Satellites: Orbits and Energy — Question 3

Section 13-7 · Physics pages 2016–2017

Question 3 A tangential speed increase creates an ellipse rather than an immediate larger circle A satellite initially has circular speed vc = √ µ/r at radius r. A short prograde burn increases its speed to 1.2vc without changing position. Use specific energy ϵ = v2/2 −µ/r = −µ/(2a) for a bound ellipse. R r 1.2vc Spherical central body; radii are measured from its center. (a) Find the new semimajor axis and apoapsis radius. (b) Identify the burn point as periapsis and determine the speed-factor threshold for escape.
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Question 3 - Solution A tangential speed increase creates an ellipse rather than an immediate larger circle R r 1.2vc (a) Derivation and calculation Immediately after the burn, v′ = 1.2 √ µ/r, ϵ = v′2 2 −µ r = (.72 −1)µ r = −.28µ r . Hence a = −µ 2ϵ = 25r 14 . The tangential burn leaves ˙r = 0 and increases speed above circular, making this periapsis: ra = 2a −r = 18r 7 . (b) Result and interpretation The radial-coordinate acceleration verifies a local radius minimum: ¨r = v′2 r −µ r2 = (1.44 −1) µ r2 > 0. For a tangential speed kvc, ϵ = ( k2 2 −1 ) µ r . kescape = √ 2 ; k < √ 2 is bound, k > √ 2 is unbound. Physical check The new apoapsis exceeds the burn radius and the energy remains negative for k = 1.2.

Question 3

A tangential speed increase creates an ellipse rather than an immediate larger circle

A satellite initially has circular speed vc=μ/rv_c=\sqrt{\mu/r} at radius rr. A short prograde burn increases its speed to 1.2vc1.2v_c without changing position. Use specific energy ϵ=v2/2−μ/r=−μ/(2a)\epsilon=v^2/2-\mu/r=-\mu/(2a) for a bound ellipse.

Diagram shown in the original SVG worksheet.

  1. Find the new semimajor axis and apoapsis radius.

  2. Identify the burn point as periapsis and determine the speed-factor threshold for escape.

Question 3 - Solution

A tangential speed increase creates an ellipse rather than an immediate larger circle

Diagram shown in the original SVG worksheet.

(a) Derivation and calculation

Immediately after the burn, v′=1.2μ/r,ϵ=v′22−μr=(.72−1)μr=−.28μr.v'=1.2\sqrt{\mu/r},\quad \epsilon=\frac{v'^2}{2}-\frac\mu r=(.72-1)\frac\mu r=-.28\frac\mu r. Hence a=−μ2ϵ=25r14.\boxed{a=-\frac\mu{2\epsilon}=\frac{25r}{14}}. The tangential burn leaves ṙ=0\dot r=0 and increases speed above circular, making this periapsis: ra=2a−r=18r7.\boxed{r_a=2a-r=\frac{18r}{7}}.

(b) Result and interpretation

The radial-coordinate acceleration verifies a local radius minimum: r̈=v′2r−μr2=(1.44−1)μr2>0.\ddot r=\frac{v'^2}{r}-\frac\mu{r^2} =(1.44-1)\frac\mu{r^2}>0. For a tangential speed kvckv_c, ϵ=(k22−1)μr.\epsilon=\left(\frac{k^2}{2}-1\right)\frac\mu r. kescape=2;k<2 is bound,k>2 is unbound.\boxed{k_{\mathrm{escape}}=\sqrt2};\qquad k<\sqrt2\text{ is bound},\quad k>\sqrt2\text{ is unbound}.

Physical check

The new apoapsis exceeds the burn radius and the energy remains negative for k=1.2k=1.2.