Wavelength Calculator

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.

Key Takeaways

  • Wavelength and frequency are inversely related: λ = v/f — double the frequency, halve the wavelength
  • Speed of light: 299,792,458 m/s (exact by SI definition) — use this for all electromagnetic wave calculations
  • Visible light: 400–700 nm wavelength, 430–750 THz frequency, 1.7–3.1 eV photon energy
  • Sound vs. light: Sound is ~1 million times slower — sound wavelengths are measured in meters, light in nanometers
  • De Broglie wavelength: λ = h/(mv) — particles act like waves at quantum scales (electrons ~0.1–1 nm)
  • Antenna sizing: Physical length ≈ wavelength/n × velocity factor (typically 0.95 for wire antennas)
λ = v / f
Wavelength = Wave Speed ÷ Frequency
m/s
Wavelength (λ)
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Wavelength
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Frequency
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Wave Speed
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EM Spectrum Classification
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Electromagnetic Spectrum Position
γ
X
UV
Vis
IR
μW
Radio
λ = h / (m × v) = h / p
De Broglie wavelength of matter waves
De Broglie Wavelength
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--
Momentum (p)
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E = hc / λ = hf
Photon energy ↔ Wavelength (Planck-Einstein relation)
Wavelength
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Wavelength
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Energy
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Frequency
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Classification
--
λ = vsound / f
Sound wavelength in various media
Hz
A4 = 440 Hz, middle C = 262 Hz
°C
Sound Wavelength
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Meters
--
Centimeters
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Feet
--
Inches
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Speed Used
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¼ Wavelength
--
Musical Note
--
L = λ × VF / n
Antenna length with velocity factor
1.0 = free space, 0.66 = coax, 0.95 = wire
Antenna Length
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Full Wavelength
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Physical Length
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Adjusted
--
k = 1/λ   or   k = 2π/λ
Wavenumber (spectroscopic & angular)
Wavenumber (k)
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Wavenumber (m⁻¹)
--
Angular (rad/m)
--
Wavelength
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Wavelength Formula

The wavelength formula relates wavelength (λ), frequency (f), and wave speed (v):

λ = v / f

For electromagnetic waves (light, radio, X-rays), the wave speed is the speed of light:

λ = c / f   where c = 299,792,458 m/s

This fundamental relationship means higher frequency waves have shorter wavelengths, and vice versa. Understanding this inverse relationship is key to frequency to wavelength conversions.

Electromagnetic Spectrum

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.

TypeWavelengthFrequencyApplications
Gamma rays< 10 pm> 30 EHzMedical imaging, cancer treatment
X-rays10 pm - 10 nm30 PHz - 30 EHzMedical imaging, security
Ultraviolet10 nm - 400 nm750 THz - 30 PHzSterilization, black lights
Visible light400 nm - 700 nm430 THz - 750 THzHuman vision, displays
Infrared700 nm - 1 mm300 GHz - 430 THzRemote controls, thermal imaging
Microwave1 mm - 1 m300 MHz - 300 GHzWiFi, radar, cooking
Radio> 1 m< 300 MHzBroadcasting, communication

The photon energy varies across the spectrum—see how photon energy relates to wavelength through the Planck-Einstein relation (E = hc/λ).

How to Use This Calculator

This wavelength calculator provides six specialized tools for different wave physics calculations. Here's how to use each tab effectively:

Wave Basics Tab

The Wave Basics calculator uses the fundamental wave equation λ = v/f to convert between wavelength, frequency, and wave speed.

  1. Select what to solve for: Choose wavelength (λ), frequency (f), or wave speed (v) using the radio buttons at the top
  2. Set the wave speed: Keep "Speed of light" checked for electromagnetic waves (light, radio, X-rays). Uncheck it to enter a custom speed for other wave types
  3. Enter your known value: If solving for wavelength, enter the frequency. If solving for frequency, enter the wavelength. If solving for speed, enter both
  4. Select appropriate units: Use the dropdown menus to match your input (Hz, kHz, MHz, GHz, THz for frequency; m, cm, mm, μm, nm, Å for wavelength)
  5. Click Calculate: Results show wavelength, frequency, speed, electromagnetic spectrum classification, and a visual wave representation

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).

