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  2. Freezing - Wikipedia

    en.wikipedia.org/wiki/Freezing

    Most liquids freeze by crystallization, formation of crystalline solid from the uniform liquid. This is a first-order thermodynamic phase transition, which means that as long as solid and liquid coexist, the temperature of the whole system remains very nearly equal to the melting point due to the slow removal of heat when in contact with air, which is a poor heat conductor.

  3. Latent heat - Wikipedia

    en.wikipedia.org/wiki/Latent_heat

    Q is the amount of energy released or absorbed during the change of phase of the substance (in kJ or in BTU), m is the mass of the substance (in kg or in lb), and L is the specific latent heat for a particular substance (in kJ kg −1 or in BTU lb −1), either L f for fusion, or L v for vaporization.

  4. Flash freezing - Wikipedia

    en.wikipedia.org/wiki/Flash_freezing

    is the difference in free energy per unit volume between the thermodynamic phase nucleation is occurring in, and the phase that is nucleating. critical nucleus radius, at some intermediate value of r {\displaystyle {\displaystyle r}} , the free energy goes through a maximum, and so the probability of formation of a nucleus goes through a minimum.

  5. Phases of ice - Wikipedia

    en.wikipedia.org/wiki/Phases_of_ice

    Most liquids under increased pressure freeze at higher temperatures because the pressure helps to hold the molecules together. However, the strong hydrogen bonds in water make it different: for some pressures higher than 1 atm (0.10 MPa), water freezes at a temperature below 0 °C. Subjected to higher pressures and varying temperatures, ice can ...

  6. Melting point - Wikipedia

    en.wikipedia.org/wiki/Melting_point

    The melting point (or, rarely, liquefaction point) of a substance is the temperature at which it changes state from solid to liquid. At the melting point the solid and liquid phase exist in equilibrium. The melting point of a substance depends on pressure and is usually specified at a standard pressure such as 1 atmosphere or 100 kPa.

  7. Ice - Wikipedia

    en.wikipedia.org/wiki/Ice

    The amount of energy consumed in breaking hydrogen bonds in the transition from ice to water is known as the heat of fusion. [ 12 ] [ 8 ] As with water, ice absorbs light at the red end of the spectrum preferentially as the result of an overtone of an oxygen–hydrogen (O–H) bond stretch.

  8. 23 Foods to Stock Up On Before a Snow Storm - AOL

    www.aol.com/lifestyle/23-foods-stock-snow-storm...

    Snowstorm Pantry Staples. This list is a mix of shelf-stable foods, quick snacks, and emergency rations that should last you a few days. Even during a power outage, you should be able to stay ...

  9. Crystallization - Wikipedia

    en.wikipedia.org/wiki/Crystallization

    Crystallization is the process by which solids form, where the atoms or molecules are highly organized into a structure known as a crystal.Some ways by which crystals form are precipitating from a solution, freezing, or more rarely deposition directly from a gas.