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Physics essentials: 50 laws and formulas

The core laws and equations of introductory physics: Newton’s laws and kinematics, work, energy and momentum, circuits and electromagnetism, waves and light.

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Newton’s first law

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  1. 1
    Newton’s first law
    An object stays at rest or keeps moving at constant velocity unless a net external force acts on it
    Also called the law of inertia.
  2. 2
    Newton’s second law
    F⃗net=ma⃗\vec{F}_{\text{net}} = m\vec{a}
    Force is measured in newtons: 1 N=1 kg m/s21\ \mathrm{N} = 1\ \mathrm{kg\,m/s^2}.
  3. 3
    Newton’s third law
    When A exerts a force on B, B exerts an equal and opposite force on A
    The two forces act on different objects, so they don’t cancel.
  4. 4
    Velocity under constant acceleration
    v=v0+atv = v_0 + at
  5. 5
    Displacement under constant acceleration
    s=v0t+12at2s = v_0 t + \tfrac{1}{2}at^2
  6. 6
    Constant-acceleration equation without time
    v2=v02+2asv^2 = v_0^2 + 2as
  7. 7
    Gravitational acceleration at Earth’s surface
    g≈9.81 m/s2g \approx 9.81\ \mathrm{m/s^2}
  8. 8
    Weight
    W=mgW = mg
    Mass is the same everywhere; weight depends on the local gravitational field.
  9. 9
    Momentum
    p⃗=mv⃗\vec{p} = m\vec{v}
    The total momentum of a system is conserved when no external force acts on it.
  10. 10
    Impulse
    J=F Δt=ΔpJ = F\,\Delta t = \Delta p
    Why airbags help: a longer stopping time means a smaller force for the same change in momentum.
  11. 11
    Kinetic friction force
    fk=μkNf_k = \mu_k N
    NN is the normal force. Static friction can rise up to μsN\mu_s N before an object slips.
  12. 12
    Centripetal acceleration and force
    ac=v2ra_c = \dfrac{v^2}{r}, so Fc=mv2rF_c = \dfrac{mv^2}{r}
    Both point toward the center of the circle.
  13. 13
    Newton’s law of universal gravitation
    F=Gm1m2r2F = G\dfrac{m_1 m_2}{r^2}
    G≈6.674×10−11 N m2/kg2G \approx 6.674 \times 10^{-11}\ \mathrm{N\,m^2/kg^2}
  14. 14
    Torque
    τ=rFsin⁡θ\tau = rF\sin\theta
    θ\theta is the angle between the lever arm and the force.
  15. 15
    Hooke’s law
    F=−kxF = -kx
    kk is the spring constant; the minus sign means the force opposes the displacement.
  16. 16
    Pressure
    P=FAP = \dfrac{F}{A}
    Measured in pascals: 1 Pa=1 N/m21\ \mathrm{Pa} = 1\ \mathrm{N/m^2}.
  17. 17
    Pressure at a depth in a fluid
    P=P0+ρghP = P_0 + \rho g h
    P0P_0 is the pressure at the surface and ρ\rho the fluid’s density.
  18. 18
    Archimedes’ principle
    The buoyant force equals the weight of the fluid displaced: Fb=ρfluidVgF_b = \rho_{\text{fluid}} V g
  19. 19
    Kinetic energy
    Ek=12mv2E_k = \tfrac{1}{2}mv^2
  20. 20
    Gravitational potential energy near Earth’s surface
    Ep=mghE_p = mgh
  21. 21
    Elastic potential energy of a spring
    E=12kx2E = \tfrac{1}{2}kx^2
  22. 22
    Work done by a constant force
    W=Fdcos⁡θW = Fd\cos\theta
    Measured in joules: 1 J=1 N m1\ \mathrm{J} = 1\ \mathrm{N\,m}.
  23. 23
    Work–energy theorem
    The net work done on an object equals its change in kinetic energy: Wnet=ΔEkW_{\text{net}} = \Delta E_k
  24. 24
    Power
    P=WtP = \dfrac{W}{t}
    Measured in watts: 1 W=1 J/s1\ \mathrm{W} = 1\ \mathrm{J/s}. For a constant force, also P=FvP = Fv.
  25. 25
    Conservation of energy
    Energy is never created or destroyed, only converted from one form to another; the total energy of an isolated system is constant
  26. 26
    Elastic vs inelastic collisions
    Both conserve momentum; only elastic collisions also conserve kinetic energy
    In a perfectly inelastic collision the objects stick together.
  27. 27
    Mass–energy equivalence
    E=mc2E = mc^2
  28. 28
    First law of thermodynamics
    ΔU=Q−W\Delta U = Q - W
    QQ is the heat added to the system and WW the work done by it. Some textbooks write ΔU=Q+W\Delta U = Q + W, with WW the work done on the system.
