Aisha is correct: the Laplace SOI carries the ==2/5 power== of the mass ratio, the fingerprint of a tidal perturbation.
Ben's 1/2 power is the force-equality point req=Rq1/2 — where the planet's raw pull equals the Sun's raw pull. It is a different (smaller) radius and is not the SOI.
Mnemonic: "Tides are two-fifths."
Recall Solution L1.2
R = distance between the two large bodies (e.g. planet ↔ Sun).
m = mass of the smaller body — the one whose bubble we compute.
M = mass of the larger central body.
Always m≪M, so q=m/M<1 and q2/5<1, making rSOI<R as it must be (the bubble sits well inside the separation).
Step 1 — the mass ratio: q=1.989×10305.97×1024=3.00×10−6.
Step 2 — raise to 2/5using logs (recall: log turns the power into a multiply). log10q=−5.523; times 0.4 gives −2.209; so q0.4=10−2.209=6.18×10−3.
Step 3 — multiply by R:
rSOI=1.496×1011×6.18×10−3≈9.2×108 m≈924,000 km.
That's about 145 Earth radii.
Recall Solution L2.2
q=6.42×1023/1.989×1030=3.228×10−7.
log10q=−6.491; ×0.4=−2.596; q0.4=10−2.596=2.535×10−3.
rSOI=2.279×1011×2.535×10−3≈5.78×108 m≈578,000 km.
Smaller than Earth's despite Mars being farther out, because Mars is much lighter — the mass ratio wins over the distance.
Force-equality uses the 1/2 power:
req=Rq=2.279×1011×3.228×10−7.3.228×10−7=5.681×10−4, so req=2.279×1011×5.681×10−4=1.295×108 m ≈ 129,500 km.
Ratio: rSOI/req=5.78×108/1.295×108≈4.46.
The SOI is about 4.5× larger than the force-balance point — because the tidal criterion (2/5 power on the small q) beats the raw-force criterion (1/2 power).
Recall Solution L3.2
rSOI∝q2/5∝m2/5. Doubling m multiplies the radius by
22/5=20.4=1.320.
So the SOI grows by about 32%, not 100%. The 2/5 power tames the mass change — a big lever on mass gives a modest lever on the bubble. This softness is the same tidal 2/5 we pictured at the top.
Recall Solution L3.3
(1/2)1/5=2−0.2=0.8706. Applying it to L2.1's 924,000 km:
924,000×0.8706≈804,000 km.
A ~13% reduction. It comes from the factor 2 in the tidal derivative dRd(R2GM)=−R32GM. Being close to 1, convention drops it.
We are patching between an Earth-centred orbit and a Moon-centred orbit, so the SOI uses the Moon–Earth pair.
q=7.35×1022/5.97×1024=0.01231.
log10q=−1.9097; ×0.4=−0.7639; q0.4=10−0.7639=0.1722.
rSOI=3.84×108×0.1722≈6.61×107 m≈66,000 km.
A spacecraft closer than ~66,000 km to the Moon is best treated as orbiting the Moon; farther, as orbiting the Earth. This connects directly to the Patched Conic Approximation and to planning a Gravity Assist / Flyby.
Recall Solution L4.2
Rearrange rSOI=Rq2/5 for q:
q=(RrSOI)5/2.Why the 5/2 power? Undoing q2/5 means raising to the reciprocal 5/2.
R=5×1.496×1011=7.48×1011 m. Ratio rSOI/R=4.82×1010/7.48×1011=0.06444.
q=0.064442.5. log100.06444=−1.1908; ×2.5=−2.977; q=10−2.977=1.055×10−3.
m=qM=1.055×10−3×1.989×1030≈2.10×1027 kg.
That's roughly a Jupiter-mass planet.
The nested-sphere figure below makes this visual. The Moon sits 384,000 km from Earth; its bubble extends ±66,000 km, so it spans roughly 318,000 – 450,000 km from Earth. Earth's own SOI reaches 924,000 km. Since 450,000<924,000, the entire Moon SOI is nested inside Earth's SOI.
Meaning: a craft near the Moon is inside two nested bubbles. We patch conics in stages — Sun→Earth→Moon — a hierarchy the Restricted Three-Body Problem and Hill Sphere treatments make precise. The Patched Conic Approximation handles each handoff as a fresh Two-Body Problem.
Recall Solution L5.2
Hill: q/3=3.00×10−6/3=1.00×10−6; cube root =(10−6)1/3=10−2=0.01.
rH=1.496×1011×0.01=1.496×109 m≈1.50×106 km.
The Hill sphere (~1.5 million km) is larger than the SOI (~924,000 km). They answer different questions: the SOI asks "where do I switch which body I orbit for trajectory accuracy?" (a 2/5 tidal-ratio law), while the Hill Sphere asks "where can a moon stay gravitationally bound against the Sun?" (a 1/3 centrifugal-balance law in the Restricted Three-Body Problem). Different physics ⇒ different exponent ⇒ different radius. The figure below stacks the three radii to scale.
Recall Solution L5.3
Inside the SOI, Tidal Forces from the Sun are, by construction, a negligible perturbation relative to Mars's pull — so Mars's gravity alone bends the probe on a clean two-body hyperbola. Outside, Mars's pull is the negligible perturbation and the Sun dominates, so the probe follows a heliocentric conic. The SOI boundary is exactly the surface where these two "which-is-the-perturbation" verdicts flip (Laplace's equal-ratio condition). Patching the two conics at that surface — matching position and velocity — gives the flyby's net velocity change with minimal error. That is the whole point of the Patched Conic Approximation.
Recall Quick self-check summary
Forward: rSOI=Rq2/5. ::: Compute q=m/M first, then q2/5, then ×R.
Invert for mass ratio: q=(rSOI/R)5/2. ::: Reciprocal power 5/2 undoes 2/5.
Mass ×2⇒ SOI ×? ::: 22/5≈1.32 (32% bigger).
Force-equality radius? ::: req=Rq1/2 — a raw force balance, smaller than the SOI.
SOI vs Hill for Earth: ::: SOI ≈ 0.92 Mkm, Hill ≈ 1.5 Mkm — different exponents, different questions.
When does rSOI=Rq2/5 break? ::: When q→1 or the orbit is very eccentric — use the full three-body treatment.