Calculator
Example Data Table
| Energy (J) | Wavelength (nm) | Band |
|---|---|---|
| 3.20e-19 | 620.764 | Visible (orange-red) |
| 4.00e-19 | 496.611 | Visible (blue-green) |
| 2.50e-19 | 794.578 | Near‑IR |
| 1.99e-19 | 998.214 | Near‑IR (≈1 μm) |
| 6.63e-19 | 299.615 | Near‑UV |
These examples assume the default constants and photon relation E = h·c/λ.
Formula Used
For a photon, energy and wavelength are linked by: E = h·c / λ
Solving for wavelength gives: λ = (h·c) / E
- E = photon energy (joules)
- λ = wavelength (meters)
- h = Planck constant (J·s)
- c = speed of light (m/s)
How to Use This Calculator
- Enter the photon energy and pick its unit.
- Select your preferred wavelength unit for the main result.
- Choose decimal places and enable scientific notation if needed.
- Optionally enter custom values for h and c.
- Click Calculate to view results above the form.
- Use the CSV or PDF buttons to export your results.
Joules to Wavelength Guide
1) Photon energy and wavelength relationship
This calculator treats light as photons, where each photon carries energy E. Using λ = (h·c)/E, larger energy produces a shorter wavelength. For example, doubling E halves λ. This is why ultraviolet photons are more energetic than infrared photons.
2) Physical constants and numerical accuracy
The default constants use modern defined values: Planck’s constant h = 6.62607015×10⁻³⁴ J·s and the speed of light c = 299,792,458 m/s. With these, the conversion is stable and repeatable. Custom constants are included for experimental or instructional comparisons.
3) Unit scaling from meters to angstroms
Wavelength is computed in meters first, then scaled into your selected unit. 1 nm = 10⁻⁹ m, 1 µm = 10⁻⁶ m, and 1 Å = 10⁻¹⁰ m. Choosing nm is convenient for visible and UV, while µm suits infrared optics.
4) Spectrum bands you can interpret quickly
A helpful reference range is the visible band, roughly 380–740 nm. Values below that trend into ultraviolet, while higher values move into near‑infrared. The example table includes ≈300 nm (near‑UV) and ≈800–1000 nm (near‑IR) cases for comparison.
5) Worked data point from the example table
Take E = 2.50×10⁻¹⁹ J. The calculator returns about 794.6 nm, which sits in near‑IR. If you select µm, the same result becomes 0.7946 µm. This illustrates how unit choice changes the display, not the physics.
6) Reverse checking with energy in electronvolts
Many lab references quote photon energy in eV. The calculator also reports E(eV) = E(J) / 1.602176634×10⁻¹⁹. For visible light near 500 nm, energy is around 2.48 eV, which corresponds to ≈3.97×10⁻¹⁹ J.
7) Frequency and wavenumber add context
Frequency is computed using ν = c/λ. Shorter wavelengths yield higher frequencies, which matters in spectroscopy. Wavenumber in cm⁻¹ is common for infrared spectra and is simply the inverse wavelength expressed per centimeter, aiding direct comparison with spectral lines.
8) Practical tips for measurement and reporting
If your energy value comes from a detector or simulation, keep track of rounding and units. Use scientific notation when values are extremely small. Report both the chosen unit (like nm) and the meter value when publishing results. For classroom work, compare multiple energies to see the inverse trend clearly.
FAQs
1) What does this calculator convert?
It converts photon energy into wavelength using λ = (h·c)/E. You can choose energy units (like J, mJ, µJ) and output wavelength units (m, nm, µm, Å).
2) Why must energy be greater than zero?
The formula divides by energy, so zero would be undefined and negative energy is not valid for a photon’s physical energy. Enter a positive value to obtain a meaningful wavelength, frequency, and wavenumber.
3) When should I use scientific notation?
Use it when your energy is around 10⁻¹⁹ J or smaller, or when wavelengths span very large or tiny values. Scientific notation avoids rounding errors and keeps the displayed magnitude easy to read.
4) What wavelength range is visible to humans?
A common reference is about 380–740 nm. Numbers below this range are typically ultraviolet, and above it are typically infrared. Actual perception varies slightly with conditions and individual sensitivity.
5) Why does the tool show eV and cm⁻¹ too?
eV is widely used in atomic and solid‑state contexts, while cm⁻¹ is common in spectroscopy. Showing both helps you compare your result with tables, instruments, and published spectra without extra conversions.
6) Can I use custom values for h and c?
Yes. Enable “Use custom constants” and enter positive values. This is useful for demonstrations, sensitivity checks, or comparing alternate constant sets. For standard physics work, keep the default definitions for consistency.
7) Do unit changes affect the physics?
No. The calculator computes wavelength in meters first, then scales it into your selected unit. Switching between nm, µm, or Å only changes the displayed number, not the underlying wavelength.