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  2. Equations for a falling body - Wikipedia

    en.wikipedia.org/wiki/Equations_for_a_falling_body

    The first equation shows that, after one second, an object will have fallen a distance of 1/2 × 9.8 × 1 2 = 4.9 m. After two seconds it will have fallen 1/2 × 9.8 × 2 2 = 19.6 m; and so on. On the other hand, the penultimate equation becomes grossly inaccurate at great distances. If an object fell 10 000 m to Earth, then the results of both ...

  3. Three-body problem - Wikipedia

    en.wikipedia.org/wiki/Three-body_problem

    Mathematical description. [] The mathematical statement of the three-body problem can be given in terms of the Newtonian equations of motion for vector positions of three gravitationally interacting bodies with masses : where is the gravitational constant. 3 4 This is a set of nine second-order differential equations.

  4. List of Mobile Suit Gundam SEED Astray characters - Wikipedia

    en.wikipedia.org/wiki/List_of_Mobile_Suit_Gundam...

    In Gundam SEED Astray, however, after the "Umbrella of Artemis" is destroyed by the Blitz and the Archangel has escaped, he contracts the Serpent Tail mercenary company for defense of the base; holds Elijah Kiel hostage when he wants to acquire the Astray Red Frame to make up for the loss of the Strike; when Gai Murakumo fights with Lowe Guele ...

  5. List of The Lone Ranger episodes - Wikipedia

    en.wikipedia.org/wiki/List_of_The_Lone_Ranger...

    Jay Silverheels, Clayton Moore and Silver from The Lone Ranger.(1960). The Lone Ranger is an American Western television series that originally aired on the ABC network. The series starred Clayton Moore and Jay Silverheels as the Lone Ranger and Tonto, except for season three when John Hart played the role of the Lone Ranger.

  6. Equivalence principle - Wikipedia

    en.wikipedia.org/wiki/Equivalence_principle

    The equivalence principle is the hypothesis that the observed equivalence of gravitational and inertial mass is a consequence of nature. The weak form, known for centuries, relates to masses of any composition in free fall taking the same trajectories and landing at identical times. The extended form by Albert Einstein requires special ...

  7. Gravitational acceleration - Wikipedia

    en.wikipedia.org/wiki/Gravitational_acceleration

    Gravitational acceleration. In physics, gravitational acceleration is the acceleration of an object in free fall within a vacuum (and thus without experiencing drag). This is the steady gain in speed caused exclusively by gravitational attraction. All bodies accelerate in vacuum at the same rate, regardless of the masses or compositions of the ...

  8. Free fall - Wikipedia

    en.wikipedia.org/wiki/Free_fall

    Free fall. In classical mechanics, free fall is any motion of a body where gravity is the only force acting upon it. A freely falling object may not necessarily be falling down in the vertical direction. An object moving upwards might not normally be considered to be falling, but if it is subject to only the force of gravity, it is said to be ...

  9. Weightlessness - Wikipedia

    en.wikipedia.org/wiki/Weightlessness

    Weightlessness is the complete or near-complete absence of the sensation of weight, i.e., zero apparent weight. It is also termed zero g-force, or zero-g (named after the g-force) [ 1 ] or, incorrectly, zero gravity. Microgravity environment is more or less synonymous in its effects, with the recognition that g-forces are never exactly zero.