De Broglie Tab

Calculate the quantum mechanical wavelength of particles using λ = h/(mv), the de Broglie equation.

  1. Select particle type: Choose electron, proton, neutron, or custom. The calculator uses precise particle masses (electron: 9.109×10⁻³¹ kg)
  2. Enter velocity: Input the particle speed in m/s, or use "× c" to enter as a fraction of light speed (e.g., 0.01 for 1% of c)
  3. For custom particles: Enter the mass in units of 10⁻³¹ kg. An electron is 9.109, a proton is 1672.6
  4. Click Calculate: Results show the de Broglie wavelength and particle momentum

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.

Energy↔Wavelength Tab

Convert between photon energy and wavelength using the Planck-Einstein relation E = hc/λ.

  1. Select conversion direction: Choose "Wavelength from Energy" if you know the photon energy, or "Energy from Wavelength" if you know the wavelength
  2. Enter your known value: For energy, use eV (electron volts), keV, MeV, or J (joules). For wavelength, use nm, μm, Å, or m
  3. Click Calculate: Results show the converted value plus frequency and EM spectrum classification

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.

Sound Tab

Calculate acoustic wavelengths in different media using λ = v/f with the speed of sound.

  1. Enter frequency: Input the sound frequency in Hz. Common references: A4 = 440 Hz, middle C = 262 Hz, human hearing range is 20-20,000 Hz
  2. Select medium: Choose air (temperature-dependent), water (1480 m/s), steel (5960 m/s), or enter a custom speed
  3. Set temperature: For air, enter the temperature in °C. Sound speed in air is calculated as 331.3 + 0.606×T m/s
  4. Click Calculate: Results show wavelength in multiple units (m, cm, ft, in), the speed used, quarter-wavelength, and the nearest musical note

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.

Antenna Tab

Calculate antenna dimensions for radio frequency applications using L = λ × VF / n.

  1. Enter operating frequency: Input the frequency in kHz, MHz, or GHz. Common amateur bands: 2m (144-148 MHz), 70cm (420-450 MHz)
  2. Set velocity factor: Use 1.0 for free space (theoretical), 0.95 for typical wire antennas, 0.66 for coaxial cable
  3. Select antenna type: Choose ¼ wave (ground plane, vertical), ½ wave (dipole), or full wave
  4. Click Calculate: Results show the physical antenna length in both metric and imperial units

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.

Wavenumber Tab

Convert between wavelength and wavenumber using k = 1/λ (spectroscopic) or k = 2π/λ (angular).

  1. Select conversion direction: Choose wavelength to wavenumber or wavenumber to wavelength
  2. Enter your value: Wavelength in nm, μm, m, or cm. Wavenumber in cm⁻¹ or m⁻¹
  3. Click Calculate: Results show both spectroscopic wavenumber (cm⁻¹) and angular wavenumber (rad/m), plus the corresponding wavelength

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.

Common Mistakes to Avoid

  • Unit confusion: Always check that your unit selection matches your input. 500 MHz is very different from 500 THz
  • Speed of sound vs. light: Sound travels about a million times slower than light. Make sure you're using the correct speed for your wave type
  • Temperature effects: Sound speed in air varies significantly with temperature—about 0.6 m/s per degree Celsius
  • Velocity factor: Real antennas are shorter than the theoretical length. Always apply the velocity factor for accurate results
  • Relativistic particles: The de Broglie calculator uses classical equations. For particles approaching light speed, results become approximate

Pro Tip: Quick Mental Math

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.

Real-World Examples

These examples illustrate how different people use the wavelength calculator in practical situations. All calculations use the actual formulas and constants from this calculator.

Example 1: Physics Student Studying Visible Light

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:

  • Selects "Frequency (f)" as the solve target
  • Keeps "Speed of light" checked (c = 299,792,458 m/s)
  • Enters 550 in the wavelength field and selects "nm"
  • Clicks Calculate

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.

