3.2.6 · D4Orbital Mechanics & Astrodynamics

Exercises — Kepler's second law — equal areas in equal times, from angular momentum conservation

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This is the workout page for Kepler's Second Law. Each problem is graded from L1 (just recognise it) up to L5 (master everything at once). Try each one before opening its solution.

Everything on this page rests on the two facts you already built in the parent note:

Here is the radius vector from Sun to planet, its velocity, the planet's mass, the angular momentum, the angle between and , the swept area, and the polar angle. If any of those symbols feels shaky, re-read the parent note first.


Level 1 — Recognition

Problem 1.1

State, in one sentence each: (a) what quantity Kepler's second law says is constant, and (b) the physical reason it is constant.

Recall Solution

(a) The areal velocity — the area swept by the radius vector per unit time — is constant. (b) Gravity is a central force (), so it exerts zero torque about the Sun; zero torque means angular momentum is conserved, and is constant because and are both constant.

Problem 1.2

A planet is at perihelion (closest point) and later at aphelion (farthest point). At which point is it moving faster? At which point is the swept-area rate larger?

Recall Solution

Faster at perihelion. Because is fixed, a small forces a large angular rate , hence a large speed. The swept-area rate is the SAME at both points — that is the whole content of the law. Do not confuse "faster" (speed, which differs) with "area per second" (which is equal everywhere).


Level 2 — Application

Problem 2.1

Mercury has and . Its perihelion speed is . Find its aphelion speed .

Recall Solution

Both points are apsides, so and at each. Conservation of gives Why this step? Only at apsides can we drop the factor and write directly.

Problem 2.2

A comet's angular momentum per unit mass is . What area does its radius vector sweep in exactly one hour?

Recall Solution

Areal velocity is . One hour , and because is constant, area rate time: Why no integral? Constant rate means the total is just rate times elapsed time — the same reason distance speed time when speed is constant.


Level 3 — Analysis

Problem 3.1

At a certain instant a probe is at distance from the Sun, moving at speed , with the angle between and equal to . Compute its areal velocity .

Look at the figure: the shaded triangle is the tiny slice swept in time ; its "height" is the component of the displacement perpendicular to , which is why appears.

Figure — Kepler's second law — equal areas in equal times, from angular momentum conservation
Recall Solution

The magnitude of the cross product is . So With : Why and not ? The cross product measures the perpendicular piece of the two vectors — the part of that actually swings the radius vector sideways and paints area. The parallel part just lengthens/shortens and paints nothing.

Problem 3.2

Show that at the two apsides of an ellipse the speeds obey , and hence that the ratio of kinetic energies at peri- vs aphelion is .

Recall Solution

Speeds: at apsides , so , giving . Kinetic energies: , so Why square it? Kinetic energy scales with the square of speed, so any speed ratio becomes a squared ratio in energy.


Level 4 — Synthesis

Problem 4.1

Earth's orbit has semi-major axis , eccentricity , and period . The semi-minor axis is . (a) Find the total ellipse area . (b) Use to find Earth's specific angular momentum .

Recall Solution

(a) First . (b) Over one full period the radius vector sweeps the entire ellipse once, so . Solve for : Why this works: is constant, so integrating it over one orbit just multiplies by — the swept area equals the whole ellipse because the planet returns to start exactly once per period.

Problem 4.2

A satellite is in an elliptical orbit. At perihelion its speed is and . What is its speed when it is at a point where and the angle between and is ? (Use only the second law — angular momentum conservation.)

Recall Solution

Angular momentum is conserved everywhere, so at perihelion at the new point: Why: at perihelion so ; at the general point . Set equal (mass cancels). So .


Level 5 — Mastery

Problem 5.1

A comet is observed at two times. At time 1: , and it sweeps out area at some rate. At time 2 (aphelion): , speed . (a) Find the comet's areal velocity . (b) Using that constant areal velocity, find the comet's tangential speed component at position 1 (the component of perpendicular to ). (c) If the total speed at position 1 is measured to be , find the angle between and .

Look at the decomposition figure: at any point the velocity splits into a radial part (along , sweeps no area) and a tangential part (perpendicular to , does all the sweeping).

Figure — Kepler's second law — equal areas in equal times, from angular momentum conservation
Recall Solution

(a) Position 2 is aphelion, an apsis, so and (b) Areal velocity is constant, and in general (only the perpendicular part paints area). At position 1: Why and not ? Area is swept only by the sideways swing of the radius vector; that is exactly the perpendicular velocity component. (c) The perpendicular component is , so Sanity check: means the comet still has a radial velocity component — it is moving inward or outward, not at an apsis, which is consistent with being between perihelion and aphelion.

Problem 5.2

Prove that for any central force (not just gravity) the areal velocity is constant, and explain in one line why the shape of the orbit is not determined by this law alone.

Recall Solution

A central force means for some function — it always points along . Then the torque about the centre is because and are parallel (, and any vector crossed with itself is zero). Zero torque gives , so , hence .

Why the shape isn't fixed: The second law used only that points radially — it never used the form of . Different radial laws ( gravity, spring, etc.) give different orbit shapes; the ellipse-with-Sun-at-focus specifically requires the inverse-square law (that is Kepler's First Law (Ellipse)). Equal areas is universal; the ellipse is special.


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