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A Level H2 Physics Energy Power Quiz

Free A Level H2 Physics Energy Power quiz, Gemma31B Exam version, with questions, answers, and A Level-style practice for Singapore students.

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A Level H2 Physics From Real Exams Generated by Gemma 4 31B Updated 2026-08-17

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Answers

Answer Key - A-Level Physics H2 Quiz: Energy Power

  1. Binding Energy: The minimum energy required to completely separate a nucleus into its constituent protons and neutrons. [2]

  2. Calculation: KE=12mv2=12(0.50)(4.0)2=4.0 JKE = \frac{1}{2}mv^2 = \frac{1}{2}(0.50)(4.0)^2 = 4.0 \text{ J} [2]

  3. Relationship: The binding energy is the energy equivalent of the mass defect, given by E=Δmc2E = \Delta m c^2. [2]

  4. Calculation: a=F/m=15/2.0=7.5 m s2a = F/m = 15/2.0 = 7.5 \text{ m s}^{-2} v=u+at=0+(7.5)(3.0)=22.5 m s1v = u + at = 0 + (7.5)(3.0) = 22.5 \text{ m s}^{-1} KE=12(2.0)(22.5)2=506.25 JKE = \frac{1}{2}(2.0)(22.5)^2 = 506.25 \text{ J} [3]

  5. Stability: Higher binding energy per nucleon means more energy is required to remove a nucleon from the nucleus, making it more tightly bound and stable. [2]

  6. Calculation: Δm=208.980208.972=0.008 u\Delta m = 208.980 - 208.972 = 0.008 \text{ u} E=0.008×931.5=7.452 MeVE = 0.008 \times 931.5 = 7.452 \text{ MeV} [3]

  7. X-ray Significance: The minimum energy corresponds to the ionization energy of the K-shell electrons of the target metal. Electrons must have at least this energy to eject a K-shell electron to produce characteristic X-rays. [3]

  8. Calculation: E=0.20×931.5=186.3 MeVE = 0.20 \times 931.5 = 186.3 \text{ MeV} [3]

  9. Calculation: KE=12(1.67×1027)(2.0×106)2=3.34×1015 JKE = \frac{1}{2}(1.67 \times 10^{-27})(2.0 \times 10^6)^2 = 3.34 \times 10^{-15} \text{ J} KE in eV=(3.34×1015)/(1.6×1019)=20,875 eV20.9 keVKE \text{ in eV} = (3.34 \times 10^{-15}) / (1.6 \times 10^{-19}) = 20,875 \text{ eV} \approx 20.9 \text{ keV} [3]

  10. Comparison:

    • Continuous: Produced by Bremsstrahlung (braking radiation) where electrons lose varying amounts of energy as they are decelerated by the nucleus.
    • Characteristic: Produced when an incident electron knocks out an inner-shell electron, and an outer-shell electron drops down to fill the vacancy, emitting a photon of a specific energy. [3]
  11. Distribution: The energy is shared as kinetic energy between the alpha particle and the daughter nucleus. Due to conservation of momentum, the lighter alpha particle carries the majority of the kinetic energy. [2]

  12. Calculation: E=1.2×103×1.6×1019=1.92×1016 JE = 1.2 \times 10^3 \times 1.6 \times 10^{-19} = 1.92 \times 10^{-16} \text{ J} λ=hc/E=(6.63×1034×3×108)/1.92×1016=1.036×109 m=1.04 nm\lambda = hc/E = (6.63 \times 10^{-34} \times 3 \times 10^8) / 1.92 \times 10^{-16} = 1.036 \times 10^{-9} \text{ m} = 1.04 \text{ nm} [3]

  13. Gradient: The gradient represents the exponent nn. [1]

  14. Calculation: log10k=0.477\log_{10} k = 0.477 k=100.4773.0k = 10^{0.477} \approx 3.0 [2]

  15. Calculation: W=mgh=100×9.81×5.0=4905 JW = mgh = 100 \times 9.81 \times 5.0 = 4905 \text{ J} P=W/t=4905/10=490.5 WP = W/t = 4905 / 10 = 490.5 \text{ W} [3]

  16. Calculation: 8=k(2n)8 = k(2^n) and 64=k(4n)64 = k(4^n) Divide: 64/8=(4/2)n8=2nn=364/8 = (4/2)^n \Rightarrow 8 = 2^n \Rightarrow n = 3 [3]

  17. Derivation: Force F=mgsinθ+μmgcosθF = mg \sin\theta + \mu mg \cos\theta P=Fv=(mgsinθ+μmgcosθ)v=mgv(sinθ+μcosθ)P = Fv = (mg \sin\theta + \mu mg \cos\theta)v = mgv(\sin\theta + \mu \cos\theta) [4]

  18. Calculation: Δm=0.015×1.66×1027 kg=2.49×1029 kg\Delta m = 0.015 \times 1.66 \times 10^{-27} \text{ kg} = 2.49 \times 10^{-29} \text{ kg} E=Δmc2=2.49×1029×(3×108)2=2.24×1012 JE = \Delta m c^2 = 2.49 \times 10^{-29} \times (3 \times 10^8)^2 = 2.24 \times 10^{-12} \text{ J} [3]

  19. Calculation: Pout=dEdt=dmdtgh=0.10×9.81×20=19.62 WP_{\text{out}} = \frac{dE}{dt} = \frac{dm}{dt}gh = 0.10 \times 9.81 \times 20 = 19.62 \text{ W} Pin=Pout/0.70=19.62/0.70=28.03 WP_{\text{in}} = P_{\text{out}} / 0.70 = 19.62 / 0.70 = 28.03 \text{ W} [4]

  20. Proof: P=dEdt=ddt(12mv2)=mvdvdtP = \frac{dE}{dt} = \frac{d}{dt}(\frac{1}{2}mv^2) = mv \frac{dv}{dt} Pdt=mvdvP dt = mv dv Integrate: Pt=12mv2Pt = \frac{1}{2}mv^2 v2=2Ptmv=2Pmt1/2v^2 = \frac{2Pt}{m} \Rightarrow v = \sqrt{\frac{2P}{m}} t^{1/2} Thus vt1/2v \propto t^{1/2}. [4]