Example 2: Ham Radio Operator Building an Antenna

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:

  • Enters 146 in the frequency field and selects "MHz"
  • Sets velocity factor to 0.95 (standard for wire antennas)
  • Selects "¼ Wave" antenna type
  • Clicks Calculate

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.

Example 3: Audio Engineer Treating a Recording Studio

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:

  • Enters 80 in the frequency field (Hz)
  • Selects "Air (temp-dependent)" as the medium
  • Enters 22 for temperature
  • Clicks Calculate

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.

Example 4: Chemistry Student in Spectroscopy Lab

David needs to convert an infrared absorption peak from wavelength (3400 nm) to wavenumber for his IR spectroscopy report.

Using the Wavenumber tab:

  • Selects "Wavelength → Wavenumber"
  • Enters 3400 in wavelength field and selects "nm"
  • Clicks Calculate

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.

Example 5: Graduate Student Calculating Electron Wavelength

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:

  • Selects "Electron" as the particle type
  • Enters 0.005 in velocity field and selects "× c"
  • Clicks Calculate

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.

Example 6: High School Teacher Demonstrating Energy-Wavelength Relationship

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:

  • For UV-B light (300 nm): Selects "Energy from Wavelength," enters 300 nm
  • For red light (700 nm): Enters 700 nm
  • Compares results

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.

Example 7: RF Engineer Checking WiFi Antenna Design

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:

  • Enters 2.4 in frequency field and selects "GHz"
  • Sets velocity factor to 0.95 for the antenna wire
  • Selects "½ Wave Dipole"
  • Clicks Calculate

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.

Example 8: Underwater Acoustics Researcher

Dr. Patel studies whale communication and needs to know the wavelength of a 52 Hz "loneliest whale" call in seawater.

Using the Sound tab:

  • Enters 52 in frequency field (Hz)
  • Selects "Water (~1480 m/s)" as the medium
  • Clicks Calculate

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.

Example 9: Medical Physics Student Studying X-rays

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:

  • Selects "Wavelength from Energy"
  • Enters 50 in energy field and selects "keV" (typical chest X-ray)
  • Clicks Calculate

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.

Example 10: Concert Hall Acoustician

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:

  • Enters 440 in frequency field (Hz)
  • Selects "Air (temp-dependent)"
  • Enters 20 for temperature (°C)
  • Clicks Calculate

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.

When to Use This Calculator

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:

Education and Learning

  • Physics homework and exams: Verify your hand calculations for wave problems, or quickly explore "what if" scenarios to build intuition
  • Understanding the electromagnetic spectrum: See how frequency and wavelength relate across radio waves, microwaves, light, and X-rays
  • Quantum mechanics concepts: Explore de Broglie wavelengths to understand wave-particle duality
  • Lab preparation: Calculate expected values before running experiments in optics or spectroscopy labs

Amateur Radio and RF Engineering

  • Antenna design: Calculate the physical length of dipoles, verticals, and other antennas for any frequency band
  • Band planning: Convert between frequency and wavelength when discussing or documenting amateur radio bands
  • Feedline calculations: Determine wavelength for cutting coax to specific electrical lengths

Audio and Acoustics

  • Room acoustics: Calculate wavelengths for bass trapping, diffuser design, and absorber placement
  • Speaker placement: Determine quarter-wavelength distances to avoid acoustic cancellation
  • Musical instrument design: Relate pipe or string lengths to their resonant frequencies

Spectroscopy and Chemistry

  • IR spectroscopy: Convert between wavelength (nm, μm) and wavenumber (cm⁻¹) for spectral analysis
  • UV-Vis spectroscopy: Calculate photon energy from wavelength to understand electronic transitions
  • Raman spectroscopy: Work with wavenumber shifts and their corresponding wavelengths

Research and Professional Applications

  • Electron microscopy: Calculate de Broglie wavelengths for electrons at various accelerating voltages
  • X-ray crystallography: Relate X-ray energy to wavelength for diffraction experiments
  • Telecommunications: Convert between frequency allocations and wavelength (fiber optics, wireless systems)

Who Benefits Most

  • Students: From high school physics through graduate studies in physics, chemistry, engineering, and related fields
  • Educators: Teachers demonstrating wave concepts or preparing examples for class
  • Amateur radio operators: Hams designing antennas or understanding propagation
  • Audio professionals: Sound engineers, acousticians, and studio designers
  • Researchers: Scientists needing quick conversions for spectroscopy, microscopy, or wave physics
  • Hobbyists: Anyone curious about wave physics, from telescope builders to synthesizer enthusiasts

Quick Reference Tables

These reference tables are based on the constants and formulas used in this calculator. Use them for quick lookups without needing to calculate.

