Conservation of Energy Calculator

Solve conservation of energy problems involving kinetic energy, gravitational potential energy, spring energy, external work, and energy loss.

Calculator is for informational purposes only. Terms and Conditions

\[ \frac{1}{2}mv_1^2 + mgh_1 + \frac{1}{2}kx_1^2 + W – E_{loss} = \frac{1}{2}mv_2^2 + mgh_2 + \frac{1}{2}kx_2^2 \]
1

Choose what to solve for

Select the missing variable, problem type, and unit setup before entering known values.

The unknown field is hidden automatically and solved from the energy balance.

Presets simplify common physics problems while keeping the full solver available.

Unit presets update input units, gravity units, and the default answer unit.

Enter the initial and final energy-state values. Optional spring, work, and loss terms may be left blank when not needed.
2

Enter the known values

Only the fields needed for the selected setup are shown. Blank optional terms are treated as zero.

Use mass, not weight. For ideal gravity-only velocity problems, mass cancels, so the default value may be left unchanged.
Enter the speed at state 1. Use zero when the object starts from rest.
Enter the speed at state 2. This field is hidden when solving for final velocity.
Height is measured relative to the same reference level used for final height.
Only the height difference affects gravitational potential energy.
Leave blank or use zero when spring energy is not part of the problem.
Spring displacement is measured from the unstretched or uncompressed length. Leave blank when unused.
Use zero or leave blank when the spring is relaxed at the final state.
Positive work adds energy to the system. Leave blank or use zero for ideal mechanical energy conservation.
Energy loss represents friction, drag, heat, sound, or other nonconservative losses.
Default Earth gravity is 9.80665 m/s². Use custom gravity for Moon, Mars, or other systems.
Advanced Options
3

Visual Check

Compare initial energy, final energy, work added, and losses without overlapping labels.

Conservation of energy visual diagram A dynamic stacked bar chart comparing initial energy, final energy, work added, and energy loss.
4

Solution

Live result, quick checks, warnings, and full solution steps.

Solution
Real-time result updates as you type.

Quick checks

  • Energy balance
Show solution steps See the equation, substitutions, assumptions, and result path
  1. Enter values to see the full solution steps and checks.
5

Source, Standards, and Assumptions

Calculation basis, constants, assumptions, and limitations.

Standard physics energy balance

Source/standard information updates after a valid calculation.

  • Assumptions will appear after a valid calculation.
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Calculator Guide

How to Use the Conservation of Energy Calculator

The Conservation of Energy Calculator above helps solve energy-balance problems by comparing an initial state and a final state. Use it to calculate final velocity, initial velocity, height, spring displacement, spring constant, or energy loss when kinetic energy, gravitational potential energy, spring energy, work, and losses are involved.

The most common use is solving final velocity from height, but the same energy balance can also solve for height, spring compression, spring constant, or energy lost to friction. Energy can change form, but the balance must still close.

Best for Falling objects, roller coasters, spring launch problems, and energy-loss checks
Main result Velocity, height, spring value, or energy loss from an energy balance
Most important input Height difference, velocity, spring displacement, or energy loss depending on the solve mode

Quick Answer

To use the calculator, choose the unknown variable, select the problem type, enter the known initial and final state values, then review the energy balance. For a simple falling object with no losses, the common shortcut is \(v=\sqrt{2gh}\). For a full problem, use the general balance of initial energy plus work added minus energy lost equals final energy.

When not to rely on the simplified result

Do not treat an ideal conservation-of-energy result as a final design answer when friction, air resistance, rolling resistance, impact forces, deformation, safety factors, manufacturer limits, or code requirements matter. The calculator is best for educational physics, quick checks, and first-pass engineering estimates.

Inputs and Outputs Used by the Calculator

The calculator uses values from an initial state and a final state. Depending on the solve mode, one value is hidden as the unknown and the calculator rearranges the energy equation to find it.

Common inputs and outputs for conservation of energy problems
ValueWhat It MeansTypical UnitsWhy It Matters
Mass, \(m\)Amount of matter in the moving object or block.kg, g, lbm, slugNeeded for energy values, although it cancels in ideal gravity-only velocity problems.
Velocity, \(v_1\) or \(v_2\)Initial or final speed of the object.m/s, ft/s, mph, km/hKinetic energy depends on velocity squared, so speed strongly affects the result.
Height, \(h_1\) or \(h_2\)Initial or final elevation relative to the same reference level.m, cm, mm, ft, inControls gravitational potential energy through \(mgh\).
Gravity, \(g\)Acceleration due to gravity used in potential energy and falling-object calculations.m/s², ft/s²Earth uses about \(9.80665\,m/s^2\), but Moon, Mars, or custom gravity values change the result.
Spring values, \(k\) and \(x\)Spring stiffness and compression or extension from equilibrium.N/m, lbf/ft, lbf/in; m, ft, inControls elastic potential energy through \(\frac{1}{2}kx^2\).
Work and energy lossEnergy added to or removed from the simplified mechanical system.J, kJ, ft·lbf, WhAccounts for motors, pushes, friction, drag, heat, sound, and other losses.

