20 questions in 35 minutes, like Section I, marked with worked explanations.
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HSC Physics · Module 5 flashcards
83 cards. Work out each answer first, then open the card to check it and see the working.
Answer: the mass of the planet and the orbital radius
v = √(GM/r). The satellite's own mass cancels when equating gravitational force to centripetal force.
Answer: 7.6 km s-1
v = √(GM/r) = √(4.0 × 1014/7.0 × 106) = √(5.7 × 107) = 7.6 × 10³ m s-1.
Answer: −5.7 × 1010 J
U = −GMm/r = −(4.0 × 1014 × 1000)/(7.0 × 106) = −5.7 × 1010 J. Potential energy is negative because zero is set at infinity.
Answer: the same magnitude, with the vertical component reversed
Horizontal velocity is unchanged. By symmetry the vertical component returns to the same size but points downward.
Answer: 19.6 m s-1
vy = 0 at the top: 0 = uy − gt, so uy = 9.8 × 2.0 = 19.6 m s-1.
Answer: they land at the same time
Vertical motion is independent of horizontal motion. Both start with zero vertical velocity and the same acceleration, so they fall for the same time.
Answer: 11.2 km s-1
vesc = √(2GM/R) = √(2 × 4.0 × 1014/6.371 × 106) = √(1.26 × 108) = 1.12 × 104 m s-1.
Answer: 4.9 m s-2
g = GM/R². Mass × 2 and R² × 4 gives g × ½ = 4.9 m s-2.
Answer: the horizontal component of the tension
T sinθ points towards the centre of the horizontal circle. T cosθ balances the weight.
Answer: halves
KE = GMm/2r, so doubling r halves the kinetic energy. (Total energy becomes less negative; potential energy rises.)
Answer: 22 m s-1
vy² = 2gh = 392, vy = 19.8 m s-1. Speed = √(10² + 19.8²) = 22 m s-1.
Answer: horizontal velocity and downward acceleration of 9.8 m s-2
Only the vertical velocity is zero at the top. Gravity acts throughout, so acceleration is always 9.8 m s-2 downward.
Answer: 3.8 × 1027 kg
M = 4π²r³/(GT²) = 39.5 × 6.4 × 1025/(6.67 × 10-11 × 1.0 × 1010) = 3.8 × 1027 kg.
Answer: stays the same
F ∝ m1m2/r². Numerator × 4, denominator × 4: unchanged.
Answer: the same range and a longer flight time
Complementary angles give the same range. The 60° launch has a larger vertical component, so it goes higher and stays in the air longer.
Answer: friction between the tyres and the road
On a flat road the only horizontal force available is friction. Leaning keeps the net torque zero so the cyclist does not topple.
Answer: 1000 m
t = √(2 × 500/9.8) = 10.1 s. x = 100 × 10.1 = 1010 m ≈ 1000 m.
Answer: a smaller range and smaller maximum height, with an asymmetric path
Drag opposes motion in both directions, reducing height and range. The descent is steeper than the ascent, so the path is not symmetric.
Answer: 9.9 m s-1
At minimum speed the normal force is zero: v = √(gr) = √(9.8 × 10) = 9.9 m s-1.
Answer: 1.6 m s-2
g = GM/R² = 6.67 × 10-11 × 7.35 × 1022/(1.74 × 106)² = 1.6 m s-2.
Answer: increases because it moves to a lower orbit
Total energy falls, so r decreases. Since v = √(GM/r), the satellite speeds up even though drag removes energy — the lost energy comes from potential energy.
Answer: the height of launch
The vertical motion starts from zero vertical velocity, so t = √(2h/g). Launch speed only changes how far it goes horizontally.
Answer: 17 m s-1
F = mv²/r, so v = √(Fr/m) = √(7500 × 60/1500) = √300 = 17 m s-1.
Answer: zero
The force is always perpendicular to the displacement, so W = Fs cos90° = 0. This is why the speed stays constant.
Answer: 24 hours
T = √(4π²r³/GM) = √(39.5 × 7.4 × 1022/4.0 × 1014) = 8.5 × 104 s ≈ 24 h. This is the geostationary radius.
Answer: zero at infinity and negative elsewhere
U = −GMm/r. Choosing U = 0 at infinite separation makes bound objects have negative potential energy.
Answer: both have the same speed
Energy is conserved and both land at launch height, so both return to the launch speed.
Answer: is unchanged
v = √(GM/r) depends only on the central mass and radius, not on the satellite's mass.
Answer: 1 : 3
H ∝ sin²θ. sin²30° = 0.25, sin²60° = 0.75. Ratio 1 : 3.
Answer: 2.0 s
From rest vertically: h = ½gt², t = √(2 × 20/9.8) = 2.0 s.
