Before the numbers, one picture to fix the geometry in your head.
The blue arrow is v1 (before), the orange arrow is v2 (after) — same length v, rotated by Δi. The red arrow is Δv=v2−v1: the burn you must perform. Notice how the red arrow is the base of an isosceles triangle whose two equal sides are v.
Δv = the magnitude of the required burn (a change in the velocity vector, measured in m/s or km/s).
v = the orbital speed, which is the same before and after (a pure plane change keeps speed fixed).
Δi = the angle you rotate the velocity vector through = the change in inclination.
The half comes from geometry: drop a perpendicular from the triangle's apex (angle Δi) to the base Δv. It bisects the apex into Δi/2 and cuts the base in half. Each half-base is vsin(Δi/2), so the whole base is 2vsin(Δi/2).
Recall Solution L1.2
Since Δv=2vsin(Δi/2) and Δi is the same for both, Δv is directly proportional to v. So satellite A (faster) pays more. The ratio is exactly the speed ratio:
ΔvBΔvA=vBvA=3.17.7≈2.48.
A pays about 2.5× as much. (This is the reason to do plane changes where you are slow.)
Recall Solution L1.3
(a) Δi=0°: Δv=2vsin(0°)=0. No rotation, no burn — obvious.
(b) Δi=180°: Δv=2vsin(90°)=2v. You must fully reverse direction: kill your speed v, then build v the opposite way, total 2v. The formula captures this exactly.
Half-angle: Δi/2=5°. Then sin5°≈0.08716.
Δv=2(7.7)(0.08716)≈1.342 km/s=1342 m/s.
A mere 10° costs over 1.3 km/s — nearly a fifth of the orbital speed itself.
Recall Solution L2.2
Rearrange Δv=2vsin(Δi/2) for Δi. First isolate the sine:
sin(2Δi)=2vΔv=2(7.7)0.200=15.40.200=0.012987.Why arcsin? We know the sine of the half-angle and want the angle back — arcsin is the operation that undoes sine. Since 0.012987 is tiny, the angle is tiny (and positive), so no quadrant ambiguity:
2Δi=arcsin(0.012987)=0.012987 rad⇒Δi=0.025974 rad.
Convert to degrees: 0.025974×π180≈1.488°.
So the biggest change is about 1.49° — showing how stingy plane changes are with a small budget.
Recall Solution L2.3
First, unify units. The formula mixes Δv and v, so both must be in the same unit. Convert the budget Δv=400 m/s =0.400 km/s (divide by 1000), and we'll get v out in km/s.
Rearrange for v: v=2sin(Δi/2)Δv.
Half-angle Δi/2=10°, sin10°≈0.17365.
v=2(0.17365)0.400 km/s=0.347300.400≈1.152 km/s.
You must be crawling at about 1.15 km/s — the kind of speed you only reach at apoapsis of a high ellipse. Use vis-viva to find where that speed occurs.
Set Δv=v: 2vsin(Δi/2)=v⇒sin(Δi/2)=0.5⇒Δi/2=30°⇒Δi=60°.
Set Δv=2v: sin(Δi/2)=1⇒Δi/2=90°⇒Δi=180°.
So the burn first equals the whole orbital speed at exactly Δi=60°, and reaches its maximum2v only at the full reversal Δi=180°. Because sin(Δi/2) never exceeds 1 on 0°–180°, Δv=2vsin(Δi/2)never exceeds 2v — it is capped at 2v. The function is monotonically increasing on 0° to 180° (the sine of the half-angle rises steadily from 0 to 1), so bigger tilt always costs more, up to that hard ceiling of 2v. The lesson: once Δi>60° a single plane change costs more than an entire orbit's worth of speed, so engineers split large changes across slow orbit points instead.
Recall Solution L3.2
Why a derivative? We want the rated(Δv)/d(Δi) — "how much does the cost change per unit angle" — and the derivative is exactly the tool that answers "rate of change of one quantity with respect to another."
d(Δi)d[2vsin(Δi/2)]=2v⋅21cos(Δi/2)=vcos(Δi/2).
At small Δi, cos(Δi/2)≈1, so the slope ≈v=7.7 km/s per radian. Convert to per degree by multiplying by π/180≈0.01745:
7.7×0.01745≈0.1344 km/s per degree=134 m/s per degree.
Every extra degree near zero costs about 134 m/s in LEO. (Matches the parent note's 2°-GPS example scaled by speed.)
Recall Solution L3.3
Look at the figure again: the red arrow Δv is the base of an isosceles triangle. The angle between v1 and Δv equals 90°+Δi/2 measured on that triangle — i.e. the burn points almost exactly perpendicular to the velocity (it tips slightly backward by Δi/2). For an infinitesimally small change (Δi→0) the burn is purely sideways (normal to v), which makes sense: a sideways nudge rotates a vector without changing its length to first order. The sign (left vs right / north vs south) sets whether inclination increases or decreases.
