In 1896 Pickering found lines from the star Zeta Pup- pis that had not been observed on Earth. Bohr showed in 1913 that the lines were due to He. Show that an equation giving these wavelengths is 1 1 = ² ( ²1 - 22 ) R λ n What value should the Rydberg constant R have in this case?
In 1896 Pickering found lines from the star Zeta Pup- pis that had not been observed on Earth. Bohr showed in 1913 that the lines were due to He. Show that an equation giving these wavelengths is 1 1 = ² ( ²1 - 22 ) R λ n What value should the Rydberg constant R have in this case?
College Physics
1st Edition
ISBN:9781938168000
Author:Paul Peter Urone, Roger Hinrichs
Publisher:Paul Peter Urone, Roger Hinrichs
Chapter30: Atomic Physics
Section: Chapter Questions
Problem 14CQ: CT scanners do not detect details smaller than about 0.5 Is this limitation clue to the wavelength...
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Question
![In 1896 Pickering found lines from the star Zeta Pup-
pis that had not been observed on Earth. Bohr
showed in 1913 that the lines were due to He+. Show
that an equation giving these wavelengths is
1-(2)
R(
n²/²
=
λ
What value should the Rydberg constant R have in
this case?
n](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F093e7116-3e01-49ad-9157-7a22a5caeb16%2Fc2533d73-2f32-4e87-a58b-b6b45e9d2db6%2Ft8phbr_processed.png&w=3840&q=75)
Transcribed Image Text:In 1896 Pickering found lines from the star Zeta Pup-
pis that had not been observed on Earth. Bohr
showed in 1913 that the lines were due to He+. Show
that an equation giving these wavelengths is
1-(2)
R(
n²/²
=
λ
What value should the Rydberg constant R have in
this case?
n
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