💡 Illuminance Conversion Calculator 2026

Instantly convert between lux (lx), footcandles (fc), phots, millilux, nox, lumen/m², lumen/ft² and 6 more units. Trusted reference for lighting designers, photographers, architects, agronomists, and display engineers — with MathJax inverse-square law formulas, ISO/EN/IESNA recommended illuminance standards, and a 2,500+ word photometry guide.

Lux ↔ Footcandle Phot · Nox · Millilux 13+ Units Inverse Square Law ISO / IESNA Standards
⇄ Illuminance Unit Converter
Quick Presets (lux):
500 lx = 46.45 fc
Formula: value × 0.09290 (lx ÷ 10.7639)

📊 All Units — Simultaneous Conversion

📖 How to Use This Illuminance Converter

  1. 1
    Enter Your Illuminance Value

    Type any illuminance level in the Value field. The tool accepts decimals and very large or very small numbers — from starlight (0.0001 lx) to direct sunlight (100,000 lx). You can also click any Quick Preset button to instantly load a real-world reference value.

  2. 2
    Select Source and Target Units

    Choose "From Unit" (e.g., lux for international SI measurements or footcandle for US lighting specifications) and "To Unit". All 13 photometric illuminance units are available — covering SI, CGS, imperial, and derived flux-per-area formats.

  3. 3
    Read Instant Results in All Units

    The indigo result box shows your primary conversion instantly. The "All Units" panel simultaneously displays your value in every available unit — ideal for technical lighting reports, architectural specifications, or photographic exposure planning that need multiple format references.

  4. 4
    Use Quick Presets for Real-World Reference

    Six presets cover the most common illuminance scenarios — direct sunlight (100,000 lx), overcast sky (10,000 lx), office standard (500 lx), reading level (300 lx), cinema projection (100 lx), and full moonlight (0.25 lx). These let you instantly benchmark any measurement against known real-world values.

  5. 5
    Apply the Inverse Square Law Formula

    Use the MathJax formula section below to calculate how illuminance changes with distance from a point source: E = I ÷ d². If you know your luminous intensity (candela) and distance, plug into the formula to find the illuminance on a surface — crucial for architectural lighting layout, photography, and plant growth lamp positioning.

📐 Illuminance Formulas — MathJax Rendered

Illuminance — Formal Photometric Definition (SI)

\[ E_v = \frac{d\Phi_v}{dA} \quad \text{(lux, lm/m²)} \]

\( E_v = \) Illuminance (lux) · \( \Phi_v = \) Luminous flux (lumens) · \( A = \) Surface area (m²)

\( \text{Equivalently: } E_v = \frac{\Phi_v}{A} \text{ (for uniform illumination over area } A \text{)} \)

\( \text{Example: 1000 lm uniformly spread over 2 m}^2 \Rightarrow E_v = \frac{1000}{2} = 500 \text{ lux} \)

Illuminance (E_v) is defined as the luminous flux (Φ_v, in lumens) received per unit area of a surface. The SI unit is the lux (lx), equal to 1 lumen per square meter (lm/m²). This is distinct from luminous intensity (candela — how much light a source emits in a direction) and luminance (cd/m² — how bright a surface appears). Illuminance quantifies how well-lit a surface is, independently of its reflective properties. A uniformly illuminated surface with 500 lux has received 500 lumens on every square metre. The differential definition d𝚽/dA is needed for non-uniform illumination distributions (e.g., light from a nearby point source where the beam spreads unevenly).
Inverse Square Law — Distance Effect on Illuminance

\[ E_v = \frac{I_v}{d^2} \quad \text{(lux, for a point source)} \]

\( E_v = \) Illuminance (lux) · \( I_v = \) Luminous intensity (candela, cd) · \( d = \) Distance (metres)

\( \text{With angle: } E_v = \frac{I_v \cos\theta}{d^2} \quad (\theta = \text{angle between beam and surface normal}) \)

\( \text{Ratio law: } \frac{E_2}{E_1} = \left(\frac{d_1}{d_2}\right)^2 \quad \text{(double distance → quarter illuminance)} \)

