Spring energy: launch a block with a compressed spring

Compress a spring, release a block and see the stored energy ½kx² turn into motion. Find the launch speed, and how far the block slides when the floor has friction.

Keep it one tap away for everyday use.

Bookmark Spring energy?

Press Ctrl + D now. Your browser opens its own bookmark box, where you choose the name and folder.

  1. Compress
  2. Release
  3. Check
Nothing is uploadedWorks offline once open

Compress, release, launch

A teaching model: the block is only pushed, not fixed to the spring, and g = 9.8 m/s².

Energy and speed

Try this

  • Double the compression. The stored energy goes up four times, because it depends on x².
  • Double the mass. The speed falls by a factor of √2, not 2.
  • Switch friction on. The block leaves slower and stops after a sliding distance you can predict.
  • Make friction large and the compression small: the spring cannot even start the block.

Check yourself

What it does

A spring squeezed by a distance x stores energy ½ k x², where k is its stiffness in newtons per metre. When you let go, that energy pushes a block, and by the time the block leaves the spring it has kinetic energy ½ m v². With no friction the two are equal, so the launch speed is v = x √(k/m).

On a rough floor some of the energy is used up as heat. The spring must first beat friction, then it loses μ m g x while pushing, and after the block leaves it slides until friction stops it. This is a teaching model: the block is only pushed, not fixed to the spring. To see how a spring force varies, try spring combinations, and for the idea of work done by a changing force see variable force work.

How to use it

  1. Set the stiffness k, the compression x and the block’s mass m.
  2. Leave friction μ at 0 for a smooth floor, or raise it.
  3. Press Release and watch the block; Reset puts it back.
  4. Read the stored energy, the launch speed and the sliding distance under the picture.

What each setting does

  • Stiffness k: a stiffer spring stores more energy for the same squeeze.
  • Compression x: the energy grows with x squared.
  • Mass m: a heavier block ends up slower for the same energy.
  • Friction μ: how rough the floor is. Zero means smooth.

Worked example

Take k = 100 N/m, x = 10 cm and m = 0.5 kg on a smooth floor. The stored energy is ½ × 100 × 0.1² = 0.5 J, and v = 0.1 × √(100 ÷ 0.5) = 1.41 m/s.

Now add friction μ = 0.2. Then v² = (100 × 0.01 − 2 × 0.2 × 0.5 × 9.8 × 0.1) ÷ 0.5 = 1.61, so v = 1.27 m/s, and the block slides 1.61 ÷ (2 × 0.2 × 9.8) = 0.41 m before it stops.

FAQs

Why does doubling x quadruple the energy? Because the force grows with x and the distance also grows with x, so the work (area under the force graph) grows with x².

Does the block stay joined to the spring? Not in this model. It leaves where the spring reaches its natural length.

Where the numbers come from

  • Elastic potential energy ½kx², the work-energy theorem and kinetic friction μmg: standard Class 11 physics (work, energy and power). g = 9.8 m/s². The picture is fibub's own teaching model.

Standard scientific values, such as constants, atomic weights and melting points, are facts found in every textbook; we name where ours were checked. If you are an author or publisher and want a value, a credit or a table changed or removed, tell us and we will act quickly.

Last updated 2026-11-10.

Change log for Spring energy

  1. Add spring-energy (Class 11 Physics) Details on GitHub

Every change to fibub

Related tools

Variable force work #L196 Shape a force-displacement graph with your finger, or start from a steady force, a spring or a fading push, pick where the motion starts and stops, and see the work as the shaded area, with the parts above and below the axis, the formula with your numbers, and the speed it gives a cart. Spring combinations #L214 Hang a mass on one spring, two springs one below the other, or two side by side, and watch it bob. See the combined spring constant, how far it hangs, the period T = 2π√(m/k) and the energy, all with your numbers, and compare series with parallel. Mirror ray diagram #L1 Drag an object in front of a concave or convex mirror and watch the principal rays find the image: where it forms, how big it is, real or virtual, with the mirror formula and magnification worked out with signs. Lens ray diagram #L2 Drag an object in front of a convex or concave lens and watch the principal rays find the image: where it forms, how big it is, real or virtual, with the lens formula, magnification and power worked out with signs. Snell's law #L3 Aim a ray of light at the boundary between air, water, glass or diamond and see it bend by Snell's law, find the critical angle and total internal reflection, the sideways shift through a glass slab, and why a pool looks shallower than it is. Prism and dispersion #L4 Shine a ray through a glass prism and see it bend twice: the angles at both faces, the angle of deviation, the deviation graph with its minimum, and white light splitting into a spectrum from red to violet.