Universe
Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 6, Problem 41Q

(a)

To determine

The wavelength (in meters) of the emission, if the mission of the Submillimeter Wave Astronomy satellite (SWAS), launched in 1998, was to investigate clouds within which stars form and 557 GHz is one of the frequencies at which these clouds are observed (1 GHz = 1 gigahertz = 109 Hz).

(b)

To determine

The necessity for using satellite for the mission of the Submillimeter Wave Astronomy satellite (SWAS) to investigate clouds within which stars form and 557 GHz is one of the frequencies at which these clouds are observed (1 GHz = 1 gigahertz = 109 Hz).

(c)

To determine

The diameter of the primary mirror, if SWAS had an angular resolution of 4 arcmin. The mission of the Submillimeter Wave Astronomy satellite (SWAS), was to investigate clouds within which stars forms and 557 GHz is one of the frequencies at which these clouds are observed (1 GHz = 1 gigahertz = 109 Hz).

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