The inverse square law is the most fundamental formula in illuminance calculations. Because a point source emits light in all directions, the same flux spreads over an area that grows as d² (the surface area of a sphere: 4πd²). So doubling the distance reduces illuminance by a factor of 4 (not 2). This explains why a 1,000-cd spotlight at 1 m gives 1,000 lux — but at 2 m gives only 250 lux, and at 10 m gives only 10 lux. The cosθ factor applies when the surface is tilted: a surface at a 60° angle from the beam direction receives cos(60°) = 0.5× the illuminance of a perpendicular surface. This explains why sunlight is more intense at noon (θ ≈ 0°) than at dawn (θ ≈ 80°). Caveat: the inverse square law applies only to point sources (or sources far enough that they approximate a point). For extended sources (troffers, windows, sky), more complex solid-angle integration is needed.
Unit Conversion — Lux, Footcandle, Phot, Nox

\( 1 \text{ fc (footcandle)} = 1 \text{ lm/ft}^2 = \frac{1}{0.092903} \text{ lx} \approx 10.7639 \text{ lx} \)

\( 1 \text{ lx} = 0.09290 \text{ fc} \quad \Leftrightarrow \quad 1 \text{ fc} = 10.7639 \text{ lx} \)

\( 1 \text{ ph (phot)} = 1 \text{ lm/cm}^2 = 10{,}000 \text{ lx} \quad \Rightarrow \quad 1 \text{ lx} = 10^{-4} \text{ ph} \)

\( 1 \text{ nx (nox)} = 10^{-3} \text{ lx} = 1 \text{ millilux} \quad \Rightarrow \quad 1 \text{ lx} = 1000 \text{ nx} \)

\( \text{General: } E_B = E_A \times \frac{F_A}{F_B} \quad (F = \text{lux-equivalent factor}) \)

All illuminance unit conversions use lux as the pivot. The footcandle factor derives from unit area: 1 ft² = 0.092903 m², so 1 lm/ft² = 1/0.092903 lm/m² = 10.7639 lux. The phot (CGS system) is 1 lm/cm² = 10,000 lm/m² = 10,000 lux — powerful enough for direct sunlight (approximately 10 phots). The nox (from Latin "nox" = night) is 1 millilux, used historically for very dim nighttime environments where starlight measures ~0.001 lux = 1 nox. The lumen/m² is identical to lux (they are the same unit stated two ways). The metercandle is an older synonym for lux (1 lux = illuminance from 1 standard candle at 1 metre distance, in an era when candela was defined from flame standards).
Luminous Efficacy and Lumen-to-Lux Calculation

\( \Phi_v = P \times \eta \quad \text{(lumens from power and efficacy)} \)

\( P = \text{Power (watts)} \quad \eta = \text{Luminous efficacy (lm/W)} \)

\( E_v = \frac{\Phi_v}{A} = \frac{P \times \eta}{A} \quad \text{(lux, uniformly lit area)} \)

\( \text{Number of luminaires: } N = \frac{E_{\text{required}} \times A}{\Phi_{\text{per luminaire}} \times \text{LLF} \times \text{UF}} \)

\( \text{LLF} = \text{Light Loss Factor} \quad \text{UF} = \text{Utilisation Factor} \)

The lumen method (also called the zonal cavity method) is standard practice in architectural lighting design for calculating the number of luminaires needed to achieve a target illuminance. Luminous efficacy (η, in lm/W) describes how efficiently a light source converts electrical power to visible light: a 10W LED at 100 lm/W produces 1,000 lumens. The Light Loss Factor (LLF, typically 0.7–0.85) accounts for lamp depreciation, dirt accumulation, and ballast losses over the luminaire's service life. The Utilisation Factor (UF, also called Coefficient of Utilisation in the US) accounts for room geometry — high-reflectance ceilings and walls "recycle" light more effectively, increasing effective lux per lumen. In DIALUX/Relux software, these factors are computed automatically from photometric IES/EULUMDAT files. For quick manual calculations: if you need 500 lux in a 20 m² room with LLF=0.75 and UF=0.65, you need N = (500 × 20)/(3,500 × 0.75 × 0.65) = 10,000/1,706 ≈ 5.9, so 6 luminaires of 3,500 lumens each.

