DP Physics Questionbank
D.4 – Stellar processes (HL only)
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Description
Nature of science:
Observation and deduction: Observations of stellar spectra showed the existence of different elements in stars. Deductions from nuclear fusion theory were able to explain this. (1.8)
Understandings:
- The Jeans criterion
- Nuclear fusion
- Nucleosynthesis off the main sequence
- Type Ia and II supernovae
Applications and skills:
- Applying the Jeans criterion to star formation
- Describing the different types of nuclear fusion reactions taking place off the main sequence
- Applying the mass–luminosity relation to compare lifetimes on the main sequence relative to that of our Sun
- Describing the formation of elements in stars that are heavier than iron including the required increases in temperature
- Qualitatively describe the s and r processes for neutron capture
- Distinguishing between type Ia and II supernovae
Guidance:
- Only an elementary application of the Jeans criterion is required, ie collapse of an interstellar cloud may begin if
- Students should be aware of the use of type Ia supernovae as standard candles
Aims:
- Aim 10: analysis of nucleosynthesis involves the work of chemists
Directly related questions
- 18M.3.HL.TZ2.18b: Explain how neutron capture can produce elements with an atomic number greater than iron.
- 18M.3.HL.TZ2.18a: Outline, with reference to the Jeans criterion, why a cold dense gas cloud is more likely to form...
- 18M.3.HL.TZ1.18b.ii: State one assumption made in your calculation.
- 18M.3.HL.TZ1.18b.i: Show that the distance to the supernova is approximately 3.1 × 1018 m.
- 18M.3.HL.TZ1.18a: Describe the formation of a type Ia supernova.
- 17N.3.HL.TZ0.20a: The Sun is a second generation star. Outline, with reference to the Jeans criterion (MJ), how the...
- 17M.3.HL.TZ1.16c: Massive stars that have left the main sequence have a layered structure with different chemical...
- 17M.3.HL.TZ1.16b: In the proton–proton cycle, four hydrogen nuclei fuse to produce one nucleus of helium releasing...
- 17M.3.HL.TZ1.16a: Outline, with reference to star formation, what is meant by the Jeans criterion.
- 16N.3.HL.TZ0.24c: Explain how the observation of type Ia supernovae led to the hypothesis that dark energy exists.
- 16N.3.HL.TZ0.24b: Hence, explain why a type Ia supernova is used as a standard candle.
- 16N.3.HL.TZ0.24a: Describe how some white dwarf stars become type Ia supernovae.
- 16M.3.HL.TZ0.20b: Describe three differences between type Ia and type II supernovae.
- 16M.3.HL.TZ0.20a: State the Jeans criterion for star formation.
- 15N.3.HL.TZ0.2e.i: Outline why the Sun will leave the main sequence, and describe the nuclear processes that occur...
- 15N.3.HL.TZ0.2e.ii: Describe two physical changes that the Sun will undergo as it enters the red giant stage.