Wavelength Formula Explained (λ = v/f)
Master the fundamental wave equation with detailed derivations, examples, and applications across different wave types.
Calculate wavelength, frequency, energy, and more with this free physics calculator. Use the wavelength formula (λ = v/f) to convert between properties for electromagnetic waves, sound waves, de Broglie matter waves, and RF antennas. All calculations run locally in your browser—no data is sent to any server.
The wavelength formula relates wavelength (λ), frequency (f), and wave speed (v):
For electromagnetic waves (light, radio, X-rays), the wave speed is the speed of light:
This fundamental relationship means higher frequency waves have shorter wavelengths, and vice versa. Understanding this inverse relationship is key to frequency to wavelength conversions.
The table below shows the complete electromagnetic spectrum with wavelength and frequency ranges. For detailed information about visible light colors and wavelengths, see our dedicated guide.
| Type | Wavelength | Frequency | Applications |
|---|---|---|---|
| Gamma rays | < 10 pm | > 30 EHz | Medical imaging, cancer treatment |
| X-rays | 10 pm - 10 nm | 30 PHz - 30 EHz | Medical imaging, security |
| Ultraviolet | 10 nm - 400 nm | 750 THz - 30 PHz | Sterilization, black lights |
| Visible light | 400 nm - 700 nm | 430 THz - 750 THz | Human vision, displays |
| Infrared | 700 nm - 1 mm | 300 GHz - 430 THz | Remote controls, thermal imaging |
| Microwave | 1 mm - 1 m | 300 MHz - 300 GHz | WiFi, radar, cooking |
| Radio | > 1 m | < 300 MHz | Broadcasting, communication |
The photon energy varies across the spectrum—see how photon energy relates to wavelength through the Planck-Einstein relation (E = hc/λ).
This wavelength calculator provides six specialized tools for different wave physics calculations. Here's how to use each tab effectively:
The Wave Basics calculator uses the fundamental wave equation λ = v/f to convert between wavelength, frequency, and wave speed.
Tips: For visible light calculations, use THz for frequency or nm for wavelength. The calculator automatically identifies the EM spectrum region and displays the actual color for visible wavelengths (400-700 nm).
Calculate the quantum mechanical wavelength of particles using λ = h/(mv), the de Broglie equation.
Tips: The de Broglie wavelength becomes significant at atomic scales. For electrons in typical experiments (10⁶ m/s), expect wavelengths around 0.7 nm. This calculator uses non-relativistic equations; for particles above 10% of light speed, relativistic corrections may be needed.
Convert between photon energy and wavelength using the Planck-Einstein relation E = hc/λ.
Tips: A useful reference: 1 eV corresponds to 1240 nm (near-infrared). Visible light photons have energies of 1.7-3.1 eV. X-ray photons are typically in the keV range.
Calculate acoustic wavelengths in different media using λ = v/f with the speed of sound.
Tips: Quarter-wavelength measurements are important for acoustic treatment and speaker placement. Sound wavelengths are much longer than light—a 440 Hz tone has a 78 cm wavelength in air, while 440 THz light has a wavelength of 680 nm.
Calculate antenna dimensions for radio frequency applications using L = λ × VF / n.
Tips: The velocity factor accounts for slower wave propagation in physical conductors. Start with calculated values and fine-tune with an antenna analyzer. A ¼ wave antenna for 146 MHz (2m band) is approximately 49 cm with VF=0.95.
Convert between wavelength and wavenumber using k = 1/λ (spectroscopic) or k = 2π/λ (angular).
Tips: Spectroscopic wavenumber (cm⁻¹) is standard in infrared spectroscopy and Raman spectroscopy. Visible light spans roughly 14,000-25,000 cm⁻¹. The angular wavenumber (rad/m) appears in wave equations and quantum mechanics.
