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  2. Phases of ice - Wikipedia

    en.wikipedia.org/wiki/Phases_of_ice

    Ice, water, and water vapour can coexist at the triple point, which is exactly 273.16 K (0.01 °C) at a pressure of 611.657 Pa. [14] [15] The kelvin was defined as ⁠ 1 / 273.16 ⁠ of the difference between this triple point and absolute zero, [16] though this definition changed in May 2019. [17] Unlike most other solids, ice is difficult to ...

  3. Solar granule - Wikipedia

    en.wikipedia.org/wiki/Solar_granule

    According to the Stefan–Boltzmann law, luminosity increases with the fourth power of temperature, causing even a small loss of heat to produce a large luminosity contrast.) In addition to the visible appearance, which can be explained by convective motion , Doppler shift measurements of the light from individual granules provides evidence for ...

  4. Stefan problem - Wikipedia

    en.wikipedia.org/wiki/Stefan_problem

    The classical Stefan problem aims to describe the evolution of the boundary between two phases of a material undergoing a phase change, for example the melting of a solid, such as ice to water. This is accomplished by solving heat equations in both regions, subject to given boundary and initial conditions. At the interface between the phases ...

  5. Phase transition - Wikipedia

    en.wikipedia.org/wiki/Phase_transition

    Below the boiling point, the liquid is the more stable state of the two, whereas above the boiling point the gaseous form is the more stable. Common transitions between the solid, liquid, and gaseous phases of a single component, due to the effects of temperature and/or pressure are identified in the following table:

  6. State of matter - Wikipedia

    en.wikipedia.org/wiki/State_of_matter

    A simplified phase diagram for water, showing whether solid ice, liquid water, or gaseous water vapor is the most stable at different combinations of temperature and pressure In physics , a state of matter is one of the distinct forms in which matter can exist.

  7. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The coolest layer of the Sun is a temperature minimum region extending to about 500 km above the photosphere, and has a temperature of about 4,100 K. [77] This part of the Sun is cool enough to allow for the existence of simple molecules such as carbon monoxide and water. [81]

  8. Solar activity and climate - Wikipedia

    en.wikipedia.org/wiki/Solar_activity_and_climate

    The updated figure (right) shows the variations and contrasts solar cycles 14 and 24, a century apart, that are quite similar in all solar activity measures (in fact cycle 24 is slightly less active than cycle 14 on average), yet the global mean air surface temperature is more than 1 degree Celsius higher for cycle 24 than cycle 14, showing the ...

  9. Water vapor - Wikipedia

    en.wikipedia.org/wiki/Water_vapor

    Water vapor is the "working medium" of the atmospheric thermodynamic engine which transforms heat energy from sun irradiation into mechanical energy in the form of winds. Transforming thermal energy into mechanical energy requires an upper and a lower temperature level, as well as a working medium which shuttles forth and back between both.