Understanding Lamberts to Apostilbs Conversion
The lambert (L) is a CGS unit of luminance defined so that a perfectly diffusing surface emitting or reflecting 1 lumen per square centimetre has a luminance of 1 lambert. The apostilb (asb) is a photometric unit of luminance equal to one lumen per square metre of a perfect diffuser, or equivalently candela per square metre. Both belong to the older brightness-measurement conventions still encountered in optics, illumination engineering, and historical instrument documentation.
Conversion Formula
To convert Lamberts to Apostilbs, multiply by this factor:
Step-by-Step Example
Convert 25 Lamberts to Apostilbs.
How to Convert Lamberts to Apostilbs
Both units measure luminance, so conversion is a clean multiplication by a whole number.
- Record the luminance in lamberts: note the value in L.
- Multiply by 10,000: this scales from lumens per cm² to lumens per m².
- Calculate: for 25 L, compute .
- Report the result: the luminance is 250,000 asb.
lamberts to apostilbs conversion table
| lamberts (L) | apostilbs (asb) |
|---|---|
| 0 | 0 |
| 1 | 10000 |
| 2 | 20000 |
| 3 | 30000 |
| 4 | 40000 |
| 5 | 50000 |
| 6 | 60000 |
| 7 | 70000 |
| 8 | 80000 |
| 9 | 90000 |
| 10 | 100000 |
| 15 | 150000 |
| 20 | 200000 |
| 25 | 250000 |
| 30 | 300000 |
| 40 | 400000 |
| 50 | 500000 |
| 60 | 600000 |
| 70 | 700000 |
| 80 | 800000 |
| 90 | 900000 |
| 100 | 1000000 |
| 150 | 1500000 |
| 200 | 2000000 |
| 250 | 2500000 |
| 300 | 3000000 |
| 400 | 4000000 |
| 500 | 5000000 |
| 600 | 6000000 |
| 700 | 7000000 |
| 800 | 8000000 |
| 900 | 9000000 |
| 1000 | 10000000 |
| 2000 | 20000000 |
| 3000 | 30000000 |
| 4000 | 40000000 |
| 5000 | 50000000 |
| 10000 | 100000000 |
| 25000 | 250000000 |
| 50000 | 500000000 |
| 100000 | 1000000000 |
| 250000 | 2500000000 |
| 500000 | 5000000000 |
| 1000000 | 10000000000 |
What is the Lambert?
The lambert is a non-SI unit of luminance, describing how much light is emitted or reflected from a surface toward an observer. It is named after the Swiss-German polymath Johann Heinrich Lambert and appears mainly in older optics, photometry, and lighting literature.
Definition
The lambert is defined so that a perfectly diffusing (Lambertian) surface emitting or reflecting a total luminous flux of one lumen per square centimetre has a luminance of one lambert.
Equivalently, . The factor of enters because luminance in candela per unit area relates to the emitted lumens per unit area through the geometry of a Lambertian (cosine-law) emitter. Sub-multiples such as the millilambert (mL) and microlambert are common in practice.
Origin and History
The unit honors Johann Heinrich Lambert (1728–1777), whose 1760 work Photometria laid the mathematical foundations of photometry, including the cosine emission law of diffuse surfaces. The lambert itself was proposed in the early 20th century as photometry was being systematized, and it saw wide use before the SI candela-per-square-metre (nit) became standard.
Law and Notable Facts
The lambert is not part of the SI and is discouraged in modern metrology, but it survives in legacy instruments and texts. A key convenience of the lambert family is that a perfect diffuse reflector illuminated by one lux has a luminance of exactly lambert, tidily linking illuminance and luminance for ideal surfaces.
Real-World Examples and Conversions
- A surface of 1 lambert equals about 3183 cd/m², roughly the brightness of a bright fluorescent lamp diffuser.
- 1 millilambert = 3.18310 cd/m², close to comfortable indoor lighting levels.
- The closely related foot-lambert (used for cinema screens) equals about 3.426 cd/m²; standard theater screen luminance of 14 fL corresponds to roughly 48 cd/m².
- 1 lambert ≈ 929.03 foot-lamberts.
What is the apostilb?
The apostilb is an obsolete unit of luminance once used to describe the brightness of diffusely reflecting or emitting surfaces. It belongs to a family of "1/π" luminance units designed to simplify calculations for perfectly diffuse (Lambertian) surfaces.
Definition
One apostilb is defined as one lumen per square metre emitted from a perfectly diffusing surface, which equals 1/π candela per square metre.
Exactly, .
Origin and History
The apostilb was part of an early-20th-century set of photometric units (alongside the lambert and foot-lambert) built around the factor 1/π so that a Lambertian surface illuminated to a given number of lux would have a numerically equal luminance. The prefix "apo-" distinguished it from the stilb.
Law and Notable Facts
The apostilb is not an SI unit and is now essentially obsolete, replaced by the candela per square metre. Its defining convenience was that a perfect diffuser receiving an illuminance of one lux has a luminance of exactly one apostilb.
Real-World Examples and Conversions
- A white matte surface at 1 lux illuminance: about 1 apostilb.
- .
- .
- .
Frequently Asked Questions
How many apostilbs are in one lambert?
Exactly 10,000 apostilbs equal one lambert, a factor that comes directly from the square-centimetre to square-metre area ratio in their definitions.
How do I convert lamberts to apostilbs?
Multiply the lambert value by 10,000. So 3 L equals 30,000 asb.
Why is the factor exactly 10,000?
Because the lambert is based on lumens per square centimetre while the apostilb is based on lumens per square metre, and there are 10,000 cm² in one m².
Where are lamberts and apostilbs used?
They appear in classical photometry, older lighting and display engineering references, and instrument calibration documents predating the SI candela-per-square-metre standard.
How do I go back from apostilbs to lamberts?
Divide the apostilb value by 10,000, which is the same as multiplying by 0.0001.
People also convert
Complete lamberts conversion table
| Unit | Result |
|---|---|
| candelas per square metre (cd/m2) | 3183.099 cd/m2 |
| nits (nt) | 3183.099 nt |
| stilbs (sb) | 0.3183099 sb |
| apostilbs (asb) | 10000 asb |
| foot-lamberts (fL) | 929.0304 fL |