Audited ·Last updated 27 Jul 2026·5 citations·Tier 1·0 uses

Coulomb's Law Calculator

Calculate electrostatic force between point charges with Coulomb's law. Solve for force, charge, or distance using CODATA constants and step-by-step arithmetic.

Coulomb's Law Calculator

Solve for
Electrostatic force magnitude (F)
0.1997
Magnitude of the electrostatic force between the two point charges, in newtons.

Background.

The Coulomb's law calculator computes the electrostatic force between two stationary point charges, or solves for any one variable—charge magnitude or separation distance—when the other three are known. It is the foundational quantitative relationship in electrostatics, preceding field concepts and Gauss's law in most physics curricula. Students in Advanced Placement Physics C, introductory university physics, and electrical engineering courses encounter this calculation repeatedly, both in conceptual problem sets and in laboratory exercises involving Coulomb balances or charged pith balls. Beyond the classroom, the law governs the design of electrostatic precipitators, the modeling of ionic bonding potentials, and the baseline force estimates in vacuum microelectromechanical systems where gravitational and inertial effects are negligible compared with electric interactions.

Search demand for Coulomb's law calculators is sustained by the sheer volume of STEM enrollments globally. Every academic year, millions of students complete problem sets that require evaluating the force between two charges separated by a given distance, or inferring an unknown charge from a measured force and known geometry. Unlike more specialized engineering calculators, the audience here is broad: high school seniors, undergraduates, teaching assistants creating answer keys, and hobbyists building high-voltage demonstrations. The calculation is simple in principle—an inverse-square law with a proportionality constant—but students frequently struggle with unit conversions, scientific notation, and the sign conventions that determine attractive versus repulsive forces.

The historical context matters because Coulomb's law is not merely an approximation; it is the electrostatic limit of quantum electrodynamics, validated to extraordinary precision. Charles-Augustin de Coulomb published his findings in 1785 after experiments with a torsion balance, measuring the torque on charged spheres as a function of their separation. His result—that force varies as the inverse square of distance—was anticipated by Joseph Priestley and Daniel Bernoulli, but Coulomb provided the first direct quantitative evidence. The proportionality constant, now written k_e, was not isolated as a distinct fundamental constant until the development of the SI system and the explicit definition of the ampere. Modern values derive from CODATA recommended values, where k_e is exact by definition because it equals 1/(4πε₀) and ε₀ is fixed by the defined speed of light and the defined magnetic constant. This definitional exactness means that, unlike the gravitational constant G, k_e carries no measurement uncertainty in SI.

When using the calculator, it is important to recognize the domain of validity. Coulomb's law applies exactly to point charges in a vacuum. For extended conductors or dielectric media, the net force can be computed by integration or by introducing a relative permittivity factor, but the point-charge formula itself is no longer exact. At atomic scales, the law breaks down because charge is quantized and quantum effects dominate; at relativistic velocities, magnetic fields and retardation effects enter. Nevertheless, for the macroscopic, static, vacuum-scale problems that dominate homework and introductory design, Coulomb's law remains the correct starting point. The calculator therefore serves both as a computational shortcut and as a pedagogical reinforcement of the inverse-square relationship that underlies much of classical electromagnetism. Modern Coulomb balances used in national metrology institutes to realize the ampere rely on this same force law, achieving relative uncertainties below one part in 10⁸.

What is coulomb's law calculator?

Coulomb's law states that the magnitude of the electrostatic force between two point charges is directly proportional to the product of the charge magnitudes and inversely proportional to the square of the distance between them. The force acts along the straight line joining the charges. If the charges have the same sign, the force is repulsive; if opposite, attractive. The scalar magnitude is expressed as F = k_e |q₁ q₂| / r², where q₁ and q₂ are the charge values in coulombs, r is the center-to-center separation in meters, and k_e is Coulomb's constant. In SI units, k_e equals 8.9875517923 × 10⁹ newton meter squared per coulomb squared, exact by definition.

The coulomb is the SI unit of electric charge, defined by the fixed numerical value of the elementary charge e = 1.602176634 × 10⁻¹⁹ C. Consequently, one coulomb corresponds to roughly 6.242 × 10¹⁸ elementary charges. The law assumes charges are stationary or moving slowly enough that magnetic effects are negligible. It also assumes the medium is vacuum or air; for other materials, the force is reduced by a factor of the relative permittivity κ. The range of validity extends from submillimeter charged-particle traps to planetary-scale charge distributions, provided the problem remains in the electrostatic regime and quantum corrections are unnecessary.

How to use this calculator.

  1. Enter the magnitude of the first point charge in coulombs, using scientific notation if needed.
  2. Enter the magnitude of the second point charge in coulombs.
  3. Input the center-to-center separation distance in meters.
  4. Select the quantity to solve for: force, first charge, second charge, or distance.
  5. Review the computed result, which uses the exact CODATA value of Coulomb's constant.
  6. Interpret the sign: like charges yield a positive (repulsive) force magnitude; opposite charges yield attraction.

The formula.

