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  2. Naismith's rule - Wikipedia

    en.wikipedia.org/wiki/Naismith's_rule

    Pace [6] in minutes per kilometre or mile vs. slope angle resulting from Naismith's rule [7] for basal speeds of 5 and 4 km / h. [n 1]The original Naismith's rule from 1892 says that one should allow one hour per three miles on the map and an additional hour per 2000 feet of ascent.

  3. Fourth, fifth, and sixth derivatives of position - Wikipedia

    en.wikipedia.org/wiki/Fourth,_fifth,_and_sixth...

    Snap, [6] or jounce, [2] is the fourth derivative of the position vector with respect to time, or the rate of change of the jerk with respect to time. [4] Equivalently, it is the second derivative of acceleration or the third derivative of velocity, and is defined by any of the following equivalent expressions: = ȷ = = =.

  4. Battenberg course indicator - Wikipedia

    en.wikipedia.org/wiki/Battenberg_Course_Indicator

    The rear of the device had a separate rotating calculator, where if the ship's speed was set against the 60-minute guide mark, then the distance travelled at any time 0–60 minutes could be read off against the logarithmic time scale.

  5. Equations for a falling body - Wikipedia

    en.wikipedia.org/wiki/Equations_for_a_falling_body

    Instantaneous velocity of a falling object that has travelled distance on a planet with mass , with the combined radius of the planet and altitude of the falling object being , this equation is used for larger radii where is smaller than standard at the surface of Earth, but assumes a small distance of fall, so the change in is small and ...

  6. Motion graphs and derivatives - Wikipedia

    en.wikipedia.org/wiki/Motion_graphs_and_derivatives

    Since the velocity of the object is the derivative of the position graph, the area under the line in the velocity vs. time graph is the displacement of the object. (Velocity is on the y-axis and time on the x-axis. Multiplying the velocity by the time, the time cancels out, and only displacement remains.)

  7. Orders of magnitude (speed) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude_(speed)

    Approaching velocity of Messier 98 to our galaxy. 192,000: 690,000: 430,000 0.00064: Predicted [needs update] top speed of the Parker Solar Probe at its closest perihelion in 2024. [29] [30] 200,000: 700,000: 450,000 0.00070: Orbital speed of the Solar System in the Milky Way galaxy. 308,571: 1,080,000: 694,288 0.001: Approaching velocity of ...

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    Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

  9. Proper acceleration - Wikipedia

    en.wikipedia.org/wiki/Proper_acceleration

    For example, imagine a spaceship that can accelerate its passengers at "1 gee" (10 m/s 2 or about 1.0 light year per year squared) halfway to their destination, and then decelerate them at "1 gee" for the remaining half so as to provide earth-like artificial gravity from point A to point B over the shortest possible time. [8] [9] For a map ...

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