Visible Light Colors and Wavelengths

The visible spectrum spans wavelengths from approximately 380 nm to 780 nm. This table shows the color ranges as defined in the calculator.

ColorWavelength RangeFrequency RangePhoton Energy
Violet380–450 nm668–789 THz2.76–3.26 eV
Blue450–485 nm618–668 THz2.56–2.76 eV
Cyan485–500 nm600–618 THz2.48–2.56 eV
Green500–565 nm531–600 THz2.19–2.48 eV
Yellow565–590 nm508–531 THz2.10–2.19 eV
Orange590–625 nm480–508 THz1.98–2.10 eV
Red625–780 nm384–480 THz1.59–1.98 eV

Speed of Sound in Different Media

Sound speed varies dramatically depending on the medium. These values are used by the Sound tab calculator.

MediumSpeed (m/s)Speed (ft/s)440 Hz Wavelength
Air at 0°C331.3108775.3 cm
Air at 20°C343.4112778.0 cm
Air at 30°C349.5114779.4 cm
Water (20°C)1,4804,8563.36 m
Steel5,96019,55413.5 m

For air, the calculator uses the formula: v = 331.3 + 0.606 × T (where T is temperature in °C).

Particle Masses for De Broglie Calculations

These are the exact mass values used by the De Broglie tab. The masses are from CODATA 2018 values.

ParticleMass (kg)Mass (×10⁻³¹ kg)λ at 1×10⁶ m/s
Electron9.1093837 × 10⁻³¹9.1090.727 nm
Proton1.6726219 × 10⁻²⁷1,672.60.396 pm
Neutron1.6749275 × 10⁻²⁷1,674.90.395 pm

Common Amateur Radio Bands and Antenna Lengths

Quick reference for ¼ wave vertical antenna lengths on popular amateur radio bands (with VF = 0.95).

BandFrequencyFull λ¼ Wave (VF=0.95)
160m1.9 MHz157.8 m37.5 m (123 ft)
80m3.7 MHz81.0 m19.2 m (63 ft)
40m7.15 MHz41.9 m9.96 m (32.7 ft)
20m14.2 MHz21.1 m5.01 m (16.4 ft)
10m28.5 MHz10.5 m2.50 m (8.2 ft)
2m146 MHz2.05 m48.8 cm (19.2 in)
70cm440 MHz68.1 cm16.2 cm (6.4 in)

Full Electromagnetic Spectrum Reference

The electromagnetic spectrum spans over 15 orders of magnitude in wavelength. This table shows each region with its properties and common applications.