Conservation of Energy Formula

The most useful calculator form compares the energy at state 1 with the energy at state 2. The calculator adds external work and subtracts energy loss so it can handle ideal and non-ideal problems.

General Energy Balance

\[ \frac{1}{2}mv_1^2 + mgh_1 + \frac{1}{2}kx_1^2 + W – E_{loss} = \frac{1}{2}mv_2^2 + mgh_2 + \frac{1}{2}kx_2^2 \]

This form includes kinetic energy, gravitational potential energy, spring potential energy, work added, and energy loss.

Common Falling-Object Shortcut

\[ v_2=\sqrt{v_1^2+2g(h_1-h_2)} \]

If an object starts from rest and falls through height \(h\), this becomes \(v=\sqrt{2gh}\). This is why mass does not affect ideal fall speed when air resistance is ignored.

Spring Launch Shortcut

\[ \frac{1}{2}kx^2=\frac{1}{2}mv^2 \qquad\Rightarrow\qquad v=x\sqrt{\frac{k}{m}} \]

Use this simplified spring relationship only when spring energy becomes kinetic energy with no height change and no losses. For spring force and stiffness background, review Hooke’s Law.

Formula reference note

For a student-friendly explanation of mechanical energy as kinetic plus potential energy, see The Physics Classroom mechanical energy guide. For falling-object impact velocity from conservation of energy, see HyperPhysics on falling-object energy.

What the Variables Mean

Each variable must use the same physical reference system. Heights must share the same zero datum, spring displacement must be measured from the unstretched position, and energy terms must use consistent units.

\(KE=\frac{1}{2}mv^2\)

Kinetic energy is energy of motion. Because velocity is squared, a small speed change can create a large energy change. If you only need energy from mass and speed, use the Kinetic Energy Calculator.

\(PE_g=mgh\)

Gravitational potential energy depends on mass, gravity, and height. Only the height difference matters when the same reference level is used.

\(PE_s=\frac{1}{2}kx^2\)

Spring potential energy depends on spring constant and displacement from equilibrium. Compression and extension are entered as positive magnitudes.

\(W\) and \(E_{loss}\)

Work added increases the available energy. Energy loss represents mechanical energy converted into heat, sound, drag-related fluid motion, vibration, or deformation.

How to Use the Calculator

Use the calculator by matching the solve mode to your unknown, entering the known state values, selecting units, and checking whether the energy balance closes.

1

Select the unknown

Choose final velocity, initial velocity, height, spring displacement, spring constant, or energy loss. The calculator hides the unknown field and solves for it.

2

Choose the problem type

Use general energy balance for full problems, falling object for height-to-speed checks, spring launch for elastic energy, or energy loss when friction or drag is the missing value.

3

Enter known values and units

Enter speeds, heights, mass, gravity, spring values, work, and losses. Optional spring, work, and loss terms may be left blank when they do not apply.

4

Review the balance check

Compare initial mechanical energy, final mechanical energy, energy added, and losses. A valid setup should make the left and right sides of the energy balance agree within rounding.

How the controls work

When you change the solve mode, the calculator hides the unknown input and updates the required known values. When you change the unit preset, the calculator converts values internally to SI units before solving and then displays the answer in your selected output unit.

How to Interpret the Result

A conservation-of-energy result tells you what value makes the energy balance work. It does not automatically prove that the physical situation is safe, efficient, or realistic.

What to do with the result

Use the answer to check homework, compare scenarios, estimate speed from height, estimate spring launch speed, or identify how much mechanical energy was lost.

What changes the result most?

Velocity and spring displacement often dominate because both are squared. Height difference is also important because it directly changes gravitational potential energy.

Practical sanity check

If an object falls from \(10\,m\) from rest near Earth with no losses, the speed should be about \(14\,m/s\). A result far from that usually means a unit or input mistake.

Energy loss does not mean energy disappeared

When the calculator reports energy loss, it means mechanical energy left the simplified mechanical model. It may have become heat, sound, vibration, deformation, or drag-related energy.

Why mass cancels in ideal falling-object speed problems

In ideal gravity-only problems, mass cancels because both \(mgh\) and \(\frac{1}{2}mv^2\) contain \(m\). Mass still affects kinetic energy, but it does not affect ideal fall speed when air resistance is ignored.

Input Checklist Before You Trust the Answer

Most wrong conservation-of-energy answers come from mixing units, using inconsistent height references, forgetting losses, or entering spring displacement incorrectly.

