Question

In radio astronomy, hydrogen atoms are observed in which, for example, radiative transitions from n=109 to...

In radio astronomy, hydrogen atoms are observed in which, for example, radiative transitions from n=109 to n=108 occur. What are the frequency and wavelength of the radiation emitted in this transition?

Homework Answers

Answer #1

n = 109 to n = 108

using equation

En = 13.6 ( 1 - 1/n2 ) eV

E109 = 13.6 ( 1 - 1/1092 )

= 13.59885532 eV

En = 13.6 ( 1 - 1/n2 ) eV

E108 = 13.6 ( 1 - 1/1082 )

= 13.59883402 eV

dE = E109 - E108  

dE = 13.59885532 - 13.59883402

dE = 2.1296 X 10-5 eV

or

dE = 2.1296 X 10-5 X 1.6 X 10-19

dE = 3.40736 X 10-24 J

= hC/ dE

= 6.627 X 10-34 X 3 X 108 / 3.40736 X 10-24

= 0.05834 m

or

= 5.834 cm

f = C /

f = 3 X 108 / 0.05834

f = 5.142269455 X 109 Hz

f = 5.142269455 GHz

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