RegionWavelengthFrequencyPhoton EnergyKey Applications
Gamma rays< 10 pm> 30 EHz> 124 keVCancer radiotherapy, nuclear imaging (PET), sterilization
Hard X-rays10–100 pm3–30 EHz12.4–124 keVMedical CT scans, industrial inspection, crystallography
Soft X-rays0.1–10 nm30 PHz–3 EHz124 eV–12.4 keVDental X-rays, security scanners, material analysis
Extreme UV10–121 nm2.5–30 PHz10.2–124 eVSemiconductor lithography (EUV), solar physics
UV-C100–280 nm1.07–3 PHz4.43–12.4 eVGermicidal lamps, water purification
UV-B280–315 nm952 THz–1.07 PHz3.94–4.43 eVVitamin D production, sunburns
UV-A315–400 nm750–952 THz3.10–3.94 eVBlack lights, tanning, photolithography
Violet380–450 nm668–789 THz2.76–3.26 eVBlu-ray lasers (405 nm)
Blue450–485 nm618–668 THz2.56–2.76 eVBlue LEDs, LCD backlights
Cyan485–500 nm600–618 THz2.48–2.56 eVArgon laser (488 nm)
Green500–565 nm531–600 THz2.19–2.48 eVGreen laser pointers (532 nm), traffic lights
Yellow565–590 nm508–531 THz2.10–2.19 eVSodium lamps (589 nm), warning lights
Orange590–625 nm480–508 THz1.98–2.10 eVNeon signs, amber LEDs
Red625–780 nm384–480 THz1.59–1.98 eVHeNe laser (633 nm), CD/DVD players, fiber optics
Near-IR780 nm–2.5 μm120–384 THz0.50–1.59 eVFiber optics (1310/1550 nm), night vision, remote controls
Mid-IR2.5–25 μm12–120 THz50–500 meVIR spectroscopy, thermal cameras, heat seeking
Far-IR25 μm–1 mm300 GHz–12 THz1.2–50 meVTerahertz imaging, astronomy
Microwave (EHF)1–10 mm30–300 GHz124–1240 μeV5G mmWave, satellite, radar
Microwave (SHF)1–10 cm3–30 GHz12.4–124 μeVWiFi, radar, satellite dishes
Microwave (UHF)10 cm–1 m300 MHz–3 GHz1.24–12.4 μeVTV, cellular, GPS, Bluetooth
Radio (VHF)1–10 m30–300 MHz124–1240 neVFM radio, aircraft, amateur radio
Radio (HF)10–100 m3–30 MHz12.4–124 neVShortwave radio, amateur radio, aviation
Radio (MF)100–1000 m300 kHz–3 MHz1.24–12.4 neVAM radio, maritime navigation
Radio (LF/VLF)1–100 km3–300 kHz12.4 peV–1.24 neVNavigation (LORAN), submarine comms, time signals

Wireless Technology Frequencies

Common wireless standards and their operating frequencies and wavelengths.

TechnologyFrequencyWavelength¼ Wave Antenna
AM Radio540–1700 kHz176–556 m44–139 m
FM Radio88–108 MHz2.78–3.41 m69–85 cm
GPS (L1)1.575 GHz19.0 cm4.76 cm
Bluetooth2.4 GHz12.5 cm3.12 cm
WiFi 2.4G2.4 GHz12.5 cm3.12 cm
WiFi 5G5.0 GHz6.0 cm1.50 cm
WiFi 6E6.0 GHz5.0 cm1.25 cm
4G LTE700 MHz–2.6 GHz11.5–42.8 cm2.9–10.7 cm
5G Sub-63.5 GHz8.6 cm2.14 cm
5G mmWave28 GHz10.7 mm2.68 mm
LoRa868/915 MHz33–35 cm8.2–8.6 cm
Starlink10.7–12.7 GHz2.4–2.8 cm0.6–0.7 cm

Real-World Wavelength Scale Comparisons

Putting wavelengths in perspective by comparing them to familiar objects.

WavelengthWave TypeSize Comparison
0.001 nm (1 pm)Gamma raySmaller than an atomic nucleus
0.1 nm (1 Å)X-raySize of a hydrogen atom
10 nmExtreme UVWidth of cell membrane
400–700 nmVisible lightSmaller than a bacterium (1 μm)
10 μmMid-infraredSize of a red blood cell
1 mmFar-IR / microwaveThickness of a credit card
12.5 cmWiFi (2.4 GHz)Width of a smartphone
3 mFM radio (100 MHz)Height of a room ceiling
78 cmSound: A4 (440 Hz)Width of a desk
17 mSound: 20 Hz (bass)Length of a bowling lane
3,945 kmELF radio (76 Hz)Distance: LA to New York

Common Laser Wavelengths

Standard laser types and their emission wavelengths, used in industry, medicine, and research.

