IB Physics SL E.1 Structure of the Atom Question Bank
Practise IB Physics SL E.1 by modelling nuclei, isotopes, spectra, binding energy and the evidence for atomic structure.
- Syllabus
- First assessment 2025
- Course
- Physics SL
- Level
- SL
Practise IB Physics SL E.1 by modelling nuclei, isotopes, spectra, binding energy and the evidence for atomic structure.
This question is in two parts. Part 1 is about the nuclear model of the atom and radioactive decay. Part 2 is about waves.
Part 1 Nuclear model of the atom and radioactive decay
Outline how the evidence supplied by the Geiger-Marsden experiment supports the nuclear model of the atom.
most undeflected/pass straight through; hence mostly empty space; few deflected; hence small dense nucleus; positive / positively charged;
Tritium may be produced by bombarding a nucleus of the isotope lithium-7 with a high-energy neutron. The reaction equation for this interaction is
Identify the proton number Z of X.
2;
This question is about atomic energy levels.
Outline a laboratory procedure for producing and observing the atomic absorption spectrum of a gas.
shine white light through;
a tube of the gas; then observe with spectroscope/grating/prism;
Describe the appearance of an atomic absorption spectrum.
continuous spectrum crossed by dark lines;
Explain why the spectrum in (a) provides evidence for quantization of energy in atoms.
dark lines formed by the absorption of photons; the absorbed photons have specific/discreet wavelengths; indicating discreet differences in energy; which can only be explained by existence of energy levels;
The principal energy levels of the hydrogen atom in electronvolt ( eV ) are given by
where n is a positive integer.
Determine the wavelength of the absorption line that corresponds to an electron transition from the energy level given by n=1 to the level given by n=3.
E=13.6[121−321]=12.1eV;
12.1eV=12.1×1.6×10−19 J=λhc;
λ=102 nm or 103 nm ;
Marking guidance:
Award [3] for a bald correct answer.