📊 Complete Illuminance Unit Conversion Reference

From UnitTo lux (lm/m²)Exact FactorNotes / Use Case
1 lux (lx)1 lx1 (exact)SI base unit — international lighting standard
1 kilolux (klx)1,000 lx1,000Outdoor / horticultural grow lighting
1 millilux (mlx)0.001 lx0.001Starlight, nighttime sky glow
1 footcandle (fc)10.7639 lx1/0.092903US/Canada lighting standard — IESNA specs
1 phot (ph)10,000 lx10,000CGS unit; 1 lm/cm². Direct sunlight ≈10 phots
1 milliphot (mph)10 lx10CGS sub-unit; 0.001 phot
1 nox (nx)0.001 lx0.001Scotopic (dim) lighting; identical to millilux
1 lm/m²1 lx1 (same unit)Explicit flux-per-area form of lux
1 lm/cm²10,000 lx10,000Same as phot
1 lm/ft²10.7639 lx10.7639Same as footcandle
1 lm/in²1,550.003 lx1,550.003High-intensity spot illuminance
1 metercandle (mc)1 lx1 (exact)Historical synonym for lux

🏛️ ISO / EN / IESNA Recommended Illuminance Levels

Work Area / EnvironmentLux (lx)Footcandles (fc)Standard
☀️ Direct sunlight100,0009,290Natural
🌤️ Full daylight (overcast)10,000–20,000929–1,858Natural
🌳 Shaded outdoor area1,000–5,00093–465Natural
🏥 Operating theatre10,000–40,000929–3,716EN 12464-1 / HTM 08-03
💊 Pharmaceutical clean room500–2,00046–186GMP Guidelines / ISO 14644
🖥️ Office — screen-based work300–50028–46EN 12464-1, ISO 8995-1
📐 Drawing / technical work500–75046–70EN 12464-1 / IESNA RP-1
🏫 Classroom / lecture theatre300–50028–46EN 12464-1
📖 Library reading room300–50028–46EN 12464-1, IESNA RP-4
🏪 Retail — general merchandise300–75028–70IESNA RP-2, EN 12464-1
🍽️ Restaurant / hospitality100–3009–28IESNA RP-16
🏠 Domestic — kitchen task300–50028–46BS 8206-2
🏠 Domestic — living room50–3005–28BS 8206-2
🛣️ Road — motorway lighting1–20.09–0.19EN 13201, CIE 115
🌱 Plant growth (low light)500–2,50046–232Horticultural guidance
🌱 Plant growth (high light)10,000–50,000929–4,645Horticultural guidance
🌙 Full moon (approx.)0.1–0.30.009–0.028Natural
⭐ Starlight only0.0001–0.0010.000009–0.0001Natural

💡 Understanding Illuminance Units

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Lux (lx) — The SI Standard

The SI unit of illuminance, defined as 1 lumen per square metre (lm/m²). Adopted by the International System of Units (SI) in 1948, published in CIE Standard 017.3. Used globally in lighting engineering, architectural standards (EN 12464, ISO 8995), photography, and agriculture. The lux enables internationally consistent lighting specifications — a requirement for multinational construction projects and medical facility standards that cross regulatory jurisdictions.

🇺🇸

Footcandle (fc) — The Imperial Standard

Defined as 1 lumen per square foot (lm/ft²). 1 fc = 10.7639 lux. The name derives from the original definition: the illuminance produced by a standard candle at a distance of one foot. This unit remains dominant in the United States across all lighting sectors — IESNA publications (RP-1 through RP-31), architectural lighting contracts, building code compliance inspections, and theater/stage lighting specifications all use footcandles. The conversion factor 10.7639 = 1/(0.3048)² since 1 foot = 0.3048 m.

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Phot (ph) — CGS Extreme Unit

1 phot = 1 lm/cm² = 10,000 lux. The CGS (centimetre-gram-second) unit of illuminance — like the stilb for luminance. Direct sunlight at solar noon is approximately 10 phots (100,000 lux). The milliphot (1 mph = 10 lux) was used in some European photometry literature before SI adoption. Today both units are deprecated in favour of lux, but they still appear in pre-1970 laboratory notebooks, optics research papers, and some government archives.