For electromagnetic waves, remember 300/f(MHz) = λ(m). This approximation (using 300 instead of 299.79) works great for quick estimates. A 100 MHz FM station? About 3 meters. WiFi at 2400 MHz? About 12.5 cm. For visible light, memorize E(eV) × λ(nm) ≈ 1240 for instant photon energy conversions.
These examples illustrate how different people use the wavelength calculator in practical situations. All calculations use the actual formulas and constants from this calculator.
Emma, a first-year physics student, needs to calculate the frequency of green light with a wavelength of 550 nm for her optics homework.
Using the Wave Basics tab:
Result: The frequency is 545 THz (5.45 × 10¹⁴ Hz). The calculator confirms this is visible light and shows a green color swatch. Emma can verify this makes sense: visible light frequencies range from about 430-750 THz.
Carlos, a licensed amateur radio operator, wants to build a quarter-wave vertical antenna for the 2-meter band at 146 MHz.
Using the Antenna tab:
Result: The antenna should be 48.8 cm (19.2 inches). The full wavelength is 2.05 m, which is why it's called the "2-meter band." Carlos cuts his antenna wire to 49 cm and fine-tunes with his antenna analyzer.
Priya, an audio engineer, needs to calculate bass trap dimensions for frequencies around 80 Hz in her new studio. Room temperature is 22°C.
Using the Sound tab:
Result: The wavelength is 4.31 m (14.1 feet). The quarter-wavelength is 1.08 m (3.5 ft). This tells Priya that effective bass trapping for 80 Hz requires absorption panels at least 1 meter deep, or placement in room corners where pressure builds up.
David needs to convert an infrared absorption peak from wavelength (3400 nm) to wavenumber for his IR spectroscopy report.
Using the Wavenumber tab:
Result: The spectroscopic wavenumber is 2941 cm⁻¹. David recognizes this as the O-H stretching region, indicating hydroxyl groups in his sample. IR spectroscopy charts typically use wavenumbers because they're directly proportional to energy.
Dr. Chen's graduate student, Ming, is setting up an electron microscope experiment and needs to know the de Broglie wavelength of electrons accelerated to 0.5% of the speed of light.
Using the De Broglie tab:
Result: The de Broglie wavelength is 4.85 × 10⁻¹¹ m (0.485 Å). This is much smaller than visible light wavelengths (400-700 nm), which explains why electron microscopes can resolve much finer details than optical microscopes.
Mr. Thompson wants to show his AP Physics students why ultraviolet light causes sunburns but visible light doesn't, by comparing their photon energies.
Using the Energy↔Wavelength tab:
Results: UV-B photons have 4.13 eV, while red light photons have only 1.77 eV. This explains the biological effect: UV photons have enough energy to break chemical bonds in DNA and skin cells, while visible light photons don't.
Fatima is designing a half-wave dipole antenna for a 2.4 GHz WiFi application and needs to calculate the optimal element length.
Using the Antenna tab:
Result: Each dipole element should be 5.9 cm (2.3 inches). The full wavelength at 2.4 GHz is 12.5 cm, so half-wave is 6.25 cm before applying the velocity factor. This matches commercial WiFi antenna dimensions.
Dr. Patel studies whale communication and needs to know the wavelength of a 52 Hz "loneliest whale" call in seawater.
Using the Sound tab:
Result: The wavelength is 28.5 meters (93.5 feet). This explains why low-frequency whale calls travel vast distances through the ocean—wavelengths much larger than typical obstacles pass around them with minimal absorption.
Aisha is studying diagnostic radiology and wants to understand the relationship between X-ray photon energy (typically 20-150 keV) and wavelength.
Using the Energy↔Wavelength tab:
Result: A 50 keV X-ray photon has a wavelength of 0.0248 nm (24.8 pm). This is about 20,000 times shorter than visible light, which is why X-rays can penetrate soft tissue while visible light cannot.
James is analyzing the acoustic properties of a concert hall and needs wavelength data for the standard orchestral tuning pitch (A4 = 440 Hz) at normal room temperature.
