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      "body": "Desde hace muchos años la física clásica ha intentado describir uno de los enigmas más importantes, la gravedad, unos de los autores principales en tratar de deducir dicho fenómeno fue Isaac Newton, quien describía de manera sencilla que, dos objetos pueden atraerse de acuerdo a su masa y a la distancia entre sus centros, es decir, si la masa aumenta su volumen la fuerza de atracción aumentará, y si la distancia entre los dos objetos aumenta la fuerza disminuirá. Sin embargo, esta teoría encuentra su propio límite en escenarios donde los objetos son supermasivos, en ese momento la teoría de Newton no hace predicciones exactas. \n\n<center>\n![](https://steemitimages.com/DQmQCWEJcmudu4fUEvjtXDnnbnCbqwTBbb7Lun9XRVEfSN6/image.png)\n[FUENTE](http://www.astromia.com/astronomia/gravita.htm)\n</center>\n<center>\n![](https://steemitimages.com/DQmdYYKvhtmvD9q3jM3pEQhQbX2p8nL8HWG3o91HegHea5P/image.png)\n</center>\n\nUna interpretación sencilla de la teoría de Newton es pensar en el siguiente escenario: el sol y la tierra son dos masas las cuales tienen entre si una distancia x que las separa y cada una de ellas tiene una masa determinada, es decir, la tierra se encuentra en la órbita alrededor del sol debido a la fuerza de atracción que ejerce una sobre la otra, supongamos que el sol desapareciera de repente, la tierra saldría expulsada de inmediato sin rumbo en el basto universo, esto debido a que el sol tiene mayor volumen en masa.\n\n<center>\n![](https://steemitimages.com/DQmZdQcuAnhckTHJCyxRsG7YemHYia3S1caVfA4dSB75aAK/image.png)\n[FUENTE](https://es.wikipedia.org/wiki/Gravedad)\n</center>\n\nNo fue hasta 1905 cuando Albert Einstein en su teoría de la relatividad especial introdujo conceptos que revolucionaron la forma de entender el universo. Esta teoría se presenta basándose en que la velocidad de la luz es igual en todos los sistemas de referencia inerciales. Dicha teoría Einstein la presenta como relatividad “especial” porque solo se aplica donde la curvatura del espacio-tiempo debido a la gravedad es despreciable. \n<center>\n![](https://steemitimages.com/DQmcmCN69oMufoed2DPUWxUjq6vr3xV1fLtPFsocb2h17ov/image.png)\n[FUENTE](https://es.wikipedia.org/wiki/Albert_Einstein)\n</center>\n\nLa teoría de la relatividad especial se basa en ecuaciones que chocan con el sentido común de las personas, entre ellas tenemos: contracción espacial, dilatación del tiempo y otras. \n\n<h1>Contracción espacial</h1>\n\nBásicamente representa un efecto relativista donde la longitud de un cuerpo en movimiento se contrae a medida que la velocidad va tendiendo a la velocidad de la luz.\n<center>\n![](https://steemitimages.com/DQmdZ1oZkWB8KAsDvvYjTW6bmei6YVzrhs1rihQNfRdT6gV/image.png)\n[FUENTE](https://es.wikipedia.org/wiki/Contracci%C3%B3n_de_Lorentz)\n</center>\n\n<h1>Dilatación del tiempo</h1>\n\nEste es un fenómeno planteado por la teoría de la relatividad, en el cual se dice que un observador en reposo que tiene un reloj exactamente igual a otro reloj donde el observador está en movimiento, pasará más lento el tiempo donde esté el observador en movimiento. \n\nEn este caso se aplica el ejemplo de los gemelos, donde ambos tienen un reloj exactamente igual, uno de ellos hace un viaje espacial en el cual va a velocidades cercanas a la velocidad de la luz, y el otro se queda en la tierra. De regreso el gemelo viajero es más joven que el gemelo que se quedó en la tierra.\n<center>\nhttps://upload.wikimedia.org/wikipedia/commons/e/eb/Time_dilation02.gif\n[FUENTE](https://es.wikipedia.org/wiki/Dilataci%C3%B3n_del_tiempo)\n</center>\n\nNo fue hasta 1915-1916 donde Albert Einstein introdujo el concepto de gravedad en la teoría, llamándola así Teoría de la relatividad general. Ésta es una teoría del campo gravitatorio y los sistemas de referencia generales. Esta teoría generaliza la llamada teoría de la relatividad especial. Los principios fundamentales de esta teoría son: el principio de equivalencia, la noción de la curvatura del espacio-tiempo y el principio de la covariancia.