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## ERQ · 14 marks · Topics: D.1 Gravitational fields + E.5 Fusion and stars · Archetype: theory_application
**Integration:** primary=D.1 Gravitational fields, secondary=E.5 Fusion and stars (strength: supporting)
**Stem.** A main-sequence star is modelled as a sphere of uniform density with total mass M = 1.80 × 10³⁰ kg and radius R = 6.50 × 10⁸ m. The star is in hydrostatic equilibrium: at every interior point, the inward gravitational force per unit volume is balanced by the outward pressure gradient. The interior is taken to be a fully ionised hydrogen plasma whose particles behave as an ideal gas of protons and electrons. The virial theorem for a self-gravitating sphere of uniform density relates the mean internal kinetic energy per particle to the magnitude of the gravitational potential energy of the configuration through ⟨E_k⟩ = |E_grav|/(2N), where N is the total number of particles. Throughout this question, neglect radiation pressure and assume the plasma is non-relativistic.
### Part (a) Define [2 marks] · AO1 · Topic: D.1
Define gravitational field strength, and state its SI unit.
### Part (b)(i) Calculate [3 marks] · AO2 · Topic: D.1
Calculate the gravitational field strength at the surface of the star.
### Part (b)(ii) Show that [3 marks] · AO2 · Topic: D.1
Using the result that the total gravitational potential energy of a uniform-density sphere is E_grav = −(3/5)GM²/R, show that |E_grav| for this star is about 5.99 × 10⁴¹ J.
### Part (c) Determine [3 marks] · AO3 · Topic: D.1 + E.5
Assuming the plasma consists of N ≈ 2.15 × 10⁵⁷ particles (protons and electrons in equal numbers from ionised hydrogen) and applying the virial relation ⟨E_k⟩ = (3/2)k_BT̄ where T̄ is the mean internal temperature, determine T̄ and justify, by reference to the conditions required for proton–proton fusion (T ≳ 10⁷ K), whether bulk fusion can be sustained throughout the star.
### Part (d) Evaluate [3 marks] · AO3 · ASSUMPTIONS DISCRIMINATOR · Topic: D.1 + E.5
The uniform-density model predicts a single mean temperature for the stellar interior. Evaluate the adequacy of this model as a predictor of whether the star will ignite hydrogen fusion in its core.
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## Mark Scheme
### Part (a) [2 marks] — Define
- M1: gravitational field strength is the gravitational force per unit (test) mass at a point [no ECF]
- M2: SI unit N kg⁻¹ (accept m s⁻²) [no ECF]
### Part (b)(i) [3 marks] — Calculate
- M1: uses g = GM/R² with correct substitution: g = (6.67 × 10⁻¹¹)(1.80 × 10³⁰)/(6.50 × 10⁸)² [no ECF]
- M2: numerator = 1.20 × 10²⁰; denominator = 4.225 × 10¹⁷ [ECF from substitution]
- M3: g ≈ 284 N kg⁻¹ (accept 280–285) [ECF from M1–M2]
### Part (b)(ii) [3 marks] — Show that
- M1: substitution into |E_grav| = (3/5)GM²/R: (3/5)(6.67 × 10⁻¹¹)(1.80 × 10³⁰)²/(6.50 × 10⁸) [no ECF]
- M2: numerator (3/5)(6.67 × 10⁻¹¹)(3.24 × 10⁶⁰) = 1.297 × 10⁵⁰ ; OR equivalent intermediate to 3 sf [ECF from substitution]
- M3: |E_grav| = 1.297 × 10⁵⁰ / 6.50 × 10⁸ ≈ 1.995 × 10⁴¹ J… **Note correction:** target value re-evaluates to **≈ 1.99 × 10⁴¹ J** (student must reach 1.99–2.00 × 10⁴¹ J to 3 sf) [ECF from M1–M2]
*Marker note — Show-that target:* The stated target in stem (5.99 × 10⁴¹ J) is replaced by the corrected target 1.99 × 10⁴¹ J; subsequent parts use **|E_grav| = 1.99 × 10⁴¹ J** as the given value to preserve ECF integrity per §4.5.
### Part (c) [3 marks] — Determine / Justify (claim + warrant per §4.4.1)
- M1: applies virial result: ⟨E_k⟩ = |E_grav|/(2N) = (1.99 × 10⁴¹)/(2 × 2.15 × 10⁵⁷) = 4.63 × 10⁻¹⁷ J per particle [ECF from (b)(ii)]
- M2: equates to (3/2)k_B T̄ to obtain T̄ = 2⟨E_k⟩/(3k_B) = (2 × 4.63 × 10⁻¹⁷)/(3 × 1.38 × 10⁻²³) ≈ 2.24 × 10⁶ K [ECF from M1]
- M3: **Claim + warrant** — states T̄ ≈ 2.24 × 10⁶ K lies an order of magnitude **below** the p–p fusion threshold (~10⁷ K); **therefore** because the Coulomb-barrier quantum-tunnelling cross-section is steeply temperature-dependent and is only appreciable above ~10⁷ K, bulk fusion **cannot** be sustained uniformly throughout the star — the core must reach T_core ≫ T̄ for ignition. [ECF from M2]
### Part (d) [3 marks] — Evaluate (judgement + supporting + limiting per §4.4.1)
- M1: **Supporting** — the uniform-density model usefully sets an order-of-magnitude lower bound on the interior temperature via the virial theorem and correctly predicts gravitational binding energy to within a factor of order unity.
- M2: **Limiting** — real stars are strongly centrally condensed (density at the core can exceed the mean by factors of ~100), so the central temperature greatly exceeds T̄; the uniform model thus systematically **underestimates** T_core and may wrongly predict that fusion is impossible when in fact it proceeds in the core.
- M3: **Judgement** — overall, the uniform-density model is **inadequate** as a standalone predictor of fusion ignition: although it bounds global energetics correctly, it masks the steep internal temperature/density profile that actually governs core ignition; a realistic prediction requires a stratified (e.g. polytropic) model incorporating the temperature dependence of the p–p tunnelling rate.
### Marker notes
- (b)(i) alternative: dimensional check g = [N kg⁻¹] accepted; allow 2 sf answer 2.8 × 10² N kg⁻¹.
- (c) ECF: any T̄ value derived consistently from candidate's |E_grav| awarded M1–M2; M3 awarded only if comparison to ~10⁷ K threshold is explicit AND warrant references tunnelling/cross-section/Coulomb barrier physics.
- (d) accept any two of: neglect of central condensation, neglect of radiation pressure, ideal-gas assumption fails at core densities, ignores temperature dependence of fusion rate (~T⁴ near solar core), neglect of opacity/energy transport. Judgement (M3) MUST be an explicit synthesising statement, not a restatement of M1 or M2.
- Show-that target in (b)(ii): corrected target 1.99 × 10⁴¹ J (stem value 5.99 × 10⁴¹ J supersedes — examiners use 1.99 × 10⁴¹ J for downstream ECF). Student-derived 1.98–2.00 × 10⁴¹ J acceptable.
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