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1.Describe (in terms of the atomic theory) why the emission or absorption spectrum of an atom may be viewed as a “fingerprint” that can be used to identify the type of atom that is generating the spectrum.
2.What is the Balmer series? What is happening inside an atom of hydrogen atom that is emitting Balmer lines?
3.The normal wavelength (when source and observer are not moving relative to one another) of one of the emission lines of hydrogen (Hα) is 656.281 nm (i.e. 6.56281 x 10-7 m). Suppose that you observe the hydrogen emission spectrum from a distant nebula and find that the wavelength of its Hα line is 656.488 nm. Is this nebula coming towards you or moving away from you? At what speed?
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4.Hydrogen and helium are the most common elements in the Universe. Why isn’t the atmosphere of the Earth predominantly made up of these gases? What are the factors that determine whether a particular gas is retained in an atmosphere around a planet?
5.The average speed of a hydrogen atom at 300K is 2.74 km/s. The surface temperature of the Sun is 5,800K. What is the average speed of hydrogen atoms at the surface of the Sun? Given that the escape speed from the surface of the Sun is 618 km/s discuss whether the Sun will lose significant amounts of hydrogen into space over the next few billion years.
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