Satellites: Orbits and Energy — Question 4

Section 13-7 · Physics pages 2018–2019

Question 4 A radial impulse changes energy while preserving angular momentum A satellite in a circular orbit of radius r and speed vc = √ µ/r receives an outward radial velocity increment u = .5vc. Its transverse speed stays vc. Use ϵ = −µ/(2a) and e2 = 1 + 2ϵh2/µ2, where h = rvt. R r u vc Spherical central body; radii are measured from its center. (a) Find its new a and e. (b) Find both apsis radii and explain why the burn point is not an apsis.
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Question 4 - Solution A radial impulse changes energy while preserving angular momentum R r u vc (a) Derivation and calculation The radial impulse is perpendicular to the original velocity: v′2 = v2 c + u2 = 1.25µ r , ϵ = v′2 2 −µ r = −3µ 8r . Thus a = 4r 3 , h2 = (rvc)2 = µr, e2 = 1 + 2ϵh2 µ2 = 1 −3 4, e = 1 2 . (b) Result and interpretation The new apsides are rp = a(1 −e) = 2r 3 , ra = a(1 + e) = 2r . The burn radius lies strictly between them because ˙r = u̸ = 0. The angular-momentum change is ∆⃗h =⃗r × (uˆr) =⃗0, while the specific energy increases by u2/2. Physical check The radial impulse preserves angular momentum but cannot leave a circular orbit when the radial speed is nonzero.

Question 4

A radial impulse changes energy while preserving angular momentum

A satellite in a circular orbit of radius rr and speed vc=μ/rv_c=\sqrt{\mu/r} receives an outward radial velocity increment u=.5vcu=.5v_c. Its transverse speed stays vcv_c. Use ϵ=−μ/(2a)\epsilon=-\mu/(2a) and e2=1+2ϵh2/μ2e^2=1+2\epsilon h^2/\mu^2, where h=rvth=rv_t.

Diagram shown in the original SVG worksheet.

  1. Find its new aa and ee.

  2. Find both apsis radii and explain why the burn point is not an apsis.

Question 4 - Solution

A radial impulse changes energy while preserving angular momentum

Diagram shown in the original SVG worksheet.

(a) Derivation and calculation

The radial impulse is perpendicular to the original velocity: v′2=vc2+u2=1.25μr,ϵ=v′22−μr=−3μ8r.v'^2=v_c^2+u^2=1.25\frac\mu r,\qquad \epsilon=\frac{v'^2}{2}-\frac\mu r=-\frac{3\mu}{8r}. Thus a=4r3,h2=(rvc)2=μr,\boxed{a=\frac{4r}{3}},\qquad h^2=(rv_c)^2=\mu r, e2=1+2ϵh2μ2=1−34,e=12.e^2=1+\frac{2\epsilon h^2}{\mu^2}=1-\frac34, \qquad\boxed{e=\frac12}.

(b) Result and interpretation

The new apsides are rp=a(1−e)=2r3,ra=a(1+e)=2r.\boxed{r_p=a(1-e)=\frac{2r}{3}},\qquad \boxed{r_a=a(1+e)=2r}. The burn radius lies strictly between them because ṙ=u≠0\dot r=u\ne0. The angular-momentum change is Δh→=r→×(ur̂)=0→,\Delta\vec h=\vec r\times(u\hat r)=\vec0, while the specific energy increases by u2/2u^2/2.

Physical check

The radial impulse preserves angular momentum but cannot leave a circular orbit when the radial speed is nonzero.