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Allgemeinbildung, Lexikon, Wörterbücher & Reiseführer - wissen.de

Allgemeinbildung, Lexikon, Wörterbücher & Reiseführer - wissen.de
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Hebrew for Christians - Learn Hebrew for FREE! La voiture autonome pourrait bouleverser l'immobilier Bien qu'il soit encore distant de plusieurs années, l'avènement de la voiture autonome provoque déjà des questionnements quant à ses effets secondaires dans toutes sortes de domaines. Un analyste prédit notamment un impact important sur l'immobilier. Mais pourquoi au juste ? Il ne fait aucun doute que la voiture électrique ainsi que la voiture autonome vont profondément bouleverser notre rapport à l'automobile. Mais celles-ci auront aussi un impact dans toutes sortes de domaines inattendus. Par exemple, certains observateurs pensent que la voiture électrique pourrait menacer l’industrie de la boisson en faisant disparaître les stations-service. Concernant la voiture autonome, on sait déjà qu'elle va entraîner de grandes évolutions au niveau des infrastructures urbaines. Donc, si de moins en moins de personnes possèdent une voiture, cela entraînera, de fait, une diminution du nombre de places de stationnement nécessaires. Cela vous intéressera aussi

Einführung in die Theoretische Physik - Ein Lehrbuch in mehreren Bänden – Wikibooks, Sammlung freier Lehr-, Sach- und Fachbücher Einführung in die Theoretische Physik - Ein Lehrbuch in mehreren Bänden Aus Wikibooks Wechseln zu: Navigation, Suche Dieses mehrbändige Werk steht im Regal Physik sowie im Regal Maschinenbau. Hier gibt es eine PDF-Version [1]. Von „ Kategorie: Mehrbändiges Werk Navigationsmenü Meine Werkzeuge Namensräume Varianten Ansichten Mehr Navigation Mitmachen Werkzeuge Sprachen Drucken/exportieren Diese Seite wurde zuletzt am 21.

Wikileaks - WikiLeaks welcome - library.nu L'accueil | LA GRANDE GUERRE EN DESSINS Light-time correction Light-time correction is a displacement in the apparent position of a celestial object from its true position (or geometric position) caused by the object's motion during the time it takes its light to reach an observer. Light-time correction occurs in principle during the observation of any moving object, because the speed of light is finite. The magnitude and direction of the displacement in position depends upon the distance of the object from the observer and the motion of the object, and is measured at the instant at which the object's light reaches the observer. Light-time correction can be applied to any object whose distance and motion are known. Calculation[edit] A calculation of light-time correction usually involves an iterative process. Discovery[edit] The effect of the finite speed of light on observations of celestial objects was first recognised by Ole Rømer in 1675, during a series of observations of eclipses of the moons of Jupiter. References[edit] P.

The Eucharist --It's Origin IntroductionThis paper will not prove a thing. Too much time has past, too many books and manuscripts burned, to many tracks covered by the dust of twenty centuries. We do, however, have enough information at hand to draw some reasonable conclusions concerning where Paul obtained the Eucharist and why he instituted it in the church. The previous paper entitled The Eucharist -- Not from Jesus exposed Paul as the one who instituted the Eucharist or, as he named it, the Lord's Supper. He claims to have received it directly from the Lord. We therefore accord to Paul the institution of the Eucharist in his churches -- specifically in the Corinthian church. Where Did Paul Get It? I Cor.11:23 FNTFor I received from the Lord what I have also delivered up to you, that the Lord Jesus, in the night in which he was delivered up, took bread,24and having given thanks he broke [it] and said: This is my body being broken in your behalf. Did he blatantly lie in claiming the Lord as his source? 1. 2.

Cartographie numérique Tests of special relativity Special relativity is a physical theory that plays a fundamental role in the description of all physical phenomena, as long as gravitation is not significant. Many experiments played (and still play) an important role in its development and justification. The strength of the theory lies in its unique ability to correctly predict to high precision the outcome of an extremely diverse range of experiments. Repeats of many of those experiments are still being conducted with steadily increased precision, with modern experiments focusing on effects such as at the Planck scale and in the neutrino sector. Their results are consistent with the predictions of special relativity. Collections of various tests were given by Jakob Laub,[1] Zhang,[2] Mattingly,[3] Clifford Will,[4] and Roberts/Schleif.[5] Special relativity is restricted to flat spacetime, i.e., to all phenomena without significant influence of gravitation. Experiments paving the way to relativity[edit] First-order experiments[edit]

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