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Download Burnham's Celestial Handbook: An Observer's Guide to the by Robert Burnham Jr. PDF

By Robert Burnham Jr.

Quantity III of this three-part complete consultant to the hundreds of thousands of celestial items outdoors our sun procedure concludes with listings from Pavo through Vulpecula. Objects are grouped in keeping with constellation, and their definitions function names, coordinates, classifications, and actual descriptions. extra notes provide interesting old details. hundreds and hundreds of visible aids. 1977 version.

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Extra resources for Burnham's Celestial Handbook: An Observer's Guide to the Universe Beyond the Solar System, Vol. 3

Sample text

After a number of failed attempts 36 , on 10 October 1946, the rocket reached an altitude of 173 kilometres. By recovering the capsule, from the nosecone of the rocket it was possible to observe the first UV spectrum of the Sun in the range between 210–300 nm (Tousey et al. 1947) . 14). Alltogether, NRL spectrographs were flown on ten V–2 rockets during 1946–1948, of which four flights were successful. De Vorkin (1992) describes scientific research with V–2 rockets. In a letter to Leo Goldberg, Henry Norris Russell (1877–1955) expressed his excitement after seeing the photographs: these rocket spectra are certainly fascinating.

Aldrich, launched these balloons which reached heights of up to 25 km from the Californian coast during several campaigns in 1913 and 1914.

After a number of failed attempts 36 , on 10 October 1946, the rocket reached an altitude of 173 kilometres. By recovering the capsule, from the nosecone of the rocket it was possible to observe the first UV spectrum of the Sun in the range between 210–300 nm (Tousey et al. 1947) . 14). Alltogether, NRL spectrographs were flown on ten V–2 rockets during 1946–1948, of which four flights were successful. De Vorkin (1992) describes scientific research with V–2 rockets. In a letter to Leo Goldberg, Henry Norris Russell (1877–1955) expressed his excitement after seeing the photographs: these rocket spectra are certainly fascinating.

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