🌙

Nox (nx) — Night Illuminance

1 nox = 0.001 lux = 1 millilux. From Latin nox (night). Proposed for very low light levels in the scotopic range — below 0.01 lux where rod vision dominates. Full moonlight: ~0.25 lx = 250 nox. Starlit night without moon: ~0.001 lux = 1 nox. Overcast starless night: ~0.0001 lux. The nox was recognised by the IEC but never widely standardised — millilux is now preferred. Relevant to: night photography, astronomy (sky brightness measurement in magnitudes per arcsecond²), military night vision equipment, and wildlife research on nocturnal animal behaviour.

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Lumens vs Lux — The Critical Distinction

Lumens (lm) measure total light output from a source — a property of the light fixture, independent of space. Lux (lx) measures how much of that light arrives at a surface per unit area — a property of the illuminated surface, dependent on distance and geometry. A 1,000-lumen bulb produces 1,000 lux on 1 m² (theoretical perfect sphere). In a 10 m² room it might produce only 60–80 lux (accounting for surface absorption, fixture efficiency, and room geometry). Lux is what matters for vision; lumens determine the source power required to achieve target lux levels.

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Illuminance in Photography

Camera exposure relates to illuminance via the reflected-light equation: EV = log₂(L × S / K) where L is scene luminance (cd/m²). But incident light meters measure illuminance (lux), then derive exposure using the incident-light formula: EV = log₂(E × S / C) where C = 250 (Minolta standard) or 320 (Canon/Nikon). At ISO 100 and f/8 at 1/125s, the EV is approximately 13. Direct sunlight at solar noon yields ~EV 15 (100,000 lux). Deep shade: ~EV 10 (1,000 lux). Tungsten interior: ~EV 5–7 (100–500 lux). Understanding lux-to-EV relationships allows manual exposure calculation independent of camera metering systems.

💡 Quick Conversion Memory Aid: 1 fc ≈ 10.76 lux · 1 lux ≈ 0.093 fc · 1 phot = 10,000 lux · 1 nox = 0.001 lux · 1 klx = 1,000 lux. When designing for US clients, multiply lux by 0.0929 for footcandles. When converting IESNA footcandle specs to European EN 12464 format, multiply footcandles by 10.764.

📚 Complete Guide to Illuminance — Science, Standards, and Real-World Applications

Illuminance is the foundation of all lighting design — the single numerical quantity that describes how much light arrives at a surface, and the primary metric used in every professional lighting standard worldwide. Whether you are an architect specifying luminaire layouts for an open-plan office, a horticulturalist calculating grow light intensities for a vertical farm, a photographer selecting an exposure value, or a healthcare manager ensuring surgical theatre compliance with HTM 08-03, you are working with illuminance measured in lux (or fotcandles in North American practice). Understanding illuminance — its definition, measurement, real-world reference values, and relationship to other photometric quantities — is the entry point to all of applied photometry.

The formal definition of illuminance was codified by the International Commission on Illumination (Commission Internationale de l'Éclairage — CIE) in CIE Standard 017.3:2011, the International Lighting Vocabulary. The definition: illuminance (symbol E_v) is the quotient of the luminous flux (Φ_v, in lumens) incident on a surface element divided by the area of that element: E_v = dΦ_v/dA. The SI unit is the lux (lx), equal to one lumen per square metre (1 lx = 1 lm/m²). The lux was formally adopted at the 9th meeting of the Conférence Générale des Poids et Mesures (CGPM) in 1948, consolidating earlier French, German, and British illuminance standards into a single international unit. Before 1948, illuminance was measured in metercandles (France), lux (Germany), and foot-candles (UK/US), all numerically equivalent to what we now call lux or footcandles respectively.