F = kₑ |q₁ q₂| ⁄ r²

The modern form of Coulomb's law, F = k_e |q₁ q₂| / r², emerged from decades of refinement after Coulomb's 1785 torsion-balance experiments. The inverse-square dependence on distance was the critical discovery, consistent with the geometric spreading of electric flux that later enabled Gauss's law. The proportionality to the product of charges reflects the superposition principle: the force exerted by a collection of charges on a test charge is the vector sum of the individual pairwise forces, each scaling linearly with the test charge.

The constant k_e is not an independently measured empirical quantity in the current SI; it is exact because the vacuum electric permittivity ε₀ is fixed by definition. Since k_e = 1/(4πε₀) and ε₀ is defined through the magnetic constant μ₀ and the speed of light c (with c exact and μ₀ = 4π × 10⁻⁷ N/A² exact), k_e inherits exactness. This definitional architecture, adopted in the 2019 SI revision, means that a Coulomb's law calculation in SI units carries no uncertainty from k_e itself; any uncertainty enters only through the measured charges and distances.

The formula can be algebraically rearranged to solve for any isolated variable. Solving for separation gives r = √(k_e |q₁ q₂| / F), which is useful when a known force is measured between calibrated charges. Solving for an unknown charge gives |q₁| = F r² / (k_e |q₂|), the basis of historical charge measurement before the electron's charge was known. The vector form introduces unit vectors: F₁₂ = k_e q₁ q₂ / r² r̂₁₂, where r̂₁₂ points from charge 1 to charge 2. This vector formulation is essential when combining Coulomb forces with other vectors, but the scalar magnitude suffices for collinear problems.

An important subtlety is that Coulomb's law describes the force between point charges. For continuous charge distributions, the total force requires integrating the pairwise force over both distributions, which reduces to the point-charge result when the separation is large compared with the charge dimensions. Inside a uniform spherical shell, the enclosed charge contributes nothing by symmetry, a result that generalizes to Newton's shell theorem and its electrostatic analogue.

A worked example.

Example

Consider two small conducting spheres carrying charges of 1.00 microcoulomb and 2.00 microcoulomb, placed 30.0 centimeters apart in air. To find the electrostatic force, first convert the charges to coulombs: q₁ = 1.00 × 10⁻⁶ C and q₂ = 2.00 × 10⁻⁶ C. The separation is r = 0.300 m. Multiply the charges to obtain |q₁ q₂| = 2.00 × 10⁻¹² C². Multiply by Coulomb's constant, k_e = 8.9875517923 × 10⁹ N·m²/C², yielding 0.0179751036 N·m². Divide by r² = 0.0900 m² to obtain F = 0.1997 N, which rounds to 0.200 N. Because both charges are positive, the force is repulsive. This result is consistent with the worked example in Halliday, Resnick, and Walker, Fundamentals of Physics, 10th edition, Chapter 21, which uses similar magnitudes to illustrate the substantial forces that even microcoulomb-scale charges generate at modest distances. For physical context, a force of 0.200 newtons is comparable to the weight of a small paperclip, yet it arises from charges smaller than those produced by rubbing a balloon against hair.

q10
q20
r0.3

Frequently asked questions.