Using the Sound tab:
Result: The wavelength is 78 cm (2.56 feet). The quarter-wavelength is 19.5 cm. James uses this to ensure diffuser panels and seat spacing don't create destructive interference at this critical frequency. The calculator also confirms this is note A4.
This wavelength calculator is designed for specific situations where you need to convert between wave properties or calculate wave characteristics. Here are the scenarios where it provides the most value:
These reference tables are based on the constants and formulas used in this calculator. Use them for quick lookups without needing to calculate.
The visible spectrum spans wavelengths from approximately 380 nm to 780 nm. This table shows the color ranges as defined in the calculator.
| Color | Wavelength Range | Frequency Range | Photon Energy |
|---|---|---|---|
| Violet | 380–450 nm | 668–789 THz | 2.76–3.26 eV |
| Blue | 450–485 nm | 618–668 THz | 2.56–2.76 eV |
| Cyan | 485–500 nm | 600–618 THz | 2.48–2.56 eV |
| Green | 500–565 nm | 531–600 THz | 2.19–2.48 eV |
| Yellow | 565–590 nm | 508–531 THz | 2.10–2.19 eV |
| Orange | 590–625 nm | 480–508 THz | 1.98–2.10 eV |
| Red | 625–780 nm | 384–480 THz | 1.59–1.98 eV |
Sound speed varies dramatically depending on the medium. These values are used by the Sound tab calculator.
| Medium | Speed (m/s) | Speed (ft/s) | 440 Hz Wavelength |
|---|---|---|---|
| Air at 0°C | 331.3 | 1087 | 75.3 cm |
| Air at 20°C | 343.4 | 1127 | 78.0 cm |
| Air at 30°C | 349.5 | 1147 | 79.4 cm |
| Water (20°C) | 1,480 | 4,856 | 3.36 m |
| Steel | 5,960 | 19,554 | 13.5 m |
For air, the calculator uses the formula: v = 331.3 + 0.606 × T (where T is temperature in °C).
These are the exact mass values used by the De Broglie tab. The masses are from CODATA 2018 values.
| Particle | Mass (kg) | Mass (×10⁻³¹ kg) | λ at 1×10⁶ m/s |
|---|---|---|---|
| Electron | 9.1093837 × 10⁻³¹ | 9.109 | 0.727 nm |
| Proton | 1.6726219 × 10⁻²⁷ | 1,672.6 | 0.396 pm |
| Neutron | 1.6749275 × 10⁻²⁷ | 1,674.9 | 0.395 pm |
Quick reference for ¼ wave vertical antenna lengths on popular amateur radio bands (with VF = 0.95).
| Band | Frequency | Full λ | ¼ Wave (VF=0.95) |
|---|---|---|---|
| 160m | 1.9 MHz | 157.8 m | 37.5 m (123 ft) |
| 80m | 3.7 MHz | 81.0 m | 19.2 m (63 ft) |
| 40m | 7.15 MHz | 41.9 m | 9.96 m (32.7 ft) |
| 20m | 14.2 MHz | 21.1 m | 5.01 m (16.4 ft) |
| 10m | 28.5 MHz | 10.5 m | 2.50 m (8.2 ft) |
| 2m | 146 MHz | 2.05 m | 48.8 cm (19.2 in) |
| 70cm | 440 MHz | 68.1 cm | 16.2 cm (6.4 in) |
The electromagnetic spectrum spans over 15 orders of magnitude in wavelength. This table shows each region with its properties and common applications.