  29. 29
    Heat needed to change an object’s temperature
    Q=mc ΔTQ = mc\,\Delta T
    cc is the specific heat capacity; for water it is about 4.18 kJ kg−1 K−14.18\ \mathrm{kJ\,kg^{-1}\,K^{-1}}.
  30. 30
    Ohm’s law
    V=IRV = IR
  31. 31
    Electric power
    P=IV=I2R=V2RP = IV = I^2R = \dfrac{V^2}{R}
  32. 32
    Resistors in series
    Rtotal=R1+R2+⋯R_{\text{total}} = R_1 + R_2 + \cdots
    The same current flows through each resistor.
  33. 33
    Resistors in parallel
    1Rtotal=1R1+1R2+⋯\dfrac{1}{R_{\text{total}}} = \dfrac{1}{R_1} + \dfrac{1}{R_2} + \cdots
    Each has the same voltage across it, and the total is less than the smallest resistance.
  34. 34
    Coulomb’s law
    F=kq1q2r2F = k\dfrac{q_1 q_2}{r^2}
    k=14πε0≈8.99×109 N m2/C2k = \dfrac{1}{4\pi\varepsilon_0} \approx 8.99 \times 10^9\ \mathrm{N\,m^2/C^2}
  35. 35
    Electric current
    I=QtI = \dfrac{Q}{t}
    Measured in amperes: 1 A=1 C/s1\ \mathrm{A} = 1\ \mathrm{C/s}.
  36. 36
    Elementary charge
    e≈1.602×10−19 Ce \approx 1.602 \times 10^{-19}\ \mathrm{C}
    The charge of a proton; an electron carries −e-e.
  37. 37
    Capacitance
    C=QVC = \dfrac{Q}{V}
    Measured in farads. A capacitor stores energy E=12CV2E = \tfrac{1}{2}CV^2.
  38. 38
    Kirchhoff’s circuit laws
    Current law: the current into a junction equals the current out (charge is conserved). Voltage law: the voltages around any closed loop sum to zero (energy is conserved)
  39. 39
    Resistance of a wire
    R=ρLAR = \rho\dfrac{L}{A}
    ρ\rho is the material’s resistivity, LL the length and AA the cross-sectional area.
  40. 40
    Faraday’s law of induction
    E=−dΦBdt\mathcal{E} = -\dfrac{d\Phi_B}{dt}
    A changing magnetic flux induces an EMF. The minus sign is Lenz’s law: the induced current opposes the change that caused it.
  41. 41
    Magnetic force on a moving charge
    F⃗=qv⃗×B⃗\vec{F} = q\vec{v} \times \vec{B}
    Its magnitude is qvBsin⁡θqvB\sin\theta. It is perpendicular to the velocity, so it does no work.
  42. 42
    Wave speed, frequency and wavelength
    v=fλv = f\lambda
    Period and frequency are reciprocals: T=1fT = \dfrac{1}{f}.
  43. 43
    Transverse vs longitudinal waves
    Transverse: the medium oscillates perpendicular to the direction of travel (waves on a string, light). Longitudinal: it oscillates along it (sound)
  44. 44
    Speed of light in a vacuum
    c=299 792 458 m/s≈3.00×108 m/sc = 299\,792\,458\ \mathrm{m/s} \approx 3.00 \times 10^8\ \mathrm{m/s}
    Exact by definition: the metre is defined from it.
  45. 45
    Speed of sound in air at 20 °C
    About 343 m/s343\ \mathrm{m/s}
  46. 46
    Energy of a photon
    E=hf=hcλE = hf = \dfrac{hc}{\lambda}
    Planck constant h≈6.626×10−34 J sh \approx 6.626 \times 10^{-34}\ \mathrm{J\,s}
  47. 47
    Snell’s law
    n1sin⁡θ1=n2sin⁡θ2n_1 \sin\theta_1 = n_2 \sin\theta_2
    Angles are measured from the normal to the surface.
  48. 48
    Doppler effect
    The observed frequency rises when source and observer move toward each other and falls when they move apart
    It is why a passing siren drops in pitch.
  49. 49
    Period of a simple pendulum
    T=2πLgT = 2\pi\sqrt{\dfrac{L}{g}}
    Valid for small swings; it doesn’t depend on the mass.
  50. 50
    Period of a mass on a spring
    T=2πmkT = 2\pi\sqrt{\dfrac{m}{k}}

Frequently asked questions

Is this deck for high school or university physics?

Both. It covers algebra-based introductory physics, as in AP Physics 1 and 2 or a first university course, plus a few calculus-based results such as Faraday’s law.

Why do some symbols differ from my textbook?

Notation varies: kinetic energy is written KE, K or E_k, and the first law of thermodynamics has two sign conventions. The cards note the common alternatives where it matters.

Should I memorize formulas or derive them?

Both. Knowing the core equations by heart frees your attention for the physics of a problem; knowing where they come from tells you when they apply.