Combined (law of cosines, two different sides at angle Δi):
Δvcomb=v12+v22−2v1v2cosΔi.
With cos28°≈0.88295:
Δvcomb=1.62+3.12−2(1.6)(3.1)(0.88295)=2.56+9.61−8.7589=3.4111≈1.847 km/s.Separate = speed change first, then a pure plane change at the new speed v2=3.1:
Δvsep=speed(3.1−1.6)+plane2(3.1)sin14°=1.5+6.2(0.24192)=1.5+1.500=3.000 km/s.
Combined (1.85 km/s) beats separate (3.00 km/s) by over a km/s — the triangle inequality in action: one straight step is shorter than two legs of a bent path. This is why Hohmann transfers fold the plane change into the apogee burn.
Recall Solution L4.2
One shot: Δv=2(7.7)sin20°=15.4(0.34202)≈5.267 km/s.
Split into two 20° burns: each costs 2(7.7)sin10°=15.4(0.17365)≈2.674 km/s, total 2×2.674=5.348 km/s.
Splitting at the same speed is slightly worse (5.35>5.27): each small chord is shorter, but two chords sum to more than the single larger chord (again the triangle inequality, now the other way). Splitting only helps if you do the sub-burns where v is smaller — the real saving comes from lower speed, not from subdividing the angle.
Recall Solution L4.3
Why Tsiolkovsky? It's the tool that turns a required Δv into a mass ratio. See Tsiolkovsky rocket equation.
mfm0=eΔv/ve=e1.342/3.0=e0.44733≈1.5641.
Propellant fraction =1−m0mf=1−1.56411=1−0.6393=0.3607.
About 36% of the spacecraft's mass is burned as fuel — for a single 10° tilt. Plane changes are ruinous.
(a) Combined burn. Two sides va=1.60, vGEO=3.07, included angle 27°, cos27°≈0.89101:
Δv=1.602+3.072−2(1.60)(3.07)(0.89101)=2.5600+9.4249−8.7526=3.2323≈1.798 km/s.
(b) Separate burns. Circularize: ∣3.07−1.60∣=1.47 km/s. Then a pure plane change at the GEO speed 3.07: 2(3.07)sin13.5°=6.14(0.23345)=1.433 km/s. Total:
Δvsep=1.47+1.433=2.903 km/s.
Combining saves 2.903−1.798=1.105 km/s — a huge margin.
(c) Propellant fraction (combined). Use Tsiolkovsky with Δv=1.798 km/s and ve=3.1 km/s:
mfm0=e1.798/3.1=e0.58000≈1.7860,fraction=1−1.78601=1−0.5599=0.4401.
About 44% of the mass is propellant with the combined burn. For comparison, the separate strategy (Δv=2.903 km/s) gives mfm0=e2.903/3.1=e0.93645≈2.551, a fraction 1−1/2.551=0.6081, i.e. about 61% — far worse.
(d) Design lesson. Do the plane change (i) at the slowest point — apogee, where v is smallest — and (ii) combined with the circularization burn, exploiting the law-of-cosines triangle. Both tricks stack to slash the propellant bill from ~61% to ~44%. That is why real GEO missions fold the inclination removal into the apogee kick.
Recall Solution L5.2
Separate cost, as a function of Δi:
Δvsep(Δi)=∣vGEO−va∣+2vGEOsin(Δi/2)=1.47+6.14sin(Δi/2).
Combined cost:
Δvcomb(Δi)=1.602+3.072−2(1.60)(3.07)cosΔi=11.9849−9.8248cosΔi.
At Δi=0: combined =∣3.07−1.60∣=1.47, separate =1.47 — equal (as they must, no plane change). For allΔi>0 the combined value is strictly below separate (triangle inequality), so combining is always at least as cheap and strictly cheaper whenever Δi>0.
Numerical check at Δi=27°: combined =11.9849−9.8248(0.89101)=11.9849−8.7538=3.2311≈1.797 km/s vs separate 1.47+6.14(0.23345)=2.903 km/s. So there is no break-even where separate wins — combining dominates for every Δi>0, and the two are equal only at the trivial Δi=0.
Speed change from 2° tilt at 7.7 km/s? ::: ≈269 m/s (using 2⋅7.7⋅sin1°)
Largest Δi for a 200 m/s budget at 7.7 km/s? ::: ≈1.49°Δv per degree near zero at 7.7 km/s? ::: ≈134 m/s per degree
Combined burn formula? ::: Δv=v12+v22−2v1v2cosΔi
Why does combining always win for Δi>0? ::: triangle inequality — one vector leg is shorter than two sequential legs