The inverse square law is the governing physics for illuminance from point sources — and it is perhaps the most important relationship in practical lighting design. If a point source has luminous intensity I_v (measured in candela), the illuminance at distance d from the source is E_v = I_v / d². This follows directly from the geometry of spherical wave propagation: the same luminous flux spreads over the surface area of an expanding sphere (4πd²), so flux per unit area decreases as 1/d². Practical consequence: doubling the distance from a fixture to a work surface reduces the illuminance by a factor of four, not two. A 1,000 cd spotlight at 1 m produces 1,000 lux. At 2 m: 250 lux. At 3 m: 111 lux. At 10 m: 10 lux. This dramatic fall-off is why architectural lighting design positions luminaires much closer to work surfaces than casual intuition suggests — to achieve 500 lux on a desk from a single luminaire at 3 m height, you need a luminous intensity of 500 × 3² = 4,500 cd per steradian toward the work surface.

International illuminance standards are published by three primary organisations: (1) The CIE (International Commission on Illumination) publishes foundational photometric standards (CIE 115, CIE 232); (2) ISO and CEN (European Committee for Standardisation) publish binational standards — most significantly EN 12464-1:2021 "Light and Lighting — Lighting of Work Places", which specifies maintained average illuminance (Ēm), uniformity ratio (U₀ = E_min/Ēm ≥ 0.6 for most areas), and Unified Glare Rating (UGR ≤ 19 for offices); (3) the IESNA (Illuminating Engineering Society of North America) publishes the Lighting Handbook (10th edition, 2011) and Reference Publications (RP series) specifying footcandle-based targets for the North American market. For most office environments, EN 12464-1 and IESNA RP-1 converge on 300–500 lux / 28–46 fc as the Maintained Average Illuminance.

The natural illuminance range spans approximately 10 orders of magnitude — from 0.0001 lux (starlit night) to 100,000 lux (tropical direct sunlight). The human visual system adapts to this range through pupillary constriction (a factor of ~16× in retinal light flux) and neural sensitivity adaptation (another ~5 orders of magnitude through photoreceptor gain control). The switchover between rod-dominated (scotopic) and cone-dominated (photopic) vision occurs in the mesopic range: approximately 0.001–10 lux. Below 0.01 lux, only rods function, giving high sensitivity but no colour discrimination and poor acuity. Above 10 lux, cones dominate, enabling colour vision and high spatial resolution. This transition zone is critical for road lighting design — EN 13201 specifies road lighting classes from M1 (2.0 cd/m² for motorways) down to P6 (0.5 lux for cycle paths), carefully balancing energy efficiency with safe visibility in the mesopic range.

Horticultural lighting is one of the fastest-growing applications of illuminance measurement, driven by the rapid expansion of vertical farms, greenhouse supplemental lighting, and indoor cannabis cultivation. Plants respond to photosynthetically active radiation (PAR, 400–700 nm) — measured in μmol/m²/s (PPFD), not lux. However, lux remains useful for approximating plant light requirements when spectrally calibrated PAR meters are unavailable. General conversions for common light sources: sunlight ≈ 54 μmol/m²/s per 1,000 lux; LED grow lights ≈ 15–25 μmol/m²/s per 1,000 lux (spectrum-dependent). Low-light plants (ferns, pothos): 500–2,500 lux (27–135 μmol/m²/s). Medium-light plants (ficuses, orchids): 2,500–10,000 lux. High-light food crops (lettuce, herbs): 10,000–30,000 lux. Fruiting crops (tomatoes, peppers): 30,000–80,000 lux — approaching full sunlight intensity. Modern ISO/DIS 21461 provides guidance on measuring plant-relevant light metrics including PPFD, DLI (Daily Light Integral), and spectral distribution.

Photography and cinematography use illuminance extensively for exposure planning and lighting consistency. A standard cinematography incident light meter (such as the Sekonic L-858D-U) measures illuminance at the subject position in lux or footcandles, then translates to EV (Exposure Value). The incident-light exposure formula: EV = log₂(E_v × S / C_i) where E_v is illuminance (lux), S is ISO, and C_i is the incident-light calibration constant (typically 330 for modern lux-calibrated meters, giving the key-light value that drives the exposure decision). Photography studio lighting: typically 500–2,000 lux at subject position — corresponding to EV 8–11 at ISO 100. High-speed sports photography may require 5,000–10,000 lux minimum. Motion picture production historically specified lighting levels in "book values" — a standard scene lit for ISO 400 film at T2.8 requires approximately 1,100 lux (100 fc). Modern digital cinematography at ISO 6,400, T2.8 can achieve acceptable exposure at 70 lux — enabling documentary-style "available light" shooting that was impossible on film.

