Explore reflectivity for Earth, planets, and experiments easily. Switch modes to solve any missing value. Export results, verify ranges, and learn the physics here.
Albedo is a dimensionless reflectivity ratio. For the same wavelength band and geometry, it is the fraction of incoming radiant flux that is reflected.
For physical realism, check that incoming radiation is positive and that reflected radiation does not exceed incoming radiation for the same measurement conditions.
| Surface | Incoming (W/m²) | Reflected (W/m²) | Albedo | Absorbed (W/m²) |
|---|---|---|---|---|
| Fresh snow | 1000 | 850 | 0.85 | 150 |
| Dry sand | 1000 | 400 | 0.40 | 600 |
| Open ocean | 1000 | 60 | 0.06 | 940 |
Values are illustrative and vary with sun angle and wavelength band.
Albedo is the fraction of incoming radiation reflected by a surface, so it directly controls how much energy is available for heating, melting, or driving evaporation. It is central to surface energy budgeting in many applications. In field work, albedo is often computed from measured irradiance and reflected flux collected over the same interval.
Bright surfaces tend to have higher albedo. Fresh snow can reach about 0.80 to 0.85, while open ocean is commonly below 0.10. Dry sand is often near 0.40 and new concrete can be around 0.55. These ranges help you spot unrealistic inputs quickly.
Earth’s average planetary albedo is about 0.30, meaning roughly 30% of incoming sunlight is reflected back to space. With a solar constant near 1361 W/m², the globally averaged incoming flux is about 340 W/m² after spherical averaging. A 0.30 albedo implies about 102 W/m² reflected and about 238 W/m² absorbed before greenhouse effects redistribute energy.
The core relationship is ρ = R / I, where R is reflected radiation and I is incoming radiation in the same band and geometry. The tool also reports absorptivity (1 − ρ) and absorbed flux (I − R), which are useful when you connect albedo to heating rates.
Albedo is not a single constant for most materials. It changes with solar zenith angle, surface roughness, moisture, and wavelength. For water, reflection increases at low sun angles, while snow albedo can drop as grains grow or become dirty. Keep your measurement conditions consistent.
In climate studies, albedo helps explain feedbacks such as melting ice lowering reflectivity and accelerating warming. In engineering, roof coatings and pavements are compared by albedo to estimate cooling potential, peak surface temperature reduction, and comfort improvements.
Incoming radiation should be positive, and reflected radiation should not exceed incoming radiation for the same timestamp and sensor alignment. If you compute albedo outside 0 to 1, it often indicates unit mismatch, shading, saturation, or a time offset between measurements.
Use the dataset box to process many observations at once. The calculator returns per-line albedo plus summary statistics such as mean, minimum, maximum, and standard deviation. This is helpful for comparing sites, quantifying variability during the day, or validating remote-sensing estimates against ground measurements.
It depends on the surface. Snow can be near 0.85, sand near 0.40, vegetation near 0.15 to 0.25, and open ocean often below 0.10. Use local conditions and wavelength band.
Usually a measurement issue: mismatched units, sensor tilt, shading, time mismatch, or reflected flux contaminated by nearby bright objects. Confirm both readings use the same unit and time window.
No. Albedo is reflectivity for incoming radiation, typically solar wavelengths. Emissivity describes how efficiently a surface emits thermal infrared radiation. Some materials can have low albedo but high emissivity.
Classical albedo refers to reflected shortwave sunlight. If you use longwave values, you are mixing concepts and results may not represent reflectivity. Use consistent bands for both incoming and reflected terms.
Clouds change the incoming spectrum and add diffuse light, which can shift apparent albedo. Rapidly varying clouds can also desynchronize sensors. Average over stable intervals and record sky conditions.
Absorbed flux (I − R) is the energy per area retained by the surface in that band. Higher absorbed flux generally means stronger surface heating, assuming similar wind, moisture, and thermal properties.
Include enough to capture variability. For stable lab surfaces, a few dozen may suffice. For outdoor campaigns, hundreds across different sun angles improve statistics and help identify outliers.
Generated: 2026-01-25 05:34
No computed result to print.
Important Note: All the Calculators listed in this site are for educational purpose only and we do not guarentee the accuracy of results. Please do consult with other sources as well.