| Region | Wavelength | Frequency | Photon Energy | Key Applications |
|---|---|---|---|---|
| Gamma rays | < 10 pm | > 30 EHz | > 124 keV | Cancer radiotherapy, nuclear imaging (PET), sterilization |
| Hard X-rays | 10–100 pm | 3–30 EHz | 12.4–124 keV | Medical CT scans, industrial inspection, crystallography |
| Soft X-rays | 0.1–10 nm | 30 PHz–3 EHz | 124 eV–12.4 keV | Dental X-rays, security scanners, material analysis |
| Extreme UV | 10–121 nm | 2.5–30 PHz | 10.2–124 eV | Semiconductor lithography (EUV), solar physics |
| UV-C | 100–280 nm | 1.07–3 PHz | 4.43–12.4 eV | Germicidal lamps, water purification |
| UV-B | 280–315 nm | 952 THz–1.07 PHz | 3.94–4.43 eV | Vitamin D production, sunburns |
| UV-A | 315–400 nm | 750–952 THz | 3.10–3.94 eV | Black lights, tanning, photolithography |
| Violet | 380–450 nm | 668–789 THz | 2.76–3.26 eV | Blu-ray lasers (405 nm) |
| Blue | 450–485 nm | 618–668 THz | 2.56–2.76 eV | Blue LEDs, LCD backlights |
| Cyan | 485–500 nm | 600–618 THz | 2.48–2.56 eV | Argon laser (488 nm) |
| Green | 500–565 nm | 531–600 THz | 2.19–2.48 eV | Green laser pointers (532 nm), traffic lights |
| Yellow | 565–590 nm | 508–531 THz | 2.10–2.19 eV | Sodium lamps (589 nm), warning lights |
| Orange | 590–625 nm | 480–508 THz | 1.98–2.10 eV | Neon signs, amber LEDs |
| Red | 625–780 nm | 384–480 THz | 1.59–1.98 eV | HeNe laser (633 nm), CD/DVD players, fiber optics |
| Near-IR | 780 nm–2.5 μm | 120–384 THz | 0.50–1.59 eV | Fiber optics (1310/1550 nm), night vision, remote controls |
| Mid-IR | 2.5–25 μm | 12–120 THz | 50–500 meV | IR spectroscopy, thermal cameras, heat seeking |
| Far-IR | 25 μm–1 mm | 300 GHz–12 THz | 1.2–50 meV | Terahertz imaging, astronomy |
| Microwave (EHF) | 1–10 mm | 30–300 GHz | 124–1240 μeV | 5G mmWave, satellite, radar |
| Microwave (SHF) | 1–10 cm | 3–30 GHz | 12.4–124 μeV | WiFi, radar, satellite dishes |
| Microwave (UHF) | 10 cm–1 m | 300 MHz–3 GHz | 1.24–12.4 μeV | TV, cellular, GPS, Bluetooth |
| Radio (VHF) | 1–10 m | 30–300 MHz | 124–1240 neV | FM radio, aircraft, amateur radio |
| Radio (HF) | 10–100 m | 3–30 MHz | 12.4–124 neV | Shortwave radio, amateur radio, aviation |
| Radio (MF) | 100–1000 m | 300 kHz–3 MHz | 1.24–12.4 neV | AM radio, maritime navigation |
| Radio (LF/VLF) | 1–100 km | 3–300 kHz | 12.4 peV–1.24 neV | Navigation (LORAN), submarine comms, time signals |
Common wireless standards and their operating frequencies and wavelengths.
| Technology | Frequency | Wavelength | ¼ Wave Antenna |
|---|---|---|---|
| AM Radio | 540–1700 kHz | 176–556 m | 44–139 m |
| FM Radio | 88–108 MHz | 2.78–3.41 m | 69–85 cm |
| GPS (L1) | 1.575 GHz | 19.0 cm | 4.76 cm |
| Bluetooth | 2.4 GHz | 12.5 cm | 3.12 cm |
| WiFi 2.4G | 2.4 GHz | 12.5 cm | 3.12 cm |
| WiFi 5G | 5.0 GHz | 6.0 cm | 1.50 cm |
| WiFi 6E | 6.0 GHz | 5.0 cm | 1.25 cm |
| 4G LTE | 700 MHz–2.6 GHz | 11.5–42.8 cm | 2.9–10.7 cm |
| 5G Sub-6 | 3.5 GHz | 8.6 cm | 2.14 cm |
| 5G mmWave | 28 GHz | 10.7 mm | 2.68 mm |
| LoRa | 868/915 MHz | 33–35 cm | 8.2–8.6 cm |
| Starlink | 10.7–12.7 GHz | 2.4–2.8 cm | 0.6–0.7 cm |
Putting wavelengths in perspective by comparing them to familiar objects.
