Satellites: Orbits and Energy — Question 10

Section 13-7 · Physics pages 2030–2031

Question 10 An effective-potential graph separates radial turning points from zero speed A satellite has specific angular momentum h2 = µr0 and energy ϵ = −µ/(4r0). Use ˙r2/2 + Veff(r) = ϵ, where Veff = h2/(2r2) −µ/r. r/r0 Veff/(µ/r0) ϵ −1/2 −1/4 1 The dashed energy level intersects the effective potential at both radial turning points. (a) Find the two radial turning points and the allowed radial interval. (b) At a turning point, is the satellite at rest? Locate the stable circular radius for this fixed h.
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Question 10 - Solution An effective-potential graph separates radial turning points from zero speed r/r0 Veff/(µ/r0) ϵ −1/2 −1/4 1 (a) Derivation and calculation At a radial turning point, ˙r = 0. Set x = r/r0: r0Veff µ = 1 2x2 −1 x = −1 4. Multiplication by 4x2 gives x2 −4x + 2 = 0, hence r± = (2 ± √ 2)r0 . The radial kinetic energy is nonnegative only for r−≤r ≤r+ . (b) Result and interpretation At either turning point, ˙r = 0 but vt = h/r̸ = 0. For a circular orbit at fixed h, V ′ eff= −h2 r3 + µ r2 = 0 =⇒ rc = h2/µ = r0 . Vmin = −µ 2r0 , V ′′ eff(r0) = µ r3 0 > 0. The minimum is radially stable, and the given higher energy produces two distinct turning points. Physical check The energy lies between the negative minimum and zero, consistent with a bound noncircular orbit.

Question 10

An effective-potential graph separates radial turning points from zero speed

A satellite has specific angular momentum h2=μr0h^2=\mu r_0 and energy ϵ=−μ/(4r0)\epsilon=-\mu/(4r_0). Use ṙ2/2+Veff(r)=ϵ\dot r^2/2+V_{eff}(r)=\epsilon, where Veff=h2/(2r2)−μ/rV_{eff}=h^2/(2r^2)-\mu/r.

Diagram shown in the original SVG worksheet.

  1. Find the two radial turning points and the allowed radial interval.

  2. At a turning point, is the satellite at rest? Locate the stable circular radius for this fixed hh.

Question 10 - Solution

An effective-potential graph separates radial turning points from zero speed

Diagram shown in the original SVG worksheet.

(a) Derivation and calculation

At a radial turning point, ṙ=0\dot r=0. Set x=r/r0x=r/r_0: r0Veffμ=12x2−1x=−14.\frac{r_0V_{\mathrm{eff}}}\mu=\frac1{2x^2}-\frac1x=-\frac14. Multiplication by 4x24x^2 gives x2−4x+2=0x^2-4x+2=0, hence r±=(2±2)r0.\boxed{r_\pm=(2\pm\sqrt2)r_0}. The radial kinetic energy is nonnegative only for r−≤r≤r+.\boxed{r_-\le r\le r_+}.

(b) Result and interpretation

At either turning point, ṙ=0\dot r=0 but vt=h/r≠0v_t=h/r\ne0. For a circular orbit at fixed hh, Veff′=−h2r3+μr2=0⇒rc=h2/μ=r0.V'_{\mathrm{eff}}=-\frac{h^2}{r^3}+\frac\mu{r^2}=0 \quad\Longrightarrow\quad\boxed{r_c=h^2/\mu=r_0}. Vmin=−μ2r0,Veff″(r0)=μr03>0.V_{\mathrm{min}}=-\frac\mu{2r_0},\qquad V''_{\mathrm{eff}}(r_0)=\frac\mu{r_0^3}>0. The minimum is radially stable, and the given higher energy produces two distinct turning points.

Physical check

The energy lies between the negative minimum and zero, consistent with a bound noncircular orbit.