front cover of Big and Bright
Big and Bright
A History of the McDonald Observatory
By David S. Evans and J. Derral Mulholland
University of Texas Press, 1986

By day, every year over 40,000 visitors pour in. Across the Rio Grande, a hundred miles away, Mexican mountaineers use the white domes as landmarks. By night, perched almost 7,000 feet above the sleeping, earthbound world, astronomers probe the secrets of the night sky. This is the University of Texas McDonald Observatory, one of the world's largest university-operated astronomical installations.

Big and Bright: A History of the McDonald Observatory is the story of a remarkable collaboration between two major universities, one a prestigious private school, the other a growing southwestern state institution. The University of Chicago had astronomers, but its Yerkes Observatory was aging and underfunded; the University of Texas had money for an observatory but no working astronomer to staff it. Out of their mutual need, they formed a thirty-year compact for a joint venture. Unusual in its day, the Yerkes-McDonald connection presaged the future. In this arrangement, one can see some of the beginnings of today's consortium "big science."

Now the McDonald Observatory's early history can be put in proper perspective. Blessed with a gifted and driving founding director, the world's (then) second-largest telescope, and an isolation that permitted it to be virtually the only major astronomical observatory that continued operations throughout World War II, the staff of McDonald Observatory helped lay the foundations of modern astrophysics during the 1940s. For over a decade after the war, a lonely mountaintop in West Texas was the mecca that drew nearly all the most important astronomers from all over the world.

Based on personal reminiscences and archival material, as well as published historical sources, Big and Bright is one of the few histories of a major observatory, unique in its focus on the human side of the story.

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The Last of the Great Observatories
Spitzer and the Era of Faster, Better, Cheaper at NASA
George H. Rieke
University of Arizona Press, 2006
The Spitzer Space Observatory, originally known as the Space Infrared Telescope Facility (SIRTF), is the last of the four “Great Observatories”, which also include the Hubble Space Telescope, the Chandra X-ray Observatory, and the Compton Gamma Ray Observatory. Developed over twenty years and dubbed the “Infrared Hubble", Spitzer was launched in the summer of 2003 and has since contributed significantly to our understanding of the universe.

George Rieke played a key role in Spitzer and now relates the story of how that observatory was built and launched into space. Telling the story of this single mission within the context of NASA space science over two turbulent decades, he describes how, after a tortuous political trail to approval, Spitzer was started at the peak of NASA’s experiment with streamlining and downsizing its mission development process, termed “faster better cheaper.” Up to its official start and even afterward, Spitzer was significant not merely in terms of its scientific value but because it stood at the center of major changes in space science policy and politics. Through interviews with many of the project participants, Rieke reconstructs the political and managerial process by which space missions are conceived, approved, and developed. He reveals that by the time Spitzer had been completed, a number of mission failures had undermined faith in “faster-better-cheaper” and a more conservative approach was imposed. Rieke examines in detail the premises behind “faster better cheaper,” their strengths and weaknesses, and their ultimate impact within the context of NASA’s continuing search for the best way to build future missions.

Rieke’s participant’s perspective takes readers inside Congress and NASA to trace the progress of missions prior to the excitement of the launch, revealing the enormously complex and often disheartening political process that needs to be negotiated. He also shares some of the new observations and discoveries made by Spitzer in just its first year of operation. As the only book devoted to the Spitzer mission, The Last of the Great Observatories is a story at the nexus of politics and science, shedding new light on both spheres as it contemplates the future of mankind’s exploration of the universe.
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Observatories of the Southwest
A Guide for Curious Skywatchers
Douglas Isbell and Stephen E. Strom
University of Arizona Press, 2009
With its clear skies and low humidity, the southwestern United States is an astronomer’s paradise where observatories like Kitt Peak have redefined the art of skywatching. The region is unique in its loose federation of like-minded research outposts and in the quantity and diversity of its observatories—places captured in this unique guidebook.

Douglas Isbell and Stephen Strom, both intimately involved in southwestern astronomy, have written a practical guide to the major observatories of the region for those eager to learn what modern telescopes are doing, to understand the role each of these often quirky places has played in advancing our understanding of the cosmos, and hopefully to visit and see the tools of the astronomer up close. For each observatory, the authors describe its history, highlights of its contributions to astronomy—with an emphasis on recent results—and information for visitors. Also included are wide-ranging interviews with astronomers closely associated with each site.

Observatories covered range from McDonald in Texas to Palomar in California, with significant outposts in between: Arizona’s Kitt Peak National Observatory southwest of Tucson, the Lowell Observatory in Flagstaff, and the Whipple Observatory outside Amado; and New Mexico’s Very Large Array near Socorro and Sacramento Peak close to Sunspot. In addition to describing these established institutions, they also take a look ahead to the most powerful ground-based telescope in the world just beginning to operate at full power on Mount Graham in Safford, Arizona.

With more than three dozen illustrations, Observatories of the Southwest is accessible to amateur astronomers, tourists, students, and teachers—anyone fascinated with the contributions that astronomy has made to deepening our understanding of humanity’s place in the universe, whether exploring the solar system from Lowell Observatory or studying the birth of stars using the army of giant radio telescopes at the Very Large Array. This book aims to inspire visits to these sites by illuminating the major scientific questions being pursued every clear night beneath the dark skies of the Southwest and the amazing machinery that makes these pursuits possible.
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The Sun in the Church
Cathedrals as Solar Observatories
J. L. Heilbron
Harvard University Press, 1999

Between 1650 and 1750, four Catholic churches were the best solar observatories in the world. Built to fix an unquestionable date for Easter, they also housed instruments that threw light on the disputed geometry of the solar system, and so, within sight of the altar, subverted Church doctrine about the order of the universe.

A tale of politically canny astronomers and cardinals with a taste for mathematics, The Sun in the Church tells how these observatories came to be, how they worked, and what they accomplished. It describes Galileo's political overreaching, his subsequent trial for heresy, and his slow and steady rehabilitation in the eyes of the Catholic Church. And it offers an enlightening perspective on astronomy, Church history, and religious architecture, as well as an analysis of measurements testing the limits of attainable accuracy, undertaken with rudimentary means and extraordinary zeal. Above all, the book illuminates the niches protected and financed by the Catholic Church in which science and mathematics thrived.

Superbly written, The Sun in the Church provides a magnificent corrective to long-standing oversimplified accounts of the hostility between science and religion.

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