as among these great Englishmen.” At the society’s meeting a few days later, she gave a formal presentation about her recent investigation into the spectra of gaseous nebulae.
 
Mrs. Marshall understandably avoided the scientific sessions, at which Miss Cannon inured herself to being the sole woman in a roomful of as many as ninety men. In Germany, she reported, “Not a single German woman attended these Hamburg meetings” of the Astronomische Gesellschaft. “Once or twice, two or three would come in for a few minutes but I was generally the only woman to sit through a session. This was not so pleasant but at the recesses the men were so kind that nothing seemed to matter, and at the luncheon women appeared in great numbers.”
 
In Bonn, where the Solar Union gathered from July 30 to August 5, the astronomers were treated to a flyby visit of a military zeppelin, a side trip to the Gothic cathedral at Cologne, a riverboat ride up the Rhine, and a gala night in the Bonn observatory that prompted the English-speaking delegates to sing “They Are Jolly Good Fellows” to Director Friedrich Küstner and his wife and daughters. “Luncheon and indeed all meals in Germany,” observed Canadian astrophysicist John Stanley Plaskett, “are a much more important and solemn function than with us and take at least twice the time.”
 
Pickering, an elder statesman in this community, spoke at several banquets during the week. He shared impressions of his previous stays in Bonn, a city he had long regarded as the world capital of photometry. It was here that the legendary Friedrich Wilhelm Argelander assembled the Bonner Durchmusterung star catalogue and perfected the Argelander method of studying variables by comparing them to their steady neighbors. Argelander’s own small telescope, still mounted at the Bonn observatory, proved an object of veneration for the visiting astronomers.
 
Only about half the members of Pickering’s Committee on Spectral Classification, first convened at Mount Wilson, had come to the Bonn meeting. Those present included Henry Norris Russell, Karl Schwarzschild, Herbert Hall Turner, and of course Küstner, of the local observatory. They met Thursday afternoon, July 31, to polish their report before Friday’s discussion and vote. The group had considered incorporating some symbols into the Draper classification that would account for the widths of spectral lines, but ultimately rejected the idea. Rather than retrofit the Draper system, they preferred to look forward and explore the possibility of an entirely new design for stellar taxonomy.
 
On Friday morning Chairman Pickering read the committee’s recommendation to the full assembly at the Physical Institute. He proposed postponing “the permanent and universal adoption” of any system until the committee could formulate a suitable revision. In the interim, however, everyone should foster the well-known and widely praised Draper classification. Approval of the resolution was swift and unanimous. Ditto the subresolution regarding a refinement originally suggested by Ejnar Hertzsprung and already practiced by Miss Cannon. It consisted of a zero subscript for lone letters. Going forward, A0 would denote a star of purely A‑category attributes, showing no B tendencies whatever. The new A0 reduced plain A to a “rough” categorization.
 
At the final session on August 5, the Solar Union dissolved its old committees and regrouped into new ones for the work to be done over the next three years, before they would all meet again in Rome. “When the names of committees were read,” wrote Miss Cannon, “I was very much surprised to find that I was put on the Committee on Classification of Stellar Spectra—and one of the novel experiences of the summer was to meet with this Committee. They sat at a long table, these men of many nations, and I was the only woman. Since I have done almost all the world’s work in this one branch, it was necessary for me to do most of the talking.”

Table of Contents

Preface xi

Part 1 The Colors of Starlight

Chapter 1 Mrs. Draper's Intent 3

Chapter 2 What Miss Maury Saw 21

Chapter 3 Miss Bruce's Largesse 40

Chapter 4 Stella Nova 56

Chapter 5 Bailey's Pictures from Peru 71

Part 2 Oh, Be A Fine Girl, Kiss Me!

Chapter 6 Mrs. Fleming's Title 89

Chapter 7 Pickering's "Harem" 105

Chapter 8 Lingua Franca 123

Chapter 9 Miss Leavitt's Relationship 141

Chapter 10 The Pickering Fellows 159

Part 3 In the Depths Above

Chapter 11 Shapley's "Kilo-Girl" Hours 179

Chapter 12 Miss Payne's Thesis 196

Chapter 13 The Observatory Pinafore 215

Chapter 14 Miss Cannon's Prize 232

Chapter 15 The Lifetimes of Stars 249

Appreciation 267

Sources 269

Some Highlights in the History of the Harvard College Observatory 273

Glossary 281

A Catalogue of Harvard Astronomers, Assistants, and Associates 285

Remarks 293

Bibliography 299

Index 307

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