Laser TypeWavelengthFrequencyCommon Applications
ArF excimer193 nm1,553 THzSemiconductor lithography, eye surgery (LASIK)
KrF excimer248 nm1,209 THzLithography, micromachining
Nitrogen (N2)337 nm890 THzDye laser pumping, spectroscopy
Blu-ray diode405 nm740 THzData storage, 3D printing
Argon-ion488 nm614 THzConfocal microscopy, flow cytometry
Nd:YAG (doubled)532 nm564 THzGreen laser pointers, LIDAR
HeNe633 nm474 THzAlignment, interferometry, holography
Ruby694 nm432 THzTattoo removal, holography
GaAs diode850 nm353 THzShort-range fiber optics, CD players
Nd:YAG1,064 nm282 THzCutting, welding, medical surgery
Telecom (C-band)1,550 nm193 THzLong-haul fiber optic communications
CO210,600 nm28.3 THzIndustrial cutting, engraving, surgery

Formula Reference

This calculator uses standard physics equations. Here are the formulas with explanations and worked examples.

Wave Equation (Wave Basics Tab)

λ = v / f
Wavelength equals wave speed divided by frequency
  • λ (lambda) = wavelength in meters (m)
  • v = wave speed in meters per second (m/s)
  • f = frequency in Hertz (Hz, cycles per second)

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

De Broglie Equation (De Broglie Tab)

λ = h / (m × v) = h / p
De Broglie wavelength equals Planck's constant divided by momentum
  • λ = de Broglie wavelength in meters (m)
  • h = Planck's constant = 6.62607015 × 10⁻³⁴ J·s
  • m = particle mass in kilograms (kg)
  • v = velocity in meters per second (m/s)
  • p = momentum = m × v (kg·m/s)

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

Planck-Einstein Relation (Energy↔Wavelength Tab)

E = hc / λ = hf
Photon energy equals Planck's constant times the speed of light, divided by wavelength
  • E = photon energy in joules (J) or electron volts (eV)
  • h = Planck's constant = 6.626 × 10⁻³⁴ J·s = 4.136 × 10⁻¹⁵ eV·s
  • c = speed of light = 299,792,458 m/s
  • λ = wavelength in meters (m)
  • f = frequency in Hertz (Hz)

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

Sound Wavelength (Sound Tab)

λ = vsound / f
Same wave equation, using speed of sound instead of light

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

Antenna Length (Antenna Tab)

L = (λ × VF) / n
Physical antenna length with velocity factor adjustment
  • L = physical antenna length in meters
  • λ = free-space wavelength = c / f
  • VF = velocity factor (typically 0.95 for wire, 0.66 for coax)
  • n = divisor (4 for ¼ wave, 2 for ½ wave, 1 for full wave)

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)

Wavenumber Conversions (Wavenumber Tab)

k = 1/λ (spectroscopic)    k = 2π/λ (angular)
Wavenumber is the spatial frequency of a wave
  • k (spectroscopic) = wavenumber in m⁻¹ or cm⁻¹
  • k (angular) = angular wavenumber in rad/m
  • λ = wavelength

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

Understanding Your Results

After calculating, you may wonder: "Is this result reasonable?" Here's how to interpret results from each tab.

Wave Basics Results

What the numbers mean:

  • Wavelength: The physical distance between wave peaks. For EM waves, this determines how the wave interacts with matter
  • Frequency: How many wave cycles pass a point per second. Higher frequency = more energy (for photons)
  • EM Classification: Shows where your wave falls on the electromagnetic spectrum

Sanity checks:

  • Radio waves: wavelengths > 1 m, frequencies < 300 MHz
  • Visible light: wavelengths 400-700 nm, frequencies 430-750 THz
  • X-rays: wavelengths < 10 nm, frequencies > 30 PHz
  • If your EM wave has a wavelength in kilometers, it's very low frequency radio (VLF)
  • If your wavelength is in picometers, you're in the X-ray/gamma ray range

De Broglie Results

What the numbers mean:

  • De Broglie wavelength: The scale at which quantum wave behavior becomes significant
  • Momentum: The classical momentum (mass × velocity) of the particle

Typical ranges:

  • Electrons at typical lab velocities (10⁶ m/s): λ ≈ 0.7 nm
  • Electrons in electron microscopes: λ ≈ 0.01-0.1 nm (much smaller than visible light)
  • Thermal neutrons: λ ≈ 0.1-0.2 nm (useful for diffraction studies)
  • Macroscopic objects: λ is so small it's unmeasurable (quantum effects invisible)

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).

