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.
The mass defect is the difference between the sum of the masses of the free nucleons and the actual mass of the nucleus; the binding energy is the energy equivalent of that difference. The curve rises for the lightest nuclei because adding nucleons increases the number of short-range attractions, and falls for the heaviest because the long-range electrostatic repulsion of the many protons grows faster; the balance is best near iron.
No citable source has been recorded for this record. Treat it as practice material, not as fact.
This is why fusion releases energy below the peak and fission above it.
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
Calculate the energy of an electron in the second orbit of a hydrogen atom.
Atoms and Nuclei
State the postulates of Bohr's model of the atom.
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