Find the wavelength of the radiation emitted when an electron in a hydrogen atom falls from the third orbit to the second. Take the Rydberg constant as 1.097 × 107 m−1.
Atoms and Nuclei
Original Khojo Papers practice question — not from a past board paper.
−3.4 eV
No citable source has been recorded for this record. Treat it as practice material, not as fact.
En = −13.6/n2 eV, so for n = 2 the energy is −13.6/4 = −3.4 eV.
From the same topic and chapter, at a similar level.
Find the wavelength of the radiation emitted when an electron in a hydrogen atom falls from the third orbit to the second. Take the Rydberg constant as 1.097 × 107 m−1.
Atoms and Nuclei
The half-life of a radioactive nuclide is 4 days. What fraction of a sample remains after 16 days, and what is its decay constant?
Atoms and Nuclei
State the postulates of Bohr's model of the atom.
Atoms and Nuclei
Define mass defect and binding energy, and explain why the binding energy per nucleon curve peaks near iron.
Atoms and Nuclei
State two limitations of Bohr's model of the atom.
Atoms and Nuclei
State Kirchhoff's two laws and say what conservation principle each expresses.
Current Electricity