1. Replace constant gravity when the distance changes greatly
The gravity and circular-orbit workshop finds speed from an inward-force equation. Here the question changes: how far can an object climb, and can it escape? An energy balance connects two positions without solving for the travel time. Review work and energy first if choosing a system is unfamiliar.
Model: a fixed, nonrotating planet has spherically symmetric mass, radius R and gravitational parameter , where G is the gravitational constant and M is the planet's mass. The moving object's mass m is negligible compared with the planet's mass. Work only outside the planet, , where r is distance from its centre and altitude is . Neglect atmosphere and other bodies. After a launch, there is no thrust. These are idealized mechanics exercises, not spacecraft flight plans.
The gravitational-force magnitude is . Taking increasing r as outward gives the signed radial component . Choose potential energy zero at infinite separation:
The potential energy increases by as separation grows from r to infinity; that increase can come from initial kinetic energy or external work. The negative sign of U does not mean a negative force magnitude or a negative speed. Potential energy belongs to their interaction. With gravity as the only force doing work, E is conserved. If another force does work, include its work instead of claiming conservation.
Calculus check: , which recovers the inward force. Equivalently, the work by gravity from to is . For an outward move, gravity does negative work and potential energy increases.
Near a starting radius r, a small outward displacement gives the exact change . The approximation , with , follows only when . Using a fixed surface value of g over a planet-sized climb overestimates the required energy.
Use one set of units: has units ; has units . The specific mechanical energy is convenient because the nonzero test mass cancels. It is energy per kilogram, not force per kilogram.
2. Worked example: where does a radial launch stop rising?
Use a hypothetical planet with and . An object starts at , moving radially outward at . Find its greatest radius and altitude before it returns.
First calculate energy per kilogram, keeping the potential term negative:
Because the motion is radial, the entire speed is zero at the outer turning point. Conservation then gives , so
The maximum altitude is . The object rises by , a different distance. Check: its potential energy per kilogram increases from −16 million to −8 million J/kg, exactly matching the 8 million J/kg of kinetic energy lost.
Zero speed at the top does not mean equilibrium. Gravity still points inward, so the object begins returning. Our calculation stops at the planet's surface on its return; the exterior model is not a description of motion through the planet.
Do not transfer the zero-speed step to an arbitrary orbit. At the farthest point of a nonradial bound orbit, radial speed is zero but tangential speed generally is not. The same 4000 m/s directed tangentially at this starting radius gives a circular orbit instead. Energy alone does not determine the trajectory; direction and angular momentum matter.
3. Worked example: escape is an energy threshold
At the same starting radius, find the ideal minimum escape speed. Then find the limiting speed far away if the object launches radially outward at 6000 m/s.
At the threshold, the object can approach infinite separation with speed approaching zero. Because , its total energy is zero. Setting the initial specific energy to zero gives
This threshold is independent of the test mass, under our assumptions. For 6000 m/s, the initial specific energy is . At infinity, potential energy approaches zero, leaving
Check directly: . Do not subtract the two speeds; subtract their squared contributions in the energy equation. No finite outer turning radius exists for these outward radial launches with . At the exact threshold the object keeps moving outward at every finite radius and slows toward zero only asymptotically; it does not reach infinity in a finite time.
Negative energy means the separation has an upper bound, not that a safe satellite orbit is guaranteed. A radial launch can return into the planet. For nonnegative energy, an outward collision-free trajectory is needed to escape; an inward launch may hit the surface first. Escape also does not mean gravity switches off at some altitude.
4. Worked example: a higher circular orbit has more energy but less speed
Compare a 250 kg satellite in two possible circular orbits around the same planet: and . For circular motion only, the inward-force equation gives . Substitute into kinetic and total energy:
In the lower orbit, , and . In the higher orbit these values are respectively , and .
The higher state has 1 billion joules more total energy, despite having 1 billion joules less kinetic energy. Its potential energy increased by 2 billion joules. Its circular speed is about 2828 m/s rather than 4000 m/s. Comparing only speeds misses the larger potential-energy change.
This is a comparison of two states, not a maneuver plan or fuel calculation. An engine burn initially changes velocity at the satellite's current position. The circular-speed formula does not describe every point of the transfer trajectory, and the net mechanical-energy difference alone does not specify thrust, fuel, or timing.