Answer: tanθ = v²/(rg)
N sinθ = mv²/r and N cosθ = mg. Dividing gives tanθ = v²/(rg).
Answer: 2.7 × 10-3 m s-2
a = 4π²r/T² = 39.5 × 3.84 × 108/(2.36 × 106)² = 2.7 × 10-3 m s-2.
Answer: 6.7 × 10-5 N
F = Gm1m2/r² = 6.67 × 10-11 × 106/1 = 6.7 × 10-5 N.
Answer: twice as large
v = √(GM/r). Four times the mass gives √4 = 2 times the speed.
Answer: moves in a straight line along the tangent
With no force, Newton's first law applies: it keeps its instantaneous velocity, which is tangential.
Answer: 1.6 × 1010 J
ΔU = GMm(1/R − 1/2R) = GMm/2R = 4.0 × 1014 × 500/(2 × 6.371 × 106) = 1.6 × 1010 J. (Using mgh would be wrong — g is not constant over this range.)
Answer: 25 m s-1 at 53°
Speed = √(15² + 20²) = 25 m s-1. tanθ = 20/15, θ = 53°.
Answer: the passenger's inertia — their body tends to continue in a straight line while the car turns
No outward force acts. The seat and door must push the passenger inward to make them follow the curve; what they feel is their own inertia.
Answer: is independent of the mass of the escaping object
½mv² = GMm/R; m cancels, giving v = √(2GM/R).
Answer: 81 m
t = √(2 × 80/9.8) = 4.04 s. Range = 20 × 4.04 = 81 m.
Answer: 6 times larger
R = u² sin2θ/g. Range ∝ 1/g, and 9.8/1.6 ≈ 6.
Answer: becomes half as negative
U = −GMm/r. Doubling r halves the magnitude, so U goes from −GMm/R to −GMm/2R.
Answer: 1.0 × 103 m s-1
v = √(GM/r) = √(4.0 × 1014/3.84 × 108) = √(1.04 × 106) = 1.0 × 10³ m s-1.
Answer: 28 m s-1
uy = √(2gH) = √196 = 14 m s-1. u = uy/sin30° = 28 m s-1.
Answer: 31 m s-1
R = u²/g at 45°, so u = √(Rg) = √980 = 31 m s-1.
Answer: 8.2 N
At the top T + mg = mv²/r, so T = 1.0 × 36/2.0 − 9.8 = 8.2 N.
Answer: the net torque is zero
Rotational equilibrium means no net turning effect: the sum of clockwise torques equals the sum of anticlockwise torques.
Answer: fastest when closest to the Sun
To sweep the same area in the same time when the radius is short, the planet must cover more arc, so it moves faster near perihelion.
Answer: 40 m
Total flight time = 4.0 s. Range = 10 × 4.0 = 40 m.
Answer: have the same vertical motion
Both have zero initial vertical velocity and the same acceleration g, so their vertical motions are identical.
Answer: three times
g = GM/R². Mass × 3 with R unchanged gives g × 3.
Answer: 90 minutes
At r ≈ 6.8 × 106 m, T = 2π√(r³/GM) ≈ 5500 s ≈ 90 min.
Answer: 610 N
g = GM/r² = 4.0 × 1014/(6.77 × 106)² = 8.7 m s-2. F = 70 × 8.7 = 610 N. 'Weightlessness' is free fall, not absence of gravity.
Answer: its kinetic energy decreases, its potential energy increases, and net energy must be supplied
KE = GMm/2r falls, U = −GMm/r rises by twice as much, so total energy rises — the rocket must supply it.
Answer: its launch speed and the height of the cliff
Energy conservation: ½mv² = ½mu² + mgh, so v depends only on u and h — not on the angle.
Answer: 99 m s-2
v = 2πrf = 3.14 m s-1. a = v²/r = 9.87/0.10 = 99 m s-2.
Answer: 1.5 m
Torques balance: 30 × 9.8 × 2.0 = 40 × 9.8 × d, so d = 1.5 m.
Answer: 3.1 km s-1
v = 2πr/T = 2π × 4.22 × 107/86 400 = 3.1 × 10³ m s-1.
Answer: 12 m
uy = 20 sin50° = 15.3 m s-1. H = 15.3²/19.6 = 12 m.
Answer: tanθ = v²/(rg)
T sinθ = mv²/r and T cosθ = mg. Dividing gives tanθ = v²/(rg) — the same relation as a banked curve.
Answer: +7.1 × 109 J
ΔU = GMm(1/r1 − 1/r2) = 4.0 × 1017 × (1.43 × 10-7 − 1.25 × 10-7) = +7.1 × 109 J. U increases (becomes less negative).
20 questions in 35 minutes, like Section I, marked with worked explanations.
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317 cards across Modules 5–8.
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