What is Coulomb's constant and where does its value come from?
Coulomb's constant, denoted k_e, is the proportionality factor in Coulomb's law that relates charge product and separation to electrostatic force in SI units. Its value is 8.9875517923 × 10⁹ N·m²/C². In the current International System of Units, adopted in 2019, this value is exact by definition rather than measured. It derives from the exact definition of the vacuum electric permittivity ε₀, with k_e = 1/(4πε₀). Because the speed of light c and the magnetic constant μ₀ are themselves exact in SI, ε₀ and therefore k_e carry no experimental uncertainty. Prior to 2019, k_e was determined experimentally through measurements of the force between known charges.
Does Coulomb's law work for charges in water or other materials?
Coulomb's law in its standard form applies to point charges in a vacuum. When charges are immersed in a material medium, the medium polarizes in response to the electric field, reducing the net force between the charges by a factor equal to the relative permittivity κ of the material. For water at room temperature, κ is approximately 80, so the force is roughly one-eightieth of its vacuum value. The modified formula is F = k_e |q₁ q₂| / (κ r²). This reduction assumes the medium is uniform, isotropic, and linear. In non-uniform media or at interfaces between dielectrics, the problem requires solving Poisson's equation or using the method of images rather than the simple point-charge formula.
Why is the force inversely proportional to the square of the distance?
The inverse-square dependence arises from the geometric fact that electric field lines emanating from a point charge spread uniformly over the surface of an imaginary sphere centered on the charge. As the sphere's radius r increases, its surface area grows as 4πr², diluting the flux per unit area as 1/r². Since force is proportional to the electric field strength experienced by the second charge, the force inherits the same 1/r² scaling. Coulomb verified this experimentally in 1785 using a torsion balance. Modern tests of the inverse-square law, through measurements of the photon rest mass limit, confirm the exponent is 2 to within a few parts in 10¹⁶, making it one of the most precisely verified laws in physics.
Can Coulomb's law be used for moving charges?
Coulomb's law strictly applies to stationary charges. When charges move, they constitute electric currents that generate magnetic fields, and the moving charges experience additional magnetic forces governed by the Lorentz force law. Furthermore, electromagnetic information propagates at the finite speed of light, so the force on a charge depends on the retarded position of the source charge, not its instantaneous position. For non-relativistic speeds much less than the speed of light, Coulomb's law remains an excellent approximation for the electric component of the force, but the full interaction must be described by Maxwell's equations and, for relativistic velocities, by quantum electrodynamics.
How does Coulomb's law relate to Newton's law of universal gravitation?
Both laws describe inverse-square central forces proportional to the product of a source property and a test property. Coulomb's law uses the product of electric charges and the constant k_e, while Newton's gravitation uses the product of masses and the constant G. Despite this formal similarity, the two forces differ dramatically in magnitude and sign. The electrostatic force between two protons is approximately 10³⁶ times stronger than their gravitational attraction. Additionally, mass is always positive, so gravity is universally attractive, whereas electric charge can be positive or negative, allowing electrostatic forces to be either attractive or repulsive. The mathematical parallel breaks down at relativistic scales, where gravity requires general relativity rather than a simple static force law.
What is the difference between the scalar and vector forms of Coulomb's law?
The scalar form, F = k_e |q₁ q₂| / r², gives only the magnitude of the force and is sufficient when the charges are aligned along a single axis or when only the force size is needed. The vector form, F₁₂ = k_e q₁ q₂ / r² r̂₁₂, encodes both magnitude and direction. Here r̂₁₂ is the unit vector pointing from charge 1 toward charge 2. If the product q₁ q₂ is positive, the force vector points in the direction of r̂₁₂, indicating repulsion; if negative, it points opposite, indicating attraction. The vector form is essential for calculating the net force on a charge from multiple sources using vector superposition, as required in two- and three-dimensional arrangements.
Can I use this calculator for charged spheres instead of point charges?
Yes, provided the spheres are small compared with their separation and the charge is distributed uniformly on the surface. Under these conditions, each sphere behaves electrostatically as if its entire charge were concentrated at its center, a result known as the shell theorem. If the spheres are close enough that charge redistribution occurs due to mutual induction, the simple point-charge formula becomes inaccurate. For conducting spheres in contact, charge sharing and induction effects require solving Laplace's equation or using numerical methods. The calculator assumes the point-charge approximation holds, which is valid for most textbook problems and for macroscopic charged objects separated by distances large relative to their radii.
What units should I use with this calculator?
The calculator expects SI units: charge in coulombs, distance in meters, and force in newtons. One microcoulomb equals 10⁻⁶ coulombs, one nanocoulomb equals 10⁻⁹ coulombs, and one centimeter equals 10⁻² meters. Using consistent SI units ensures the proportionality constant k_e = 8.9875517923 × 10⁹ N·m²/C² applies without conversion factors. If you input charge in microcoulombs and distance in centimeters without converting, the result will be off by orders of magnitude. The calculator handles scientific notation, so values such as 3.50 × 10⁻⁶ C should be entered as 3.50e-6. Always verify that your inputs are in base SI units before interpreting the output.
Why is Coulomb's law called an inverse-square law?
The term inverse-square law refers to any physical relationship in which a quantity decreases proportionally to the square of the distance from the source. In Coulomb's law, the electrostatic force F is proportional to 1/r², meaning doubling the separation reduces the force to one-quarter of its original value, and tripling the separation reduces it to one-ninth. This scaling distinguishes Coulomb forces from other potentials, such as the spring force which varies linearly with displacement or the van der Waals interaction which falls off as 1/r⁶. The inverse-square character is deeply tied to three spatial dimensions; in a hypothetical two-dimensional world, Gauss's law would yield a 1/r force law instead.
How accurate is Coulomb's law at very small distances?
At subatomic scales, Coulomb's law ceases to be exact because charge is quantized into elementary units carried by electrons and quarks, and because quantum mechanical effects dominate. The force between an electron and a proton in a hydrogen atom is not purely classical; vacuum polarization and the exchange of virtual photons modify the interaction at distances comparable to the Compton wavelength of the electron. These corrections are captured by quantum electrodynamics. At distances below roughly 10⁻¹⁵ meters, the strong nuclear force overwhelms the electrostatic repulsion between protons in a nucleus. For all macroscopic and most atomic calculations, however, Coulomb's law remains accurate to many decimal places.

References& sources.

  1. [1]CODATA (2018). "CODATA Recommended Values of the Fundamental Physical Constants: 2018." Journal of Physical and Chemical Reference Data, 50(3), 033105.
  2. [2]Coulomb, C.A. (1785). "Premier mémoire sur l'électricité et le magnétisme." Histoire de l'Académie Royale des Sciences, 569-577.
  3. [3]Halliday, D., Resnick, R., & Walker, J. (2013). Fundamentals of Physics, 10th ed. Wiley. Ch. 21.
  4. [4]BIPM (2019). The International System of Units (SI Brochure), 9th ed.
  5. [5]Jackson, J.D. (1999). Classical Electrodynamics, 3rd ed. Wiley. Ch. 1.

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