5. Six problems with progressively less guidance
Use the same hypothetical planet unless the question says otherwise. Attempt each problem before revealing its solution. State whether you are comparing positions, following a radial launch, or comparing circular states.
1. Guided: lift without changing endpoint speed
An external device moves a 100 kg object from rest at to rest at . Find the net work by the device, with no losses. Why is not exact?
Hint 1
The endpoint kinetic energies are equal. Find the change in the negative potential energy.
Explained solution 1
The device supplies . Gravity does the opposite work. A constant surface-gravity estimate gives , twice the exact result. Gravity becomes weaker during the outward motion; this displacement is not small compared with the starting radius.
2. Diagnose: negative does not mean decreasing
A student writes, “At , million J/kg. At , it is −8 million J/kg. Potential energy therefore decreases by 8 million J/kg, and gravity does positive work during an outward move.” Repair both signs.
Hint 2
Subtract the initial signed value from the final one, then use .
Explained solution 2
The change per kilogram is million J/kg. Potential energy increases toward zero. Gravity's work per kilogram is −8 million J/kg because force is inward while displacement is outward. Choosing zero potential at infinity fixes the values; the physically relevant change has the same meaning under any consistent additive shift of the zero.
3. Independent: a slower radial launch
From , launch radially outward at 2000 m/s. Find the greatest radius, greatest altitude and outward rise. Check that the turning point is outside the planet.
Hint 3
Find specific energy first. At the radial turning point, use .
Explained solution 3
Here . Thus , , and the rise is about . The radius exceeds both the starting radius and . A smaller launch speed than in example 1 gives a smaller rise, as expected.
4. Reverse the question: choose a finite target
What radial outward launch speed at makes the outer turning radius exactly ? Compare it with escape speed at the same starting point.
Hint 4
Set final speed to zero at the target and equate the two energies. Do not set final potential energy to zero at a finite radius.
Explained solution 4
The ratio is less than one. The object reaches a finite maximum radius and returns; reaching that target is not escaping. This answer is a speed at launch, not the speed at the turning point.
5. Transfer: keep the energy left at infinity
A 50 kg object launches radially outward from . It must have limiting speed 3000 m/s far away. Find its launch speed and total mechanical energy. Would doubling its mass change either result?
Hint 5
Use , then multiply specific energy by mass.
Explained solution 5
The launch speed is . Specific energy is , so . Doubling mass leaves both specified speeds and specific energy unchanged but doubles total energy. The total is positive because nonzero kinetic energy remains at infinite separation.
6. Challenge: identical energy, different motion
Two equal-mass objects start at the same with speed . Object A moves tangentially; B moves radially outward. Show that their energies are equal but their paths are different. What is B's outer turning radius?
Hint 6
Energy contains speed, not velocity direction. Use the circular-force condition for A and the zero-speed condition only for B.
Explained solution 6
Both have . A follows a circle in the stated gravity-only model; its speed stays nonzero. B rises radially, reaches , and returns. A has nonzero angular momentum about the planet's centre; B has zero angular momentum. Negative energy alone does not establish a circular or collision-free orbit. Setting total speed to zero at the farthest point of every orbit would erase this distinction.
6. Check the model before the arithmetic
- Use centre-to-centre radius, not altitude, in the potential.
- Keep one zero of potential energy and use joules or joules per kilogram consistently.
- Use zero total speed at a turning point only when the motion is radial.
- Use circular-state formulas only for circular states. Energy alone does not specify direction or angular momentum.
- Distinguish a finite turning radius, threshold escape and escape with excess speed.
For curriculum context, John Abbott's Science description of Mechanics 203-SN1-RE includes forces, energy and the gravitational field. That supports the topic connection, not a claim that every section assesses escape speed or orbit energy. Use your current outline to choose these extensions. Return to the John Abbott mechanics guide for the broader course context.
Further reading: OpenStax, gravitational potential and total energy and satellite orbits and energy. The explanations and exercises here are original Nablio teaching, not official examination questions. Tutoring is currently offered in English.
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John Abbott's 203-SN1-RE description includes forces, energy and the gravitational field. This is focused supplemental practice, not complete course coverage or confirmation that escape speed and orbit energy are assessed in your section. Follow your current outline.
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