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单词 effective temperature
释义
effective temperature

Physics
  • See luminosity.


Astronomy
  • The temperature of a black body that radiates the same total energy per unit area as a given object, such as a star. It is the most useful measure of a star’s surface temperature. The effective temperature of the Sun, for example, is 5800 K. However, in other circumstances it may be misleading, such as for a planetary nebula which may have a kinetic temperature (obtained from the mean energies of the particles) of 10 000 K, but an effective temperature of only 50 K because of the low density of particles. See also Colour Temperature.


Geology and Earth Sciences
  • 1. The temperature of a planetary surface in the absence of an atmosphere. The effective temperature of Earth is some 35–40  °C lower than the actual Earth surface temperature (Ts): the latter is approximately 15 °C owing to the greenhouse effect of the Earth’s atmosphere.

    2. The temperature of saturated air that, with a wind speed no greater than 0.2 m/s, would produce the same sensation of comfort in a sedentary person wearing indoor clothes as the air to which that person is actually exposed.


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