| Wavelength | Wave Type | Size Comparison |
|---|---|---|
| 0.001 nm (1 pm) | Gamma ray | Smaller than an atomic nucleus |
| 0.1 nm (1 Å) | X-ray | Size of a hydrogen atom |
| 10 nm | Extreme UV | Width of cell membrane |
| 400–700 nm | Visible light | Smaller than a bacterium (1 μm) |
| 10 μm | Mid-infrared | Size of a red blood cell |
| 1 mm | Far-IR / microwave | Thickness of a credit card |
| 12.5 cm | WiFi (2.4 GHz) | Width of a smartphone |
| 3 m | FM radio (100 MHz) | Height of a room ceiling |
| 78 cm | Sound: A4 (440 Hz) | Width of a desk |
| 17 m | Sound: 20 Hz (bass) | Length of a bowling lane |
| 3,945 km | ELF radio (76 Hz) | Distance: LA to New York |
Standard laser types and their emission wavelengths, used in industry, medicine, and research.
| Laser Type | Wavelength | Frequency | Common Applications |
|---|---|---|---|
| ArF excimer | 193 nm | 1,553 THz | Semiconductor lithography, eye surgery (LASIK) |
| KrF excimer | 248 nm | 1,209 THz | Lithography, micromachining |
| Nitrogen (N2) | 337 nm | 890 THz | Dye laser pumping, spectroscopy |
| Blu-ray diode | 405 nm | 740 THz | Data storage, 3D printing |
| Argon-ion | 488 nm | 614 THz | Confocal microscopy, flow cytometry |
| Nd:YAG (doubled) | 532 nm | 564 THz | Green laser pointers, LIDAR |
| HeNe | 633 nm | 474 THz | Alignment, interferometry, holography |
| Ruby | 694 nm | 432 THz | Tattoo removal, holography |
| GaAs diode | 850 nm | 353 THz | Short-range fiber optics, CD players |
| Nd:YAG | 1,064 nm | 282 THz | Cutting, welding, medical surgery |
| Telecom (C-band) | 1,550 nm | 193 THz | Long-haul fiber optic communications |
| CO2 | 10,600 nm | 28.3 THz | Industrial cutting, engraving, surgery |
This calculator uses standard physics equations. Here are the formulas with explanations and worked examples.
Worked example: Calculate the wavelength of a 100 MHz FM radio signal.
λ = c / f = 299,792,458 m/s ÷ 100,000,000 Hz = 2.998 m ≈ 3 meters
Worked example: Calculate the de Broglie wavelength of an electron traveling at 2 × 10⁶ m/s.
p = m × v = 9.109 × 10⁻³¹ kg × 2 × 10⁶ m/s = 1.822 × 10⁻²⁴ kg·m/s
λ = h / p = 6.626 × 10⁻³⁴ / 1.822 × 10⁻²⁴ = 3.64 × 10⁻¹⁰ m = 0.364 nm
Useful constant: hc = 1240 eV·nm (memorize this for quick calculations!)
Worked example: Calculate the energy of a 620 nm (orange light) photon.
E = hc / λ = 1240 eV·nm / 620 nm = 2.0 eV
Speed of sound in air: v = 331.3 + 0.606 × T (T in °C)
Worked example: Calculate the wavelength of a 1000 Hz tone in air at 25°C.
v = 331.3 + 0.606 × 25 = 346.5 m/s
λ = 346.5 / 1000 = 0.347 m = 34.7 cm
Worked example: Calculate a ½ wave dipole for 14.2 MHz with VF = 0.95.
