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In a standard polar conic, e<1 gives an ellipse, e=1 a parabola, and e>1 a hyperbola.
Worked example 1
Classify r=1+0.5cosθ2.
r=1+0.5cosθ2; e=0.5
e<1⟹ Ellipse
Answer: Ellipse
Worked example 2
Classify r=1+1cosθ3.
r=1+1cosθ3; e=1
e=1⟹ Parabola
Answer: Parabola
Idea 2 of 3
Focus and directrix
The numerator in r=1±ecosθed is ed, not d alone. Recover the directrix distance by dividing by e.
Worked example 1
For r=1+0.5cosθ2, find the positive distance from the focus to the directrix.
ed=2; e=0.5
d=0.52=4
Answer:4
Worked example 2
For r=1+1cosθ3, find the positive distance from the focus to the directrix.
ed=3; e=1
d=13=3
Answer:3
Idea 3 of 3
Kepler’s Laws
For bodies orbiting the same central mass, a3T2 is constant, where a is semimajor axis. Equal areas are swept in equal times.
Worked example 1
Two planets orbit the same star. Planet A has semimajor axis 1 and period 1. Planet B has semimajor axis 2. Find its period.
a3T2=1312=1
TB2=23=8
TB=8=8≈2.83
Answer:8≈2.83
Worked example 2
Two planets orbit the same star. Planet A has semimajor axis 1 and period 1. Planet B has semimajor axis 3. Find its period squared.
a3T2=1312=1
TB2=33=27
TB2=27
Answer:27
Resource alignment: Larson & Edwards, Calculus of a Single Variable, Tenth Edition, §10.6,p. 734. Explanations, diagrams and numerical practice variants are original MathLab content aligned to this section.