Video Experimental Relacionado
Updated: Jul 5, 2026

10:29
Experimental Methodology for Estimation of Local Heat Fluxes and Burning Rates in Steady Laminar Boundary Layer Diffusion Flames
Published on: June 1, 2016
¿Por qué la temperatura del universo es 2.726 Kelvin?
Resumen
El satélite Cosmic Background Explorer midió la temperatura del universo en 2.726 grados Kelvin. Esta medición precisa ayuda a comprender el universo temprano, la síntesis de elementos y los misterios cosmológicos actuales como la materia oscura.
Área de la Ciencia:
- Cosmología Cosmología.
- La astrofísica es la astrofísica.
Sus antecedentes:
- La temperatura del universo es un parámetro fundamental.
- Comprender su origen es clave para la cosmología.
Objetivo del estudio:
- Para presentar la medición más precisa de la temperatura del universo.
- Para conectar esta medición con las características cosmológicas fundamentales y los problemas actuales.
Principales métodos:
- Utilizando datos del satélite Explorador del Fondo Cósmico.
- Medición de alta precisión de la radiación cósmica de fondo de microondas.
Principales resultados:
- Se ha determinado que la temperatura del universo es de 2,726 +/- 0,01 Kelvin.
- Este valor está vinculado a la época temprana dominada por la radiación.
Conclusiones:
- La medición de la temperatura apoya los modelos del universo temprano, incluida la nucleosíntesis y la asimetría materia-antimateria.
- Destaca las áreas de investigación en curso, como la formación de estructuras y la identificación de la materia oscura.
Videos de Conceptos Relacionados
Enthalpy
Chemists ordinarily use a property known as enthalpy (H) to describe the thermodynamics of chemical and physical processes. Enthalpy is defined as the sum of a system’s internal energy (E) and the mathematical product of its pressure (P) and volume (V):
Entropy
Salt particles that have dissolved in water never spontaneously come back together in solution to reform solid particles. Moreover, a gas that has expanded in a vacuum remains dispersed and never spontaneously reassembles. The unidirectional nature of these phenomena is the result of a thermodynamic state function called entropy (S). Entropy is the measure of the extent to which the energy is dispersed throughout a system, or in other words, it is proportional to the degree of disorder of a...
Radiation: Applications
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...
Entropy
The first law of thermodynamics is quantitatively formulated via an equation relating the internal energy of a system, the heat exchanged by it, and the work done on it. A quantitative formulation of the second law of thermodynamics leads to defining a state function, the entropy.
When an ideal gas expands isothermally, the disorder in the gas increases. From the molecular perspective, the gas molecules have more volume to move around in.
Consider an infinitesimal step in the expansion, which...
When an ideal gas expands isothermally, the disorder in the gas increases. From the molecular perspective, the gas molecules have more volume to move around in.
Consider an infinitesimal step in the expansion, which...
Entropy and the Second Law of Thermodynamics
The second law of thermodynamics can be stated quantitatively using the concept of entropy. Entropy is the measure of disorder of the system.
The relation between entropy and disorder can be illustrated with the example of the phase change of ice to water. In ice, the molecules are located at specific sites giving a solid state, whereas, in a liquid form, these molecules are much freer to move. The molecular arrangement has therefore become more randomized. Although the change in average...
The relation between entropy and disorder can be illustrated with the example of the phase change of ice to water. In ice, the molecules are located at specific sites giving a solid state, whereas, in a liquid form, these molecules are much freer to move. The molecular arrangement has therefore become more randomized. Although the change in average...
Entropy and the Second Law of Thermodynamics
Consider an isolated system in which a hot object is placed in contact with a cold one. This is an irreversible process that eventually leads both objects to reach the same equilibrium temperature. It is crucial to note that the constituents of any substance exhibit increased disorder at higher temperatures. As a cold substance absorbs heat, its constituents become more disordered. The energy transfer from a hotter object to a cooler one increases the system's disorder or randomness. This...

