ARlogo Annu. Rev. Astron. Astrophys. 1999. 37: 445-486
Copyright © 1999 by Annual Reviews. All rights reserved

Reprinted with kind permission from Annual Reviews, 4139 El Camino Way, Palo Alto, California, USA

For a PDF version of the article, click here.


THE FIRST 50 YEARS AT PALOMAR: 1949-1999 The Early Years of Stellar Evolution, Cosmology, and High-Energy Astrophysics

Allan Sandage


The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101

PROLOGUE

In 1999 we celebrate the 50th anniversary of the initial bringing into operation of the Palomar 200-inch Hale telescope. When this telescope was dedicated, it opened up a much larger and clearer window on the universe than any telescope that had gone before.

Because the Hale telescope has played such an important role in twentieth century astrophysics, we decided to invite one or two of the astronomers most familiar with what has been achieved at Palomar to give a scientific commentary on the work that has been done there in the first fifty years.

The first article of this kind which follows is by Allan Sandage, who has been an active member of the staff of what was originally the Mount Wilson and Palomar Observatories, and later the Carnegie Observatories for the whole of these fifty years.

The article is devoted to the topics which covered the original goals for the Palomar telescope, namely observational cosmology and the study of galaxies, together with discoveries that were not anticipated, but were first made at Palomar and which played a leading role in the development of high energy astrophysics.

The Palomar work first showed how optical astronomy would be the key to our understanding of observations made in other parts of the electromagnetic spectrum, particularly at radio wavelengths and at X-ray energies.

--Geoffrey Burbidge, Editor

Abstract. An account is given of the history of two observational programs set for the Palomar 200-inch telescope, one by Walter Baade and the other by Edwin Hubble near the start of the scheduled operation of the telescope 50 years ago. The review is partly an assessment of whether, and how well, these programs have been carried to completion, and partly an account of the response of Palomar to new discoveries and developments not foreseen in 1950. Stellar evolution, the discovery of variations in the metallicity of stars of different populations, the chemical evolution of the Galaxy, the Cepheid P-L relation, the redshift-distance relation of the expanding universe, and the extragalactic distance scale are discussed as they relate to the predictions for progress on the programs set out by Baade and Hubble. Not foreseen was the invention and development of radio astronomy and high energy astrophysics, leading to the discovery of radio galaxies, quasars, and the gradual realization of violent events, both in stars and in galaxies. The review is highly restricted to these subjects, covering only three areas among the totality of the work in observational astrophysics studied during the first 50 years at Palomar.


Key words: stellar evolution, observational cosmology, radio astronomy, high energy astrophysics


Table of Contents

THE BEGINNING

THE EARLY YEARS
The First Palomar Discoveries
Baade's Program Proposed

STELLAR EVOLUTION
Stars Move Off the Main Sequence Rather Than Up or Down
The Chemical Composition Connection

CALIBRATION OF THE CEPHEID P-L RELATION

COSMOLOGY
Large-Scale Distribution
The Velocity-Distance Relation

THE EXTRAGALACTIC DISTANCE SCALE
The First Step from the Local Group to NGC 2403
The Steps Series from NGC 2403 to the Global Expansion Field

EARLY DEVELOPMENTS IN HIGH ENERGY ASTROPHYSICS
Initial Identification of Radio Sources
The Discovery of Quasars and the AGN Phenomena
M82 and NGC 1275 as Prototypes of Starburst Galaxies and Other Violent Events

CONCLUSIONS

REFERENCES

Next