Kinematics, forces, energy, waves, electricity and heat

Grade 11 Physics

0 of 230 stars · 0 of 46 lessons done · your report card →

Kinematics

  • L1
    Lesson 1
    Reading the problem
    Which number is which quantity

    Every number in a physics problem arrives wearing its units, and the units tell you what kind of thing it is before you do any math at all.

  • L2
    Lesson 2
    Choosing the tool
    Pick the right formula, fast

    Say them out loud once — a formula you can SAY is a formula you own. The fastest way to pick the right machine is to ask what the story GIVES you — not what it asks for.

    The formulas in this lesson
    v=dtv = \dfrac{d}{t},a=Δvta = \dfrac{\Delta v}{t}
  • L3
    Lesson 3
    Speed, distance, time
    v = d/t, asked every way

    The rearranging is the physics — the arithmetic afterward is just bookkeeping.

    The formula in this lesson
    v=dtv = \dfrac{d}{t}
  • L4
    Lesson 4
    Acceleration
    Signs matter

    Acceleration is not about how fast you are going — it is about how fast that is changing.

    The formula in this lesson
    a=Δvta = \dfrac{\Delta v}{t}
  • L5
    Lesson 5
    Units in flight
    km/h ↔ m/s · the ×3.6 bridge

    Two speeds rule the road: physics thinks in m/s, road signs shout in km/h. The bridge between them is exact: an hour is 3600 s and a kilometre is 1000 m, and 3600/1000 = 3.6.

    The formula in this lesson
    v=dtv = \dfrac{d}{t}
  • L6
    Lesson 6
    Displacement
    The half matters

    The picture explains the half: distance is the area under the speed line.

    The formula in this lesson
    d=v0t+12at2d = v_0 t + \tfrac{1}{2}at^2
  • L7
    Lesson 7
    Two steps to the answer
    find it, then use it · estimate first

    From here the paper stops asking one thing at a time. A two-step problem hands the answer of line one to line two as a given — so write each answer down, with its units, before moving on.

  • ★
    Boss lesson
    The Final Bell
    the boss · no calculator · everything carries

    No calculator — the numbers are chosen to fit in your head, the way a well-set final always is. One long problem, worked line by line, and every answer feeds the next: write them down as you go.

    The formula in this lesson
    a=Δvta = \dfrac{\Delta v}{t}

Forces & Newton's laws

  • L9
    Lesson 9
    Reading the forces
    Newtons, kilograms and what pushes what

    Chapter one watched things move. This chapter asks WHY they move: something pushed.

  • L10
    Lesson 10
    Choosing the force tool
    F = ma, W = mg, or last chapter's machines

    All through kinematics, F = ma sat in the option deck as a trap — nothing had a mass, so it never applied. That diagnosis just flipped.

    The formulas in this lesson
    F=maF = ma,W=mgW = mg,v=dtv = \dfrac{d}{t}
  • L11
    Lesson 11
    F = ma, asked every way
    force, mass or acceleration in turn

    The ladder is the one you know: pick the formula, rearrange it for what you want, put the numbers in their sockets, and only then compute.

    The formula in this lesson
    F=maF = ma
  • L12
    Lesson 12
    Weight is not mass
    The kilogram-newton confusion

    Every kilogram gets charged 9.8 newtons, no exceptions, like a tax. On the Moon the same kilograms would be charged less; the stuff itself never changes.

    The formula in this lesson
    W=mgW = mg
  • L13
    Lesson 13
    Friction holds on
    The first naked number

    A coefficient carries none — if your μ ever wears newtons, a rearrangement upstream is lying to you. The subscripts name the state, not a first-and-second: k is kinetic, already sliding, and s is static, still at rest.

    The formulas in this lesson
    fk=μkNf_k = \mu_k N,fs,max⁡=μsNf_{s,\max} = \mu_s N
  • L14
    Lesson 14
    The spring pushes back
    Stiffness in N/m · mind the cm

    Stretch a spring and it answers in proportion: F = kx — F equals k x, where F is the force the spring pulls back with, in newtons, and x is the stretch — how far it has been pulled past its rest length, in metres.

    The formula in this lesson
    F=kxF = kx
  • L15
    Lesson 15
    Unbalanced
    net the forces first, then Newton answers

    Real objects never feel one force at a time. The push fights friction; the cable fights the weight.

  • ★
    Boss lesson
    The Loading Dock
    the boss · no calculator · one crate, every law

    One crate, one long problem, and every answer feeds the next: weight, then the normal force, then friction's cut, then the net, then Newton, then the speed it all buys.