⚠️ Illuminance vs Luminance — The Most Common Confusion in Lighting: Illuminance (lux) measures the light arriving at a surface — it is a property of the lighting environment. Luminance (cd/m²/nits) measures the light leaving a surface toward a viewer — it is a property of both the illuminance and the surface reflectance. Relationship: L_v = E_v × ρ / π (for a Lambertian reflector with reflectance ρ). A white wall (ρ = 0.85) under 500 lux has luminance ≈ 500 × 0.85 / π = 135 cd/m². A black wall (ρ = 0.05) under the same 500 lux has luminance ≈ 8 cd/m². Same illuminance, vastly different perceived brightness. This distinction matters for WCAG web accessibility (which uses relative luminance from screen pixel values, not room illuminance), for photography (reflected-light meters measure luminance; incident meters measure illuminance), and for display calibration standards.
Energy Efficiency and the Move to LED Lighting: Modern LED luminaires achieve luminous efficacies of 150–220 lm/W — compared to 15 lm/W for incandescent, 60–80 lm/W for fluorescent (T8), and 100–130 lm/W for metal halide. To maintain 500 lux in a 100 m² open-plan office (requiring ≈ 50,000 lm total with typical UF = 0.55 and LLF = 0.8): with T8 fluorescents at 80 lm/W: 50,000/80 = 625W of lamp power (plus 10–20% ballast loss: ~700W). With LEDs at 150 lm/W: 50,000/150 = 333W — a 53% energy saving. ASHRAE 90.1-2022 and EU Regulation 2019/2015 mandate maximum Lighting Power Densities (LPD) of 0.7–0.9 W/m² for offices, achievable only with current LED technology. For lighting design verification, use our Luminance Conversion Calculator alongside this illuminance tool.
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Written & Reviewed by Num8ers Editorial Team — Photometry, Architectural Lighting & Standards Researchers Last updated: April 2026 · Sources: CIE Standard 017.3:2011 — International Lighting Vocabulary (lux, illuminance definitions, CIE publication S 017/E) · ISO 8995-1:2002 (CIE 8995-1:2002) — Lighting of indoor workplaces, maintained illuminance values · EN 12464-1:2021 — Light and Lighting: Lighting of workplaces — indoor, EU mandatory standard · IESNA Lighting Handbook, 10th Edition (2011) — Illuminating Engineering Society of North America, footcandle-based specifications · IESNA RP-1 2012 — Recommended Practice for Office Lighting · IESNA RP-2 2012 — Illuminance recommendations for merchandising areas · ANSI/ASHRAE/IES 90.1-2022 — Energy Standard for buildings, maximum LPD values · EN 13201:2015 — Road Lighting Standard, series 1–5 · DIN 5035-3:2006 — Interior lighting standard (DE) · BS 8206-2:2008 — Lighting for buildings, daylighting, UK · HTM 08-03 (2017) — Health Technical Memorandum: Lighting in healthcare premises, DHSC UK · ISO/DIS 21461 — Lighting for plants (in development) · CIE 115:2010 — Lighting of roads for motor and pedestrian traffic · CIE 232:2019 — Discomfort Caused by Glare from Luminaires with a non-uniform Source Luminance · BIPM — Candela definition (1979, updated 2019 SI): 683 lm/W at 540 THz = maximum luminous efficacy · National Physical Laboratory (NPL) UK — Realisation of the lux, SI unit of illuminance · NIST — Special Publication 250-37, illuminance measurement procedures · Sekonic Corporation — L-858D-U Digital Master Light Meter specification (C_i = 330 constant, incident lux mode) · Peter Boyce, "Human Factors in Lighting" (3rd edition, 2014) — empirical illuminance requirements for visual tasks · DIAL GmbH — DIALUX 4.13 photometric calculation reference manual.

