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Books > Science & Mathematics > Astronomy, space & time > Cosmology & the universe

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The Milky Way Galaxy and Statistical Cosmology, 1890-1924 (Hardcover) Loot Price: R3,082
Discovery Miles 30 820
You Save: R375 (11%)
The Milky Way Galaxy and Statistical Cosmology, 1890-1924 (Hardcover): Erich Robert Paul

The Milky Way Galaxy and Statistical Cosmology, 1890-1924 (Hardcover)

Erich Robert Paul

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Was R3,457 Loot Price R3,082 Discovery Miles 30 820 | Repayment Terms: R289 pm x 12* You Save R375 (11%)

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Between the years 1890 and 1924, the dominant view of the universe suggested a cosmology largely foreign to contemporary ideas. First, astronomers believed they had confirmed that the sun was roughly in the centre of the Milky Way galaxy. Second, considerable evidence indicated that the size of the galaxy was only about one-third the value now accepted by today's astronomers. Third, it was thought that interstellar space was completely transparent, that there was no absorbing material between the stars. Fourth, astronomers believed that the universe was composed of numerous star systems comparable to the Milky Way galaxy. The method that provided this picture and came to dominate cosmology was 'statistical' in nature, because it was based on the counts of stars and their positions, motions, brightnesses and stellar spectra. Professor Paul describes the rise of this statistical cosmology in light of developments in nineteenth-century astronomy and explains how this cosmology set the stage for many of the most significant developments of twentieth-century astronomy.

General

Imprint: Cambridge UniversityPress
Country of origin: United Kingdom
Release date: November 1993
First published: 1993
Authors: Erich Robert Paul
Dimensions: 229 x 152 x 19mm (L x W x T)
Format: Hardcover
Pages: 280
ISBN-13: 978-0-521-35363-2
Categories: Books > Science & Mathematics > Science: general issues > History of science
Books > Science & Mathematics > Astronomy, space & time > Cosmology & the universe
LSN: 0-521-35363-7
Barcode: 9780521353632

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