  • Use the same height reference for \(h_1\) and \(h_2\).
  • Enter mass, not weight, unless the calculator specifically asks for weight.
  • Check that velocity units match the value entered, especially mph versus m/s or ft/s.
  • Set spring constant to zero when spring energy is not part of the problem.
  • Use spring displacement from the relaxed spring length, not total spring length.
  • Add energy loss when friction, drag, heat, sound, or deformation matters.

Worked Examples

These examples follow the same logic as the calculator so users can verify the calculation manually.

Example 1: Final velocity from height

Initial velocity
\(v_1=0\,m/s\)
Initial height
\(h_1=10\,m\)
Final height
\(h_2=0\,m\)
Gravity
\(g=9.80665\,m/s^2\)
Losses
\(E_{loss}=0\,J\)

Formula

\[ v_2=\sqrt{v_1^2+2g(h_1-h_2)} \]

Substitution

\[ v_2=\sqrt{0^2+2(9.80665)(10-0)} \]
\[ v_2=\sqrt{196.133}=14.0\,m/s \]

Final answer

The final velocity is \(14.0\,m/s\). This is reasonable because a 10 m fall near Earth gives a speed a little over 30 mph when air resistance is ignored. For a narrower falling-object workflow, use the Free Fall Calculator.

Reverse check

Use \(KE=\frac{1}{2}mv^2\) and \(PE=mgh\). For any mass \(m\), the equality \(\frac{1}{2}m(14.0)^2 \approx m(9.80665)(10)\) checks the answer. The mass cancels because both sides include \(m\).

Example 2: Spring launch

For a \(2\,kg\) block launched by a \(500\,N/m\) spring compressed \(0.20\,m\), use \(v=x\sqrt{\frac{k}{m}}\).

\[ v=0.20\sqrt{\frac{500}{2}}=3.16\,m/s \]

The result is reasonable because the spring stores \(\frac{1}{2}(500)(0.20)^2=10\,J\), and \(\frac{1}{2}(2)(3.16)^2\approx10\,J\).

Example 3: Energy loss

If a system starts with \(1000\,J\) of mechanical energy and ends with \(850\,J\), the missing mechanical energy is the loss.

\[ E_{loss}=E_1-E_2=1000-850=150\,J \]

The \(150\,J\) may have become heat, sound, vibration, drag-related fluid motion, or deformation.

How to Visualize the Energy Balance

Think of conservation of energy as two energy states connected by work and loss. Energy can move between forms, but the balance must still close.

Reference Checks for Common Energy Problems

Conservation-of-energy problems do not have one universal “typical” result because the answer depends on height, speed, mass, spring stiffness, and losses. Use quick reference checks instead of memorized ranges.

Falling object check

A fall from \(10\,m\) with no air resistance gives about \(14.0\,m/s\). A fall from \(1\,m\) gives about \(4.43\,m/s\).

Spring energy check

Doubling spring compression quadruples the stored spring energy because \(PE_s\) depends on \(x^2\).

Source note: Educational physics references commonly define total mechanical energy as kinetic plus potential energy. The Physics Classroom mechanical energy conservation examples show how kinetic and potential energy trade off while total mechanical energy remains constant under ideal assumptions.

Practical Limits of Conservation of Energy

For classroom problems, conservation of energy is often enough. For engineering design or real-world prediction, the simplified result may overestimate speed or underestimate losses.

Ideal mechanics

Use the basic equation when friction, drag, rolling resistance, and deformation are intentionally ignored.

Real motion

Add energy loss when contact friction, air resistance, heat, sound, or vibration is important.

Impact or safety problems

Energy can estimate speed or kinetic energy before impact, but impact force requires stopping distance, time, material deformation, and professional judgment.

Units and Conversions

Energy calculations are safest when everything is converted internally to SI units: kg, m, s, N/m, and J. The calculator can return the final answer in selected display units, but the physical balance still depends on consistent units.

Useful unit conversions for conservation of energy
QuantityCommon UnitsConversion Reminder
Masskg, g, lbm, slug\(1\,lbm=0.45359237\,kg\), \(1\,slug\approx14.5939\,kg\)
Length or heightm, cm, mm, ft, in\(1\,ft=0.3048\,m\), \(1\,in=0.0254\,m\)
Velocitym/s, ft/s, mph, km/h\(1\,mph=0.44704\,m/s\)
EnergyJ, kJ, ft·lbf, Wh\(1\,ft{\cdot}lbf\approx1.35582\,J\), \(1\,Wh=3600\,J\)
Spring constantN/m, lbf/ft, lbf/inUse units of force per length, not just force.

Common unit trap

Do not mix pound-mass, pound-force, and slugs. They are not interchangeable. If a problem gives weight instead of mass, convert carefully or use a force-based work relationship instead of treating weight as kilograms or pound-mass.