Energy↔Wavelength Results

What the numbers mean:

  • Photon energy: The amount of energy a single photon carries. Higher energy photons can break chemical bonds or ionize atoms
  • Wavelength: Inversely related to energy—shorter wavelengths carry more energy

Reference points:

  • Chemical bond energies: 1-10 eV (this is why UV and X-rays can damage DNA)
  • Visible light: 1.7-3.1 eV (not enough to break most bonds)
  • Infrared: < 1.7 eV (causes molecular vibrations, perceived as heat)
  • X-rays: 100 eV - 100 keV (ionizing radiation)
  • Gamma rays: > 100 keV (highly penetrating, used in cancer treatment)

Sound Results

What the numbers mean:

  • Wavelength: The physical size of sound waves—important for acoustic design
  • Quarter-wavelength: Key dimension for acoustic treatment. Bass traps need thickness ~¼λ to absorb effectively
  • Musical note: Helps identify the pitch corresponding to your frequency

Practical ranges:

  • Bass frequencies (20-200 Hz): wavelengths 1.7-17 m (difficult to control in small rooms)
  • Midrange (200-2000 Hz): wavelengths 17 cm - 1.7 m
  • Treble (2000-20000 Hz): wavelengths 1.7-17 cm (easily absorbed/reflected)
  • Ultrasound (>20 kHz): wavelengths < 1.7 cm (used in medical imaging)

Antenna Results

What the numbers mean:

  • Physical length: The actual length to cut your antenna element
  • Velocity factor adjustment: Real antennas are shorter than the theoretical free-space calculation due to end effects and conductor properties

Practical considerations:

  • The calculated length is a starting point; final tuning requires an antenna analyzer
  • ¼ wave antennas need a ground plane (radials or car body)
  • ½ wave dipoles are balanced; feed point impedance is ~73Ω
  • Higher frequencies = shorter antennas (easier to build)
  • HF antennas (3-30 MHz) can be physically large; consider space constraints

Wavenumber Results

What the numbers mean:

  • Spectroscopic wavenumber (cm⁻¹): Number of wavelengths per centimeter. Standard unit in infrared spectroscopy
  • Angular wavenumber (rad/m): Related to spatial frequency; appears in wave equations

Typical ranges in spectroscopy:

  • Far-IR / THz: 10-400 cm⁻¹
  • Mid-IR (most common for organic chemistry): 400-4000 cm⁻¹
  • Near-IR: 4000-14000 cm⁻¹
  • Visible: 14000-25000 cm⁻¹
  • UV: 25000-50000 cm⁻¹

Comparison: Electromagnetic vs. Sound vs. Matter Waves

This calculator handles three fundamentally different types of waves. Understanding their differences helps you choose the right calculation.

PropertyEM WavesSound WavesMatter Waves
What oscillatesElectric and magnetic fieldsPressure in mediumQuantum probability amplitude
Requires mediumNo (travels through vacuum)Yes (air, water, solid)No (quantum phenomenon)
Typical speed299,792,458 m/s (in vacuum)343 m/s in airParticle-dependent
Speed varies withMedium (slower in glass, water)Medium, temperatureParticle velocity
Wavelength range10⁻¹² m to 10⁴ m0.017 m to 17 m (audible)10⁻¹² m to 10⁻⁹ m (typical)
Formulaλ = c/fλ = vsound/fλ = h/(mv)
Governing equationMaxwell's equationsWave equation in fluidsSchrödinger equation
ApplicationsRadio, light, X-raysMusic, sonar, ultrasoundElectron 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.

Related Guides

Dive deeper into wave physics with our comprehensive guides. Each article expands on the concepts used in this calculator.

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More Physics Resources

Expand your understanding with these additional guides covering related topics:

Frequently Asked Questions

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.

Did You Know?

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