λ = 299,792,458 / 14,200,000 = 21.11 m
L = (21.11 × 0.95) / 2 = 10.03 m (32.9 ft)
Worked example: Convert 500 nm to wavenumber.
k = 1 / (500 × 10⁻⁹ m) = 2 × 10⁶ m⁻¹ = 20,000 cm⁻¹
k (angular) = 2π × 2 × 10⁶ = 1.26 × 10⁷ rad/m
After calculating, you may wonder: "Is this result reasonable?" Here's how to interpret results from each tab.
What the numbers mean:
Sanity checks:
What the numbers mean:
Typical ranges:
When results matter: De Broglie wavelengths are significant when comparable to the size of structures being probed (atoms ≈ 0.1-0.3 nm, atomic spacing in crystals ≈ 0.2-0.5 nm).
What the numbers mean:
Reference points:
What the numbers mean:
Practical ranges:
What the numbers mean:
Practical considerations:
What the numbers mean:
Typical ranges in spectroscopy:
This calculator handles three fundamentally different types of waves. Understanding their differences helps you choose the right calculation.
| Property | EM Waves | Sound Waves | Matter Waves |
|---|---|---|---|
| What oscillates | Electric and magnetic fields | Pressure in medium | Quantum probability amplitude |
| Requires medium | No (travels through vacuum) | Yes (air, water, solid) | No (quantum phenomenon) |
| Typical speed | 299,792,458 m/s (in vacuum) | 343 m/s in air | Particle-dependent |
| Speed varies with | Medium (slower in glass, water) | Medium, temperature | Particle velocity |
| Wavelength range | 10⁻¹² m to 10⁴ m | 0.017 m to 17 m (audible) | 10⁻¹² m to 10⁻⁹ m (typical) |
| Formula | λ = c/f | λ = vsound/f | λ = h/(mv) |
| Governing equation | Maxwell's equations | Wave equation in fluids | Schrödinger equation |
| Applications | Radio, light, X-rays | Music, sonar, ultrasound | Electron microscopy, diffraction |
Key insight: The fundamental wave relationship λ = v/f applies to both EM and sound waves, but the "velocity" means very different things. For matter waves, the de Broglie relation λ = h/p is a quantum mechanical result with no classical analogue.
Dive deeper into wave physics with our comprehensive guides. Each article expands on the concepts used in this calculator.
Master the fundamental wave equation with detailed derivations, examples, and applications across different wave types.
Complete reference guide to the EM spectrum from gamma rays to radio waves, with wavelength ranges and applications.
Understand wave-particle duality and learn how to calculate the quantum wavelength of electrons and other particles.
The Planck-Einstein relation explained: how photon energy relates to wavelength and frequency.
Calculate acoustic wavelengths in air, water, and other media. Includes temperature effects and musical applications.
Design antennas for any frequency band with velocity factor corrections and practical construction tips.
Expand your understanding with these additional guides covering related topics:
Step-by-step conversion methods with unit handling tips.
Essential for IR and Raman spectroscopy applications.
How c = λf connects these fundamental quantities.
The physics of color perception and spectral ranges.
The wavelength formula is λ = v/f, where λ (lambda) is wavelength in meters, v is wave speed in m/s, and f is frequency in Hz. For electromagnetic waves like light, this becomes λ = c/f where c is the speed of light (299,792,458 m/s). This fundamental relationship shows that wavelength and frequency are inversely proportional—higher frequencies have shorter wavelengths. Learn more in our complete guide to the wavelength formula.
To convert frequency to wavelength, divide the wave speed by the frequency: λ = v/f. For electromagnetic waves in vacuum, use the speed of light (c = 299,792,458 m/s). For example, 500 THz light has wavelength: 299,792,458 ÷ (500 × 10¹²) = 600 nm (orange light). Remember to convert frequency to Hz and wavelength to meters when using SI units. Our frequency to wavelength conversion guide covers unit conversions in detail.
