temperature$82144$ - definizione. Che cos'è temperature$82144$
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Cosa (chi) è temperature$82144$ - definizione

ESTIMATED TEMPERATURE OF AN ASTRONOMICAL BODY
Effective Temperature; Stellar temperature; Surface temperature (star); Solar temperature
  • The effective temperature of the [[Sun]] (5777 [[kelvin]]s) is the temperature a black body of the same size must have to yield the same total emissive power.

Absolute Temperature         
  • '''Figure 2.5''' This simulation illustrates an argon atom as it would appear through a 400-power optical microscope featuring a reticle graduated with 50-micron (0.05 mm) tick marks. This atom is moving with a velocity of 14.43 microns per second, which gives the atom a kinetic temperature of one-trillionth of a kelvin. The atom requires 13.9 seconds to travel 200 microns (0.2 mm). Though the atom is being invisibly jostled due to zero-point energy, its translational motion seen here comprises all its kinetic energy.
  • '''Figure 7''' Water's temperature does not change during phase transitions as heat flows into or out of it. The total heat capacity of a mole of water in its liquid phase (the green line) is 7.5507 kJ.
  • [[Joseph Louis Gay-Lussac]]
  • [[Guillaume Amontons]]
  • [[Johann Heinrich Lambert]]
  • [[Jacques Alexandre César Charles]]
  • [[Macquorn Rankine]]
ABSOLUTE MEASURE OF TEMPERATURE
Absolute temperature; Absolute Temperature; Thermodynamic temperature scale; Kelvin temperature; Temperature (thermodynamic); Atoms can have zero kinetic velocity and simultaneously be vibrating due to zero-point energy
Temperature reckoned from absolute zero (see "Zero, Absolute"). It is obtained by adding for the centigrade scale 273, and for the Fahrenheit scale 459, to the degree readings of the regular scale.
absolute temperature         
  • '''Figure 2.5''' This simulation illustrates an argon atom as it would appear through a 400-power optical microscope featuring a reticle graduated with 50-micron (0.05 mm) tick marks. This atom is moving with a velocity of 14.43 microns per second, which gives the atom a kinetic temperature of one-trillionth of a kelvin. The atom requires 13.9 seconds to travel 200 microns (0.2 mm). Though the atom is being invisibly jostled due to zero-point energy, its translational motion seen here comprises all its kinetic energy.
  • '''Figure 7''' Water's temperature does not change during phase transitions as heat flows into or out of it. The total heat capacity of a mole of water in its liquid phase (the green line) is 7.5507 kJ.
  • [[Joseph Louis Gay-Lussac]]
  • [[Guillaume Amontons]]
  • [[Johann Heinrich Lambert]]
  • [[Jacques Alexandre César Charles]]
  • [[Macquorn Rankine]]
ABSOLUTE MEASURE OF TEMPERATURE
Absolute temperature; Absolute Temperature; Thermodynamic temperature scale; Kelvin temperature; Temperature (thermodynamic); Atoms can have zero kinetic velocity and simultaneously be vibrating due to zero-point energy
¦ noun a temperature measured from absolute zero in kelvins.
Thermodynamic temperature         
  • '''Figure 2.5''' This simulation illustrates an argon atom as it would appear through a 400-power optical microscope featuring a reticle graduated with 50-micron (0.05 mm) tick marks. This atom is moving with a velocity of 14.43 microns per second, which gives the atom a kinetic temperature of one-trillionth of a kelvin. The atom requires 13.9 seconds to travel 200 microns (0.2 mm). Though the atom is being invisibly jostled due to zero-point energy, its translational motion seen here comprises all its kinetic energy.
  • '''Figure 7''' Water's temperature does not change during phase transitions as heat flows into or out of it. The total heat capacity of a mole of water in its liquid phase (the green line) is 7.5507 kJ.
  • [[Joseph Louis Gay-Lussac]]
  • [[Guillaume Amontons]]
  • [[Johann Heinrich Lambert]]
  • [[Jacques Alexandre César Charles]]
  • [[Macquorn Rankine]]
ABSOLUTE MEASURE OF TEMPERATURE
Absolute temperature; Absolute Temperature; Thermodynamic temperature scale; Kelvin temperature; Temperature (thermodynamic); Atoms can have zero kinetic velocity and simultaneously be vibrating due to zero-point energy
Thermodynamic temperature is a quantity defined in thermodynamics as distinct from kinetic theory or statistical mechanics.

Wikipedia

Effective temperature

The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation. Effective temperature is often used as an estimate of a body's surface temperature when the body's emissivity curve (as a function of wavelength) is not known.

When the star's or planet's net emissivity in the relevant wavelength band is less than unity (less than that of a black body), the actual temperature of the body will be higher than the effective temperature. The net emissivity may be low due to surface or atmospheric properties, including greenhouse effect.