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  • Liquid Density: Definition, Factors & Units
    Liquid density is a physical property that measures the mass of a liquid per unit volume. It is defined as the ratio of the mass of a liquid to its volume and is expressed in units such as grams per cubic centimeter (g/cm³), kilograms per liter (kg/L), or pounds per gallon (lb/gal).

    The density of a liquid can vary depending on its temperature and pressure. In general, the density of a liquid decreases as the temperature increases and increases as the pressure increases. This is because as the temperature increases, the molecules of the liquid move faster and take up more space, resulting in a lower density. As the pressure increases, the molecules are forced closer together, resulting in a higher density.

    The density of a liquid is important for a number of reasons. For example, it is used to determine the buoyancy of objects in water, to calculate the amount of liquid in a container, and to design ships and other vessels that float.

    Here are some examples of the densities of common liquids at room temperature (25°C) and atmospheric pressure:

    - Water: 1 g/cm³ (1000 kg/L, 8.34 lb/gal)

    - Milk: 1.03 g/cm³ (1030 kg/L, 8.59 lb/gal)

    - Olive oil: 0.91 g/cm³ (910 kg/L, 7.58 lb/gal)

    - Gasoline: 0.75 g/cm³ (750 kg/L, 6.24 lb/gal)

    - Ethanol (alcohol): 0.79 g/cm³ (790 kg/L, 6.58 lb/gal)

    - Mercury: 13.6 g/cm³ (13,600 kg/L, 113 lb/gal)

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