Article ID: CBB752540761

Francis G. Pease and the first galactic rotation curves (1916-1922) (2018)

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With the 60-inch reflector at Mount Wilson Observatory, Francis G. Pease obtained the first measurements of the rotation curves of two nearly edge-on spiral galaxies, NGC 4594 (the Sombrero Galaxy) and NGC 224 (the Andromeda Galaxy) in 1916 and 1918, respectively. Pease aligned the spectrograph's slit with the major axes of the galaxies' foreshortened elliptical figures and obtained direct measurements of the Doppler-induced radial velocity components along their axes. This technique originally had been applied in 1895 by James E. Keeler to a rotational analysis of the rings of Saturn. By subtracting out the radial velocities of their centers, Pease obtained their rotational velocities as a function of distance away from the centers. This enabled him to determine that linear relationships existed in both cases, whereby these objects appeared to show evidence of solid-body rotations out to (and beyond) the limits that could be observed spectroscopically (about 2.5 arcminutes from their centers). These relationships contradicted the behaviors of planets that orbited our Sun, and indicated that the objects' mass distributions likewise increased in direct proportion away from the centers. Pease's dynamical results were applied in two independent cases (by Ernst J. Öpik and Knut Lundmark) to a greater understanding of the distance and nature of the 'spiral nebulae' in the aftermath of the 'Great Debate'. Yet, the remaining questions posed by Pease's data were not effectively answered for two decades (or more) until Horace W. Babcock extended spectroscopic investigations into the disk region of the Andromeda Galaxy and showed that those stellar velocities were largely independent of their distances from the center. Along with many other examples, this finding was later confirmed by Vera Rubin and her colleagues and has become one of the leading forms of evidence for the existence of dark matter in galaxies.

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Authors & Contributors
Smith, Robert William
Osterbrock, Donald E.
Simpson, Emily
Crandall, Heather Stephanie
Stacy S. McGaugh
Philip Yock
Journals
Journal for the History of Astronomy
Journal of Astronomical History and Heritage
Studies in History and Philosophy of Science
Notes and Records: The Royal Society Journal of the History of Science
Leonardo
Journal of Dialectics of Nature
Publishers
Universal Publishers
University of Maryland, Baltimore County
Cambridge University Press
Concepts
Astrophysics
Astronomy
Galaxies; nebulae
Cosmology
Celestial mechanics
Dark matter
People
Hale, George Ellery
Zwicky, Fritz
Robinson, Thomas Romney
Hubble, Edwin Powell
Zanstra, Herman
Sitter, Willem de
Time Periods
20th century, early
20th century
19th century
21st century
20th century, late
Medieval
Places
United States
Bukhara (Uzbekistan)
Pasadena (California)
Spain
New Zealand
Japan
Institutions
Mount Wilson Observatory
Palomar Observatory
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