1
kg/m³
0.001
g/cm³
0.062428
lb/ft³
0.001
kg/L
1
kg/m³
1
kg/m³
0.001
g/cm³
0.062428
lb/ft³
0.001
kg/L
1
kg/m³
The Density Conversion Calculator converts density values between four commonly used units: kg/m³, g/cm³, lb/ft³, and kg/L. Density is defined as mass per unit volume:
$$\rho = \frac{m}{V}$$
It is a fundamental intensive property of matter — meaning it does not depend on the size of the sample. A drop of water and an ocean of water have the same density (approximately 1000 kg/m³ at 4 °C). Density determines whether objects float or sink, governs buoyancy forces, and is critical in materials science, fluid mechanics, and chemical engineering.
The SI unit of density is kg/m³. However, the unit g/cm³ is often more convenient for solids and liquids because common materials have densities near 1–20 g/cm³. The useful equivalence is:
$$1\text{ g/cm}^3 = 1000\text{ kg/m}^3 = 1\text{ kg/L}$$
This means that g/cm³ and kg/L are numerically identical — water has a density of 1 g/cm³ = 1 kg/L = 1000 kg/m³. In US engineering, lb/ft³ (pounds per cubic foot) is standard, with water at about 62.4 lb/ft³. The conversion factor is:
$$1\text{ lb/ft}^3 = 16.01846\text{ kg/m}^3$$
Density depends on temperature and pressure. Liquids expand slightly when heated (decreasing density), while gases are highly compressible. The density of air at sea level (20 °C) is about 1.204 kg/m³, roughly 830 times less than water. Solids span a wide range: aerogel at 1–2 kg/m³, wood at 400–700 kg/m³, steel at 7800 kg/m³, and osmium (the densest natural element) at 22,590 kg/m³.
This calculator is useful for material selection in engineering design, fluid mechanics problems, buoyancy calculations, quality control in manufacturing, and any context requiring density unit conversion.
The calculator normalizes all inputs to kg/m³, then converts to each target unit:
Step 1 — Normalize to kg/m³:
$$\rho_{base} = \begin{cases} value & \text{from kg/m}^3 \\ value \times 1000 & \text{from g/cm}^3 \\ value \times 16.01846 & \text{from lb/ft}^3 \\ value \times 1000 & \text{from kg/L} \end{cases}$$
Step 2 — Convert to each target:
$$\text{g/cm}^3 = \frac{\rho_{base}}{1000}, \quad \text{lb/ft}^3 = \frac{\rho_{base}}{16.01846}, \quad \text{kg/L} = \frac{\rho_{base}}{1000}$$
Note that g/cm³ and kg/L always give the same numerical result because 1 cm³ = 1 mL and 1000 mL = 1 L.
Water at 4 °C: 1000 kg/m³ = 1 g/cm³ = 62.43 lb/ft³ = 1 kg/L. Air at sea level (20 °C): 1.204 kg/m³. Aluminum: 2700 kg/m³ (2.7 g/cm³). Steel: 7800 kg/m³. Gold: 19,300 kg/m³. Materials with density less than water (< 1 g/cm³) float in water; those denser than water sink. Specific gravity is the ratio of a substance's density to that of water, making it a dimensionless number numerically equal to density in g/cm³.
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Water at 4 °C has a density of exactly 1000 kg/m³ = 1.000 g/cm³ = 62.43 lb/ft³. This reference value is the basis of the specific gravity scale.
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Structural steel at 490 lb/ft³ equals about 7849 kg/m³ or 7.85 g/cm³ — nearly 8 times denser than water, which is why steel sinks despite being used to build ships (the hull encloses air, reducing average density).
Density has units (kg/m³, g/cm³, etc.) and is the mass per unit volume of a substance. Specific gravity (relative density) is the dimensionless ratio of a substance's density to a reference density — usually water at 4 °C (1000 kg/m³). Since the reference is 1 g/cm³, specific gravity is numerically equal to density expressed in g/cm³. For example, gold has density 19.3 g/cm³ and specific gravity 19.3.
Because 1 cm³ = 1 mL (by definition of the millilitre) and 1000 mL = 1 L, we have 1 g/cm³ = 1 g/mL = 1000 g/L = 1 kg/L. Likewise, 1 g/cm³ = 1,000,000 g/m³ = 1000 kg/m³. This elegant relationship arises from the metric system's design, where volume and length units are consistently linked.
Most materials expand when heated, decreasing density. Water is anomalous: it reaches maximum density at 4 °C, then expands both when heated and when cooled below 4 °C (which is why ice floats). Gases are strongly affected: air density at 0 °C is about 1.293 kg/m³, decreasing to 1.204 kg/m³ at 20 °C. For precise work, always specify the temperature at which density is measured.
Osmium holds the record at 22,590 kg/m³ (22.59 g/cm³), slightly denser than iridium at 22,560 kg/m³. Both are platinum-group metals. For comparison, gold is 19,300 kg/m³ and lead is 11,340 kg/m³. The densest known substance overall is the core of a neutron star, reaching approximately 10¹⁷ kg/m³.
An object floats if its average density is less than the density of the surrounding fluid. A solid steel ball (7800 kg/m³) sinks in water (1000 kg/m³), but a hollow steel ship floats because the enclosed air brings the average density of the ship-plus-air system below 1000 kg/m³. Archimedes' principle states the buoyant force equals the weight of displaced fluid: $$F_b = \rho_{fluid} \cdot V_{submerged} \cdot g$$.
Multiply lb/ft³ by 16.01846: $$\rho_{kg/m^3} = \rho_{lb/ft^3} \times 16.01846$$. This factor comes from: 1 lb = 0.453592 kg and 1 ft³ = 0.0283168 m³, so 1 lb/ft³ = 0.453592 / 0.0283168 = 16.01846 kg/m³. For quick estimates, multiply by 16.
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