    The formula in this lesson
    W=mgW = mg

Energy, work & power

  • L17
    Lesson 17
    Paying in joules
    Which number is an energy, a force, a power

    Watch the units in every scenario: a bare N is a force waiting to act, a J is energy banked, and a W — a watt, one joule per second — is energy on the move.

    The formulas in this lesson
    W=F⋅dW = F \cdot d,Ek=12mv2E_k = \tfrac{1}{2}mv^2
  • L18
    Lesson 18
    Work is a push through a distance
    W = Fd, asked every way

    Work is not effort — it is a force times the distance it acts through: W = Fd, W equals F d: the work W in joules, the force F in newtons, the distance d in metres.

    The formula in this lesson
    W=F⋅dW = F \cdot d
  • L19
    Lesson 19
    The v-squared surprise
    double the speed, quadruple the bill

    The half is honest bookkeeping, but the square is the headline: double the speed and the energy bill QUADRUPLES. Triple it, nine times the bill.

    The formula in this lesson
    Ek=12mv2E_k = \tfrac{1}{2}mv^2
  • L20
    Lesson 20
    Height is stored energy
    Height is a battery

    Keep last chapter's warning in force: mg alone is the WEIGHT, a force in newtons. Stop there and you have not reached an energy — the height still has to be paid.

    The formula in this lesson
    U=mghU = m g h
  • L21
    Lesson 21
    The energy swap
    mgh becomes ½mv² · mass cancels

    Now watch the m on both sides — it cancels.

  • L22
    Lesson 22
    How fast is the work done
    One power, two faces

    Same bill, different clock: a kettle and a campfire can hand the water the same joules, but the kettle does it before the conversation dries up.

    The formulas in this lesson
    P=WtP = \dfrac{W}{t},P=FvP = F v
  • L23
    Lesson 23
    Nothing is perfect
    efficiency · nothing beats 100%

    No machine hands back every joule: friction, heat and noise all take their cut.

  • ★
    Boss lesson
    The Drop Tower
    the boss · no calculator · energy in, speed out

    No calculator: g rounds to 10 and every number is chosen to fit in your head, the way a well-set final always is. One ride, worked line by line, and every answer feeds the next: write them down as you go.

    The formula in this lesson
    U=mghU = m g h

Waves & sound

  • L25
    Lesson 25
    Anatomy of a wave
    name the parts · T = 1/f

    Every wave that will ever appear on your paper is described by four numbers.

  • L26
    Lesson 26
    The universal wave equation
    v = fλ, asked every way

    Run the free check before any arithmetic: hertz times metres is cycles-per-second times metres-per-cycle — the cycles cancel and m/s falls out, a speed.

    The formula in this lesson
    v=fλv = f\lambda
  • L27
    Lesson 27
    The speed of sound
    331.3 plus warmth · the echo's ÷2

    Sound has no fixed speed — it borrows one from the air. In dry air the rule is v = 331.3 + 0.606T — the speed v in m/s, and T the air temperature in °C.

  • L28
    Lesson 28
    Strings that sing
    Harmonics climb

    A guitar string is pinned at both ends, so the simplest wave it can hold is one bump — HALF a wavelength — between the pins.

    The formulas in this lesson
    f1=v2Lf_1 = \dfrac{v}{2L},v=Fμv = \sqrt{\dfrac{F}{\mu}},fn=n f1f_n = n \, f_1
  • L29
    Lesson 29
    Pipes and columns
    Odd harmonics only

    Close a pipe at one end and the rules change. The closed end pins the air still — a node — while the open mouth swings free — an antinode.

    The formula in this lesson
    f1=v4Lf_1 = \dfrac{v}{4L}
  • L30
    Lesson 30
    How loud is loud
    decibels · the inverse-square fade

    Your ear spans a trillion-to-one range of intensities, so loudness is scored on a ladder of tens.

  • L31
    Lesson 31
    Moving sources and beats
    Doppler shifts · beats

    The siren that sails past you drops its pitch the instant it passes — that is the Doppler effect, and the sanity rail you must never let go of: approach raises pitch, retreat lowers it.

    The formulas in this lesson
    f′=fvv−vsf' = \dfrac{f v}{v - v_s},f′=f(v+vo)vf' = \dfrac{f (v + v_o)}{v},fbeat=f1−f2f_{\text{beat}} = f_1 - f_2
  • ★
    Boss lesson
    The Sound Check
    the boss · no calculator · whole hertz

    No calculator — the numbers are chosen to live in your head, and 0.606 rounds to six-tenths without shame. One long sound check, worked line by line, and every answer feeds the next: write them down as you go.

