Bundle: Foundations Of Astronomy, Loose-leaf Version, 14th + Webassign, Printed Access Card, Single-term
Bundle: Foundations Of Astronomy, Loose-leaf Version, 14th + Webassign, Printed Access Card, Single-term
14th Edition
ISBN: 9780357292990
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Chapter 13, Problem 4P
To determine

Compare the brightness of Sirius B and full Moon.

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A star has a measured radial velocity of 100 km/s. If you measure the wavelength of a particular spectral line of Hydrogen as 486.42 nm, what was the laboratory wavelength (in nm) of the line? (Round your answer to at least one decimal place.) Which spectral line does this likely correspond to?   Balmer-alpha (656.3 nm) Balmer-beta (486.1 nm)     Balmer-gamma (434.0 nm) Balmer-delta (410.2 nm)
Rigel is a bright star in the night sky - its apparent magnitude is 0.12. Venus, when it isat it’s brightest, can have an apparent magnitude of -4.9. When this happens, what is theflux of Venus relative to the flux of Sirius? Use the fact that the absolute magnitude of Rigel is -7.8 to calculate its distance fromEarth.
A star has a measured radial velocity of 300 km/s. If you measure the wavelength of a particular spectral line of Hydrogen as 657.18 nm, what was the laboratory wavelength (in nm) of the line? (Round your answer to at least one decimal place.) nm Which spectral line does this likely correspond to? Balmer-alpha (656.3 nm) Balmer-beta (486.1 nm) Balmer-gamma (434.0 nm) Balmer-del ta (410.2 nm)
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