Before we start, a few reminders in plain words so no symbol appears unearned:
I is the moment of inertia — a number saying "how hard is this object to spin up", the rotational cousin of mass. (See Moment of Inertia.)
ω (lowercase omega, the Greek "w") is angular speed — how many radians of turn happen each second. A radian is just "arc length equal to the radius"; a full circle is 2π radians.
L=Iω is angular momentum — spin's version of "how much motion is stored". The little arrow means it has a direction, pointing along the spin axis. (See Angular Momentum.)
Goal: pick the right formula and plug in. No traps yet.
Recall Solution L1·Q1
What we use: the definition L=Iω. This is a definition, not a derivation — angular momentum of a symmetric rotor is just "spin-inertia times spin-rate". We want the magnitudeL, so we drop the arrows:
L=Iω=(0.8)(300)=240kg⋅m2/s.Direction: the vector L lies along the spin axis, sense given by the right-hand rule — curl the right-hand fingers the way the wheel turns, the thumb points along L.
Recall Solution L1·Q2
What we use: the magnitude form Ω=Lτ — derived in the intuition box above and boxed in the parent note. Both quantities here are magnitudes, so no arrows are needed.
Ω=0.50.002=0.004rad/s.
The axis drifts around a cone at 0.004 radians per second — very slow, which is exactly what a stable reference needs.
Goal: combine two definitions, or invert one to solve for an unknown.
Recall Solution L2·Q1
What we do: start from the magnitude form Ω=Iωτ and solve for ω. Why: the unknown is trapped in the denominator, so we rearrange to free it.
ω=IΩτ=(1×10−4)(5×10−4)1×10−3=5×10−81×10−3=2×104rad/s.
So ω=20,000rad/s (about 191,000 rpm — real precision gyros do spin this fast). A slower rotor would drift too quickly to trust.
Recall Solution L2·Q2
What we use: conservation of angular momentum (Conservation of Angular Momentum). Here we keep signs because direction is the whole question — a positive ω means one rotational sense, a negative ω the opposite sense (this is the 1-D signed shadow of the full vector statement L=0). The craft is isolated in vacuum and started at rest, so total angular momentum is 0forever:
Ibωb+Iwωw=0⇒ωw=−IwIbωb.ωw=−0.4(800)(0.015)=−0.412=−30rad/s.
The minus sign means opposite sense: to turn the body one way, spin the wheel the other way. The magnitude 30rad/s is large because the wheel is 2000× smaller in inertia.
Goal: reason about how competing quantities trade off; interpret, don't just compute.
Recall Solution L3·Q1
What we do: precession rate Ω=τ/(Iω), so with the sameτ, whoever has the larger spin magnitude L=Iω precesses less. Compute each L:
LA=(2×10−4)(5000)=1.0kg⋅m2/s,LB=(5×10−4)(3000)=1.5kg⋅m2/s.B has the larger L, so B precesses less. The factor:
ΩBΩA=τ/LBτ/LA=LALB=1.01.5=1.5.
Gyro A drifts 1.5 times faster than B, even though A spins faster — because B's larger inertia more than compensates. Read the product, not one variable.
Recall Solution L3·Q2
(a) Wheel torque. Torque is the rate of change of angular momentum (Torque and Newton's Second Law for Rotation): τ=IwΔtΔωw.
τwheel=0.4×630=0.4×5=2.0N⋅m.(b) Body torque. By Newton's third law for rotation, the reaction on the body is equal and opposite:
τbody=−τwheel=−2.0N⋅m.(c) Body angular acceleration. Using τbody=Ibαb:
αb=Ibτbody=800−2.0=−2.5×10−3rad/s2.
The body accelerates the opposite way — tiny, because it is so massive. After 6s its speed is ∣αb∣t=2.5×10−3×6=0.015rad/s, matching the conservation answer from L2·Q2. Two roads, same destination — a good consistency check.
(b) Direction — read it off the figure. The figure below is a top-down map of the horizontal plane: East is the +x^ axis, North is +y^. The teal arrow is L (spin axis, pointing East); the orange arrow is the applied torque τ (pointing North); the plum dashed arc shows the resulting sweep of the axis; and the small circled dot marks Ω pointing straight out of the page (upward). Use it to see that the axis does not tip over toward the push — it swings sideways in the horizontal plane.