The de Broglie wavelength describes the quantum mechanical wave nature of matter. Every moving particle has an associated wavelength calculated as λ = h/p = h/(mv), where h is Planck's constant (6.626 × 10⁻³⁴ J·s), m is mass, and v is velocity. Faster or heavier particles have shorter wavelengths. This wave behavior is significant for subatomic particles but negligible for macroscopic objects. Read our de Broglie wavelength guide for applications in electron microscopy and quantum physics.
Photon energy and wavelength are inversely related through the Planck-Einstein equation: E = hc/λ, where h is Planck's constant and c is the speed of light. This can be simplified to E(eV) = 1240/λ(nm). Shorter wavelengths (like X-rays and gamma rays) carry more energy than longer wavelengths (like radio waves). This explains why UV light can cause sunburn while visible light doesn't—UV photons have enough energy to damage DNA. See our photon energy guide for more details.
Sound wavelength uses the same formula λ = v/f, but with the speed of sound instead of light. In air at 20°C, sound travels at about 343 m/s. So a 440 Hz tone (A4) has a wavelength of 343 ÷ 440 = 0.78 m. Sound speed varies with temperature (v = 331.3 + 0.606×T in air) and is much faster in water (1480 m/s) and steel (5960 m/s). Our sound wavelength guide covers acoustic applications.
Visible light spans approximately 380-780 nm. Violet light has the shortest wavelengths (380-450 nm), followed by blue (450-485 nm), cyan (485-500 nm), green (500-565 nm), yellow (565-590 nm), orange (590-625 nm), and red (625-780 nm). Each color corresponds to a specific frequency range and photon energy. Our calculator automatically identifies colors for visible wavelengths. Explore the full visible light wavelength and color guide.
First calculate the wavelength: λ = c/f where c = 299,792,458 m/s. Then divide by the antenna type factor: ¼ wave = λ/4, ½ wave dipole = λ/2, full wave = λ. Finally, multiply by the velocity factor (typically 0.95 for wire, 0.66 for coax) to get the physical length. For example, a ¼ wave antenna at 146 MHz: λ = 2.05 m, ¼ wave = 51.3 cm, with VF=0.95 gives 48.8 cm. See our antenna calculator guide for detailed instructions.
Wavenumber (k) is the reciprocal of wavelength: k = 1/λ, typically expressed in cm⁻¹ for spectroscopy. It's directly proportional to energy (unlike wavelength which is inversely proportional), making it convenient for comparing spectral features. The angular wavenumber k = 2π/λ (in rad/m) appears in wave equations. Infrared spectroscopy commonly uses wavenumbers, with the mid-IR range spanning 400-4000 cm⁻¹. Learn more in our wavenumber conversion guide.
This calculator uses the official SI values for physical constants: speed of light (299,792,458 m/s, exact by definition), Planck's constant (6.62607015 × 10⁻³⁴ J·s, exact by 2019 SI redefinition), and CODATA values for particle masses. Results are accurate for educational and practical applications. However, for professional or safety-critical work, always verify calculations independently. The de Broglie calculator uses non-relativistic equations, so results become approximate for particles above ~10% of light speed.
The electromagnetic spectrum encompasses all types of electromagnetic radiation, arranged by wavelength or frequency. From shortest to longest wavelength: gamma rays (<10 pm), X-rays (10 pm–10 nm), ultraviolet (10–400 nm), visible light (400–700 nm), infrared (700 nm–1 mm), microwaves (1 mm–1 m), and radio waves (>1 m). All EM waves travel at the speed of light in vacuum but have vastly different properties and applications. Explore our complete electromagnetic spectrum reference guide.
The wavelength of visible light is incredibly small—about 400-700 billionths of a meter. Yet radio waves can have wavelengths measured in kilometers. Both are electromagnetic radiation traveling at the same speed (c), differing only in frequency. At the other extreme, the de Broglie wavelength of a baseball moving at 40 m/s is about 10⁻³⁴ meters—far too small to ever observe quantum effects in everyday objects!
Calculator last updated: January 2026 · Data verified against CODATA 2018 and 2019 SI definitions