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  2. Classical central-force problem - Wikipedia

    en.wikipedia.org/wiki/Classical_central-force...

    t. e. In classical mechanics, the central-force problem is to determine the motion of a particle in a single central potential field. A central force is a force (possibly negative) that points from the particle directly towards a fixed point in space, the center, and whose magnitude only depends on the distance of the object to the center.

  3. Two-body problem - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem

    A two-point-particle model of such a system nearly always describes its behavior well enough to provide useful insights and predictions. A simpler "one body" model, the "central-force problem", treats one object as the immobile source of a force acting on the other. One then seeks to predict the motion of the single remaining mobile object.

  4. Inertia - Wikipedia

    en.wikipedia.org/wiki/Inertia

    Inertia is the tendency of objects in motion to stay in motion and objects at rest to stay at rest, unless a force causes its speed or direction to change. It is one of the fundamental principles in classical physics, and described by Isaac Newton in his first law of motion (also known as The Principle of Inertia). [1]

  5. Philosophiæ Naturalis Principia Mathematica - Wikipedia

    en.wikipedia.org/wiki/Philosophiæ_Naturalis...

    Philosophiæ Naturalis Principia Mathematica. Philosophiæ Naturalis Principia Mathematica (English: The Mathematical Principles of Natural Philosophy) [ 1] often referred to as simply the Principia ( / prɪnˈsɪpiə, prɪnˈkɪpiə / ), is a book by Isaac Newton that expounds Newton's laws of motion and his law of universal gravitation.

  6. Central force - Wikipedia

    en.wikipedia.org/wiki/Central_force

    Central force. In classical mechanics, a central force on an object is a force that is directed towards or away from a point called center of force. [ a][ 1]: 93 where is the force, F is a vector valued force function, F is a scalar valued force function, r is the position vector, || r || is its length, and is the corresponding unit vector ...

  7. Copernican heliocentrism - Wikipedia

    en.wikipedia.org/wiki/Copernican_heliocentrism

    Copernican heliocentrism is the astronomical model developed by Nicolaus Copernicus and published in 1543. This model positioned the Sun at the center of the Universe, motionless, with Earth and the other planets orbiting around it in circular paths, modified by epicycles, and at uniform speeds. The Copernican model displaced the geocentric ...

  8. Geocentric model - Wikipedia

    en.wikipedia.org/wiki/Geocentric_model

    The geocentric model was the predominant description of the cosmos in many European ancient civilizations, such as those of Aristotle in Classical Greece and Ptolemy in Roman Egypt, as well as during the Islamic Golden Age . Two observations supported the idea that Earth was the center of the Universe.

  9. Reviving Hollywood glamor of the silent movie era, experts ...

    www.aol.com/entertainment/reviving-hollywood...

    July 14, 2024 at 12:53 AM. DETROIT (AP) — A massive pipe organ that underscored the drama and comedy of silent movies with live music in Detroit's ornate Hollywood Theatre nearly a century ago ...