\n\nEinstein básicamente postuló en esta teoría que en un punto determinado no se puede distinguir experimentalmente entre un objeto acelerado uniformemente y un objeto gravitatorio uniforme. \n<center>\n![](https://steemitimages.com/DQmaEEa9ojjb16FddZC4FJGzDucaMrkcyzY9Mmp1kSXK8zp/image.png)\n[FUENTE](https://www.investigacionyciencia.es/blogs/astronomia/17/posts/cien-aos-de-relatividad-general-fundamentos-y-cosmologa-13622)\n</center>\n\nLa teoría de la relatividad general así como la relatividad especial comparten aspectos importantes, entre ellos está el principio de que nada viaja más rápido que la luz. Esto explica que los cambios en el campo gravitatorio no pueden ocurrir en todas partes instantáneamente, estos deben propagarse. A estos cambios gravitatorios que se propagan se les llama ondas gravitacionales. \n\nLas ondas gravitacionales es un fenómeno físico planteado por Albert Einstein en 1916 en su teoría de la relatividad general. Este fenómeno trata de fluctuaciones que se generan en la curvatura del espacio-tiempo las cuales se propagan en forma de ondas alejándose de su fuente. \n<center>\n![](https://steemitimages.com/DQmXNGyCuvMc1g6X13GBMnTdcrQfLJADoEmrPwd5vTUY183/image.png)\n[FUENTE](https://medium.com/starts-with-a-bang/what-is-the-future-of-gravitational-wave-astronomy-fc9bcc9efe39)\n</center>\n\nLas ondas gravitacionales se originan cuando dos o más cuerpos masivos interactúan en el espacio. Dependiendo de la distancia de estos cuerpos con respecto a la tierra, las ondas al llegar a la tierra ya son más débiles, han perdido fuerza. Ya que son débiles al llegar a la tierra es difícil detectarlas, los científicos necesitan instrumentos muy sensible para apenas percibir dichas ondas. \n\nLas ondas gravitacionales representan una gran importancia para la comprensión y explicación de muchas leyes físicas. Este fenómeno puede dar información sobre el origen del universo y como se forman o mueren las estrellas o agujeros negros. \n\nPor otro lado, para los científicos este fenómeno podría ser una visión directa de ver el universo una fracción de segundo después del Big Bang.",
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      "body": "For many years classical physics has tried to describe one of the most important enigmas, gravity, one of the main authors in trying to deduce this phenomenon was Isaac Newton, who described in a simple way that two objects can be attracted according to their mass and the distance between their centers, that is, if the mass increases its volume the force of attraction will increase, and if the distance between the two objects increases the force will decrease. However, this theory finds its own limit in scenarios where objects are supermassive, at that time Newton's theory does not make exact predictions.\n\n<center>\n![](https://steemitimages.com/DQmQCWEJcmudu4fUEvjtXDnnbnCbqwTBbb7Lun9XRVEfSN6/image.png)\n[FUENTE](http://www.astromia.com/astronomia/gravita.htm)\n</center>\n<center>\n![](https://steemitimages.com/DQmdYYKvhtmvD9q3jM3pEQhQbX2p8nL8HWG3o91HegHea5P/image.png)\n</center>\n\nA simple interpretation of Newton's theory is to think of the following scenario: the sun and the earth are two masses which have a distance \"x\" separating them and each one of them has a certain mass, that is, the Earth is in the orbit around the sun due to the force of attraction that exerts one on the other, suppose the sun disappeared suddenly, the earth would be ejected immediately without direction in the vast universe, this because the sun has greater volume in mass. \n<center>\n![](https://steemitimages.com/DQmZdQcuAnhckTHJCyxRsG7YemHYia3S1caVfA4dSB75aAK/image.png)\n[FUENTE](https://es.wikipedia.org/wiki/Gravedad)\n</center>\n\nIt was not until 1905 when Albert Einstein in his theory of special relativity introduced concepts that revolutionized the way of understanding the universe. This theory is presented on the basis that the speed of light is the same in all inertial reference systems. This theory Einstein presents as \"special\" relativity because it only applies where the curvature of spacetime due to gravity is negligible.