Electricity & magnetism

  • L33
    Lesson 33
    Counting charge
    amps, volts, ohms, coulombs — and Q = It

    Four units run this whole chapter, and a water pipe explains them all. Current I, in amperes, is the flow — how much charge streams past per second.

    The formula in this lesson
    Q=ItQ = It
  • L34
    Lesson 34
    Ohm's law
    V = IR, asked every way

    V = IR — read aloud: V equals I R — is the chapter's centre of gravity: pressure equals flow times narrowness, with V the voltage in volts, I the current in amperes and R the resistance in ohms.

    The formula in this lesson
    V=IRV = IR
  • L35
    Lesson 35
    Series and parallel
    combine resistors, predict the meter

    Parallel is extra doors: every new branch makes the flow easier, so the total drops BELOW even the smallest branch — always.

    The formulas in this lesson
    Rt=R1+R2R_t = R_1 + R_2,Rt=R1R2R1+R2R_t = \dfrac{R_1 R_2}{R_1 + R_2}
  • L36
    Lesson 36
    Three faces of power
    P = VI, I²R, V²/R — match the face to the givens

    The original is P = VI (read aloud: P equals V I) — the push times the flow is the rate of spending energy, measured in watts.

    The formulas in this lesson
    P=VIP = VI,P=I2RP = I^{2} R,P=V2RP = \dfrac{V^2}{R}
  • L37
    Lesson 37
    The hydro bill
    kWh · the meter, the bridge, the bill

    The hydro meter does not count joules — it would need nine digits by breakfast.

  • L38
    Lesson 38
    Magnets at work
    F = BIL and the transformer's ratio

    Put a current-carrying wire square across a magnetic field and the field pushes on it — the motor effect, and the reason anything electric spins.

    The formulas in this lesson
    F=B I LF = B\,I\,L,VsVp=NsNp\dfrac{V_s}{V_p} = \dfrac{N_s}{N_p}
  • ★
    Boss lesson
    The Breaker Panel
    the boss · no calculator · trace the circuit to the bill

    No calculator — 120 V and whole ohms, chosen to fit in your head, the way a well-set final always is.

    The formulas in this lesson
    Rt=R1+R2R_t = R_1 + R_2,P=VIP = VI

Heat

  • L40
    Lesson 40
    Heat is not temperature
    joules move, degrees describe

    Same July sun, same beach: the sand scorches your feet while the water stays cool. Both collected heat all morning — but water is thermally stubborn: it takes a small mountain of energy to move its thermometer one degree.

    The formula in this lesson
    Q=mcΔTQ = m c \Delta T
  • L41
    Lesson 41
    Q = mcΔT, asked every way
    heat, mass, capacity, rise — four unknowns

    If your rearrangement's units refuse to cancel, it is wrong — no appeal. (Units that do work out never prove it right.) Two flags for this lesson.

    The formula in this lesson
    Q=mcΔTQ = m c \Delta T
  • L42
    Lesson 42
    Changing state
    Flat at the plateau

    Drop a thermometer in melting ice and watch: heat pours in, and the reading parks at 0 °C until the last crystal is gone.

    The formula in this lesson
    Q=mLQ = m L
  • L43
    Lesson 43
    Warm it, then boil it
    sensible plus latent · estimate first

    The named trap is skipping a leg — usually the plateau, because the thermometer stops advertising it. And feel the sizes before computing.

  • L44
    Lesson 44
    Heat on the move
    Watts through walls

    So far we have counted heat in lump sums. But through a window, heat runs as a steady rate — joules every second, which is to say watts, the same watts as any power.

    The formula in this lesson
    P=kA ΔTdP = \dfrac{kA\,\Delta T}{d}
  • L45
    Lesson 45
    The stretch of summer
    ΔL = αL₀ΔT · mm out of metres

    Warm a solid and it grows — every metre of it, by a tiny fixed fraction per degree.

  • ★
    Boss lesson
    The Kettle
    the boss · no calculator · everything carries

    No calculator — the numbers are chosen to carry in your head, the way a well-set final always is. One kettle, worked line by line, and every answer feeds the next: write them down as you go.

    The formula in this lesson
    Q=mcΔTQ = m c \Delta T

Nothing here is locked — the path recommends an order, and you study what you need. Progress lives in this browser (it survives cache clears, not “clear site data”); sign-in with permanent tracking is coming.

On paper: the study guide — formulas, worked examples, practice problems with the key — or the formula sheet alone. All downloads live in the study guide library.