Recollections of "Tucson Operations"


Book Description

A personal account of the evolution of millimeter-wave astronomy at the US National Radio Astronomy Observatory. The author recounts the behind-the-scenes activities of the staff from the beginnings at Kitt Peak to the closing of the Tuscon offices.




Federal Register


Book Description




Secrets of the Hoary Deep


Book Description

A Noble Prize–winning Italian astrophysicist shares his scientific autobiography and the history of the development of contemporary astronomy. The discovery of x-rays continues to have a profound effect on the field of astronomy. It has opened the cosmos to exploration in ways previously unimaginable, and fundamentally altered the methods for pursuing information about outer space. Nobel Prize–winner Riccardo Giacconi’s highly personal account of the birth and evolution of x-ray astronomy reveals the science, people, and institutional settings behind this important and influential discipline. Part history, part memoir, and part cutting-edge science, Secrets of the Hoary Deep is the tale of x-ray astronomy from its infancy through what can only be called its early adulthood. It also details how the tools, techniques, and practices designed to support and develop x-ray astronomy were transferred to optical, infrared, and radio astronomy, drastically altering the face of modern space exploration. Giacconi relates the basic techniques developed at American Science and Engineering and explains how, where, and by whom the science was advanced. From the first Earth-orbiting x-ray satellite, Uhuru, to the opening of the Space Telescope Science Institute and the lift-off of the Hubble Space Telescope to the construction of the Very Large Telescope, Giaconni recounts the ways in which the management methods and scientific methodology behind successful astronomy projects came to set the standards of operations for all subsequent space- and Earth-based observatories. Along the way he spares no criticism and holds back no praise, detailing individual as well as institutional failures and successes, reflecting upon how far astronomy has come and how far it has yet to go.




Submillimetre Astronomy


Book Description

G. M. Bernstein, M. L. Fischer, and P. L. Richards Department of Physics, University of California Berkeley, California 94720, U. S. A. J. B. Peterson Department of Physics, Princeton University Princeton, New Jersey 08540, U. S. A. T. Timusk Department of Physics, McMaster University Hamilton, Ontario L8S 4M1 , Canada ABSTRACT. Recent measurements of the diffuse background at millimeter wavelengths indicate no departure from a Planck spectrum near the peak of the blackbody curve. Anisotropy measurements indicate no structure, at the 2% level, in the recently detected submillimeter excess. We report here the results of an April 1987 balloon flight of an instrument designed to measure the spectrum of the cosmic background radiation from 1 mm to 3 mm. A description of the instrument can be found in Peterson, Richards, and Timusk (1985). Modifications were made to the apparatus and experimental procedure in order to identify and reduce systematic errors. Results from the latest flight indicate that two effects hamper the interpretation of the data. These systematic effects will be described in detail in a forthcoming publications; they are probably responsible for the non-Planckian spectrum measured by Woody and Richards (1981). Attempts to remove the systematic effects from our data yield the upper limits to the CBR brightness temperature in 4 bands from 1 mm to 3 mm. There is no evidence for an excess of radiation near the 2. 8 K blackbody peak.







Observing At A Distance - Proceedings Of A Workshop On Remote Observing


Book Description

Remote Observing is a new, important, and growing aspect of astronomy. Recent developments in global network communications have made remote observing a viable, and sometimes preferable, alternative to travel to a possibly remote and inhospitable telescope site.This workshop is the first in the world devoted to the topic. The contributors represent many of the world's major telescopes, radio, optical and infrared. The proceedings should become a standard reference for many years on the state of the art in remote control of and data acquisition from astronomical telescopes.




Stardust


Book Description

How did life originate on Earth? For over 50 years, scientists believed that life was the result of a chemical reaction involving simple molecules such as methane and ammonia cooking in a primordial soup. Recent space observations have revealed that old stars are capable of making very complex organic compounds. At some point in their evolution, stars eject those organics and spread them all over the Milky Way galaxy. There is evidence that these organic dust particles actually reached the early Solar System. Through bombardments by comets and asteroids, the young Earth inherited significant amounts of stardust. Was the development of life assisted by the arrival of these extraterrestrial materials? In this book, the author describes stunning discoveries in astronomy and solar system science made over the last 10 years that have yielded a new perspective on the origin of life. Other interesting topics discussed in this book The discovery of diamonds and other gemstones in space The origin of oil Neon signs and fluorescent lights in space Smoke from the stars Stardust in our hands Where oceans come from The possibility of bacteria in space