\n<center>\n![](https://steemitimages.com/DQmcmCN69oMufoed2DPUWxUjq6vr3xV1fLtPFsocb2h17ov/image.png)\n[FUENTE](https://es.wikipedia.org/wiki/Albert_Einstein)\n</center>\n\nThe theory of special relativity is based on equations that clash with the common sense of people, among them we have: spatial contraction, time dilation and others.\n\n<h1>Spatial contraction</h1>\n\nBasically it represents a relativistic effect where the length of a body in motion contracts as the speed tends to the speed of light.\n<center>\n![](https://steemitimages.com/DQmdZ1oZkWB8KAsDvvYjTW6bmei6YVzrhs1rihQNfRdT6gV/image.png)\n[FUENTE]( https://es.wikipedia.org/wiki/Contracci%C3%B3n_de_Lorentz)\n</center>\n\n<h1>Dilation of time</h1>\n\nThis is a phenomenon posed by the theory of relativity, in which it is said that an observer at rest who has a clock exactly like another clock where the observer is in motion, will slow down the time the observer is in motion.\n\nIn this case the example of the twins is applied, where both have a clock exactly the same, one of them makes a space trip in which it goes at speeds close to the speed of light, and the other stays on the ground. On the way back the traveling twin is younger than the twin who stayed on the earth.\n<center>\nhttps://upload.wikimedia.org/wikipedia/commons/e/eb/Time_dilation02.gif\n[FUENTE](https://es.wikipedia.org/wiki/Dilataci%C3%B3n_del_tiempo)\n</center>\n\nIt was not until 1915-1916 that Albert Einstein introduced the concept of gravity in theory, calling it Theory of General Relativity. This is a theory of the gravitational field and the general reference systems. This theory generalizes the so-called theory of special relativity. The fundamental principles of this theory are: the principle of equivalence, the notion of the curvature of space-time and the principle of covariance.\n\nEinstein basically postulated in this theory that at a certain point one can not distinguish experimentally between a uniformly accelerated object and a uniform gravitational object.\n<center>\n![](https://steemitimages.com/DQmaEEa9ojjb16FddZC4FJGzDucaMrkcyzY9Mmp1kSXK8zp/image.png)\n[FUENTE](https://www.investigacionyciencia.es/blogs/astronomia/17/posts/cien-aos-de-relatividad-general-fundamentos-y-cosmologa-13622)\n</center>\n\nThe theory of general relativity as well as special relativity share important aspects, among them is the principle that nothing travels faster than light. This explains that changes in the gravitational field can not occur everywhere instantaneously, they must propagate. These gravitational changes that propagate are called gravitational waves.\n\nGravitational waves is a physical phenomenon raised by Albert Einstein in 1916 in his theory of general relativity. \nThis phenomenon deals with fluctuations that are generated in the curvature of space-time which propagate in the form of waves moving away from their source.\n<center>\n![](https://steemitimages.com/DQmXNGyCuvMc1g6X13GBMnTdcrQfLJADoEmrPwd5vTUY183/image.png)\n[FUENTE](https://medium.com/starts-with-a-bang/what-is-the-future-of-gravitational-wave-astronomy-fc9bcc9efe39)\n</center>\n\nGravitational waves originate when two or more massive bodies interact in space. Depending on the distance of these bodies from the earth, the waves when they reach the earth are weaker, they have lost strength. Since they are weak when they reach the earth it is difficult to detect them, scientists need very sensitive instruments to barely perceive these waves.\n\nGravitational waves represent a great importance for the understanding and explanation of many physical laws. This phenomenon can give information about the origin of the universe and how stars or black holes are formed or die.\n\nOn the other hand, for scientists this phenomenon could be a direct vision of seeing the universe a fraction of a second after the Big Bang.",
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