❓ Frequently Asked Questions — Illuminance & Light Level Conversion

What is illuminance and how does it differ from brightness?
Illuminance (measured in lux or footcandles) is the amount of luminous flux received per unit area of a surface — it measures how well-lit a surface is. Brightness is the subjective perception of luminance (cd/m²) — the light reflected or emitted by the surface toward your eye. The same illuminance can appear differently bright depending on surface reflectance: white paint (90%) and black paint (5%) under identical 500 lux look completely different because their luminance differs by 18:1. Task lighting recommendations specify illuminance, but visual comfort also depends on luminance ratios between the task, its immediate surroundings, and the background.
How do I convert lux to footcandles?
Multiply lux by 0.09290 (or divide by 10.7639).
Formula: fc = lux × 0.09290 = lux / 10.7639
Examples: 500 lux = 46.45 fc · 1,000 lux = 92.90 fc · 100,000 lux = 9,290 fc
The conversion factor 10.7639 = (1/0.3048)² because 1 foot = 0.3048 m, so 1 m² = (1/0.3048)² ft² = 10.7639 ft². Therefore 1 lm/m² = 10.7639 lm/ft², i.e., 1 fc = 10.7639 lux.
How do I convert footcandles to lux?
Multiply footcandles by 10.7639.
Formula: lux = fc × 10.7639
Examples: 50 fc = 538 lux · 100 fc = 1,076 lux · 9,290 fc = 100,000 lux (sunlight)
This is the exact reverse of the lux-to-fc formula. The IESNA Lighting Handbook uses FC throughout, while EN 12464-1 uses lux — engineers working across US/European projects must convert regularly.
What is the difference between lux and lumens?
Lumens (lm) = total light output from a source. Property of the luminaire, independent of the room. Lux (lx) = lumens per square metre. Property of the illuminated surface — depends on source lumens, distance, room geometry, and reflectances. A 1,000-lumen LED produces 1,000 lux only if all light falls perfectly on exactly 1 m² (theoretical maximum). In a real 10 m² room, accounting for wall/ceiling absorption and fixture efficiency, it might produce 50–80 lux. Formula: Lux = Lumens × Utilisation Factor × Maintenance Factor ÷ Floor Area (m²).
What recommended illuminance do offices need?
EN 12464-1:2021 (Europe / international): 500 lux maintained average (Ēm) for screen-based office work with uniformity U₀ ≥ 0.6 and UGR ≤ 19.
IESNA RP-1 (North America): 30–50 footcandles (323–538 lux) for general office, 50–75 fc (538–807 lux) for detailed tasks.
Task breakdown: Corridors: 100 lux. Reception: 200 lux. General office: 300–500 lux. Technical drawing: 500–750 lux. Colour matching/inspection: 1,000–2,000 lux. Use our calculator to convert any specification between lux and footcandles instantly.
How much lux does direct sunlight provide?
About 100,000 lux at solar noon at sea level on a clear day at mid-latitudes. This varies with: solar elevation angle (maximum in summer/tropical locations), atmospheric conditions (haze, humidity reduce it by 10–30%), altitude (every 1,000 m altitude increases UV by ~10%), and latitude. At the equinox in Northern Europe: ~50,000–70,000 lux peak. Overcast sky: 1,000–20,000 lux (diffuse skylight). Indoor window: 100–1,000 lux depending on window size, tinting, and distance from window. Understanding these values helps calibrate camera exposures, size plant grow lights, and evaluate building daylighting designs.
What is the inverse square law for light?
E = I / d², where E is illuminance (lux), I is luminous intensity (candela), and d is distance (metres). Consequences: (1) Double the distance → illuminance divided by 4. (2) Triple the distance → illuminance divided by 9. (3) To compensate for doubling distance while maintaining the same lux: increase source intensity 4×, or add 3 additional identical sources. With angled beam: E = I × cosθ / d², where θ is the angle between the light beam and the surface normal. This is why direct overhead lighting (θ = 0°) is always the most efficient angle — any tilt reduces effective lux proportionally to cosθ.
How many lux do plants need to grow?
Plant light requirements depend on species and stage. Approximate lux-based guidance:
Low light (500–2,500 lux): Ferns, pothos, snake plants, ZZ plants — suitable for rooms far from windows.
Medium (2,500–10,000 lux): Fiddle leaf figs, orchids, African violets — bright indirect light near windows.
High (10,000–30,000 lux): Herbs, lettuce, seedlings — require supplemental grow lights in most homes.
Very high (30,000-80,000 lux): Tomatoes, peppers, fruiting crops — near-full-sun conditions.
Note: for precise plant science, use PPFD (μmol/m²/s) not lux — lux weights wavelengths for human vision, not plant photosynthesis.
How do I calculate lumens needed to achieve a target lux level?
Lumens = Lux × Area (m²) ÷ (Utilisation Factor × Maintenance Factor)
For a simple approximation: Lumens total = Target lux × Room area (m²).
Example: Need 500 lux in a 6 × 4 m = 24 m² office: 500 × 24 = 12,000 lumens total (theoretical). With typical UF = 0.60, LLF = 0.80: actual lumens needed = 12,000 / (0.60 × 0.80) = 25,000 lumens. Five luminaires of 5,000 lm each would achieve this. At 100 lm/W (LED): 25,000 / 100 = 250W total installed load, giving 250/24 = 10.4 W/m² lighting power density.
What is a phot?
1 phot = 10,000 lux = 1 lumen/cm². The CGS unit of illuminance, used before SI standardisation. Direct tropical sunlight at solar noon is approximately 10 phots (100,000 lux). The phot was defined in the CGS system analogously to the stilb (luminance) and gauss (magnetic flux density). After 1960 SI adoption, phot was replaced by lux in all international standards. You will encounter phots only in pre-1970 scientific literature — NIST has explicit guidance on converting historical CGS photometric measurements to SI units. The milliphot (1 mph = 10 lux) was used for intermediate values.
What is a nox?
1 nox = 0.001 lux = 1 millilux. Proposed by CIE for measuring very low illuminances in the scotopic vision range (rod-dominated vision below ~0.01 lux). Examples: full moonlight ≈ 0.1–0.3 lux = 100–300 nox; starlit night ≈ 0.001 lux = 1 nox; starless cloudy night ≈ 0.0001 lux = 0.1 nox. The nox never achieved wide adoption — millilux (mlx) is now preferred in standards. Applications include: astronomy (measuring light pollution in terms of magnitudes per arcsecond² which converts to nox-scale illuminance), wildlife ecology (nocturnal animal behaviour experiments), and military night vision equipment specifications.
How is illuminance measured in practice?
With a lux meter (photometer / light meter) — a device with a cosine-corrected silicon photodiode filtered to match the CIE photopic luminous efficiency function V(λ). The cosine correction ensures accurate readings when light arrives at an angle. Key measurement practices: (1) Position meter at the task surface (desk top, not ceiling) with the sensor facing the dominant light source. (2) For average room illuminance, take a grid of measurements (EN 12464-1 specifies a calculation grid with spacing ≤ room index/10). (3) Allow the lamp to stabilise (20–30 minutes for fluorescent, 5 minutes for LED). (4) Record at maintained illuminance — not initial (new lamps are brighter). Common instruments: Konica Minolta T-10A, Extech LT300, HIOKI 3421. For research-grade accuracy: integrating sphere spectroradiometers (NIST traceable calibration).
What is the difference between maintained and initial illuminance?
Initial illuminance is the lux produced by new, clean luminaires with new lamps. Maintained illuminance is the average illuminance over the full maintenance cycle — after lamp depreciation, dirt accumulation, and component degradation. EN 12464-1 specifies maintained average illuminance (Ēm) — the minimum that must be achieved at any point during the maintenance cycle. The Maintenance Factor (MF) = Lamp Lumen Depreciation × Luminaire Dirt Depreciation × Room Surface Depreciation × Lamp Survival Factor. Typical MF: 0.67–0.80 for offices (cleaned 12–24 monthly). So if maintained target = 500 lux with MF = 0.75, the design initial illuminance = 500/0.75 = 667 lux. You must over-design by 33% to meet the maintained target throughout the service life.

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