Now confirm with the Cross Product relation τ=Ω×L. In a right-handed frame x^×y^=z^, y^×z^=x^, z^×x^=y^.
We guessΩ=Ωz^ (pointing up, out of the page) and test:
Ω×L=(Ωz^)×(Lx^)=ΩL(z^×x^)=ΩLy^.
That points along +y^ — exactly the direction of τ. ✓ So Ω=+Ωz^: the axis sweeps horizontally, turning from East toward North, tracing a cone about the vertical — precisely the plum arc in the figure.
Recall Solution L4·Q2
(a) Phase 1 body velocity. Total angular momentum is 0 throughout (started at rest, isolated):
ωb=−IbIwωw=−600(0.5)(+40)=−60020=−0.0333rad/s.
The minus sign means: since the wheel spins counter-clockwise (+), the body turns clockwise (−).
(b) After Phase 2. When the wheel returns to ωw=0, conservation forces Ibωb=0, so ωb=0. The body stops rotating. (Spinning the wheel back undoes the body's spin — this is how a craft stops slewing.)
(c) Net angle and direction. The body reorients during Phase 1 (it rotates at −0.0333rad/s), then holds still when the wheel is braked. The net turn is the Phase-1 rotation. With constant wheel acceleration the body's speed ramps linearly from 0 to −0.0333rad/s over 8s, so the average signed velocity is half the peak:
θb=21(−0.0333)(8)=−0.1333rad≈−7.6∘.
The negative sign is the physics: the craft has turned ≈7.6∘clockwise (the sense opposite the wheel), and now sits still, pointed at a new target. Spin wheel to turn, brake wheel to hold.
Goal: full engineering scenarios — saturation, unit reasoning, multi-formula design.
Recall Solution L5·Q1
(a) Time to saturate. The wheel must absorb momentum at rate τd, and its capacity is Lmax=Iwωmax:
Lmax=(0.6)(600)=360kg⋅m2/s.
Time = capacity ÷ fill-rate:
tsat=τdLmax=3×10−4360=1.2×106s≈13.9days.Why: the tiny disturbance drips angular momentum in; the wheel's finite capacity fills over about two weeks — then it can't help any more.
(b) Desaturation time. The thruster must remove all 360kg⋅m2/s at rate 0.05N⋅m:
tdesat=τthrusterLmax=0.05360=7200s=2hours.The lesson: the wheel handled steady disturbances silently for two weeks; only occasionally must a thruster dump the accumulated momentum externally. That's exactly the "desaturation" the parent note warns about.
Recall Solution L5·Q2
Step 1 — link drift angle to precession rate. During the observation the axis precesses at a steady rate Ω, so the accumulated angle is θ=Ωt. Why: angle = rate × time when the rate is constant.
Step 2 — express Ω from the precession formula. From the intuition box, Ω=Iωτ. Substitute:
θ=Ωt=Iωτt.Step 3 — impose the budgetθ≤θmax and solve for ω. Since ω sits in the denominator, a largerω makes θsmaller, so we need ωat least the value that makes θ exactly θmax:
ω≥Iθmaxτt=(3×10−5)(1×10−4)(2×10−6)(100)=3×10−92×10−4≈6.67×104rad/s.Answer: the rotor must spin at at least ≈6.67×104rad/s (about 66,700rad/s) to keep the star image steady enough for the whole 100s exposure. Every earlier idea appears at once: the precession rate Ω=τ/(Iω), drift-as-rate×time θ=Ωt, and design-by-inequality — this is exactly what an attitude-control engineer computes when sizing a gyro.
Recall One-line summary of every formula used here
Spin momentum L=Iω, magnitude L=Iω ::: along the axis, right-hand rule.
Precession rate Ω=τ/(Iω) ::: bigger spin → slower drift.
Vector precession τ=Ω×L ::: axis sweeps perpendicular to the push.
Reaction wheel Ibωb=−Iwωw ::: spin wheel one way, body turns the other.
Torque τ=IΔω/Δt ::: rate of change of angular momentum.
Drift angle θ=Ωt ::: steady-rate precession over an interval.
Saturation Lmax=Iwωmax ::: finite momentum store.