Conservation of Energy vs. Other Physics Methods

Conservation of energy is often the fastest method when the path details are not important. Other methods are better when time, acceleration history, force history, or direction-specific motion matters.

Use energy when

You know height, speed, spring compression, or energy loss and need a state-to-state result.

Use kinematics when

You need time, acceleration, displacement, or motion under constant acceleration.

Use force analysis when

You need normal force, friction force, contact force, impact force, or detailed force direction.

Common Mistakes

Conservation of energy is powerful, but small setup mistakes can completely change the answer.

Do

  • Use the same height datum for the initial and final states.
  • Include spring energy when a spring is compressed or stretched.
  • Include loss when friction, drag, heat, sound, or deformation matters.
  • Check squared terms carefully because \(v^2\) and \(x^2\) dominate results.

Don’t

  • Do not mix meters and feet without conversion.
  • Do not confuse spring displacement with total spring length.
  • Do not assume mechanical energy is conserved when nonconservative work is significant.
  • Do not use impact velocity alone to claim an impact force.

Troubleshooting Unrealistic Results

If the result looks too high, too low, negative, or impossible, check the setup before assuming the formula is wrong.

No real velocity

The final state may require more energy than the initial state provides. Lower the final height, reduce losses, add work, or check units.

Speed too high

Look for height entered in feet while meters are selected, missing losses, or a velocity entered in mph while m/s is selected.

Energy loss is negative

A negative calculated loss usually means energy was added to the system or the final state has more mechanical energy than the initial state.

Spring answer seems wrong

Check that \(x\) is displacement from equilibrium and that spring constant is in force per length, such as N/m or lbf/in.

Assumptions and Limitations

The calculator uses a simplified mechanical energy model. It is best for educational use, problem solving, and early estimates—not for final safety or design decisions by itself.

Idealized system

The calculator assumes the energy terms you enter fully describe the system. Any omitted loss or work term is treated as zero.

Point-mass model

The basic formula does not include rotational energy unless you manually account for it as an added energy term.

No automatic drag model

Air resistance and fluid drag must be represented as energy loss or handled with a more detailed drag calculation.

Not an impact-force calculator

The tool can estimate speed or kinetic energy before impact, but impact force also depends on stopping distance and deformation.

Rotational energy note

If rotation is important, such as a rolling object or flywheel, rotational kinetic energy \( \frac{1}{2}I\omega^2 \) must be added separately. The simplified calculator focuses on translational kinetic energy, gravitational potential energy, spring energy, work, and losses.

Related Calculators and Engineering Tools

Use these related Turn2Engineering resources when your conservation-of-energy problem connects to motion, force, spring mechanics, or follow-up physics checks.

Key Terms

These terms help connect the calculator inputs, formula, and result.

Kinetic Energy

Energy due to motion, calculated as \(KE=\frac{1}{2}mv^2\).

Gravitational Potential Energy

Energy due to height in a gravitational field, calculated as \(PE_g=mgh\).

Spring Potential Energy

Energy stored in a compressed or stretched spring, calculated as \(PE_s=\frac{1}{2}kx^2\).

Energy Loss

Mechanical energy converted into heat, sound, drag, vibration, or deformation in the simplified model.

Work

Energy transferred by a force through distance. Positive work adds energy to the system.

Datum

The zero-height reference level used to measure potential energy.

FAQ

What does a Conservation of Energy Calculator do?

It compares an initial energy state and a final energy state to solve for a missing value such as final velocity, height, spring displacement, spring constant, or energy loss.

What formula does the Conservation of Energy Calculator use?

The general calculator form is \(KE_1+PE_{g1}+PE_{s1}+W-E_{loss}=KE_2+PE_{g2}+PE_{s2}\). Simpler problems may reduce to \(v=\sqrt{2gh}\) or \(\frac{1}{2}kx^2=\frac{1}{2}mv^2\).

How do you calculate final velocity from height?

For an ideal falling object, use \(v_2=\sqrt{v_1^2+2g(h_1-h_2)}\). If it starts from rest and falls through height \(h\), use \(v=\sqrt{2gh}\).

Why does mass cancel in falling-object problems?

Mass appears in both gravitational potential energy \(mgh\) and kinetic energy \(\frac{1}{2}mv^2\). In an ideal gravity-only problem, the same mass appears on both sides, so it cancels.

Can conservation of energy include friction?

Yes, but friction must be included as energy loss or nonconservative work. If friction is ignored, the calculator will return an ideal result that may overestimate real speed or height.

Is mechanical energy always conserved?

No. Mechanical energy is conserved only under ideal assumptions or when all nonconservative work and losses are accounted for. Total energy is conserved overall, but mechanical energy can become heat, sound, vibration, or deformation.

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